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2145163
10.1007/s00021-011-0075-9
We study the global existence of solutions to a two-component generalized Hunter-Saxton system in the periodic setting. We first prove a persistence result of the solutions. Then for some particular choices of parameters $(\alpha, \kappa)$, we show the precise blow-up scenarios and the existence of global solutions to the generalized Hunter-Saxton system under proper assumptions on the initial data. This significantly improves recent results obtained in [M. Wunsch, DCDS Ser. B 12 (2009), 647-656] and [M. Wunsch, SIAM J. Math. Anal. 42 (2010), 1286-1304].Comment: 22 pages; submitted in modified form on August 7, 201
Global existence for the generalized two-component Hunter-Saxton system
global existence for the generalized two-component hunter-saxton system
hunter saxton setting. persistence solutions. choices alpha kappa precise blow scenarios hunter saxton proper assumptions data. improves wunsch dcds ser. wunsch siam math. anal. .comment pages submitted august
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2256998
10.1007/s00021-012-0102-5
In order to obtain quite precise information about the shape of the particle paths below small-amplitude gravity waves travelling on irrotational deep water, analytic solutions of the nonlinear differential equation system describing the particle motion are provided. All these solutions are not closed curves. Some particle trajectories are peakon-like, others can be expressed with the aid of the Jacobi elliptic functions or with the aid of the hyperelliptic functions. Remarks on the stagnation points of the small-amplitude irrotational deep-water waves are also made.Comment: to appear in J. Math. Fluid Mech. arXiv admin note: text overlap with arXiv:1106.382
On the particle paths and the stagnation points in small-amplitude deep-water waves
on the particle paths and the stagnation points in small-amplitude deep-water waves
precise paths travelling irrotational analytic describing provided. curves. trajectories peakon jacobi elliptic hyperelliptic functions. remarks stagnation irrotational math. mech. admin overlap
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24765735
10.1007/s00021-012-0115-0
For inviscid fluid flow in any n-dimensional Riemannian manifold, new conserved vorticity integrals generalizing helicity, enstrophy, and entropy circulation are derived for lower-dimensional surfaces that move along fluid streamlines. Conditions are determined for which the integrals yield constants of motion for the fluid. In the case when an inviscid fluid is isentropic, these new constants of motion generalize Kelvin's circulation theorem from closed loops to closed surfaces of any dimension.Comment: 14 pages; typos correcte
New conserved vorticity integrals for moving surfaces in multi-dimensional fluid flow
new conserved vorticity integrals for moving surfaces in multi-dimensional fluid flow
inviscid riemannian manifold conserved vorticity integrals generalizing helicity enstrophy circulation move streamlines. integrals fluid. inviscid isentropic generalize kelvin circulation loops pages typos correcte
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5237496
10.1007/s00021-013-0145-2
In this paper we investigate the issue of the inviscid limit for the compressible Navier-Stokes system in an impermeable fixed bounded domain. We consider two kinds of boundary conditions. The first one is the no-slip condition. In this case we extend the famous conditional result obtained by Kato in the homogeneous incompressible case. Kato proved that if the energy dissipation rate of the viscous flow in a boundary layer of width proportional to the viscosity vanishes then the solutions of the incompressible Navier-Stokes equations converge to some solutions of the incompressible Euler equations in the energy space. We provide here a natural extension of this result to the compressible case. The other case is the Navier condition which encodes that the fluid slips with some friction on the boundary. In this case we show that the convergence to the Euler equations holds true in the energy space, as least when the friction is not too large. In both cases we use in a crucial way some relative energy estimates proved recently by Feireisl, Ja Jin and Novotn{\'y}
On the inviscid limit for the compressible Navier-Stokes system in an impermeable bounded domain
on the inviscid limit for the compressible navier-stokes system in an impermeable bounded domain
inviscid compressible navier stokes impermeable domain. kinds conditions. slip condition. extend famous conditional kato homogeneous incompressible case. kato proved dissipation viscous viscosity vanishes incompressible navier stokes converge incompressible euler space. compressible case. navier encodes slips friction boundary. euler friction large. crucial proved feireisl novotn
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25010138
10.1007/s00021-013-0152-3
This paper is to study global-in-time existence of weak solutions to zero Mach number system which derives from the full Navier-Stokes system, under a special relationship between the viscosity coefficient and the heat conductivity coefficient such that, roughly speaking, the source term in the equation for the newly introduced divergence-free velocity vector field vanishes. In dimension two, thanks to a local-in-time existence result of a unique strong solution in critical Besov spaces given in \cite{Danchin-Liao}, for arbitrary large initial data, we will show that this unique strong solution exists globally in time, by a weak-strong uniqueness argument
A global existence result for a zero Mach number system
a global existence result for a zero mach number system
mach derives navier stokes viscosity conductivity roughly speaking newly divergence vanishes. thanks besov cite danchin liao globally uniqueness argument
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24938985
10.1007/s00021-013-0158-x
We investigate the influence of the topography on the lake equations which describe the two-dimensional horizontal velocity of a three-dimensional incompressible flow. We show that the lake equations are structurally stable under Hausdorff approximations of the fluid domain and $L^p$ perturbations of the depth. As a byproduct, we obtain the existence of a weak solution to the lake equations in the case of singular domains and rough bottoms. Our result thus extends earlier works by Bresch and M\'etivier treating the lake equations with a fixed topography and by G\'erard-Varet and Lacave treating the Euler equations in singular domains
Topography influence on the Lake equations in bounded domains
topography influence on the lake equations in bounded domains
topography lake incompressible flow. lake structurally hausdorff approximations perturbations depth. byproduct lake singular rough bottoms. extends bresch etivier treating lake topography erard varet lacave treating euler singular
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80910310
10.1007/s00021-013-0159-9
We consider the boundary-value problem for the steady isothermal flow of an incompressible viscoelastic liquid of Oldroyd type in a bounded domain with a Navier type slip boundary condition. We prove that under some restrictions on the material constants and the data, there exists a strong solution which is locally unique. The proof is based on a fixed point argument in which the boundary-value problem is decomposed into a transport equation and a Stokes system.http://link.springer.com/journal/21hb201
On flows of viscoelastic fluids of oldroyd type with wall slip
on flows of viscoelastic fluids of oldroyd type with wall slip
steady isothermal incompressible viscoelastic oldroyd navier slip condition. restrictions locally unique. argument decomposed stokes system.
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24961257
10.1007/s00021-014-0163-8
We discuss the problem of well-posedness of the compressible (barotropic) Euler system in the framework of weak solutions. The principle of maximal dissipation introduced by C.M. Dafermos is adapted and combined with the concept of admissible weak solutions. We use the method of convex integration in the spirit of the recent work of C.DeLellis and L.Szekelyhidi to show various counterexamples to well-posedness. On the other hand, we conjecture that the principle of maximal dissipation should be retained as a possible criterion of uniqueness as it is violated by the oscillatory solutions obtained in the process of convex integration
Maximal dissipation and well-posedness for the compressible Euler system
maximal dissipation and well-posedness for the compressible euler system
posedness compressible barotropic euler solutions. maximal dissipation c.m. dafermos adapted admissible solutions. convex spirit lellis l.szekelyhidi counterexamples posedness. conjecture maximal dissipation retained criterion uniqueness violated oscillatory convex
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24998933
10.1007/s00021-014-0166-5
We give an example of a well posed, finite energy, 2D incompressible active scalar equation with the same scaling as the surface quasi-geostrophic equation and prove that it can produce finite time singularities. In spite of its simplicity, this seems to be the first such example. Further, we construct explicit solutions of the 2D Boussinesq equations whose gradients grow exponentially in time for all time. In addition, we introduce a variant of the 2D Boussinesq equations which is perhaps a more faithful companion of the 3D axisymmetric Euler equations than the usual 2D Boussinesq equations.Comment: 9 pages; simplified a solution formula in section 4 and added a sentence on the time growth rate in the solutio
An incompressible 2D didactic model with singularity and explicit solutions of the 2D Boussinesq equations
an incompressible 2d didactic model with singularity and explicit solutions of the 2d boussinesq equations
posed incompressible quasi geostrophic singularities. spite simplicity example. boussinesq gradients grow exponentially time. variant boussinesq perhaps faithful companion axisymmetric euler usual boussinesq pages simplified sentence solutio
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24957897
10.1007/s00021-014-0169-2
Time-periodic solutions to the linearized Navier-Stokes system in the $n$-dimensional whole-space are investigated. For time-periodic data in $L^q$-spaces, maximal regularity and corresponding a priori estimates for the associated time-periodic solutions are established. More specifically, a Banach space of time-periodic vector fields is identified with the property that the linearized Navier-Stokes operator maps this space homeomorphically onto the $L^q$-space of time-periodic data.Comment: 19 page
Maximal regularity of the time-periodic Navier-Stokes system
maximal regularity of the time-periodic navier-stokes system
linearized navier stokes investigated. maximal regularity priori established. banach linearized navier stokes homeomorphically
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25007006
10.1007/s00021-014-0187-0
A linear stochastic vector advection equation is considered; the equation may model a passive magnetic field in a random fluid. When the driving velocity field is rough but deterministic, in particular just H\"{o}lder continuous and bounded, one can construct examples of infinite stretching of the passive field, arising from smooth initial conditions. The purpose of the paper is to prove that infinite stretching is prevented if the driving velocity field contains in addition a white noise component.Comment: 23 pages, 4 figure
Noise prevents infinite stretching of the passive field in a stochastic vector advection equation
noise prevents infinite stretching of the passive field in a stochastic vector advection equation
stochastic advection passive fluid. driving rough deterministic lder infinite stretching passive arising conditions. infinite stretching prevented driving pages
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25050886
10.1007/s00021-015-0201-1
We investigate the long-term behavior, as a certain regularization parameter vanishes, of the three-dimensional Navier-Stokes-Voigt model of a viscoelastic incompressible fluid. We prove the existence of global and exponential attractors of optimal regularity. We then derive explicit upper bounds for the dimension of these attractors in terms of the three-dimensional Grashof number and the regularization parameter. Finally, we also prove convergence of the (strong) global attractor of the 3D Navier-Stokes-Voigt model to the (weak) global attractor of the 3D Navier-Stokes equation. Our analysis improves and extends recent results obtained by Kalantarov and Titi in [31].Comment: v2: the statement and proof of Theorem 5.2 have changed. In the previous version, the proof was based on Theorem 4.9 in a book of Ladyzhenskaya, which turns out to be based on a faulty assumption. See Remark 5.5 for detail
Singular limits of Voigt models in fluid dynamics
singular limits of voigt models in fluid dynamics
regularization vanishes navier stokes voigt viscoelastic incompressible fluid. exponential attractors regularity. derive bounds attractors grashof regularization parameter. attractor navier stokes voigt attractor navier stokes equation. improves extends kalantarov titi .comment statement changed. book ladyzhenskaya turns faulty assumption. remark
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24985820
10.1007/s00021-015-0203-z
We consider the equations of motion for an incompressible Non-Newtonian fluid in a bounded Lipschitz domain $G\subset\mathbb R^d$ during the time intervall $(0,T)$ together with a stochastic perturbation driven by a Brownian motion $W$. The balance of momentum reads as $$dv=\mathrm{div}\, S\,dt-(\nabla v)v\,dt+\nabla\pi \,dt+f\,dt+\Phi(v)\,dW_t,$$ where $v$ is the velocity, $\pi$ the pressure and $f$ an external volume force. We assume the common power law model $S(\varepsilon(v))=\big(1+|\varepsilon(v)|\big)^{p-2} \varepsilon(v)$ and show the existence of weak (martingale) solutions provided $p>\tfrac{2d+2}{d+2}$. Our approach is based on the $L^\infty$-truncation and a harmonic pressure decomposition which are adapted to the stochastic setting
Existence theory for stochastic power law fluids
existence theory for stochastic power law fluids
incompressible newtonian lipschitz mathbb intervall stochastic perturbation brownian balance reads mathrm nabla nabla force. varepsilon varepsilon varepsilon martingale tfrac infty truncation harmonic decomposition adapted stochastic
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29499669
10.1007/s00021-015-0213-x
We study the Euler equations with the so-called Ekman damping in the whole 2D space. The global well-posedness and dissipativity for the weak infinite energy solutions of this problem in the uniformly local spaces is verified based on the further development of the weighted energy theory for the Navier-Stokes and Euler type problems. In addition, the existence of weak locally compact global attractor is proved and some extra compactness of this attractor is obtained.Comment: arXiv admin note: text overlap with arXiv:1203.573
Infinite energy solutions for Dissipative Euler equations in R^2
infinite energy solutions for dissipative euler equations in r^2
euler ekman damping space. posedness dissipativity infinite uniformly verified weighted navier stokes euler problems. locally attractor proved extra compactness attractor admin overlap
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25013184
10.1007/s00021-015-0214-9
As in our previous paper, the 3D Navier-Stokes equations with a translationally bounded force contain pullback attractors in a weak sense. Moreover, those attractors consist of complete bounded trajectories. In this paper, we present a sufficient condition under which the pullback attractors are degenerate. That is, if the Grashof constant is small enough, the pullback attractor will be a single point on a unique, complete, bounded, strong solution. We then apply our results to provide a new proof of the existence of a unique, strong, periodic solution to the 3D Navier-Stokes with a small, periodic forcing term
