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Sound speed induced production of primordial black holes

We study different mechanisms by which the speed of primordial curvature perturbations can produce an enhancement of the curvature spectrum, which could lead to the production of primordial black holes (PBH). One possibility is the growth of the sound speed in single scalar field models, which can i...

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Autor principal: Romano, Antonio Enea
Lenguaje:eng
Publicado: 2020
Materias:
Acceso en línea:http://cds.cern.ch/record/2723433
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author Romano, Antonio Enea
author_facet Romano, Antonio Enea
author_sort Romano, Antonio Enea
collection CERN
description We study different mechanisms by which the speed of primordial curvature perturbations can produce an enhancement of the curvature spectrum, which could lead to the production of primordial black holes (PBH). One possibility is the growth of the sound speed in single scalar field models, which can induce super-horizon growth of curvature perturbations. The other is the momentum dependent effective sound (MESS) of curvature perturbations, which can arise in multi-fields models or modified gravity theories. Future gravitational waves observatories such as LISA will allow to set constraints of the space and time dependency of the sound speed, and on the different theoretical scenarios from which it can originate.
id cern-2723433
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2020
record_format invenio
spelling cern-27234332020-07-16T03:29:32Zhttp://cds.cern.ch/record/2723433engRomano, Antonio EneaSound speed induced production of primordial black holesastro-ph.COAstrophysics and AstronomyWe study different mechanisms by which the speed of primordial curvature perturbations can produce an enhancement of the curvature spectrum, which could lead to the production of primordial black holes (PBH). One possibility is the growth of the sound speed in single scalar field models, which can induce super-horizon growth of curvature perturbations. The other is the momentum dependent effective sound (MESS) of curvature perturbations, which can arise in multi-fields models or modified gravity theories. Future gravitational waves observatories such as LISA will allow to set constraints of the space and time dependency of the sound speed, and on the different theoretical scenarios from which it can originate.arXiv:2006.07321oai:cds.cern.ch:27234332020-06-12
spellingShingle astro-ph.CO
Astrophysics and Astronomy
Romano, Antonio Enea
Sound speed induced production of primordial black holes
title Sound speed induced production of primordial black holes
title_full Sound speed induced production of primordial black holes
title_fullStr Sound speed induced production of primordial black holes
title_full_unstemmed Sound speed induced production of primordial black holes
title_short Sound speed induced production of primordial black holes
title_sort sound speed induced production of primordial black holes
topic astro-ph.CO
Astrophysics and Astronomy
url http://cds.cern.ch/record/2723433
work_keys_str_mv AT romanoantonioenea soundspeedinducedproductionofprimordialblackholes