Transport Properties in Magnetized Compact Stars

Transport properties of dense quark matter are discussed in the strong magnetic field, <i>B</i>. <i>B</i> dependence as well as density dependence of the Hall conductivity is discussed, based on the microscopic Kubo formula. We took into account the possibility of the inhomog...

Full description

Bibliographic Details
Main Authors: Toshitaka Tatsumi, Hiroaki Abuki
Format: Article
Language:English
Published: MDPI AG 2021-02-01
Series:Particles
Subjects:
Online Access:https://www.mdpi.com/2571-712X/4/1/9
Description
Summary:Transport properties of dense quark matter are discussed in the strong magnetic field, <i>B</i>. <i>B</i> dependence as well as density dependence of the Hall conductivity is discussed, based on the microscopic Kubo formula. We took into account the possibility of the inhomogeneous chiral phase at moderate densities, where anomalous Hall effect is intrinsic and resembles the one in Weyl semimetals in condensed matter physics. Some theoretical aspects inherent in anomalous Hall effect are also discussed.
ISSN:2571-712X