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...
Main Authors: | , |
---|---|
Format: | Article |
Language: | English |
Published: |
MDPI AG
2021-02-01
|
Series: | Particles |
Subjects: | |
Online Access: | https://www.mdpi.com/2571-712X/4/1/9 |
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 |