Axion superradiance in rotating neutron stars

DOI10.1088/1475-7516/2019/10/051OpenAlexW3101864461MaRDI QIDQ5067142

Jamie I. McDonald, Francesca V. Day

Publication date: 1 April 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1904.08341

zbMATH Keywords

pulsar magnetospheredark matter theoryaxions

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (2)

Exploring axions through the photon ring of a spherically symmetric black hole ⋮ Superradiance in stars: non-equilibrium approach to damping of fields in stellar media

Cites Work

• ADVANCED METHODS IN BLACK-HOLE PERTURBATION THEORY
• Black holes as particle detectors: evolution of superradiant instabilities
• A new Weber-type transform
• Axion configurations around pulsars
• On long range axion hairs for black holes
• Induction Effects in Terrestrial Magnetism Part II. The Secular Variation
• Quasi-normal modes of stars and black holes

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