Degenerate pullback attractors for the 3D Navier-Stokes equations
degenerate pullback attractors for the 3d navier-stokes equations
navier stokes translationally pullback attractors sense. attractors consist trajectories. pullback attractors degenerate. grashof pullback attractor solution. navier stokes forcing
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77019802
10.1007/s00021-015-0218-5
The purpose of this work is to analyze the mathematical model governing motion of n-component, heat conducting reactive mixture of compressible gases. We prove sequential stability of weak variational entropy solutions when the state equation essentially depends on the species concentration and the species diffusion fluxes depend on gradients of partial pressures. Of crucial importance for our analysis is the fact that viscosity coefficients vanish on vacuum and the source terms enjoy the admissibility condition dictated by the second law of thermodynamics
Mixtures: Sequential Stability of Variational Entropy Solutions
mixtures: sequential stability of variational entropy solutions
analyze mathematical governing conducting reactive mixture compressible gases. sequential variational essentially fluxes gradients pressures. crucial viscosity vanish enjoy admissibility dictated thermodynamics
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29531053
10.1007/s00021-015-0221-x
We investigate the stabilizing effects of the magnetic fields in the linearized magnetic Rayleigh-Taylor (RT) problem of a nonhomogeneous incompressible viscous magnetohydrodynamic fluid of zero resistivity in the presence of a uniform gravitational field in a three-dimensional bounded domain, in which the velocity of the fluid is non-slip on the boundary. By adapting a modified variational method and careful deriving \emph{a priori} estimates, we establish a criterion for the instability/stability of the linearized problem around a magnetic RT equilibrium state. In the criterion, we find a new phenomenon that a sufficiently strong horizontal magnetic field has the same stabilizing effect as that of the vertical magnetic field on growth of the magnetic RT instability. In addition, we further study the corresponding compressible case, i.e., the Parker (or magnetic buoyancy) problem, for which the strength of a horizontal magnetic field decreases with height, and also show the stabilizing effect of a sufficiently large magnetic field.Comment: 33 page
On Linear Instability and Stability of the Rayleigh-Taylor Problem in Magnetohydrodynamics
on linear instability and stability of the rayleigh-taylor problem in magnetohydrodynamics
stabilizing linearized rayleigh taylor nonhomogeneous incompressible viscous magnetohydrodynamic resistivity gravitational slip boundary. adapting variational careful deriving emph priori establish criterion instability linearized state. criterion phenomenon sufficiently stabilizing instability. compressible i.e. parker buoyancy stabilizing sufficiently
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25015624
10.1007/s00021-015-0222-9
The Hall-magnetohydrodynamics (Hall-MHD) equations, rigorously derived from kinetic models, are useful in describing many physical phenomena in geophysics and astrophysics. This paper studies the local well-posedness of classical solutions to the Hall-MHD equations with the magnetic diffusion given by a fractional Laplacian operator, $(-\Delta)^\alpha$. Due to the presence of the Hall term in the Hall-MHD equations, standard energy estimates appear to indicate that we need $\alpha\ge 1$ in order to obtain the local well-posedness. This paper breaks the barrier and shows that the fractional Hall-MHD equations are locally well-posed for any $\alpha>\frac12$. The approach here fully exploits the smoothing effects of the dissipation and establishes the local bounds for the Sobolev norms through the Besov space techniques. The method presented here may be applicable to similar situations involving other partial differential equations.Comment: 13 pages, this version improves the previous on
Local well-posedness for the Hall-MHD equations with fractional magnetic diffusion
local well-posedness for the hall-mhd equations with fractional magnetic diffusion
hall magnetohydrodynamics hall rigorously describing phenomena geophysics astrophysics. posedness hall fractional laplacian delta alpha hall hall alpha posedness. breaks barrier fractional hall locally posed alpha frac exploits smoothing dissipation establishes bounds sobolev norms besov techniques. applicable situations involving pages improves
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29530119
10.1007/s00021-015-0225-6
We introduce a continuous data assimilation (downscaling) algorithm for the two-dimensional Navier-Stokes equations employing coarse mesh measurements of only one component of the velocity field. This algorithm can be implemented with a variety of finitely many observables: low Fourier modes, nodal values, finite volume averages, or finite elements. We provide conditions on the spatial resolution of the observed data, under the assumption that the observed data is free of noise, which are sufficient to show that the solution of the algorithm approaches, at an exponential rate asymptotically in time, to the unique exact unknown reference solution, of the 2D Navier-Stokes equations, associated with the observed (finite dimensional projection of) velocity
Abridged continuous data assimilation for the 2D Navier-Stokes equations utilizing measurements of only one component of the velocity field
abridged continuous data assimilation for the 2d navier-stokes equations utilizing measurements of only one component of the velocity field
assimilation downscaling navier stokes employing coarse mesh field. implemented finitely observables fourier nodal averages elements. exponential asymptotically unknown navier stokes projection
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29541150
10.1007/s00021-015-0245-2
As a continuation of the previous work [40], in this paper we focus on the Cauchy problem of the two-dimensional (2D) incompressible Boussinesq equations with fractional Laplacian dissipation. We give an elementary proof of the global regularity of the smooth solutions of the 2D Boussinesq equations with a new range of fractional powers of the Laplacian. The argument is based on the nonlinear lower bounds for the fractional Laplacian established in [12]. Consequently, this result significantly improves the recent works [12, 38, 40].Comment: This version fix several typos of the previous one. 25 page
Global well-posedness of the 2D Boussinesq equations with fractional Laplacian dissipation
global well-posedness of the 2d boussinesq equations with fractional laplacian dissipation
continuation cauchy incompressible boussinesq fractional laplacian dissipation. elementary regularity boussinesq fractional powers laplacian. argument bounds fractional laplacian improves .comment typos one.
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29565710
10.1007/s00021-016-0249-6
In this paper we investigate the qualitative behaviour of the pressure function beneath an extreme Stokes wave over infinite depth. The presence of a stagnation point at the wave-crest of an extreme Stokes wave introduces a number of mathematical difficulties resulting in the irregularity of the free surface profile. It will be proven that the pressure decreases in the horizontal direction between a crest-line and subsequent trough-line, except along these lines themselves where the pressure is stationary with respect to the horizontal coordinate. In addition we will prove that the pressure strictly increases with depth throughout the fluid body.Comment: 12 pages, 2 figures. To appear in Journal of Mathematical Fluid Mechanic
The pressure in a deep-water Stokes wave of greatest height
the pressure in a deep-water stokes wave of greatest height
qualitative beneath extreme stokes infinite depth. stagnation crest extreme stokes introduces mathematical difficulties irregularity profile. proven crest trough stationary coordinate. strictly pages figures. mathematical mechanic
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80912935
10.1007/s00021-016-0254-9
This work is concerned with the time discrete analysis of the Oseen system of equations driven by nonlinear slip boundary conditions of friction type. We study the existence of solutions of the time discrete model and derive several a priori estimates needed to recover the solution of the continuous problem by means of weak compactness. Moreover, for the difference between the exact and approximate solutions, we obtainhttp://link.springer.com/journal/212017-12-31hb2016Mathematics and Applied Mathematic
Analysis of a time implicit scheme for the Oseen model driven by nonlinear slip boundary conditions
analysis of a time implicit scheme for the oseen model driven by nonlinear slip boundary conditions
concerned oseen slip friction type. derive priori recover compactness. approximate obtainhttp mathematics mathematic
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29527044
10.1007/s00021-016-0256-7
In the present paper we study a singular perturbation problem for a Navier-Stokes-Korteweg model with Coriolis force. Namely, we perform the incompressible and fast rotation asymptotics simultaneously, while we keep the capillarity coefficient constant in order to capture surface tension effects in the limit. We consider here the case of variable rotation axis: we prove the convergence to a linear parabolic-type equation with variable coefficients. The proof of the result relies on compensated compactness arguments. Besides, we look for minimal regularity assumptions on the variations of the axis.Comment: Section 5 of the previous version was remove
A singular limit problem for rotating capillary fluids with variable rotation axis
a singular limit problem for rotating capillary fluids with variable rotation axis
singular perturbation navier stokes korteweg coriolis force. incompressible asymptotics simultaneously keep capillarity capture tension limit. parabolic coefficients. relies compensated compactness arguments. besides look regularity assumptions remove
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42655925
10.1007/s00021-016-0265-6
We make a consistent derivation, from the governing equations, of the pressure transfer function in the small-amplitude Stokes wave regime and the hydrostatic approximation in the small-amplitude solitary water wave regime, in the presence of a background shear flow. The results agree with the well-known formulae in the zero vorticity case,but they incorporate the effects of vorticity through solutions to the Rayleigh equation. We extend the results to permit continuous density stratification and to internal waves between two constant-density fluids. Several examples are discussed.Comment: 20 page
Pressure transfer functions for interfacial fluid problems
pressure transfer functions for interfacial fluid problems
derivation governing stokes hydrostatic solitary flow. agree formulae vorticity incorporate vorticity rayleigh equation. extend permit stratification fluids.
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29555463
10.1007/s00021-016-0268-3
Because pressure is determined globally for the incompressible Euler equations, a localized change to the initial velocity will have an immediate effect throughout space. For solutions to be physically meaningful, one would expect such effects to decrease with distance from the localized change, giving the solutions a type of stability. Indeed, this is the case for solutions having spatial decay, as can be easily shown. We consider the more difficult case of solutions lacking spatial decay, and show that such stability still holds, albeit in a somewhat weaker form.Comment: Revised statement of Theorem 1 to include a missing definitio
Incompressible Euler Equations and the Effect of Changes at a Distance
incompressible euler equations and the effect of changes at a distance
globally incompressible euler localized immediate space. physically meaningful localized giving stability. shown. lacking albeit somewhat weaker revised statement missing definitio
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25014055
10.1007/s00021-016-0271-8
In 2000 Constantin showed that the incompressible Euler equations can be written in an "Eulerian-Lagrangian" form which involves the back-to-labels map (the inverse of the trajectory map for each fixed time). In the same paper a local existence result is proved in certain H\"older spaces $C^{1,\mu}$. We review the Eulerian-Lagrangian formulation of the equations and prove that given initial data in $H^s$ for $n\geq2$ and $s>\frac{n}{2}+1$, a unique local-in-time solution exists on the $n$-torus that is continuous into $H^s$ and $C^1$ into $H^{s-1}$. These solutions automatically have $C^1$ trajectories. The proof here is direct and does not appeal to results already known about the classical formulation. Moreover, these solutions are regular enough that the classical and Eulerian-Lagrangian formulations are equivalent, therefore what we present amounts to an alternative approach to some of the standard theory.Comment: 17 pages, to appear in J. Math. Fluid Mech. Lemmas 4 and 6 revised, several minor change
An Eulerian-Lagrangian Form for the Euler Equations in Sobolev Spaces
an eulerian-lagrangian form for the euler equations in sobolev spaces
constantin incompressible euler eulerian lagrangian involves labels trajectory proved older eulerian lagrangian formulation frac torus automatically trajectories. appeal formulation. eulerian lagrangian formulations amounts pages math. mech. lemmas revised minor
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29565067
10.1007/s00021-016-0277-2
New results are obtained for global regularity and long-time behavior of the solutions to the 2D Boussinesq equations for the flow of an incompressible fluid with positive viscosity and zero diffusivity in a smooth bounded domain. Our first result for global boundedness of the solution $(u, \theta) \in D(A)\times H^1$ improves considerably the main result of the recent article [7]. Our second result on global regularity of the solution $(u, \theta) \in V \times H^1$ for both bounded domain and the whole space ${\mathbb R}^2$ is a new one. It has been open and also seems much more challenging than the first result. Global regularity of the solution $(u, \theta) \in D(A) \times H^2$ is also proved
Global Regularity and Long-time Behavior of the Solutions to the 2D Boussinesq Equations without Diffusivity in a Bounded Domain
global regularity and long-time behavior of the solutions to the 2d boussinesq equations without diffusivity in a bounded domain
regularity boussinesq incompressible viscosity diffusivity domain. boundedness theta improves considerably regularity theta mathbb one. challenging result. regularity theta proved
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73418350
10.1007/s00021-016-0283-4
A two-dimensional water wave system is examined consisting of two discrete incompressible fluid domains separated by a free common interface. In a geophysical context this is a model of an internal wave, formed at a pycnocline or thermocline in the ocean. The system is considered as being bounded at the bottom and top by a flatbed and wave-free surface respectively. A current profile with depth-dependent currents in each domain is considered. The Hamiltonian of the system is determined and expressed in terms of canonical wave-related variables. Limiting behaviour is examined and compared to that of other known models. The linearised equations as well as long-wave approximations are presented.Comment: LaTeX, 21 pages, 1 figure, available online in J. Math. Fluid Mech. (2016
The Dynamics of Flat Surface Internal Geophysical Waves with Currents
the dynamics of flat surface internal geophysical waves with currents
consisting incompressible separated interface. geophysical pycnocline thermocline ocean. flatbed respectively. currents considered. canonical variables. limiting models. linearised approximations latex pages math. mech.
