Stability of the spacetime of a magnetized compact object
Abstract
We investigate the stability of scalar perturbations around a magnetized stationary compact object in General Relativity. The considered object is one of the simplest exact solutions of Einstein electrovacuum equations corresponding to a spheroidal body endowed with a dipole magnetic moment. It is effectively constructed by imposing a perfect reflection (mirror) boundary condition on a central region of the Gutsunaev-Manko spacetime. A time-domain analysis of the perturbations reveals a quasinormal phase followed by a power-law decaying tail. Our findings suggest that the exterior region of the magnetized compact object is stable in the entire parameter space. Moreover, the system tends to become generically more stable the stronger the magnetization of the central object is. Such findings can be useful for the qualitative understanding of more realistic astrophysical situations involving highly magnetized sources.
Keywords
Cite
@article{arxiv.2411.11117,
title = {Stability of the spacetime of a magnetized compact object},
author = {Eveling C. Ribeiro and L. Formigari and Marcos R. Ribeiro and Elcio Abdalla and Bertha Cuadros-Melgar and C. Molina and Amilcar R. de Queiroz and Alberto Saa},
journal= {arXiv preprint arXiv:2411.11117},
year = {2025}
}
Comments
10 pages, 5 figures. Minor corrections. Final version to appear in the PRD