A self-consistent study of magnetic field effects on hybrid stars
High Energy Astrophysical Phenomena
2017-06-28 v1 Solar and Stellar Astrophysics
Nuclear Theory
Abstract
It is understood that strong magnetic fields affect the structure of neutron stars. Nevertheless, many calculations for magnetized neutron stars are still being performed using symmetric solutions of Einstein's equations. In this conference proceeding, we review why this is not the correct procedure and we also discuss the effects of magnetic fields on the stellar population and temperature profiles.
Keywords
Cite
@article{arxiv.1702.00386,
title = {A self-consistent study of magnetic field effects on hybrid stars},
author = {V. Dexheimer and B. Franzon and S. Schramm},
journal= {arXiv preprint arXiv:1702.00386},
year = {2017}
}
Comments
Prepared for Conference "Compact Stars in the QCD phase diagram V" 23-27 May 2016 GSSI and LNGS (L'Aquila, Italy)