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73351970
10.1007/s00021-016-0301-6
It is well known that the full Navier-Stokes-Fourier system does not possess a strong solution in three dimensions which causes problems in applications. However, when modeling the flow of a fluid in a thin long pipe, the influence of the cross section can be neglected and the flow is basically one-dimensional. This allows us to deal with strong solutions which are more convenient for numerical computations. The goal of this paper is to provide a rigorous justification of this approach. Namely, we prove that any suitable weak solution to the three-dimensional NSF system tends to a strong solution to the one-dimensional system as the thickness of the pipe tends to zero.Comment: arXiv admin note: text overlap with arXiv:1111.4256 by other author
Dimension reduction for the full Navier-Stokes-Fourier system
dimension reduction for the full navier-stokes-fourier system
navier stokes fourier possess applications. pipe neglected basically dimensional. deal convenient computations. goal rigorous justification approach. tends pipe tends admin overlap
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73401751
10.1007/s00021-017-0315-8
The main subject of this paper concerns the establishment of certain classes of initial data, which grant short time uniqueness of the associated weak Leray-Hopf solutions of the three dimensional Navier-Stokes equations. In particular, our main theorem that this holds for any solenodial initial data, with finite $L_2(\mathbb{R}^3)$ norm, that also belongs to to certain subsets of $VMO^{-1}(\mathbb{R}^3)$. As a corollary of this, we obtain the same conclusion for any solenodial $u_{0}$ belonging to $L_{2}(\mathbb{R}^3)\cap \mathbb{\dot{B}}^{-1+\frac{3}{p}}_{p,\infty}(\mathbb{R}^3)$, for any $3<p<\infty$. Here, $\mathbb{\dot{B}}^{-1+\frac{3}{p}}_{p,\infty}(\mathbb{R}^3)$ denotes the closure of test functions in the critical Besov space ${\dot{B}}^{-1+\frac{3}{p}}_{p,\infty}(\mathbb{R}^3)$. Our results rely on the establishment of certain continuity properties near the initial time, for weak Leray-Hopf solutions of the Navier-Stokes equations, with these classes of initial data. Such properties seem to be of independent interest. Consequently, we are also able to show if a weak Leray-Hopf solution $u$ satisfies certain extensions of the Prodi-Serrin condition on $\mathbb{R}^3 \times ]0,T[$, then it is unique on $\mathbb{R}^3 \times ]0,T[$ amongst all other weak Leray-Hopf solutions with the same initial value. In particular, we show this is the case if $u\in L^{q,s}(0,T; L^{p,s}(\mathbb{R}^3))$ or if it's $L^{q,\infty}(0,T; L^{p,\infty}(\mathbb{R}^3))$ norm is sufficiently small, where $3<p< \infty$, $1\leq s<\infty$ and $3/p+2/q=1$.Comment: 44 pages. Submitted. Corollary 1.4, Proposition 1.6 and Section 5 have been added. Additional remarks included in the introduction and at the end of section 4. Another subsection has been added to the 'Preliminaries'. Minor typos have also been correcte
Uniqueness Results for Weak Leray-Hopf Solutions of the Navier-Stokes System with Initial Values in Critical Spaces
uniqueness results for weak leray-hopf solutions of the navier-stokes system with initial values in critical spaces
concerns establishment uniqueness leray hopf navier stokes equations. solenodial mathbb norm belongs subsets mathbb corollary solenodial belonging mathbb mathbb frac infty mathbb infty mathbb frac infty mathbb closure besov frac infty mathbb rely establishment continuity leray hopf navier stokes data. seem interest. leray hopf satisfies extensions prodi serrin mathbb mathbb amongst leray hopf value. mathbb infty infty mathbb norm sufficiently infty infty .comment pages. submitted. corollary added. remarks subsection preliminaries minor typos correcte
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73402954
10.1007/s00021-017-0328-3
We study the inviscid damping of Couette flow with an exponentially stratified density. The optimal decay rates of the velocity field and the density are obtained for general perturbations with minimal regularity. For Boussinesq approximation model, the decay rates we get are consistent with the previous results in the literature. We also study the decay rates for the full Euler equations of stratified fluids, which were not studied before. For both models, the decay rates depend on the Richardson number in a very similar way. Besides, we also study the dispersive decay due to the exponential stratification when there is no shear
Linear Inviscid Damping for Couette Flow in Stratified Fluid
linear inviscid damping for couette flow in stratified fluid
inviscid damping couette exponentially stratified density. perturbations regularity. boussinesq literature. euler stratified fluids before. richardson way. besides dispersive exponential stratification
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73359555
10.1007/s00021-017-0329-2
We present a new linearly stable solution of the Euler fluid flow on a torus. On a two-dimensional rectangular periodic domain $[0,2\pi)\times[0,2\pi / \kappa)$ for $\kappa\in\mathbb{R}^+$, the Euler equations admit a family of stationary solutions given by the vorticity profiles $\Omega^*(\mathbf{x})= \Gamma \cos(p_1x_1+ \kappa p_2x_2)$. We show linear stability for such flows when $p_2=0$ and $\kappa \geq |p_1|$ (equivalently $p_1=0$ and $\kappa{|p_2|}\leq{1}$). The classical result due to Arnold is that for $p_1 = 1, p_2 = 0$ and $\kappa \ge 1$ the stationary flow is {nonlinearly} stable via the energy-Casimir method. We show that for $\kappa \ge |p_1| \ge 2, p_2 = 0$ the flow is linearly stable, but one cannot expect a similar nonlinear stability result. Finally we prove nonlinear instability for all equilibria satisfying $p_1^2+\kappa^2{p_2^2}>\frac{{3(\kappa^2+1)}}{4(7-4\sqrt{3})}$. The modification and application of a structure-preserving Hamiltonian truncation is discussed for the $\kappa\neq 1$ case. This leads to an explicit Lie-Poisson integrator for the truncated system
Stability Results for Idealised Shear Flows on a Rectangular Periodic Domain
stability results for idealised shear flows on a rectangular periodic domain
linearly euler torus. rectangular kappa kappa mathbb euler admit stationary vorticity omega mathbf gamma kappa flows kappa equivalently kappa arnold kappa stationary nonlinearly casimir method. kappa linearly result. instability equilibria satisfying kappa frac kappa sqrt modification preserving truncation kappa case. poisson integrator truncated
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83867307
10.1007/s00021-017-0331-8
The main aim of the paper is to investigate the transitions of the thermohaline circulation in a spherical shell in a parameter regime which only allows transitions to multiple equilibria. We find that the first transition is either continuous (Type-I) or drastic (Type-II) depending on the sign of the transition number. The transition number depends on the system parameters and $l_c$, which is the common degree of spherical harmonics of the first critical eigenmodes, and it can be written as a sum of terms describing the nonlinear interactions of various modes with the critical modes. We obtain the exact formulas of this transition number for $l_c=1$ and $l_c=2$ cases. Numerically, we find that the main contribution to the transition number is due to nonlinear interactions with modes having zero wave number and the contribution from the nonlinear interactions with higher frequency modes is negligible. In our numerical experiments we encountered both types of transition for $Le<1$ but only continuous transition for $Le>1$. In the continuous transition scenario, we rigorously prove that an attractor in the phase space bifurcates which is homeomorphic to the 2$l_c$ dimensional sphere and consists entirely of degenerate steady state solutions
Transitions of Spherical Thermohaline Circulation to Multiple Equilibria
transitions of spherical thermohaline circulation to multiple equilibria
thermohaline circulation spherical equilibria. drastic number. spherical harmonics eigenmodes describing modes. formulas cases. numerically negligible. encountered rigorously attractor bifurcates homeomorphic sphere entirely degenerate steady
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73991451
10.1007/s00021-017-0334-5
Topology changes in multi-phase fluid flows are difficult to model within a traditional sharp interface theory. Diffuse interface models turn out to be an attractive alternative to model two-phase flows. Based on a Cahn-Hilliard-Navier-Stokes model introduced by Abels, Garcke and Gr\"{u}n (Math. Models Methods Appl. Sci. 2012), which uses a volume averaged velocity, we derive a diffuse interface model in a Hele-Shaw geometry, which in the case of non-matched densities, simplifies an earlier model of Lee, Lowengrub and Goodman (Phys. Fluids 2002). We recover the classical Hele-Shaw model as a sharp interface limit of the diffuse interface model. Furthermore, we show the existence of weak solutions and present several numerical computations including situations with rising bubbles and fingering instabilities.Comment: 41 pages, 75 figure
A Hele-Shaw-Cahn-Hilliard model for incompressible two-phase flows with different densities
a hele-shaw-cahn-hilliard model for incompressible two-phase flows with different densities
topology flows traditional sharp theory. diffuse attractive flows. cahn hilliard navier stokes abels garcke math. sci. averaged derive diffuse hele shaw matched densities simplifies lowengrub goodman phys. fluids recover hele shaw sharp diffuse model. computations situations rising bubbles fingering pages
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73353372
10.1007/s00021-017-0337-2
This paper concerns the instability and stability of the trivial steady states of the incompressible Navier-Stokes equations with Navier-slip boundary conditions in a slab domain in dimension two. The main results show that the stability (or instability) of this constant equilibrium depends crucially on whether the boundaries dissipate energy and the strengthen of the viscosity and slip length. It is shown that in the case that when all the boundaries are dissipative, then nonlinear asymptotic stability holds true, otherwise, there is a sharp critical viscosity, which distinguishes the nonlinear stability from instability.Comment: 34 page
Stability analysis for the incompressible Navier-Stokes equations with Navier boundary conditions
stability analysis for the incompressible navier-stokes equations with navier boundary conditions
concerns instability trivial steady incompressible navier stokes navier slip slab two. instability crucially boundaries dissipate strengthen viscosity slip length. boundaries dissipative asymptotic sharp viscosity distinguishes
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83862870
10.1007/s00021-017-0338-1
We consider the initial value problem to the Isobe-Kakinuma model for water waves and the structure of the model. The Isobe-Kakinuma model is the Euler-Lagrange equations for an approximate Lagrangian which is derived from Luke's Lagrangian for water waves by approximating the velocity potential in the Lagrangian. The Isobe-Kakinuma model is a system of second order partial differential equations and is classified into a system of nonlinear dispersive equations. Since the hypersurface $t=0$ is characteristic for the Isobe-Kakinuma model, the initial data have to be restricted in an infinite dimensional manifold for the existence of the solution. Under this necessary condition and a sign condition, which corresponds to a generalized Rayleigh-Taylor sign condition for water waves, on the initial data, we show that the initial value problem is solvable locally in time in Sobolev spaces. We also discuss the linear dispersion relation to the model
Solvability of the initial value problem to the Isobe-Kakinuma model for water waves
solvability of the initial value problem to the isobe-kakinuma model for water waves
isobe kakinuma model. isobe kakinuma euler lagrange approximate lagrangian luke lagrangian approximating lagrangian. isobe kakinuma classified dispersive equations. hypersurface isobe kakinuma restricted infinite manifold solution. rayleigh taylor solvable locally sobolev spaces.
