Scalar waves in a Topological Star spacetime: self-force and radiative losses
arXiv:2411.19612
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.
17 pages, 5 figures, revtex macros