Bound-unbound universality and the all-order semi-classical wave function in Schwarzschild

A bstract We present a systematic method for analytically computing time-dependent observables for a relativistic probe particle in Coulomb and Schwarzschild backgrounds. The method generates expressions valid both in the bound and unbound regimes, namely bound-unbound universal expressions. To demonstrate our method we compute the time-dependent radius and azimuthal angle for relativistic motion in a Coulomb background (relativistic Keplerian motion), as well as the electromagnetic field radiated by a relativistic Keplerian source. All of our calculations exhibit bound-unbound universality. Finally, we present an exact expression for the semi-classical wave function in Schwarzschild. The latter is crucial in applying our method to any time-dependent observable for probe-limit motion in Schwarzschild, to any desired order in velocity and the gravitational constant G .

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Publication Details

Journal
Journal of High Energy Physics
Published
2025-10-08
DOI
https://doi.org/10.1007/jhep10(2025)063
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
0.00

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article

Bound-unbound universality and the all-order semi-classical wave function in Schwarzschild

Ofri Telem, Chia-Hsien Shen, Majed Khalaf
Journal of High Energy Physics
Pulsars and Gravitational Waves Research
article

Bound-unbound universality and the all-order semi-classical wave function in Schwarzschild

Ofri Telem, Chia-Hsien Shen, Majed Khalaf
article en

Abstract

A bstract We present a systematic method for analytically computing time-dependent observables for a relativistic probe particle in Coulomb and Schwarzschild backgrounds. The method generates expressions valid both in the bound and unbound regimes, namely bound-unbound universal expressions. To demonstrate our method we compute the time-dependent radius and azimuthal angle for relativistic motion in a Coulomb background (relativistic Keplerian motion), as well as the electromagnetic field radiated by a relativistic Keplerian source. All of our calculations exhibit bound-unbound universality. Finally, we present an exact expression for the semi-classical wave function in Schwarzschild. The latter is crucial in applying our method to any time-dependent observable for probe-limit motion in Schwarzschild, to any desired order in velocity and the gravitational constant G .

Journal of High Energy PhysicsVol. 2025(10)
National Taiwan University (TW), Hebrew University of Jerusalem (IL), Cornell University (US), Laboratoire AstroParticule et Cosmologie (FR), National Center for Theoretical Sciences (TW), National Center for Theoretical Sciences, Physics Division
National Science Foundation, CERN, European Commission, Deutsche Forschungsgemeinschaft, Israel Science Foundation, Ministry of Education, India, Azrieli Foundation, National Science and Technology Council, HORIZON EUROPE Framework Programme
Openalex Percentile: Top 80%
Pulsars and Gravitational Waves Research
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