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83841591
10.1007/s00021-017-0342-5
The abstract theory of critical spaces developed in [22] and [20] is applied to the Navier-Stokes equations in bounded domains with Navier boundary conditions as well as no-slip conditions. Our approach unifies, simplifies and extends existing work in the $L_p$-$L_q$ setting, considerably. As an essential step, it is shown that the strong and weak Stokes operators with Navier conditions admit an $\mathcal{H}^\infty$-calculus with $\mathcal{H}^\infty$-angle 0, and the real and complex interpolation spaces of these operators are identified.Comment: 21 page
On critical spaces for the Navier-Stokes equations
on critical spaces for the navier-stokes equations
navier stokes navier slip conditions. unifies simplifies extends considerably. stokes navier admit mathcal infty calculus mathcal infty interpolation
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83845241
10.1007/s00021-017-0344-3
Consider the Navier-Stokes flow in 3-dimensional exterior domains, where a rigid body is translating with prescribed translational velocity $-h(t)u_\infty$ with constant vector $u_\infty\in \mathbb R^3\setminus\{0\}$. Finn raised the question whether his steady slutions are attainable as limits for $t\to\infty$ of unsteady solutions starting from motionless state when $h(t)=1$ after some finite time and $h(0)=0$ (starting problem). This was affirmatively solved by Galdi, Heywood and Shibata for small $u_\infty$. We study some generalized situation in which unsteady solutions start from large motions being in $L^3$. We then conclude that the steady solutions for small $u_\infty$ are still attainable as limits of evolution of those fluid motions which are found as a sort of weak solutions. The opposite situation, in which $h(t)=0$ after some finite time and $h(0)=1$ (landing problem), is also discussed. In this latter case, the rest state is attainable no matter how large $u_\infty$ is
Navier-Stokes flow past a rigid body: attainability of steady solutions as limits of unsteady weak solutions, starting and landing cases
navier-stokes flow past a rigid body: attainability of steady solutions as limits of unsteady weak solutions, starting and landing cases
navier stokes exterior rigid translating prescribed translational infty infty mathbb setminus finn raised steady slutions attainable infty unsteady motionless affirmatively solved galdi heywood shibata infty unsteady motions steady infty attainable motions sort solutions. opposite landing discussed. attainable infty
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83858312
10.1007/s00021-017-0352-3
We study the compressible and incompressible two-phase flows separated by a sharp interface with a phase transition and a surface tension. In particular, we consider the problem in $\mathbb{R}^N$, and the Navier-Stokes-Korteweg equations is used in the upper domain and the Navier-Stokes equations is used in the lower domain. We prove the existence of $\mathcal{R}$-bounded solution operator families for a resolvent problem arising from its model problem. According to Shibata \cite{GS2014}, the regularity of $\rho_+$ is $W^1_q$ in space, but to solve the kinetic equation: $\mathbf{u}_\Gamma\cdot\mathbf{n}_t = [[\rho\mathbf{u}]]\cdot\mathbf{n}_t /[[\rho]]$ on $\Gamma_t$ we need $W^{2-1/q}_q$ regularity of $\rho_+$ on $\Gamma_t$, which means the regularity loss. Since the regularity of $\rho_+$ dominated by the Navier-Stokes-Korteweg equations is $W^3_q$ in space, we eliminate the problem by using the Navier-Stokes-Korteweg equations instead of the compressible Navier-Stokes equations.Comment: Typos correcte
Compressible-incompressible two-phase flows with phase transition: model problem
compressible-incompressible two-phase flows with phase transition: model problem
compressible incompressible flows separated sharp tension. mathbb navier stokes korteweg navier stokes domain. mathcal families resolvent arising problem. shibata cite regularity solve mathbf gamma cdot mathbf mathbf cdot mathbf gamma regularity gamma regularity loss. regularity dominated navier stokes korteweg eliminate navier stokes korteweg compressible navier stokes typos correcte
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84094266
10.1007/s00021-017-0355-0
We provide the existence and asymptotic description of solitary wave solutions to a class of modified Green-Naghdi systems, modeling the propagation of long surface or internal waves. This class was recently proposed by Duch{\^e}ne, Israwi and Talhouk (Stud. Appl. Math.,137 (2016)) in order to improve the frequency dispersion of the original Green-Naghdi system while maintaining the same precision. The solitary waves are constructed from the solutions of a constrained minimization problem. The main difficulties stem from the fact that the functional at stake involves low order non-local operators, intertwining multiplications and convolutions through Fourier multipliers
Solitary wave solutions to a class of modified Green-Naghdi systems
solitary wave solutions to a class of modified green-naghdi systems
asymptotic solitary naghdi propagation waves. duch israwi talhouk stud. appl. math. naghdi maintaining precision. solitary constrained minimization problem. difficulties stake involves intertwining multiplications convolutions fourier multipliers
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83859903
10.1007/s00021-017-0358-x
We study the 3-D compressible barotropic radiation fluid dynamics system describing the motion of the compressible rotating viscous fluid with gravitation and radiation confined to a straight layer. We show that weak solutions in the 3-D domain converge to the strong solution of the rotating 2-D Navier-Stokes-Poisson system with radiation for all times less than the maximal life time of the strong solution of the 2-D system when the Froude number is small or to the strong solution of the rotating pure 2-D Navier- Stokes system with radiation
Derivation of the Navier - Stokes - Poisson system with radiation for an accretion disk
derivation of the navier - stokes - poisson system with radiation for an accretion disk
compressible barotropic describing compressible rotating viscous gravitation confined straight layer. converge rotating navier stokes poisson maximal froude rotating navier stokes
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83863068
10.1007/s00021-018-0361-x
The main objective of this article is to study the nonlinear stability and dynamic transitions of the basic (zonal) shear flows for the three-dimensional continuously stratified rotating Boussinesq model. The model equations are fundamental equations in geophysical fluid dynamics, and dynamics associated with their basic zonal shear flows play a crucial role in understanding many important geophysical fluid dynamical processes, such as the meridional overturning oceanic circulation and the geophysical baroclinic instability. In this paper, first we derive a threshold for the energy stability of the basic shear flow, and obtain a criteria for nonlinear stability in terms of the critical horizontal wavenumbers and the system parameters such as the Froude number, the Rossby number, the Prandtl number and the strength of the shear flow. Next we demonstrate that the system always undergoes a dynamic transition from the basic shear flow to either a spatiotemporal oscillatory pattern or circle of steady states, as the shear strength $\Lambda$ of the basic flow crosses a critical threshold $\Lambda_c$. Also we show that the dynamic transition can be either continuous or catastrophic, and is dictated by the sign of a transition parameter $A$, fully characterizing the nonlinear interactions of different modes. A systematic numerical method is carried out to explore transition in different flow parameter regimes. We find that the system admits only critical eigenmodes with horizontal wave indices $(0,m_y)$. Such modes, horizontally have the pattern consisting of $m_y$-rolls aligned with the x-axis. Furthermore, numerically we encountered continuous transitions to multiple steady states, continuous and catastrophic transitions to spatiotemporal oscillations.Comment: 20 pages, 7 figure
Dynamic Transitions and Baroclinic Instability for 3D Continuously Stratified Boussinesq Flows
dynamic transitions and baroclinic instability for 3d continuously stratified boussinesq flows
zonal flows continuously stratified rotating boussinesq model. geophysical zonal flows crucial geophysical meridional overturning oceanic circulation geophysical baroclinic instability. derive wavenumbers froude rossby prandtl flow. undergoes spatiotemporal oscillatory circle steady lambda crosses lambda catastrophic dictated characterizing modes. explore regimes. admits eigenmodes indices horizontally consisting rolls aligned axis. numerically encountered steady catastrophic spatiotemporal pages
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161229574
10.1007/s00021-018-0367-4
The paper deals with the non-stationary Oseen system of equations for the generalized Newtonian incompressible fluid with multivalued and nonmonotone frictional slip boundary conditions. First, we provide a result on existence of a unique solution to an abstract evolutionary inclusion involving the Clarke subdifferential term for a nonconvex function. We employ a method based on a surjectivity theorem for multivalued L-pseudomonotone operators. Then, we exploit the abstract result to prove the weak unique solvability of the Oseen system
Evolutionary Oseen model for generalized Newtonian fluid with Multivalued Nonmonotone Friction Law
evolutionary oseen model for generalized newtonian fluid with multivalued nonmonotone friction law
deals stationary oseen newtonian incompressible multivalued nonmonotone frictional slip conditions. evolutionary inclusion involving clarke subdifferential nonconvex function. employ surjectivity multivalued pseudomonotone operators. exploit solvability oseen
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83865645
10.1007/s00021-018-0370-9
This paper presents existence theories for several families of axisymmetric solitary waves on the surface of an otherwise cylindrical ferrofluid jet surrounding a stationary metal rod. The ferrofluid, which is governed by a general (nonlinear) magnetisation law, is subject to an azimuthal magnetic field generated by an electric current flowing along the rod. The ferrohydrodynamic problem for axisymmetric travelling waves is formulated as an infinite-dimensional Hamiltonian system in which the axial direction is the time-like variable. A centre-manifold reduction technique is employed to reduce the system to a locally equivalent Hamiltonian system with a finite number of degrees of freedom, and homoclinic solutions to the reduced system, which correspond to solitary waves, are detected by dynamical-systems methods
Spatial dynamics methods for solitary waves on a ferrofluid jet
spatial dynamics methods for solitary waves on a ferrofluid jet
presents families axisymmetric solitary cylindrical ferrofluid surrounding stationary rod. ferrofluid governed magnetisation azimuthal flowing rod. ferrohydrodynamic axisymmetric travelling formulated infinite axial variable. manifold locally freedom homoclinic solitary
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93940553
10.1007/s00021-018-0372-7
In this paper, we reconsider a circular cylinder horizontally floating on an unbounded reservoir in a gravitational field directed downwards, which was studied by Bhatnargar and Finn in 2006. We follow their approach but with some modifications. We establish the relation between the total energy relative to the undisturbed state and the total force. There is a monotone relation between the height of the centre and the wetting angle. We study the number of equilibria, the floating configurations and their stability for all parameter values. We find that the system admits at most two equilibrium points for arbitrary contact angle, the one with smaller wetting angle is stable and the one with larger wetting angle is unstable. The initial model has a limitation that the fluid interfaces may intersect. We show that the stable equilibrium point never lies in the intersection region, while the unstable equilibrium point may lie in the intersection region.Comment: 40 pages, 27 figure
A Floating Cylinder on An Unbounded Bath
a floating cylinder on an unbounded bath
reconsider circular cylinder horizontally floating unbounded reservoir gravitational directed downwards bhatnargar finn modifications. establish undisturbed force. monotone wetting angle. equilibria floating configurations values. admits wetting wetting unstable. limitation interfaces intersect. never lies intersection unstable intersection pages
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2064916
10.1007/s00022-012-0139-x
Almost hypercomplex manifolds with Hermitian and Norden metrics and more specially the corresponding quaternionic Kaehler manifolds are considered. Some necessary and sufficient conditions the investigated manifolds be isotropic hyper-Kaehlerian and flat are found. It is proved that the quaternionic Kaehler manifolds with the considered metric structure are Einstein for dimension at least 8. The class of the non-hyper-Kaehler quaternionic Kaehler manifold of the considered type is determined.Comment: 10 page
Quaternionic Kaehler manifolds with Hermitian and Norden metrics
quaternionic kaehler manifolds with hermitian and norden metrics
hypercomplex manifolds hermitian norden metrics specially quaternionic kaehler manifolds considered. manifolds isotropic hyper kaehlerian found. proved quaternionic kaehler manifolds einstein hyper kaehler quaternionic kaehler manifold
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10186076
10.1007/s00022-013-0189-8
Codes from Hall planes of even order, J. D. Key, T. P. McDonough and V. C. Mavron, Journal of Geometry, volume 105, issue 1, April 2014, pages 33?41.We show that the binary code C of the projective Hall plane Hq2 of even order q 2 where q = 2 t , for t?2 has words of weight 2q 2 in its hull that are not the difference of the incidence vectors of two lines of Hq2 ; together with an earlier result for the dual Hall planes of even order, this shows that for all t?2 the Hall plane and its dual are not tame. We also deduce that dim(C)>32t+1, the dimension of the binary code of the desarguesian projective plane of order 22t , thus supporting the Hamada?Sachar conjecture for this infinite class of planes.authorsversionPeer reviewe
Codes from Hall planes of even order
codes from hall planes of even order
codes hall planes mcdonough mavron april pages projective hall hull incidence hall planes hall tame. deduce desarguesian projective supporting hamada sachar conjecture infinite thorsversionpeer reviewe
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25015663
10.1007/s00022-014-0257-8
We derive several results in classical Euclidean elementary geometry using the steering ellipsoid formalism from quantum mechanics. This gives a physically motivated derivation of very non-trivial geometric results, some of which are entirely new. We consider a sphere of radius $r$ contained inside another sphere of radius $R$, with the sphere centres separated by distance $d$. When does there exist a nested tetrahedron circumscribed about the smaller sphere and inscribed in the larger? We derive the Grace-Danielsson inequality $d^2 \leq (R+r)(R-3r)$ as the sole necessary and sufficient condition for the existence of a nested tetrahedron. Our method also gives the condition $d^2 \leq R(R-2r)$ for the existence of a nested triangle in the analogous 2-dimensional scenario. These results imply the Euler inequality in 2 and 3 dimensions. Furthermore, we formulate a new inequality that applies to the more general case of ellipses and ellipsoids.Comment: 8 pages, 1 figure. Published versio
The Euler and Grace-Danielsson inequalities for nested triangles and tetrahedra: a derivation and generalisation using quantum information theory
the euler and grace-danielsson inequalities for nested triangles and tetrahedra: a derivation and generalisation using quantum information theory
derive euclidean elementary steering ellipsoid formalism mechanics. physically motivated derivation trivial geometric entirely new. sphere sphere sphere centres separated nested tetrahedron circumscribed sphere inscribed derive grace danielsson inequality sole nested tetrahedron. nested triangle analogous scenario. imply euler inequality dimensions. formulate inequality applies ellipses pages figure. versio
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29519229
10.1007/s00022-015-0268-0
