Superradiance in stars: non-equilibrium approach to damping of fields in stellar media
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Publication:5878840
DOI10.1088/1475-7516/2022/12/008OpenAlexW4310727176MaRDI QIDQ5878840
Björn Garbrecht, Jamie I. McDonald, Francesca Chadha-Day
Publication date: 23 February 2023
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2207.07662
Cites Work
- (Re-)inventing the relativistic wheel: gravity, cosets, and spinning objects
- A modern approach to superradiance
- Transport equations for chiral fermions to order \(\hbar\) and electroweak baryogenesis. I
- Transport equations for chiral fermions to order \(\hbar\) and electroweak baryogenesis. II
- Oscillating scalar dissipating in a medium
- Consequences of the order of the limit of infinite spacetime volume and the sum over topological sectors for \textit{CP} violation in the strong interactions
- Effective action for cosmological scalar fields at finite temperature
- Gravitational radiation from an axion cloud around a black hole: Superradiant phase
- Brownian Motion of a Quantum Oscillator
- Effective action for composite operators
- Bosenova Collapse of Axion Cloud around a Rotating Black Hole
- Axion configurations around pulsars
- Axion-photon conversion in strongly magnetised plasmas
- Axion superradiance in rotating neutron stars
- Superradiance initiated inside the ergoregion
- Nonequilibrium Quantum Field Theory
- The quark-gluon plasma: Collective dynamics and hard thermal loops
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