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In numerically solving the Helmholtz equation inside a connected plane domain with Dirichlet boundary conditions (the problem of the quantum billiard) one surprisingly faces enormous difficulties if the domain has a problematic geometry…

chao-dyn · Physics 2008-02-03 Baowen Li , Marko Robnik

The arithmetic triangular billiards are classically chaotic but have Poissonian energy level statistics, in ostensible violation of the BGS conjecture. We show that the length spectra of their periodic orbits divides into subspectra…

Chaotic Dynamics · Physics 2015-08-11 Petr Braun

In this paper we consider (n+1)-dimensional cosmological model with scalar field and antisymmetric (p+2)-form. Using an electric composite Sp-brane ansatz the field equations for the original system reduce to the equations for a Toda-like…

High Energy Physics - Theory · Physics 2008-11-26 V. D. Ivashchuk , D. Singleton

A multidimensional gravitational model containing scalar fields and antisymmetric forms is considered. The manifold is chosen in the form $M = M_0 \times M_1 \times \cdots \times M_n$, where $M_i$ are Einstein spaces ($i \geq 1$). The…

High Energy Physics - Theory · Physics 2009-07-07 Vladimir D. Ivashchuk , Vitaly N. Melnikov

We perform a detailed numerical study of energy-level and wavefunction statistics of a deformable quantum billiard focusing on properties relevant to semiconductor quantum dots. We consider the family of Robnik billiards generated by simple…

Condensed Matter · Physics 2009-10-22 Henrik Bruus , A. D. Stone

Integrability of a square billiard is spontaneously broken as it rotates about one of its corners. The system becomes quasi-integrable where the invariant tori are broken with respect to a certain parameter, $\lambda = 2E/\omega^{2}$ where…

Chaotic Dynamics · Physics 2014-06-13 Nandan Jha , Sudhir R. Jain

This paper implements the idea of considering the instantonic creation of brane worlds whose five-dimensional bulk contains a negative cosmological constant and a scalar quintessence field with time-dependent equation of state, restricting…

Astrophysics · Physics 2009-11-06 Pedro F. González-Diáz

We establish a duality between the quantum wave vector spectrum and the eigenmodes of the classical Liouvillian dynamics for integrable billiards. Signatures of the classical eigenmodes appear as peaks in the correlation function of the…

Exactly Solvable and Integrable Systems · Physics 2007-05-23 W. T. Lu , Weiqiao Zeng , S. Sridhar

We analyze the quantum cosmology of one--loop string effective models which exhibit an $O(d,d)$ symmetry. It is shown that due to the large symmetry of these models the Wheeler--de Witt equation can completely be solved. As a result, we…

High Energy Physics - Theory · Physics 2009-10-30 Alexandros A. Kehagias , Andre Lukas

The poles of the S-matrix and the wave functions of open 2D quantum billiards with convex boundary of different shape are calculated by the method of complex scaling. Two leads are attached to the cavities. The conductance of the cavities…

Mesoscale and Nanoscale Physics · Physics 2009-02-06 R. G. Nazmitdinov , K. N. Pichugin , I. Rotter , P. Seba

We study quantum field theories with boundary by utilizing non-invertible symmetries. We consider three kinds of boundary conditions of the four dimensional $\mathbb{Z}_2$ lattice gauge theory at the critical point as examples. The weights…

High Energy Physics - Theory · Physics 2023-09-26 Masataka Koide , Yuta Nagoya , Satoshi Yamaguchi

The Wheeler-DeWitt (WDW) equation is analyzed using two boundary proposals: the Hartle-Hawking no-boundary condition and tunneling condition. By compactifying the scale factor $a$ into $ x = a/(1+a) $, we reformulate the WDW equation to…

General Relativity and Quantum Cosmology · Physics 2025-03-28 Jie Jiang , Deog Ki Hong , Dong-han Yeom

We discuss an extra-dimensional braneworld with a 5th dimension compactified on a circle. As a characteristic feature, the warp factor is hyperbolic and separates the hidden and visible branes by a bulk horizon without a singularity. The…

High Energy Physics - Phenomenology · Physics 2025-03-20 Jeffrey Kuntz , Andreas Trautner

This work presents some results regarding three-dimensional billiards having a non-constant potential of Keplerian type inside a regular domain $D\subset \mathcal R^3$. Two models will be analysed: in the first one, only an inner Keplerian…

Chaotic Dynamics · Physics 2024-10-22 Irene De Blasi

For two-dimensional quantum billiards we derive the partial Weyl law, i.e. the average density of states, for a subset of eigenstates concentrating on an invariant region $\Gamma$ of phase space. The leading term is proportional to the area…

Quantum Physics · Physics 2011-05-03 Arnd Bäcker , Roland Ketzmerick , Steffen Löck , Holger Schanz

We study the quantum dynamics of a supersymmetric squashed three-sphere by dimensionally reducing to one timelike dimension the action of D=4 simple supergravity for a Bianchi IX cosmological model. After imposition of the diffeomorphism…

General Relativity and Quantum Cosmology · Physics 2014-11-11 Thibault Damour , Philippe Spindel

A quantum mesoscopic billiard can be viewed as a bounded electronic system due to some external confining potential. Since, in general, we do not have access to the exact expression of this potential, it is usually replaced by a set of…

Mesoscale and Nanoscale Physics · Physics 2017-02-08 E. Akkermans , R. Narevich

In this paper we consider $(n+1)$-dimensional cosmological model with scalar field and antisymmetric $(p+2)$-form. Using an electric composite $Sp$-brane ansatz the field equations for the original system reduce to the equations for a…

General Relativity and Quantum Cosmology · Physics 2007-05-23 V. D. Ivashchuk , D. Singleton

Rational polygonal billiards are one of the key models among the larger class of pseudo-integrable billiards. Their billiard flow may be lifted to the geodesic flow on a translation surface. Whereas such classical billiards have been much…

Mathematical Physics · Physics 2018-12-21 Omer Friedland , Henrik Ueberschaer

We study the thick brane model within $f(R)\sim R^n$ modified gravity in $D$-dimensional spacetimes with $D\geq 6$. The system under consideration consists of two branes orthogonal to each other: the four-dimensional Lorentzian brane and…

General Relativity and Quantum Cosmology · Physics 2020-04-03 Vladimir Dzhunushaliev , Vladimir Folomeev , Galia Nurtaeva , Sergei D. Odintsov
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