We study geodesics in generalized Wallach spaces which are expressed as orbits of products of three exponential terms. These are homogeneous spaces $M=G/K$ whose isotropy representation decomposes into a direct sum of three submodules $\frak{m}=\frak{m}_1\oplus\frak{m}_2\oplus\frak{m}_3$, satisfying the relations $[\frak{m}_i,\frak{m}_i]\subset \frak{k}$. Assuming that the submodules $\frak{m}_i$ are pairwise non isomorphic, we study geodesics on such spaces of the form $\gamma (t)=\exp (tX)\exp (tY)\exp (tZ)\cdot o$, where $X\in\fr{m}_1, Y\in\fr{m}_2, Z\in\fr{m}_3$ ($o=eK$), with respect to a $G$-invariant metric. Our investigation imposes certain restrictions on the $G$-invariant metric, so the geodesics turn out to be orbits of two exponential terms. We give a point of view using Riemannian submersions. As an application, we describe geodesics in generalized flag manifolds with three isotropy summands and with second Betti number $b_2(M)=2$, and in the Stiefel manifolds $SO(n+2)/S(n)$. We relate our results to geodesic orbit spaces (g.o. spaces).Comment: Journal of Geometry (2015
Geodesics in generalized Wallach spaces
geodesics in generalized wallach spaces
geodesics wallach orbits exponential terms. homogeneous isotropy decomposes submodules frak frak oplus frak oplus frak satisfying frak frak frak submodules frak pairwise isomorphic geodesics gamma cdot metric. imposes restrictions geodesics orbits exponential terms. riemannian submersions. geodesics flag manifolds isotropy summands betti stiefel manifolds relate geodesic orbit g.o. .comment
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29547290
10.1007/s00022-015-0291-1
Applications of harmonic analysis on finite groups were recently introduced to measure partition problems, with a variety of equipartition types by convex fundamental domains obtained as the vanishing of prescribed Fourier transforms. Considering the circle group, we extend this approach to the compact Lie group setting, in which case the annihilation of transforms in the classical Fourier series produces measure transversality similar in spirit to the classical centerpoint theorem of Rado: for any $q\geq 2$, the existence of a complex hyperplane whose surrounding regular $q$-fans are close -- in an $L^2$-sense -- to equipartitioning a given set of measures. The proofs of these results represent the first application of continuous as opposed to finite group actions in the usual equivariant topological reductions prevalent in combinatorial geometry.Comment: 7 page
Measure Partitions via Fourier Analysis II: Center Transversality in the $L^2$-norm for Complex Hyperplanes
measure partitions via fourier analysis ii: center transversality in the $l^2$-norm for complex hyperplanes
harmonic partition equipartition convex vanishing prescribed fourier transforms. circle extend annihilation transforms fourier produces transversality spirit centerpoint rado hyperplane surrounding fans equipartitioning measures. proofs opposed usual equivariant topological reductions prevalent combinatorial
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42647794
10.1007/s00022-016-0325-3
The purpose of this paper is to study $\mathcal{P}\mathcal{R}$-semi-invariant warped product submanifolds of a paracosymplectic manifold $\widetilde{M}$. We prove that the distributions associated with the definition of $\mathcal{P}\mathcal{R}$-semi-invariant warped product submanifold $M$ are always integrable. A necessary and sufficient condition for an isometrically immersed $\mathcal{P}\mathcal{R}$-semi-invariant submanifold of $\widetilde{M}$ to be a $\mathcal{P}\mathcal{R}$-semi-invariant warped product submanifold is obtained in terms of the shape operator.Comment: 15 pages. arXiv admin note: text overlap with arXiv:1510.0204
Geometry of $\mathcal{P}\mathcal{R}$-semi-invariant warped product submanifolds in paracosymplectic manifold
geometry of $\mathcal{p}\mathcal{r}$-semi-invariant warped product submanifolds in paracosymplectic manifold
mathcal mathcal warped submanifolds paracosymplectic manifold widetilde mathcal mathcal warped submanifold integrable. isometrically immersed mathcal mathcal submanifold widetilde mathcal mathcal warped submanifold pages. admin overlap
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129362656
10.1007/s00022-016-0333-3
In this paper, we consider the CPE conjecture in the frame-work of $K$-contact and $(\kappa, \mu)$-contact manifolds. First, we prove that if a complete $K$-contact metric satisfies the CPE is Einstein and is isometric to a unit sphere $S^{2n+1}$. Next, we prove that if a non-Sasakian $ (\kappa, \mu) $-contact metric satisfies the CPE, then $ M^{3} $ is flat and for $ n > 1 $, $ M^{2n+1} $ is locally isometric to $ E^{n+1}\times S^{n}(4)$.Comment: In the published version there was a sign error in Eq. (1.3). We have fixed it her
The Critical Point Equation And Contact Geometry
the critical point equation and contact geometry
conjecture kappa manifolds. satisfies einstein isometric sphere sasakian kappa satisfies locally isometric .comment
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29546933
10.1007/s00022-016-0350-2
In this paper, the third in the series, we define the generalized orthocenter $H$ corresponding to a point $P$, with respect to triangle $ABC$, as the unique point for which the lines $HA, HB, HC$ are parallel, respectively, to $QD, QE, QF$, where $DEF$ is the cevian triangle of $P$ and $Q=K \circ \iota(P)$ is the $isotomcomplement$ of $P$, both with respect to $ABC$. We prove a generalized Feuerbach Theorem, and characterize the center $Z$ of the cevian conic $\mathcal{C}_P$, defined in Part II, as the center of the affine map $\Phi_P = T_P \circ K^{-1} \circ T_{P'} \circ K^{-1}$, where $T_P$ is the unique affine map for which $T_P(ABC)=DEF$; $T_{P'}$ is defined similarly for the isotomic conjugate $P'=\iota(P)$ of $P$; and $K$ is the complement map. The affine map $\Phi_P$ fixes $Z$ and takes the nine-point conic $\mathcal{N}_H$ for the quadrangle $ABCH$ (with respect to the line at infinity) to the inconic $\mathcal{I}$, defined to be the unique conic which is tangent to the sides of $ABC$ at the points $D, E, F$. The point $Z$ is therefore the point where the nine-point conic $\mathcal{N}_H$ and the inconic $\mathcal{I}$ touch. This theorem generalizes the usual Feuerbach theorem and holds in all cases where the point $P$ is not on a median, whether the conics involved are ellipses, parabolas, or hyperbolas, and also holds when $Z$ is an infinite point. We also determine the locus of points $P$ for which the generalized orthocenter $H$ coincides with a vertex of $ABC$; this locus turns out to be the union of three conics minus six points. All our proofs are synthetic, and combine affine and projective arguments.Comment: 34 pages, 7 figure
Synthetic foundations of cevian geometry, III: The generalized orthocenter
synthetic foundations of cevian geometry, iii: the generalized orthocenter
orthocenter triangle cevian triangle circ iota isotomcomplement feuerbach characterize cevian conic mathcal affine circ circ circ affine isotomic conjugate iota complement map. affine fixes nine conic mathcal quadrangle abch infinity inconic mathcal conic tangent sides nine conic mathcal inconic mathcal touch. generalizes usual feuerbach conics ellipses parabolas hyperbolas infinite point. locus orthocenter coincides locus turns union conics minus points. proofs synthetic combine affine projective pages
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42736951
10.1007/s00022-016-0352-0
Minimal surfaces with planar curvature lines are classical geometric objects, having been studied since the late 19th century. In this paper, we revisit the subject from a different point of view. After calculating their metric functions using an analytical method, we recover the Weierstrass data, and give clean parametrizations for these surfaces. Then, using these parametrizations, we show that there exists a single continuous deformation between all minimal surfaces with planar curvature lines. In the process, we establish the existence of axial directions for these surfaces
Deformation of minimal surfaces with planar curvature lines
deformation of minimal surfaces with planar curvature lines
planar curvature geometric century. revisit view. calculating recover weierstrass clean parametrizations surfaces. parametrizations deformation planar curvature lines. establish axial directions
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73956286
10.1007/s00022-017-0391-1
An $n$-arc in a projective plane is a collection of $n$ distinct points in the plane, no three of which lie on a line. Formulas counting the number of $n$-arcs in any finite projective plane of order $q$ are known for $n \le 8$. In 1995, Iampolskaia, Skorobogatov, and Sorokin counted $9$-arcs in the projective plane over a finite field of order $q$ and showed that this count is a quasipolynomial function of $q$. We present a formula for the number of $9$-arcs in any projective plane of order $q$, even those that are non-Desarguesian, deriving Iampolskaia, Skorobogatov, and Sorokin's formula as a special case. We obtain our formula from a new implementation of an algorithm due to Glynn; we give details of our implementation and discuss its consequences for larger arcs.Comment: 19 pages, to appear in Journal of Geometr
Counting Arcs in Projective Planes via Glynn's Algorithm
counting arcs in projective planes via glynn's algorithm
projective line. formulas counting arcs projective iampolskaia skorobogatov sorokin counted arcs projective count quasipolynomial arcs projective desarguesian deriving iampolskaia skorobogatov sorokin case. glynn consequences pages geometr
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42750500
10.1007/s00022-017-0398-7
In this work we are interested in the characterization of curves that belong to a given surface. To the best of our knowledge, there is no known general solution to this problem. Indeed, a solution is only available for a few examples: planes, spheres, or cylinders. Generally, the characterization of such curves, both in Euclidean ($E^3$) and in Lorentz-Minkowski ($E_1^3$) spaces, involves an ODE relating curvature and torsion. However, by equipping a curve with a relatively parallel moving frame, Bishop was able to characterize spherical curves in $E^3$ through a linear equation relating the coefficients which dictate the frame motion. Here we apply these ideas to surfaces that are implicitly defined by a smooth function, $\Sigma=F^{-1}(c)$, by reinterpreting the problem in the context of the metric given by the Hessian of $F$, which is not always positive definite. So, we are naturally led to the study of curves in $E_1^3$. We develop a systematic approach to the construction of Bishop frames by exploiting the structure of the normal planes induced by the casual character of the curve, present a complete characterization of spherical curves in $E_1^3$, and apply it to characterize curves that belong to a non-degenerate Euclidean quadric. We also interpret the casual character that a curve may assume when we pass from $E^3$ to $E_1^3$ and finally establish a criterion for a curve to lie on a level surface of a smooth function, which reduces to a linear equation when the Hessian is constant.Comment: 22 pages (23 in the published version), 3 figures; this version is essentially the same as the published on
Moving frames and the characterization of curves that lie on a surface
moving frames and the characterization of curves that lie on a surface
interested belong surface. problem. planes spheres cylinders. euclidean lorentz minkowski involves relating curvature torsion. equipping moving bishop characterize spherical relating dictate motion. ideas implicitly sigma reinterpreting hessian definite. naturally bishop frames exploiting planes casual character spherical characterize belong degenerate euclidean quadric. interpret casual character pass establish criterion reduces hessian pages essentially
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73360194
10.1007/s00022-017-0400-4
A Hopf hypersurface in a (para-)Kaehler manifold is a real hypersurface for which one of the principal directions of the second fundamental form is the (para-)complex dual of the normal vector. We consider particular Hopf hypersurfaces in the space of oriented geodesics of a non-flat space form of dimension greater than 2. For spherical and hyperbolic space forms, the oriented geodesic space admits a canonical Kaehler-Einstein and para-Kaehler-Einstein structure, respectively, so that a natural notion of a Hopf hypersurface exists. The particular hypersurfaces considered are formed by the oriented geodesics that are tangent to a given convex hypersurface in the underlying space form. We prove that a tangent hypersurface is Hopf in the space of oriented geodesics with respect to this canonical (para-)Kaehler structure iff the underlying convex hypersurface is totally umbilic and non-flat. In the case of 3 dimensional space forms, however, there exists a second canonical complex structure which can also be used to define Hopf hypersurfaces. We prove that in this dimension, the tangent hypersurface of a convex hypersurface in the space form is always Hopf with respect to this second complex structure.Comment: 10 pages AMS-TE
Hopf hypersurfaces in spaces of oriented geodesics
hopf hypersurfaces in spaces of oriented geodesics
hopf hypersurface para kaehler manifold hypersurface principal directions para vector. hopf hypersurfaces oriented geodesics spherical hyperbolic oriented geodesic admits canonical kaehler einstein para kaehler einstein notion hopf hypersurface exists. hypersurfaces oriented geodesics tangent convex hypersurface form. tangent hypersurface hopf oriented geodesics canonical para kaehler convex hypersurface totally umbilic flat. canonical hopf hypersurfaces. tangent hypersurface convex hypersurface hopf pages
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2343826
10.1007/s00023-001-8594-1
In this paper we complete the first step, namely the uniform bound on completely convergent contributions, towards proving that a three dimensional interacting system of Fermions is a Fermi liquid in the sense of Salmhofer. The analysis relies on a direct space decomposition of the propagator, on a bosonic multiscale cluster expansion and on the Hadamard inequality, rather than on a Fermionic expansion and an angular analysis in momentum space, as was used in the recent proof by two of us of Salmhofer's criterion in two dimensions.Comment: 85 pages, 13 figure
Interacting Fermi liquid in three dimensions at finite temperature: Part I: Convergent Contributions
interacting fermi liquid in three dimensions at finite temperature: part i: convergent contributions
convergent proving interacting fermions fermi salmhofer. relies decomposition propagator bosonic multiscale hadamard inequality fermionic salmhofer criterion pages
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2553660
10.1007/s00023-001-8596-z
We set up and analyze a model of radiation damping within the framework of continuum mechanics, inspired by a model of post-Newtonian hydrodynamics due to Blanchet, Damour and Schaefer. In order to simplify the problem as much as possible we replace the gravitational field by the electromagnetic field and the fluid by kinetic theory. We prove that the resulting system has a well-posed Cauchy problem globally in time for general initial data and in all solutions the fields decay to zero at late times. In particular, this means that the model is free from the runaway solutions which frequently occur in descriptions of radiation reaction
The Vlasov-Poisson system with radiation damping
the vlasov-poisson system with radiation damping
analyze damping continuum mechanics inspired newtonian hydrodynamics blanchet damour schaefer. simplify replace gravitational electromagnetic theory. posed cauchy globally times. runaway frequently descriptions
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2557211
10.1007/s00023-002-8621-x
We prove a localization theorem for continuous ergodic Schr\"odinger operators $ H_\omega := H_0 + V_\omega $, where the random potential $ V_\omega $ is a nonnegative Anderson-type perturbation of the periodic operator $ H_0$. We consider a lower spectral band edge of $ \sigma (H_0) $, say $ E= 0 $, at a gap which is preserved by the perturbation $ V_\omega $. Assuming that all Floquet eigenvalues of $ H_0$, which reach the spectral edge 0 as a minimum, have there a positive definite Hessian, we conclude that there exists an interval $ I $ containing 0 such that $ H_\omega $ has only pure point spectrum in $ I $ for almost all $ \omega $.Comment: 21 page
Localization for random perturbations of periodic Schroedinger operators with regular Floquet eigenvalues
localization for random perturbations of periodic schroedinger operators with regular floquet eigenvalues
localization ergodic schr odinger omega omega omega nonnegative anderson perturbation sigma preserved perturbation omega floquet eigenvalues definite hessian omega omega .comment
