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Effects of the shape of curvature peaks on the size of primordial black holes
We simulate numerically the formation of spherically symmetric primordial black holes (PBHs) seeded by different families of primordial curvature perturbations profiles in a radiation dominated Friedman-Robertson-Walker (FRW) Universe. We have studied the dependency on the curvature profile of the i...
Autores principales: | Escrivà, Albert, Romano, Antonio Enea |
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Lenguaje: | eng |
Publicado: |
2021
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1088/1475-7516/2021/05/066 http://cds.cern.ch/record/2759852 |
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