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Gas Heating from Spinning and Non-Spinning Evaporating Primordial Black Holes
Primordial black holes (PBHs) from the early Universe constitute a viable dark matter (DM) candidate and can span many orders of magnitude in mass. Light PBHs with masses around 10<sup loc="post">15</sup> g contribute to DM and will efficiently evaporate through Hawking radiati...
| Autores principales: | , , |
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| Lenguaje: | eng |
| Publicado: |
2020
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1016/j.physletb.2021.136459 http://cds.cern.ch/record/2734055 |