Relativistic models of magnetars: Nonperturbative analytical approach
General Relativity and Quantum Cosmology
2013-05-30 v1 High Energy Astrophysical Phenomena
Abstract
In the present paper we focus on building simple nonperturbative analytical relativistic models of magnetars. With this purpose in mind we first develop a method for generating exact interior solutions to the static and axisymmetric Einstein-Maxwell-hydrodynamic equations with anisotropic perfect fluid and with pure poloidal magnetic field. Then using an explicit exact solution we present a simple magnetar model and calculate some physically interesting quantities as the surface elipticity and the total energy of the magnetized star.
Cite
@article{arxiv.1111.3536,
title = {Relativistic models of magnetars: Nonperturbative analytical approach},
author = {Stoytcho Yazadjiev},
journal= {arXiv preprint arXiv:1111.3536},
year = {2013}
}
Comments
10 pages, LaTex