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2350464
10.1007/s00023-002-8635-4
Bose-Einstein condensation is usually modeled by nonlinear Schroedinger equations with harmonic potential. We study the Cauchy problem for these equations. We show that the local problem can be treated as in the case with no potential. For the global problem, we establish an evolution law, which is the analogue of the pseudo-conformal conservation law for the nonlinear Schroedinger equation. With this evolution law, we give wave collapse criteria, as well as an upper bound for the blow up time. Taking the physical scales into account, we finally give a lower bound for the blow up time.Comment: 16 pages, no figur
Remarks on nonlinear Schroedinger equations with harmonic potential
remarks on nonlinear schroedinger equations with harmonic potential
bose einstein condensation modeled schroedinger harmonic potential. cauchy equations. potential. establish analogue pseudo conformal conservation schroedinger equation. collapse blow time. blow pages figur
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2554236
10.1007/s00023-003-0122-z
We present a proof of the central limit theorem for a pair of mutually non-commuting operators in mixing quantum spin chains. The operators are not necessarily strictly local but quasi-local. As a corollary we obtain a direct construction of the time evolution of the algebra of normal fluctuation for Gibbs states of finite range interactions on a one-dimensional lattice. We show that the state of the algebra of normal fluctuation satisfies the $\beta$-KMS condition if the microscopic state is a $\beta$-KMS state
On the Algebra of Fluctuation in Quantum Spin Chains
on the algebra of fluctuation in quantum spin chains
mutually commuting chains. necessarily strictly quasi local. corollary fluctuation gibbs lattice. fluctuation satisfies beta microscopic beta
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2554226
10.1007/s00023-003-0128-6
We investigate the ground state energy of an electron coupled to a photon field. First, we regard the self-energy of a free electron, which we describe by the Pauli-Fierz Hamiltonian. We show that, in the case of small values of the coupling constant $\alpha$, the leading order term is represented by $2\pi^{-1} \alpha (\Lambda - \ln[1 + \Lambda])$. Next we put the electron in the field of an arbitrary external potential $V$, such that the corresponding Schr\"odinger operator $p^2 + V$ has at least one eigenvalue, and show that by coupling to the radiation field the binding energy increases, at least for small enough values of the coupling constant $\alpha$. Moreover, we provide concrete numbers for $\alpha$, the ultraviolet cut-off $\Lambda$, and the radiative correction for which our procedure works.Comment: final version, to appear in Ann. Henri Poincar
One non-relativistic particle coupled to a photon field
one non-relativistic particle coupled to a photon field
field. regard pauli fierz hamiltonian. alpha alpha lambda lambda schr odinger eigenvalue alpha concrete alpha ultraviolet lambda radiative ann. henri poincar
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2428359
10.1007/s00023-003-0133-9
We prove that there are no restrictions on the spatial topology of asymptotically flat solutions of the vacuum Einstein equations in (n+1)-dimensions. We do this by gluing a solution of the vacuum constraint equations on an arbitrary compact manifold to an asymptotically Euclidean solution of the constraints on R^n. For any compact manifold which does not admit a metric of positive scalar curvature, this provides for the existence of asymptotically flat vacuum spacetimes with no maximal slices. Our main theorem is a special case of a more general gluing construction for nondegenerate solutions of the vacuum constraint equations which have some restrictions on the mean curvature, but for which the mean curvature is not necessarily constant. This generalizes the construction [IMP] (gr-qc/0109045), which is restricted to constant mean curvature data.Comment: 14 pages, v2 is a substantial revision of the previous version: superfluous condition removed from main theorem and applications to the existence of spacetimes with no maximal Cauchy surfaces adde
On the topology of vacuum spacetimes
on the topology of vacuum spacetimes
restrictions topology asymptotically einstein dimensions. gluing manifold asymptotically euclidean manifold admit curvature asymptotically spacetimes maximal slices. gluing nondegenerate restrictions curvature curvature necessarily constant. generalizes restricted curvature pages substantial revision superfluous removed spacetimes maximal cauchy adde
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2554610
10.1007/s00023-003-0141-9
Motivated by structural issues in the AdS-CFT correspondence, the theory of generalized free fields is reconsidered. A stress-energy tensor for the generalized free field is constructed as a limit of Wightman fields. Although this limit is singular, it fulfils the requirements of a conserved local density for the Poincar'e generators. An explicit "holographic" formula relating the Klein-Gordon field on AdS to generalized free fields on Minkowski space-time is provided, and contrasted with the "algebraic" notion of holography. A simple relation between the singular stress-energy tensor and the canonical AdS stress-energy tensor is exhibited.Comment: 25 page
Generalized free fields and the AdS-CFT correspondence
generalized free fields and the ads-cft correspondence
motivated correspondence reconsidered. wightman fields. singular fulfils conserved poincar generators. holographic relating klein gordon minkowski contrasted algebraic notion holography. singular canonical
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2556141
10.1007/s00023-003-0142-8
We consider a relativistic Ansatz for the vacuum expectation values (VEVs) of a quantum field on a globally hyperbolic space-time which is motivated by certain Euclidean field theories. The Yang-Feldman asymptotic condition w.r.t. a "in"-field in a quasi-free representation of the canonic commutation relations (CCR) leads to a solution of this Ansatz for the VEVs. A GNS-like construction on a non-degenerate inner product space then gives local, covariant quantum fields with indefinite metric on a globally hyperbolic space-time. The non-trivial scattering behavior of quantum fields is analyzed by construction of the "out"-fields and calculation of the scattering matrix. A new combined effect of non-trivial quantum scattering and non-stationary gravitational forces is described for this model, as quasi-free "in"- fields are scattered to "out"-fields which form a non quasi-free representations of the CCR. The asymptotic condition, on which the construction is based, is verified for the concrete example of de Sitter space-time
An indefinite metric model for interacting quantum fields with non-stationary background gravitation
an indefinite metric model for interacting quantum fields with non-stationary background gravitation
relativistic ansatz expectation vevs globally hyperbolic motivated euclidean theories. feldman asymptotic w.r.t. quasi canonic commutation ansatz vevs. degenerate covariant indefinite globally hyperbolic time. trivial matrix. trivial stationary gravitational forces quasi scattered quasi representations ccr. asymptotic verified concrete sitter
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2554845
10.1007/s00023-003-0150-8
The general theory of simple transport processes between quantum mechanical reservoirs is reviewed and extended. We focus on thermoelectric phenomena, involving exchange of energy and particles. Entropy production and Onsager relations are relevant thermodynamic notions which are shown to emerge from the microscopic description. The theory is illustrated on the example of two reservoirs of free fermions coupled through a local interaction. We construct a stationary state and determine energy- and particle currents with the help of a convergent perturbation series. We explicitly calculate several interesting quantities to lowest order, such as the entropy production, the resistance, and the heat conductivity. Convergence of the perturbation series allows us to prove that they are strictly positive under suitable assumptions on the interaction between the reservoirs.Comment: 55 pages; 2 figure
Dissipative Transport: Thermal Contacts and Tunnelling Junctions
dissipative transport: thermal contacts and tunnelling junctions
reservoirs reviewed extended. thermoelectric phenomena involving particles. onsager thermodynamic notions emerge microscopic description. illustrated reservoirs fermions interaction. stationary currents convergent perturbation series. explicitly quantities conductivity. perturbation strictly assumptions pages
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25334563
10.1007/s00023-003-0158-0
The lattice model of scalar quantum electrodynamics (Maxwell field coupled to a complex scalar field) in the Hamiltonian framework is discussed. It is shown that the algebra of observables ${\cal O}({\Lambda})$ of this model is a $C^*$-algebra, generated by a set of gauge-invariant elements satisfying the Gauss law and some additional relations. Next, the faithful, irreducible and non-degenerate representations of ${\cal O}({\Lambda})$ are found. They are labeled by the value of the total electric charge, leading to a decomposition of the physical Hilbert space into charge superselection sectors. In the Appendices we give a unified description of spinorial and scalar quantum electrodynamics and, as a byproduct, we present an interesting example of weakly commuting operators, which do not commute strongly
Charge Superselection Sectors for Scalar QED on the Lattice
charge superselection sectors for scalar qed on the lattice
electrodynamics maxwell discussed. observables lambda satisfying gauss relations. faithful irreducible degenerate representations lambda found. labeled decomposition hilbert superselection sectors. appendices unified spinorial electrodynamics byproduct weakly commuting commute
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2469699
10.1007/s00023-003-0916-z
According to the present understanding, the observed diversity of the strong interaction phenomena is described by Quantum Chromodynamics, a gauge field theory with only very few parameters. One of the fundamental questions in this context is how precisely the world of mesons and nucleons is related to the properties of the theory at high energies, where quarks and gluons are the important degrees of freedom. The lattice formulation of QCD combined with numerical simulations and standard perturbation theory are the tools that allow one to address this issue at a quantitative level.Comment: Plenary talk, International Conference on Theoretical Physics, Paris, UNESCO, 22--27 July 2002; TeX source, 15 pages, figures include
Lattice QCD -- from quark confinement to asymptotic freedom
lattice qcd -- from quark confinement to asymptotic freedom
diversity phenomena chromodynamics parameters. precisely mesons nucleons quarks gluons freedom. formulation perturbation plenary talk paris unesco pages
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25364710
10.1007/s00023-003-0926-x
Inflation has been the driving idea in cosmology for two decades and is a pillar of the New Cosmology. The inflationary paradigm has now passed its first round of significant tests, with two of its three basics predictions confirmed at about the 10% level. The Inflationary Paradigm has some of the truth. Over the next decade the precision of these tests, most of which involve measurements of CMB anisotropy and polarization, will improve 30 fold or more(!), testing inflation more sharply and possibly elucidating the underlying cause. Especially important in this regard is detecting the inflation-produced gravitational waves, either directly or through their CMB polarization signature. While inflation has by no means been verified, its successes have raised the bar for competitor theories: Any alternative must feature the two hallmarks of inflation: superluminal expansion and entropy production
The New Cosmology: Mid-term Report Card for Inflation
the new cosmology: mid-term report card for inflation
inflation driving cosmology decades pillar cosmology. inflationary paradigm passed round basics confirmed level. inflationary paradigm truth. decade precision involve anisotropy inflation sharply possibly elucidating cause. regard detecting inflation gravitational signature. inflation verified successes raised competitor hallmarks inflation superluminal
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2356737
10.1007/s00023-003-0928-8
Over the years, problems like percolation and self-avoiding walks have provided important testing grounds for our understanding of the nature of the critical state. I describe some very recent ideas, as well as some older ones, which cast light both on these problems themselves and on the quantum field theories to which they correspond. These ideas come from conformal field theory, Coulomb gas mappings, and stochastic Loewner evolution.Comment: Plenary talk given at TH-2002, Paris. 21 pages, 9 figure
Conformal Invariance in Percolation, Self-Avoiding Walks and Related Problems
conformal invariance in percolation, self-avoiding walks and related problems
percolation avoiding walks grounds state. ideas older cast correspond. ideas come conformal coulomb mappings stochastic loewner plenary talk paris. pages
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2554990
10.1007/s00023-003-0935-9
This article will review recent results on dimensional reduction for branched polymers, and discuss implications for critical phenomena. Parisi and Sourlas argued in 1981 that branched polymers fall into the universality class of the Yang-Lee edge in two fewer dimensions. Brydges and I have proven in [math-ph/0107005] that the generating function for self-avoiding branched polymers in D+2 continuum dimensions is proportional to the pressure of the hard-core continuum gas at negative activity in D dimensions (which is in the Yang-Lee or $i \phi^3$ class). I will describe how this equivalence arises from an underlying supersymmetry of the branched polymer model. - I will also use dimensional reduction to analyze the crossover of two-dimensional branched polymers to their mean-field limit, and to show that the scaling is given by an Airy function (the same as in [cond-mat/0107223]).Comment: 15 pages, 1 eps figur
Dimensional Reduction and Crossover to Mean-Field Behavior for Branched Polymers
dimensional reduction and crossover to mean-field behavior for branched polymers
branched polymers phenomena. parisi sourlas argued branched polymers fall universality fewer dimensions. brydges proven math generating avoiding branched polymers continuum continuum equivalence arises supersymmetry branched polymer model. analyze crossover branched polymers airy cond .comment pages figur
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2362943
10.1007/s00023-003-0943-9
The study of many body physics has provided a scientific playground of surprise and continuing revolution over the past half century. The serendipitous discovery of new states and properties of matter, phenomena such as superfluidity, the Meissner, the Kondo and the fractional quantum hall effect, have driven the development of new conceptual frameworks for our understanding about collective behavior, the ramifications of which have spread far beyond the confines of terrestrial condensed matter physics- to cosmology, nuclear and particle physics. Here I shall selectively review some of the developments in this field, from the cold-war period, until the present day. I describe how, with the discovery of new classes of collective order, the unfolding puzzles of high temperature superconductivity and quantum criticality, the prospects for major conceptual discoveries remain as bright today as they were more than half a century ago.Comment: Write up of talk presented at TH-2002, July 2002, Paris. Various corrections adde
Many Body Physics: Unfinished Revolution
many body physics: unfinished revolution
playground surprise continuing revolution century. serendipitous discovery phenomena superfluidity meissner kondo fractional hall conceptual frameworks collective ramifications spread confines terrestrial condensed cosmology physics. selectively developments cold day. discovery collective unfolding puzzles superconductivity criticality prospects conceptual discoveries bright today century talk paris. adde
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2356234
10.1007/s00023-003-0961-7
