Abstract
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.
| Original language | English |
|---|---|
| Article number | 63 |
| Journal | Journal of High Energy Physics |
| Volume | 2025 |
| Issue number | 10 |
| DOIs | |
| State | Published - Oct 2025 |
Bibliographical note
Publisher Copyright:© The Author(s) 2025.
Keywords
- Black Holes
- Classical Theories of Gravity
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