Scalar waves in a Topological Star spacetime: self-force and radiative losses
General Relativity and Quantum Cosmology
2024-12-02 v1
Abstract
We study the radiated energy by a scalar particle moving on a circular orbit (smeared in the extra dimension) in the spacetime of a topological star, extending a previous study [Phys. Rev. D {\bf 110}, 084077 (2024)]. We discuss motion in the presence of self-force effects too.
Cite
@article{arxiv.2411.19612,
title = {Scalar waves in a Topological Star spacetime: self-force and radiative losses},
author = {Massimo Bianchi and Donato Bini and Giorgio Di Russo},
journal= {arXiv preprint arXiv:2411.19612},
year = {2024}
}
Comments
17 pages, 5 figures, revtex macros