Anomalous Electromagnetic Transport in Compact Stars

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, a...

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Main Authors: Efrain J. Ferrer, Vivian de la Incera
Format: Article
Language:English
Published: MDPI AG 2018-03-01
Series:Universe
Subjects:
Online Access:http://www.mdpi.com/2218-1997/4/3/54
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spelling doaj-712e6d09b03c40eaac9f66f45d3b4d9c2020-11-24T22:57:03ZengMDPI AGUniverse2218-19972018-03-01435410.3390/universe4030054universe4030054Anomalous Electromagnetic Transport in Compact StarsEfrain J. Ferrer0Vivian de la Incera1Department of Engineering Science and Physics, CUNY-College of Staten Island and CUNY-Graduate Center, New York, NY 10314, USADepartment of Engineering Science and Physics, CUNY-College of Staten Island and CUNY-Graduate Center, New York, NY 10314, USAWe 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.http://www.mdpi.com/2218-1997/4/3/54chiral symmetryaxion QEDquark-hole pairingcold-dense QCDmagnetic DCDW
collection DOAJ
language English
format Article
sources DOAJ
author Efrain J. Ferrer
Vivian de la Incera
spellingShingle Efrain J. Ferrer
Vivian de la Incera
Anomalous Electromagnetic Transport in Compact Stars
Universe
chiral symmetry
axion QED
quark-hole pairing
cold-dense QCD
magnetic DCDW
author_facet Efrain J. Ferrer
Vivian de la Incera
author_sort Efrain J. Ferrer
title Anomalous Electromagnetic Transport in Compact Stars
title_short Anomalous Electromagnetic Transport in Compact Stars
title_full Anomalous Electromagnetic Transport in Compact Stars
title_fullStr Anomalous Electromagnetic Transport in Compact Stars
title_full_unstemmed Anomalous Electromagnetic Transport in Compact Stars
title_sort anomalous electromagnetic transport in compact stars
publisher MDPI AG
series Universe
issn 2218-1997
publishDate 2018-03-01
description 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.
topic chiral symmetry
axion QED
quark-hole pairing
cold-dense QCD
magnetic DCDW
url http://www.mdpi.com/2218-1997/4/3/54
work_keys_str_mv AT efrainjferrer anomalouselectromagnetictransportincompactstars
AT viviandelaincera anomalouselectromagnetictransportincompactstars
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