Small Spins of Primordial Black Holes from Random Geometries: Bekenstein-Hawking Entropy and Gravitational Wave Observations
Autor: | Bianchi, Eugenio, Gupta, Anuradha, Haggard, Hal M., Sathyaprakash, B. S. |
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Rok vydání: | 2018 |
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Druh dokumentu: | Working Paper |
Popis: | Black hole entropy is a robust prediction of quantum gravity with no established phenomenological consequences to date. We use the Bekenstein-Hawking entropy formula and general-relativistic statistical mechanics to determine the probability distribution of random geometries uniformly sampled in phase space. We show that this statistics (in the limit $\hbar\to 0$) is relevant to large curvature perturbations, resulting in a population of primordial black holes with zero natal spin. In principle, the identification of such a population at LIGO, Virgo, and future gravitational wave observatories could provide the first observational evidence for the statistical nature of black hole entropy. Comment: 9 pages, 3 figures; v2: New section on general-relativistic statistical mechanics |
Databáze: | arXiv |
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