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Artículo

Extended primordial black hole mass functions with a spike

Magaña, J; San Martín, M.; Sureda, J; Rubio, M; Araya, I; Padilla, Nelson DavidIcon
Fecha de publicación: 04/2023
Editorial: Oxford University Press
Revista: Monthly Notices of the Royal Astronomical Society
ISSN: 0035-8711
Idioma: Inglés
Tipo de recurso: Artículo publicado
Clasificación temática:
Astronomía

Resumen

We introduce a modification of the Press–Schechter formalism aimed to derive general mass functions for primordial black holes (PBHs). In this case, we start from primordial power spectra (PPS) which include a monochromatic spike, typical of ultra slow-roll inflation models. We consider the PBH formation as being associated to the amplitude of the spike on top of the linear energy density fluctuations coming from a PPS with a blue index. By modelling the spike with a lognormal function, we study the properties of the resulting mass function spikes, and compare these to the underlying extended mass distributions. When the spike is at PBH masses, which are much lower than the exponential cut-off of the extended distribution, very little mass density is held by the PBHs within the spike, and it is not ideal to apply the Press–Schechter formalism in this case as the resulting characteristic overdensity is too different from the threshold for collapse. It is more appropriate to do so when the spike mass is similar to, or larger than the cut-off mass. Additionally, it can hold a similar mass density as the extended part. Such particular mass functions also contain large numbers of small PBHs, especially if stable PBH relics are considered, and they can provide ∼1000 M☉ seeds for the supermassive black holes at the centres of present-day galaxies. The constraints on the fraction of dark matter in PBHs for monochromatic mass functions are somewhat relaxed when there is an additional underlying extended distribution of masses.
Palabras clave: DARK MATTER , THEORY , COSMOLOGY
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info:eu-repo/semantics/restrictedAccess Excepto donde se diga explícitamente, este item se publica bajo la siguiente descripción: Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Unported (CC BY-NC-SA 2.5)
Identificadores
URI: http://hdl.handle.net/11336/226163
URL: https://academic.oup.com/mnras/article/520/3/4276/7008907
DOI: http://dx.doi.org/10.1093/mnras/stad261
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Articulos de INST.DE ASTRONOMIA TEORICA Y EXPERIMENTAL
Citación
Magaña, J; San Martín, M.; Sureda, J; Rubio, M; Araya, I; et al.; Extended primordial black hole mass functions with a spike; Oxford University Press; Monthly Notices of the Royal Astronomical Society; 520; 3; 4-2023; 4276-4288
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