There exist methods to reformulate in an exact way the many-body problem of interacting bosons in terms of the stochastic evolution of single particle wave functions. For one such reformulation, the so-called simple Fock scheme, we present an elementary derivation, much simpler than the original one. Furthermore, we show that two other schemes, based on coherent states of the matter field rather than on Fock states, lead to an infinite statistical uncertainty in the continuous time limit. The simple Fock scheme is therefore, up to now, the only one that was proved to lead to a convergent Monte Carlo simulation scheme at all times.Comment: Proceedings of the Laser Physics Workshop held in Bratislava, July 2002. Submitted to Laser Physic
Exact reformulation of the bosonic many-body problem in terms of stochastic wave functions: convergence issues
exact reformulation of the bosonic many-body problem in terms of stochastic wave functions: convergence issues
reformulate interacting bosons stochastic functions. reformulation fock elementary derivation simpler one. schemes coherent fock infinite limit. fock proved convergent monte carlo workshop held bratislava submitted physic
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2362536
10.1007/s00023-003-0964-4
Arising as a fluctuation phenomenon, the equilibrium distribution of meandering steps with mean separation $<\ell>$ on a "tilted" surface can be fruitfully analyzed using results from RMT. The set of step configurations in 2D can be mapped onto the world lines of spinless fermions in 1+1D using the Calogero-Sutherland model. The strength of the ("instantaneous", inverse-square) elastic repulsion between steps, in dimensionless form, is $\beta(\beta-2)/4$. The distribution of spacings $s< \ell>$ between neighboring steps (analogous to the normalized spacings of energy levels) is well described by a {\it "generalized" Wigner surmise}: $p_{\beta}(0,s) \approx a s^{\beta}\exp(-b s^2)$. The value of $\beta$ is taken to best fit the data; typically $2 \le \beta \le 10$. The procedure is superior to conventional Gaussian and mean-field approaches, and progress is being made on formal justification. Furthermore, the theoretically simpler step-step distribution function can be measured and analyzed based on exact results. Formal results and applications to experiments on metals and semiconductors are summarized, along with open questions. (conference abstract)Comment: 7 pages, 2 figures; based on talk presented at TH-2002, UNESCO, Paris, July 2002; to be published in Ann. Henri Poincare
Applications of Ideas from Random Matrix Theory to Step Distributions on "Misoriented" Surfaces
applications of ideas from random matrix theory to step distributions on "misoriented" surfaces
arising fluctuation phenomenon meandering tilted fruitfully rmt. configurations mapped spinless fermions calogero sutherland model. instantaneous elastic repulsion dimensionless beta beta spacings neighboring analogous spacings wigner surmise beta approx beta beta beta superior progress formal justification. theoretically simpler results. formal metals semiconductors summarized questions. comment pages talk unesco paris ann. henri poincare
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2357119
10.1007/s00023-003-0966-2
We discuss recently discovered links of the statistical models of normal random matrices to some important physical problems of pattern formation and to the quantum Hall effect. Specifically, the large $N$ limit of the normal matrix model with a general statistical weight describes dynamics of the interface between two incompressible fluids with different viscousities in a thin plane cell (the Saffman-Taylor problem). The latter appears to be mathematically equivalent to the growth of semiclassical 2D electronic droplets in a strong uniform magnetic field with localized magnetic impurities (fluxes), as the number of electrons increases. The equivalence is most easily seen by relating the both problems to the matrix model.Comment: 10 pages, 3 figures, Talk given at TH-2002, Paris, UNESCO, July 200
New applications of non-hermitian random matrices
new applications of non-hermitian random matrices
discovered links hall effect. describes incompressible fluids viscousities saffman taylor mathematically semiclassical droplets localized impurities fluxes increases. equivalence relating pages talk paris unesco
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2355057
10.1007/s00023-003-0975-1
We show for a model of scale-free graphs with biased partner choice that knowing the exponent for the degree distribution is in general not sufficient to decide epidemic threshold properties for exponents less than three.We show that the connectivity between the high degree vertices and therefore the diameter is the relevant geometric quantity for epidemic threshold estimations.Absence of epidemic threshold happens precisely when a positive fraction of the nodes form a cluster of bounded diameter.Comment: 10 page
Epidemic thresholds on scale-free graphs: the interplay between exponent and preferential choice
epidemic thresholds on scale-free graphs: the interplay between exponent and preferential choice
biased partner knowing exponent decide epidemic exponents three.we connectivity geometric quantity epidemic estimations.absence epidemic happens precisely
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2570528
10.1007/s00023-004-0160-1
This is the first in a series of works devoted to small non-selfadjoint perturbations of selfadjoint $h$-pseudodifferential operators in dimension 2. In the present work we treat the case when the classical flow of the unperturbed part is periodic and the strength $\epsilon$ of the perturbation is $\gg h$ (or sometimes only $\gg h^2$) and bounded from above by $h^{\delta}$ for some $\delta>0$. We get a complete asymptotic description of all eigenvalues in certain rectangles $[-1/C, 1/C]+ i\epsilon [F_0-1/C,F_0+1/C]$.Comment: 81 page
Non-selfadjoint perturbations of selfadjoint operators in 2 dimensions I
non-selfadjoint perturbations of selfadjoint operators in 2 dimensions i
devoted selfadjoint perturbations selfadjoint pseudodifferential treat unperturbed epsilon perturbation sometimes delta delta asymptotic eigenvalues rectangles epsilon .comment
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2555149
10.1007/s00023-004-0165-9
The asymptotic properties at future null infinity of the solutions of the relativistic Vlasov-Maxwell system whose global existence for small data has been established by the author in a previous work are investigated. These solutions describe a collisionless plasma isolated from incoming radiation. It is shown that a non-negative quantity associated to the plasma decreases as a consequence of the dissipation of energy in form of outgoing radiation. This quantity represents the analogue of the Bondi mass in general relativity.Comment: 13 pages; version in press. This paper continues the analysis started in math-ph/021101
Outgoing radiation from an isolated collisionless plasma
outgoing radiation from an isolated collisionless plasma
asymptotic infinity relativistic vlasov maxwell investigated. collisionless incoming radiation. quantity dissipation outgoing radiation. quantity analogue bondi pages press. continues started math
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2568752
10.1007/s00023-004-0166-8
We consider the system of $N$ ($\ge2$) hard balls with masses $m_1,...,m_N$ and radius $r$ in the flat torus $\Bbb T_L^\nu=\Bbb R^\nu/L\cdot\Bbb Z^\nu$ of size $L$, $\nu\ge3$. We prove the ergodicity (actually, the Bernoulli mixing property) of such systems for almost every selection $(m_1,...,m_N; L)$ of the outer geometric parameters. This theorem complements my earlier result that proved the same, almost sure ergodicity for the case $\nu=2$. The method of that proof was primarily dynamical-geometric, whereas the present approach is inherently algebraic.Comment: 31 pages, no figure
Proof of the Ergodic Hypothesis for Typical Hard Ball Systems
proof of the ergodic hypothesis for typical hard ball systems
balls torus cdot ergodicity bernoulli outer geometric parameters. complements proved sure ergodicity primarily geometric inherently pages
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2555158
10.1007/s00023-004-0170-z
We present an implementation in conformal field theory (CFT) of local finite conformal transformations fixing a point. We give explicit constructions when the fixed point is either the origin or the point at infinity. Both cases involve the exponentiation of a Borel subalgebra of the Virasoro algebra. We use this to build coherent state representations and to derive a close analog of Wick's theorem for the Virasoro algebra. This allows to compute the conformal partition function in non trivial geometries obtained by removal of hulls from the upper half plane. This is then applied to stochastic Loewner evolutions (SLE). We give a rigorous derivation of the equations, obtained previously by the authors, that connect the stochastic Loewner equation to the representation theory of the Virasoro algebra. We give a new proof that this construction enumerates all polynomial SLE martingales. When one of the hulls removed from the upper half plane is the SLE hull, we show that the partition function is a famous local martingale known to probabilists, thereby unravelling its CFT origin.Comment: 41 pages, 4 figure
Conformal transformations and the SLE partition function martingale
conformal transformations and the sle partition function martingale
conformal conformal transformations fixing point. constructions infinity. involve exponentiation borel subalgebra virasoro algebra. build coherent representations derive analog wick virasoro algebra. conformal partition trivial geometries removal hulls plane. stochastic loewner evolutions rigorous derivation connect stochastic loewner virasoro algebra. enumerates martingales. hulls removed hull partition famous martingale probabilists thereby unravelling pages
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2555065
10.1007/s00023-004-0180-x
The Pauli operator describes the energy of a nonrelativistic quantum particle with spin 1/2 in a magnetic field and an external potential. A new Lieb-Thirring type inequality on the sum of the negative eigenvalues is presented. The main feature compared to earlier results is that in the large field regime the present estimate grows with the optimal (first) power of the strength of the magnetic field. As a byproduct of the method, we also obtain an optimal upper bound on the pointwise density of zero energy eigenfunctions of the Dirac operator. The main technical tools are: (i) a new localization scheme for the square of the resolvent of a general class of second order elliptic operators; (ii) a geometric construction of a Dirac operator with a constant magnetic field that approximates the original Dirac operator in a tubular neighborhood of a fixed field line. The errors may depend on the regularity of the magnetic field but they are uniform in the field strength.Comment: latex file. Revised final version: typos corrected, the definition of the lengthscale simplified, references added/update
Uniform Lieb-Thirring inequality for the three dimensional Pauli operator with a strong non-homogeneous magnetic field
uniform lieb-thirring inequality for the three dimensional pauli operator with a strong non-homogeneous magnetic field
pauli describes nonrelativistic potential. lieb thirring inequality eigenvalues presented. grows field. byproduct pointwise eigenfunctions dirac operator. localization resolvent elliptic geometric dirac approximates dirac tubular neighborhood line. regularity latex file. revised typos corrected lengthscale simplified update
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2555292
10.1007/s00023-004-0182-8
We study a system of a quantum particle interacting with a singular time-dependent uniformly rotating potential in 2 and 3 dimensions: in particular we consider an interaction with support on a point (rotating point interaction) and on a set of codimension 1 (rotating blade). We prove the existence of the Hamiltonians of such systems as suitable self-adjoint operators and we give an explicit expression for their unitary semigroups. Moreover we analyze the asymptotic limit of large angular velocity and we prove strong convergence of the time-dependent propagator to some one-parameter unitary group as (\omega \to \infty).Comment: Minor changes, to appear in Ann. H. Poincare', 35 pages, LaTe
Rotating Singular Perturbations of the Laplacian
rotating singular perturbations of the laplacian
interacting singular uniformly rotating rotating codimension rotating blade hamiltonians adjoint unitary semigroups. analyze asymptotic propagator unitary omega infty .comment minor ann. poincare pages
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2555284
10.1007/s00023-004-0183-7
The method of scaling algebras, which has been introduced earlier as a means for analyzing the short-distance behaviour of quantum field theories in the setting of the model-independent, operator-algebraic approach, is extended to the case of fields carrying superselection charges. In doing so, consideration will be given to strictly localizable charges ("DHR-type" superselection charges) as well as to charges which can only be localized in regions extending to spacelike infinity ("BF-type" superselection charges). A criterion for the preservance of superselection charges in the short-distance scaling limit is proposed. Consequences of this preservance of superselection charges are studied. The conjugate charge of a preserved charge is also preserved, and for charges of DHR-type, the preservance of all charges of a quantum field theory in the scaling limit leads to equivalence of local and global intertwiners between superselection sectors.Comment: Latex 2e, 57 pages. Supersedes hep-th/030114
Scaling algebras for charged fields and short-distance analysis for localizable and topological charges
scaling algebras for charged fields and short-distance analysis for localizable and topological charges
algebras analyzing algebraic carrying superselection charges. consideration strictly localizable charges superselection charges charges localized extending spacelike infinity superselection charges criterion preservance superselection charges proposed. consequences preservance superselection charges studied. conjugate preserved preserved charges preservance charges equivalence intertwiners superselection latex pages. supersedes
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2430409
10.1007/s00023-004-0189-1
A positive cosmological constant simplifies the asymptotics of forever expanding cosmological solutions of the Einstein equations. In this paper a general mathematical analysis on the level of formal power series is carried out for vacuum spacetimes of any dimension and perfect fluid spacetimes with linear equation of state in spacetime dimension four. For equations of state stiffer than radiation evidence for development of large gradients, analogous to spikes in Gowdy spacetimes, is found. It is shown that any vacuum solution satisfying minimal asymptotic conditions has a full asymptotic expansion given by the formal series. In four spacetime dimensions, and for spatially homogeneous spacetimes of any dimension, these minimal conditions can be derived for appropriate initial data. Using Fuchsian methods the existence of vacuum spacetimes with the given formal asymptotics depending on the maximal number of free functions is shown without symmetry assumptions.Comment: 23 page
Asymptotics of solutions of the Einstein equations with positive cosmological constant
asymptotics of solutions of the einstein equations with positive cosmological constant
cosmological simplifies asymptotics forever expanding cosmological einstein equations. mathematical formal spacetimes perfect spacetimes spacetime four. stiffer gradients analogous spikes gowdy spacetimes found. satisfying asymptotic asymptotic formal series. spacetime spatially homogeneous spacetimes data. fuchsian spacetimes formal asymptotics maximal
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2555738
10.1007/s00023-004-0190-8
Within the algebraic setting of quantum field theory, a condition is given which implies that the intersection of algebras generated by field operators localized in wedge--shaped regions of two--dimensional Minkowski space is non--trivial; in particular, there exist compactly localized operators in such theories which can be interpreted as local observables. The condition is based on spectral (nuclearity) properties of the modular operators affiliated with wedge algebras and the vacuum state and is of interest in the algebraic approach to the formfactor program, initiated by Schroer. It is illustrated here in a simple class of examples.Comment: 14 pages, no figure
Modular Nuclearity and Localization
modular nuclearity and localization
