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Constraining primordial black hole masses with the isotropic gamma ray background
Primordial black holes (PBHs) can represent all or most of the dark matter in the window 1017–1022 g. Here we present an extension of the constraints on PBHs of masses 1013–1018 g arising from the isotropic diffuse gamma-ray background. Primordial black holes evaporate by emitting Hawking radiatio...
| Autores principales: | , , |
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| Lenguaje: | eng |
| Publicado: |
2019
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| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1103/PhysRevD.101.023010 http://cds.cern.ch/record/2678422 |