Cosmological black holes are not described by the Thakurta metric: LIGO-Virgo bounds on PBHs remain unchanged
Abstract We show that the physical conditions which induce the Thakurta metric, recently studied by Bœhm et al. in the context of time-dependent black hole masses, correspond to a single accreting compact object in the entire Universe filled with isotropic non-interacting dust. In such a case, accre...
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Autores principales: | , , , , |
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Formato: | article |
Lenguaje: | EN |
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SpringerOpen
2021
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Materias: | |
Acceso en línea: | https://doaj.org/article/73b42544e89843baa2f51299a56ff776 |
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