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arXiv · 2101.09874

Transport properties in magnetized compact stars

Toshitaka Tatsumi·Hiroaki Abuki
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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.

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Toshitaka Tatsumi, Hiroaki Abuki. 2021-01-25. Transport properties in magnetized compact stars. https://arxiv.org/abs/2101.09874

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