Approximate Metric for a Rotating Deformed Mass
Cosmology and Nongalactic Astrophysics
2015-09-15 v3 General Relativity and Quantum Cosmology
Abstract
A new Kerr-like metric with quadrupole moment is obtained by means of perturbing the Kerr spacetime. The form of this new metric is simple as the Kerr metric. By comparison with the exterior Hartle-Thorne metric, it is shown that it could be matched to an interior solution. This approximate metric may represent the spacetime of a real astrophysical object with any Kerr rotation parameter a and slightly deformed.
Cite
@article{arxiv.1405.1776,
title = {Approximate Metric for a Rotating Deformed Mass},
author = {Francisco Frutos-Alfaro and Paulo Montero-Camacho and Miguel Araya-Arguedas and Javier Bonatti-Gonzalez},
journal= {arXiv preprint arXiv:1405.1776},
year = {2015}
}
Comments
arXiv admin note: substantial text overlap with arXiv:1401.0866