Transport properties in magnetized compact stars
High Energy Physics - Phenomenology
2021-01-26 v1 High Energy Astrophysical Phenomena
Abstract
Transport properties of dense quark matter are discussed in the strong magnetic field, B. B dependence as well as density dependence of the Hall conductivity is discussed in the inhomogeneous chiral phase. Anomalous Hall effect is intrinsic to the inhomogeneous chiral phase and resembles the one in Weyl semimetals in condensed matter physics. Some theoretical aspects inherent in anomalous Hall effect are revealed.
Cite
@article{arxiv.2101.09874,
title = {Transport properties in magnetized compact stars},
author = {Toshitaka Tatsumi and Hiroaki Abuki},
journal= {arXiv preprint arXiv:2101.09874},
year = {2021}
}
Comments
11 pages, 4 figures, Submitted to "Particles"