Results 91 to 100 of about 7,066 (206)
Heun’s differential equation and its q-deformation [PDF]
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Schrödinger equation as a confluent Heun equation
Abstract This article deals with two classes of quasi-exactly solvable (QES) trigonometric potentials for which the one-dimensional Schrödinger equation reduces to a confluent Heun equation (CHE) where the independent variable takes only finite values.
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In this paper, we present the exact analytical solution of the Dirac equation with equal scalar and vector generalized Cornell potential plus a novel angle-dependent potential in the framework of quasi-exactly solvable problems.
Djahida Bouchefra, Badredine Boudjedaa
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The 192 solutions of the Heun equation [PDF]
A machine-generated list of 192 local solutions of the Heun equation is given. They are analogous to Kummer's 24 solutions of the Gauss hypergeometric equation, since the two equations are canonical Fuchsian differential equations on the Riemann sphere with four and three singular points, respectively. Tabulation is facilitated by the identification of
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The Dirac equation with both scalar and vector couplings describing the dynamics of a two-dimensional Dirac oscillator in the cosmic string spacetime is considered.
Daniel F. Lima +4 more
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We consider Klein–Gordon equation in the Dyonic Kerr–Sen black hole background, which is the charged rotating axially symmetric solution of the Einstein–Maxwell–Dilaton–Axion theory of gravity.
David Senjaya +2 more
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On spectral polynomials of the Heun equation. I
The classical Heun equation has the form {Q(z) d^2/dz^2 +P(z) d/dz +V(z)}S(z)=0 where Q(z) is a cubic, P(z) at most quadratic and V(z) linear polynomials resp. In the second half of the 19-th century E.Heine and T.STieltjes initiated the study of the set of all V(z) such that the above equation has a polynomial solution S(z) of a given degree n.
Shapiro, Boris, Tater, Milos
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Scalar quasi-normal modes of accelerating Kerr-Newman-AdS black holes
We study linear scalar perturbations of slowly accelerating Kerr-Newman-anti-de Sitter black holes using the method of isomonodromic deformations.
Julián Barragán Amado, Bogeun Gwak
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We investigate the dynamics of a relativistic scalar field in a static spherically symmetric Einstein-Maxwell-Bumblebee black hole spacetime in (3+1) dimensions, incorporating non-minimal Maxwell-Bumblebee coupling. The covariant Klein-Gordon equation is
David Senjaya
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The domain of convergence of a Heun function obtained through the Poincar\'{e}--Perron (P--P) theorem is not absolute convergence but conditional one [2].
Choun, Yoon-Seok
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