Extended primordial black hole mass functions with a spike

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dc.contributor.authorMagana, J.
dc.contributor.authorSan Martin, M.
dc.contributor.authorSureda, J.
dc.contributor.authorRubio, M.
dc.contributor.authorAraya, I.
dc.contributor.authorPadilla, N.
dc.date.accessioned2025-01-20T20:07:19Z
dc.date.available2025-01-20T20:07:19Z
dc.date.issued2023
dc.description.abstractWe 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 similar to 1000 M-circle dot 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.
dc.fuente.origenWOS
dc.identifier.doi10.1093/mnras/stad261
dc.identifier.eissn1365-2966
dc.identifier.issn0035-8711
dc.identifier.urihttps://doi.org/10.1093/mnras/stad261
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/91789
dc.identifier.wosidWOS:001043810000035
dc.issue.numero3
dc.language.isoen
dc.pagina.final4288
dc.pagina.inicio4276
dc.revistaMonthly notices of the royal astronomical society
dc.rightsacceso restringido
dc.subjecttheory
dc.subjectdark matter
dc.titleExtended primordial black hole mass functions with a spike
dc.typeartículo
dc.volumen520
sipa.indexWOS
sipa.trazabilidadWOS;2025-01-12
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