algebraic intersection algebras localized wedge shaped minkowski trivial compactly localized interpreted observables. nuclearity modular affiliated wedge algebras algebraic formfactor initiated schroer. illustrated pages
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2555238
10.1007/s00023-004-0194-4
We consider an external potential, $-\lambda \phi$, due to one or more nuclei. Following the Dirac picture such a potential polarizes the vacuum. The polarization density as derived in physics literature, after a well known renormalization procedure, depends decisively on the strength of $\lambda$. For small $\lambda$, more precisely as long as the lowest eigenvalue, $e_1(\lambda)$, of the corresponding Dirac operator stays in the gap of the essential spectrum, the integral over the density vanishes. In other words the vacuum stays neutral. But as soon as $e_1(\lambda)$ dives into the lower continuum the vacuum gets spontaneously charged with charge $ 2e$. Global charge conservation implies that two positrons were emitted out of the vacuum, this is, a large enough external potential can produce electron-positron pairs. We give a rigorous proof of that phenomenon.Comment: proofs correcte
On the Vacuum Polarization Density Caused by an External Field
on the vacuum polarization density caused by an external field
lambda nuclei. dirac picture polarizes vacuum. renormalization decisively lambda lambda precisely eigenvalue lambda dirac stays vanishes. stays neutral. soon lambda dives continuum gets spontaneously conservation positrons emitted positron pairs. rigorous proofs correcte
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2555901
10.1007/s00023-004-0195-3
Products of random matrices associated to one-dimensional random media satisfy a central limit theorem assuring convergence to a gaussian centered at the Lyapunov exponent. The hypothesis of single parameter scaling states that its variance is equal to the Lyapunov exponent. We settle discussions about its validity for a wide class of models by proving that, away from anomalies, single parameter scaling holds to lowest order perturbation theory in the disorder strength. However, it is generically violated at higher order. This is explicitely exhibited for the Anderson model.Comment: minor corrections to previous version, to appear in Annales H. Poincar
Perturbative test of single parameter scaling for 1D random media
perturbative test of single parameter scaling for 1d random media
satisfy assuring centered lyapunov exponent. lyapunov exponent. settle discussions validity proving away anomalies perturbation disorder strength. generically violated order. explicitely exhibited anderson minor annales poincar
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2555414
10.1007/s00023-004-0196-2
We present a rigorous proof of an ordering transition for a two-component two-dimensional antiferromagnet with nearest and next-nearest neighbor interactions. The low-temperature phase contains two states distinguished by local order among columns or, respectively, rows. Overall, there is no magnetic order in accord with the classic Mermin-Wagner theorem. The method of proof employs a rigorous version of "order by disorder," whereby a high degeneracy among the ground states is lifted according to the differences in their associated spin-wave spectra.Comment: 22 pages, 1 eps fi
Order by disorder, without order, in a two-dimensional spin system with O(2) symmetry
order by disorder, without order, in a two-dimensional spin system with o(2) symmetry
rigorous ordering antiferromagnet nearest nearest neighbor interactions. distinguished columns rows. accord classic mermin wagner theorem. employs rigorous disorder whereby degeneracy lifted pages
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2555724
10.1007/s00023-005-0199-7
We study the ground state solutions of the Dirac-Fock model in the case of weak electronic repulsion, using bifurcation theory. They are solutions of a min-max problem. Then we investigate a max-min problem coming from the electron-positron field theory of Bach-Barbaroux-Helffer-Siedentop. We show that given a radially symmetric nuclear charge, the ground state of Dirac-Fock solves this max-min problem for certain numbers of electrons. But we also exhibit a situation in which the max-min level does not correspond to a solution of the Dirac-Fock equations together with its associated self-consistent projector
Some connections between Dirac-Fock and Electron-Positron Hartree-Fock
some connections between dirac-fock and electron-positron hartree-fock
dirac fock repulsion bifurcation theory. problem. coming positron bach barbaroux helffer siedentop. radially dirac fock solves electrons. exhibit dirac fock projector
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2430810
10.1007/s00023-005-0202-3
We prove that generic solutions of the vacuum constraint Einstein equations do not possess any global or local space-time Killing vectors, on an asymptotically flat Cauchy surface, or on a compact Cauchy surface with mean curvature close to a constant, or for CMC asymptotically hyperbolic initial data sets. More generally, we show that non-existence of global symmetries implies, generically, non-existence of local ones. As part of the argument, we prove that generic metrics do not possess any local or global conformal Killing vectors.Comment: latex2e, 38 pages in A4 now, minor corrections throughou
KIDs are non-generic
kids are non-generic
generic einstein possess killing asymptotically cauchy cauchy curvature asymptotically hyperbolic sets. symmetries generically ones. argument generic metrics possess conformal killing latex pages minor throughou
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2554968
10.1007/s00023-005-0203-2
We prove a product formula which involves the unitary group generated by a semibounded self-adjoint operator and an orthogonal projection $P$ on a separable Hilbert space $\HH$, with the convergence in $L^2_\mathrm{loc}(\mathbb{R};\HH)$. It gives a partial answer to the question about existence of the limit which describes quantum Zeno dynamics in the subspace \hbox{$\mathrm{Ran} P$}. The convergence in $\HH$ is demonstrated in the case of a finite-dimensional $P$. The main result is illustrated in the example where the projection corresponds to a domain in $\mathbb{R}^d$ and the unitary group is the free Schr\"odinger evolution.Comment: LaTeX 2e, 24 pages, with substantial modifications, to appear in Ann. H. Poincar
Product formula related to quantum Zeno dynamics
product formula related to quantum zeno dynamics
involves unitary semibounded adjoint orthogonal projection separable hilbert mathrm mathbb answer describes zeno subspace hbox mathrm illustrated projection mathbb unitary schr odinger latex pages substantial modifications ann. poincar
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2555825
10.1007/s00023-005-0204-1
It is known that for multi-level time-dependent quantum systems one can construct superadiabatic representations in which the coupling between separated levels is exponentially small in the adiabatic limit. For a family of two-state systems with real-symmetric Hamiltonian we construct such a superadiabatic representation and explicitly determine the asymptotic behavior of the exponentially small coupling term. First order perturbation theory in the superadiabatic representation then allows us to describe the time-development of exponentially small adiabatic transitions. The latter result rigorously confirms the predictions of Sir Michael Berry for our family of Hamiltonians and slightly generalizes a recent mathematical result of George Hagedorn and Alain Joye.Comment: 24 page
Precise coupling terms in adiabatic quantum evolution
precise coupling terms in adiabatic quantum evolution
superadiabatic representations separated exponentially adiabatic limit. superadiabatic explicitly asymptotic exponentially term. perturbation superadiabatic exponentially adiabatic transitions. rigorously confirms michael berry hamiltonians generalizes mathematical george hagedorn alain
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2555876
10.1007/s00023-005-0208-x
We consider continuum random Schr\"odinger operators of the type $H_{\omega} = -\Delta + V_0 + V_{\omega}$ with a deterministic background potential $V_0$. We establish criteria for the absence of continuous and absolutely continuous spectrum, respectively, outside the spectrum of $-\Delta +V_0$. The models we treat include random surface potentials as well as sparse or slowly decaying random potentials. In particular, we establish absence of absolutely continuous surface spectrum for random potentials supported near a one-dimensional surface (``random tube'') in arbitrary dimension.Comment: 14 pages, 2 figure
Absence of continuous spectral types for certain nonstationary random models
absence of continuous spectral types for certain nonstationary random models
continuum schr odinger omega delta omega deterministic establish absolutely delta treat potentials sparse slowly decaying potentials. establish absolutely potentials tube pages
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2555916
10.1007/s00023-005-0209-9
We consider the magnetic Schrodinger operator in a two-dimensional strip. On the boundary of the strip the Dirichlet boundary condition is imposed except for a fixed segment (window), where it switches to magnetic Neumann boundary condition (see Section 2, Eq. (2.2) for the definition of this boundary condition}. We deal with a smooth compactly supported field as well as with the Aharonov-Bohm field. We give an estimate on the maximal length of the window, for which the discrete spectrum of the considered operator will be empty. In the case of a compactly supported field we also give a sufficient condition for the presence of eigenvalues below the essential spectrum
Spectrum of the Magnetic Schrodinger Operator in a Waveguide with Combined Boundary Conditions
spectrum of the magnetic schrodinger operator in a waveguide with combined boundary conditions
schrodinger strip. strip dirichlet imposed segment window switches neumann deal compactly aharonov bohm field. maximal window empty. compactly eigenvalues
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2523650
10.1007/s00023-005-0210-3
We show how the Hopf algebra of rooted trees encodes the combinatorics of Epstein-Glaser renormalization and coordinate space renormalization in general. In particular we prove that the Epstein-Glaser time-ordered products can be obtained from the Hopf algebra by suitable Feynman rules, mapping trees to operator-valued distributions. Twisting the antipode with a renormalization map formally solves the Epstein-Glaser recursion and provides local counterterms due to the Hochschild 1-closedness of the grafting operator $B_+$.Comment: 19p, minor corrections and improvements. To appear in AH
The Hopf algebra of rooted trees in Epstein-Glaser renormalization
the hopf algebra of rooted trees in epstein-glaser renormalization
hopf rooted trees encodes combinatorics epstein glaser renormalization coordinate renormalization general. epstein glaser ordered hopf feynman trees valued distributions. twisting antipode renormalization formally solves epstein glaser recursion counterterms hochschild closedness grafting .comment minor improvements.
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2373314
10.1007/s00023-005-0213-0
We prove that the two dimensional Hubbard model at finite temperature T and half-filling is analytic in the coupling constant in a radius at least $c/(\log T)^2$. We also study the self-energy through a new two-particle irreducible expansion and prove that this model is not a Fermi liquid, but a Luttinger liquid with logarithmic corrections. The techniques used are borrowed from constructive field theory so the result is mathematically rigorous and completely non-perturbative. Together with earlier results on the existence of two dimensional Fermi liquids, this new result proves that the nature of interacting Fermi systems in two dimensions depends on the shape of the Fermi surface.Comment: 45 pages, 28 figure
Renormalization of the 2-point function of the Hubbard model at half-filling
renormalization of the 2-point function of the hubbard model at half-filling
hubbard filling analytic irreducible fermi luttinger logarithmic corrections. borrowed constructive mathematically rigorous perturbative. fermi liquids proves interacting fermi fermi pages
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2576264
10.1007/s00023-005-0215-y
In this paper we construct star products on Marsden-Weinstein reduced spaces in case both the original phase space and the reduced phase space are (symplectomorphic to) cotangent bundles. Under the assumption that the original cotangent bundle $T^*Q$ carries a symplectique structure of form $\omega_{B_0}=\omega_0 + \pi^*B_0$ with $B_0$ a closed two-form on $Q$, is equipped by the cotangent lift of a proper and free Lie group action on $Q$ and by an invariant star product that admits a $G$-equivariant quantum momentum map, we show that the reduced phase space inherits from $T^*Q$ a star product. Moreover, we provide a concrete description of the resulting star product in terms of the initial star product on $T^*Q$ and prove that our reduction scheme is independent of the characteristic class of the initial star product. Unlike other existing reduction schemes we are thus able to reduce not only strongly invariant star products. Furthermore in this article, we establish a relation between the characteristic class of the original star product and the characteristic class of the reduced star product and provide a classification up to $G$-equivalence of those star products on $(T^*Q,\omega_{B_0})$, which are invariant with respect to a lifted Lie group action. Finally, we investigate the question under which circumstances `quantization commutes with reduction' and show that in our examples non-trivial restrictions arise
Phase Space Reduction of Star Products on Cotangent Bundles
phase space reduction of star products on cotangent bundles
marsden weinstein symplectomorphic cotangent bundles. cotangent bundle carries symplectique omega omega equipped cotangent lift proper admits equivariant inherits product. concrete product. unlike schemes products. establish equivalence omega lifted action. circumstances quantization commutes trivial restrictions arise
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2555940
10.1007/s00023-005-0217-9
We study spontaneous symmetry breaking for field algebras on Minkowski space in the presence of a condition of geometric modular action (CGMA) proposed earlier as a selection criterion for vacuum states on general space-times. We show that any internal symmetry group must commute with the representation of the Poincare group (whose existence is assured by the CGMA) and each translation-invariant vector is also Poincare invariant. The subspace of these vectors can be centrally decomposed into pure invariant states and the CGMA holds in the resulting sectors. As positivity of the energy is not assumed, similar results may be expected to hold for other space--times.Comment: Dedicated to the memory of Siegfried Schlieder. 17 pages, no figures. Revised version: simplified arguments and improved results; as to appear in Annales H. Poincar
Geometric modular action and spontaneous symmetry breaking
geometric modular action and spontaneous symmetry breaking
spontaneous breaking algebras minkowski geometric modular cgma criterion times. commute poincare assured cgma translation poincare invariant. subspace centrally decomposed cgma sectors. positivity hold dedicated siegfried schlieder. pages figures. revised simplified arguments annales poincar
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2555771
10.1007/s00023-005-0218-8
We study semiclassical approximations to the time evolution of coherent states for general spin-orbit coupling problems in two different semiclassical scenarios: The limit \hbar to zero is first taken with fixed spin quantum number s and then with \hbar*s held constant. In these two cases different classical spin-orbit dynamics emerge. We prove that a coherent state propagated with a suitable classical dynamics approximates the quantum time evolution up to an error of size \sqrt{\hbar} and identify an Ehrenfest time scale. Subsequently an improvement of the semiclassical error to an arbitray order \hbar^{N/2} is achieved by a suitable deformation of the state that is propagated classically
Semiclassical propagation of coherent states with spin-orbit interaction
semiclassical propagation of coherent states with spin-orbit interaction
semiclassical approximations coherent orbit semiclassical scenarios hbar hbar held constant. orbit emerge. coherent propagated approximates sqrt hbar ehrenfest scale. subsequently semiclassical arbitray hbar deformation propagated classically
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