2022
DOI: 10.1103/physrevd.106.023503
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Axion electrodynamics and magnetohydrodynamics

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Cited by 7 publications
(6 citation statements)
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“…In realistic astrophysical situations, Maxwell's equations should be dynamically combined with Einstein's equation with accompanying fluids and other fields. The complete sets of Einstein's equation with a fluid and a scalar field (with additional helical coupling with the EM fields) in the covariant, the ADM, and the FNLE formulations are presented in [9]. Maxwell's equations in the general curved spacetime derived in different forms in this work are applicable in all these situations.…”
Section: Discussionmentioning
confidence: 99%
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“…In realistic astrophysical situations, Maxwell's equations should be dynamically combined with Einstein's equation with accompanying fluids and other fields. The complete sets of Einstein's equation with a fluid and a scalar field (with additional helical coupling with the EM fields) in the covariant, the ADM, and the FNLE formulations are presented in [9]. Maxwell's equations in the general curved spacetime derived in different forms in this work are applicable in all these situations.…”
Section: Discussionmentioning
confidence: 99%
“…φ is a scalar field with f = φ for the conventional axion coupling [8]. A system together with Einstein's gravity, scalar field, and a general fluid is studied in [9].…”
Section: Covariant and Adm Formulationsmentioning
confidence: 99%
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“…This approximation is relevant in many astrophysical situations including cosmology; in observable universe, except for nearby compact objects like neutron stars and black holes, the gravity represented by a dimensionless metric parameter Φ/c 2 is extremely small with typical value less than 10 −5 [12]. The weak gravity limit of a general scalar field (including axion) in cosmology is presented in [13] in the context of electrodynamics and magnetohydrodynamics.…”
Section: Introductionmentioning
confidence: 99%