Upper limits on the temperature of inspiraling astrophysical black holes
Abstract We present a method to constrain the temperature of astrophysical black holes through detecting the inspiral phase of binary black hole coalescences. At sufficient separation, inspiraling black holes can be regarded as isolated objects, hence their temperature can still be defined. Due to t...
Main Authors: | , |
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Format: | Article |
Language: | English |
Published: |
SpringerOpen
2021-07-01
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Series: | European Physical Journal C: Particles and Fields |
Online Access: | https://doi.org/10.1140/epjc/s10052-021-09391-3 |