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This paper presents an exact analytical solution for a relativistic finite-difference equation within a specific quantum mechanical potential, deriving discrete energy spectra and wavefunctions using advanced polynomial methods and SU(1,1) symmetry. The work contributes to fundamental theoretical physics by establishing the correct nonrelativistic limits and providing an algebraic approach to solving complex radial equations. While mathematically rigorous, the research remains highly specialized for theoretical physicists rather than offering immediate applications for broader technology sectors.
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Bound State Solutions of the Relativistic Finite-difference Equation for the Ring-shaped Quesne Oscillator Potential

arXiv2 min read

arXiv:2606.12082v1 Announce Type: new Abstract: We solve exactly the relativistic finite-difference equation for the quantum three-dimensional ring-shaped Quesne oscillator potential. Our investigation is based on a finite-difference version of relativistic quantum mechanics. So-called relativistic configurational r-space is a key concept here. We show that the radial wavefunctions and angular wavefunctions are expressed through the continuous dual Hahn polynomials and Jacobi polynomials, respectively. A discrete energy spectrum has been found. The radial wave functions and energy spectrum have the correct nonrelativistic limit. We also build a dynamical symmetry group SU (1, 1) for the radial part of the equation of motion, which allows us to find the energy spectrum purely algebraically.

Abstract:We solve exactly the relativistic finite-difference equation for the quantum three-dimensional ring-shaped Quesne oscillator potential. Our investigation is based on a finite-difference version of relativistic quantum mechanics. So-called relativistic configurational r-space is a key concept here. We show that the radial wavefunctions and angular wavefunctions are expressed through the continuous dual Hahn polynomials and Jacobi polynomials, respectively. A discrete energy spectrum has been found. The radial wave functions and energy spectrum have the correct nonrelativistic limit. We also build a dynamical symmetry group SU (1, 1) for the radial part of the equation of motion, which allows us to find the energy spectrum purely algebraically.

arXiv:2606.12082 [quant-ph]

(or arXiv:2606.12082v1 [quant-ph] for this version)

https://doi.org/10.48550/arXiv.2606.12082 Focus to learn more arXiv-issued DOI via DataCite (pending registration)

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Full text under the publisher's open licence · 196 words

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