Abstract
We provide a (simplified) quantum description of primordial black holes at the time of their formation. Specifically, we employ the horizon quantum mechanics to compute the probability of black hole formation starting from a simple quantum mechanical characterization of primordial density fluctuations given by a Planckian spectrum. We then estimate the initial number of primordial black holes in the early universe as a function of their typical mass, spatial width and temperature of the fluctuation.
Dokumententyp: | Zeitschriftenartikel |
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Fakultät: | Physik |
Themengebiete: | 500 Naturwissenschaften und Mathematik > 530 Physik |
ISSN: | 0001-7701 |
Sprache: | Englisch |
Dokumenten ID: | 82714 |
Datum der Veröffentlichung auf Open Access LMU: | 15. Dez. 2021, 15:02 |
Letzte Änderungen: | 15. Dez. 2021, 15:02 |