Axion configurations around pulsars
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Publication:5023077
DOI10.1088/1475-7516/2018/07/044OpenAlexW3105437629WikidataQ129508880 ScholiaQ129508880MaRDI QIDQ5023077
Jamie I. McDonald, Björn Garbrecht
Publication date: 20 January 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1804.04224
Related Items (4)
Axion superradiance in rotating neutron stars ⋮ On long range axion hairs for black holes ⋮ Diluted axion star collisions with neutron stars ⋮ Superradiance in stars: non-equilibrium approach to damping of fields in stellar media
Cites Work
- Decay of massive scalar field in a Schwarzschild background
- Axions and ``light shining through a wall: A detailed theoretical analysis
- Probing axions with neutron star inspirals and other stellar processes
- Spectral decomposition of the perturbation response of the Schwarzschild geometry
- Quasinormal modes of Schwarzschild black holes: Defined and calculated via Laplace transformation
- Black holes as particle detectors: evolution of superradiant instabilities
- The bosenova and axiverse
- Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
- Bosenova Collapse of Axion Cloud around a Rotating Black Hole
- Exact Space-Times in Einstein's General Relativity
- Dynamical boson stars
- Quasi-normal modes of stars and black holes
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