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Evolution of primordial black hole spin due to Hawking radiation
Near extremal Kerr black holes (BHs) are subject to the Thorne limit |$a\lt a^*_{\rm lim}=0.998$| in the case of thin disc accretion, or some generalized version of this in other disc geometries. However, any limit that differs from the thermodynamics limit a* < 1 can in principle be evaded in ot...
| Autores principales: | , , |
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| Lenguaje: | eng |
| Publicado: |
2019
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1093/mnras/staa765 http://cds.cern.ch/record/2678273 |