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We find and analyse solutions of Einstein's equations in arbitrary d dimensions and in the presence of a scalar field with a Liouville potential coupled to a Maxwell field. We consider spacetimes of cylindrical symmetry or again subspaces…

General Relativity and Quantum Cosmology · Physics 2010-06-29 Christos Charmousis , Blaise Goutéraux , Jiro Soda

We construct exact localised solutions of the PT-symmetric Gross-Pitaevskii equation with an attractive cubic nonlinearity. The trapping potential has the form of two $\delta$-function wells, where one well loses particles while the other…

Pattern Formation and Solitons · Physics 2016-07-12 I. V. Barashenkov , D. A. Zezyulin

In dimension N=3 the cubic nonlinear Schrodinger equation has solutions which become singular, i.e. at a spatial point they blow up to infinity in finite time. In 1972 Zakharov famously investigated finite time singularity formation in the…

Analysis of PDEs · Mathematics 2022-10-12 William C. Troy

For the 3D focusing cubic nonlinear Schrodinger equation, Scattering of $H^1$ solutions inside the (scale invariant) potential well was established by Holmer and Roudenko~\cite{HR2} (radial case) and Duyckaerts, Holmer and…

Analysis of PDEs · Mathematics 2011-01-18 Daoyuan Fang , Jian Xie , Thierry Cazenave

We consider the stationary solutions for a class of Schrodinger equations with a N-well potential and a nonlinear perturbation. By means of semiclassical techniques we prove that the dominant term of the ground state solutions is described…

Quantum Physics · Physics 2015-05-30 Andrea Sacchetti

We construct new solutions in series of confluent hypergeometric functions for the confluent Heun equation (CHE). Some of these solutions are applied to the one-dimensional stationary Schr\"{o}dinger equation with hyperbolic and…

Mathematical Physics · Physics 2013-12-02 Léa Jaccoud El-Jaick , Bartolomeu D. B. Figueiredo

One examines the infinitely deep quantum cavity, also known as the quantum infinite square well, within the framework of the real Hilbert space. The solutions are considered in terms of complex wave functions, and also in terms of…

Quantum Physics · Physics 2026-02-19 Sergio Giardino

Exactly solvable models play an extremely important role in many fields of quantum physics. In this study, the Schr\"{o}dinger equation is applied for a solution of a two--dimensional (2D) problem for two particles interacting via Kratzer,…

Quantum Physics · Physics 2023-11-21 Roman Ya. Kezerashvili , Jianning Luo , Claudio R. Malvino

We develop the formalism of quantum mechanics on three dimensional fuzzy space and solve the Schr\"odinger equation for a free particle, finite and infinite fuzzy wells. We show that all results reduce to the appropriate commutative limits.…

High Energy Physics - Theory · Physics 2015-06-22 N Chandra , H W Groenewald , J N Kriel , F G Scholtz , S Vaidya

Based on the Caputo fractional derivative the classical, non relativistic Hamiltonian is quantized leading to a fractional Schroedinger type wave equation. The free particle solutions are localized in space. Solutions for the infinite well…

Mathematical Physics · Physics 2007-05-23 Richard Herrmann

We present the solutions of the Schr$\ddot{o}$dinger equation with the Hulth$\acute{e}$n potential plus ring-shape potential for $\ell\neq 0$ states within the framework of an exponential approximation of the centrifugal potential.Solutions…

Mathematical Physics · Physics 2015-05-13 D. Agboola

We consider the time-dependent non linear Schrodinger equations with a double well potential in dimensions d =1 and d=2. We prove, in the semiclassical limit, that the finite dimensional eigenspace associated to the lowest two eigenvalues…

Mathematical Physics · Physics 2007-05-23 Dario Bambusi , Andrea Sacchetti

Stationary 1D Schr\"odinger equations with polynomial potentials are reduced to explicit countable closed systems of exact quantization conditions, which are selfconsistent constraints upon the zeros of zeta-regularized spectral…

Mathematical Physics · Physics 2009-10-31 A. Voros

We prove optimal (that is, without loss of derivatives) dispersive estimates for the Schrodinger group $e^{it(-\Delta+V)}$ for a class of real-valued potentials $V\in C^k(R^n)$ with $k>(n-3)/2$, where $n=4,5$.

Analysis of PDEs · Mathematics 2008-03-31 Fernando Cardoso , Claudio Cuevas , Georgi Vodev

A general method has been developed to solve the Schr\"odinger equation for an arbitrary derivative of the $\delta$-function potential in 1-d using cutoff regularization. The work treats both the relativistic and nonrelativistic cases. A…

High Energy Physics - Theory · Physics 2019-02-08 M. H. Al-Hashimi , M. Salman , A. M. Shalaby

We present numerically exact solutions to the full-dimensional Schrodinger Equation for the few-electron gas (few-EG) model of electronic structure theory. Our core methodology uses a Sum-of-Products (SOP) representation of singular…

Strongly Correlated Electrons · Physics 2019-11-13 Jonathan Jerke , Eric R Bittner , Bill Poirier

In the approach to the geometric quantization, based on the conversion of second-class constraints, we resolve the respective non-linear zero curvature conditions for the extended symplectic potential. From the zero curvature conditions, we…

High Energy Physics - Theory · Physics 2016-05-20 Igor A. Batalin , Peter M. Lavrov

We consider pointwise convergence of Schr\"{o}dinger means $e^{it_{n}\Delta}f(x)$ for $f \in H^{s}(\mathbb{R}^{2})$ and decreasing sequences $\{t_{n}\}_{n=1}^{\infty}$ converging to zero. The main theorem improves the previous results of…

Classical Analysis and ODEs · Mathematics 2020-11-03 Wenjuan Li , Huiju Wang , Dunyan Yan

We study the classical and quantum models of a Friedmann-Robertson-Walker (FRW) cosmology, coupled to a perfect fluid, in the context of the $f(R)$ gravity. Using the Schutz' representation for the perfect fluid, we show that, under a…

General Relativity and Quantum Cosmology · Physics 2010-04-30 Babak Vakili

We completely classify Friedmann-Lema\^{i}tre-Robertson-Walker solutions with spatial curvature $K=0,\pm 1$ and equation of state $p=w\rho$, according to their conformal structure, singularities and trapping horizons. We do not assume any…

General Relativity and Quantum Cosmology · Physics 2018-05-02 Tomohiro Harada , B. J. Carr , Takahisa Igata
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