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Primordial Black Holes from Broad Spectra: Abundance and Clustering

A common mechanism to form primordial black holes in the early universe is by enhancing at small-scales the scalar perturbations generated during inflation. If these fluctuations have a large enough amplitude, they may collapse into primordial black holes upon horizon re-entry. Such primordial black...

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Detalles Bibliográficos
Autores principales:	Moradinezhad Dizgah, Azadeh, Franciolini, Gabriele, Riotto, Antonio
Lenguaje:	eng
Publicado:	2019
Materias:	hep-ph Particle Physics - Phenomenology gr-qc General Relativity and Cosmology astro-ph.CO Astrophysics and Astronomy
Acceso en línea:	https://dx.doi.org/10.1088/1475-7516/2019/11/001 http://cds.cern.ch/record/2681923

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