Exotic Phases in Magnetars
Solar and Stellar Astrophysics
2015-04-03 v1 Nuclear Theory
Abstract
Neutron stars feature extremely high magnetic fields with deduced field strengths of G in the case of magnetars and potentially much higher values inside of the star. In this context we consider the appearance of meson condensation taking into account the effect of the magnetic field. The results show that, depending on parameters, such a condensation in magnetized neutron stars might (just) occur.
Cite
@article{arxiv.1504.00451,
title = {Exotic Phases in Magnetars},
author = {S. Schramm and A. Bhattacharyya and V. Dexheimer and R. Mallick},
journal= {arXiv preprint arXiv:1504.00451},
year = {2015}
}
Comments
Contribution to the Proceedings of CSQCD IV, Prerow (2014)