Anomalous Electromagnetic Transport in Compact Stars

Anomalous Electromagnetic Transport in Compact Stars
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DOI:
10.3390/universe4030054
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发表时间:
2018-03
期刊:
影响因子:
2.9
通讯作者:
E. J. Ferrer;V. Incera
E. J. Ferrer;V. Incera
中科院分区:
物理与天体物理3区
文献类型:
--
作者:
E. J. Ferrer;V. Incera

文献摘要

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We study the anomalous electromagnetic transport properties of a quark-matter phase that can be realized in the presence of a magnetic field in the low-temperature/moderate-high-density region of the Quantum Chromodynamics (QCD) phase map. In this so-called Magnetic Dual Chiral Density Wave phase, an inhomogeneous condensate is dynamically induced producing a nontrivial topology, a consequence of the asymmetry of the lowest Landau level modes of the quasiparticles in this phase. The nontrivial topology manifests in the electromagnetic effective action via a chiral anomaly term θ F μ ν F ˜ μ ν , with an axion field θ given by the phase of the Dual Chiral Density Wave condensate. The coupling of the axion with the electromagnetic field leads to several macroscopic effects that include, among others, an anomalous, nondissipative Hall current, an anomalous electric charge, magnetoelectricity, and the formation of a hybridized propagating mode known as an axion polariton. The possible existence of this phase in the inner core of neutron stars opens a window to search for signals of its anomalous transport properties.