Constraining inflationary potentials with inflaton PBHs Article Swipe
Luis E. Padilla
,
Juan Carlos Hidalgo
,
Gabriel Germán
·
YOU?
·
· 2023
· Open Access
·
· DOI: https://doi.org/10.48550/arxiv.2303.16428
YOU?
·
· 2023
· Open Access
·
· DOI: https://doi.org/10.48550/arxiv.2303.16428
If, after primordial inflation, the universe undergoes a relatively long reheating period, it could present a phase of matter domination supported by the oscillating inflaton field. During this epoch, small perturbations from the inflaton that reenter the cosmological horizon could virialize to form \textit{inflaton} structures. If the primordial overdensities are large enough, their associated inflaton structures could collapse to form primordial black holes (PBHs) [L.E.Padilla, J.C.Hidalgo and K.A.Malik, Phys.Rev.D, vol.106, p.023519, Jul 2022; hereinafter P1]. For this to happen at a considerable rate, the primordial power spectrum should be enhanced at small scales, a feature typically induced in single-field inflation through an ultra-slow roll phase (produced by a nearly-inflection point in the inflationary potential). In this article we consider two specific inflationary potentials that present this nearly-inflection point and we look at the PBH formation rate through the mechanism proposed in P1. We report on constraints to these two specific models from the bounds to PBH abundances. This serves as an illustration of the usefulness of the PBH formation mechanism proposed in P1.
Related Topics
Concepts
Inflaton
Physics
Primordial black hole
Inflation (cosmology)
Inflection point
Horizon
Inflationary epoch
Particle physics
Field (mathematics)
Astrophysics
Theoretical physics
Cosmology
Metric expansion of space
Astronomy
Gravitational wave
Geometry
Dark energy
Binary black hole
Mathematics
Pure mathematics
Metadata
- Type
- preprint
- Language
- en
- Landing Page
- http://arxiv.org/abs/2303.16428
- https://arxiv.org/pdf/2303.16428
- OA Status
- green
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4361806626
All OpenAlex metadata
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- DOI
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https://doi.org/10.48550/arxiv.2303.16428Digital Object Identifier
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Constraining inflationary potentials with inflaton PBHsWork title
- Type
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preprintOpenAlex work type
- Language
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enPrimary language
- Publication year
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2023Year of publication
- Publication date
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2023-03-29Full publication date if available
- Authors
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Luis E. Padilla, Juan Carlos Hidalgo, Gabriel GermánList of authors in order
- Landing page
-
https://arxiv.org/abs/2303.16428Publisher landing page
- PDF URL
-
https://arxiv.org/pdf/2303.16428Direct link to full text PDF
- Open access
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YesWhether a free full text is available
- OA status
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greenOpen access status per OpenAlex
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https://arxiv.org/pdf/2303.16428Direct OA link when available
- Concepts
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Inflaton, Physics, Primordial black hole, Inflation (cosmology), Inflection point, Horizon, Inflationary epoch, Particle physics, Field (mathematics), Astrophysics, Theoretical physics, Cosmology, Metric expansion of space, Astronomy, Gravitational wave, Geometry, Dark energy, Binary black hole, Mathematics, Pure mathematicsTop concepts (fields/topics) attached by OpenAlex
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0Total citation count in OpenAlex
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10Other works algorithmically related by OpenAlex
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| abstract_inverted_index.consider | 118 |
| abstract_inverted_index.enhanced | 89 |
| abstract_inverted_index.inflaton | 24, 33, 54 |
| abstract_inverted_index.proposed | 139, 170 |
| abstract_inverted_index.specific | 120, 149 |
| abstract_inverted_index.spectrum | 86 |
| abstract_inverted_index.universe | 5 |
| abstract_inverted_index.vol.106, | 69 |
| abstract_inverted_index.(produced | 105 |
| abstract_inverted_index.formation | 134, 168 |
| abstract_inverted_index.inflation | 99 |
| abstract_inverted_index.mechanism | 138, 169 |
| abstract_inverted_index.p.023519, | 70 |
| abstract_inverted_index.reheating | 10 |
| abstract_inverted_index.supported | 20 |
| abstract_inverted_index.typically | 95 |
| abstract_inverted_index.undergoes | 6 |
| abstract_inverted_index.virialize | 40 |
| abstract_inverted_index.K.A.Malik, | 67 |
| abstract_inverted_index.associated | 53 |
| abstract_inverted_index.domination | 19 |
| abstract_inverted_index.inflation, | 3 |
| abstract_inverted_index.potentials | 122 |
| abstract_inverted_index.primordial | 2, 47, 60, 84 |
| abstract_inverted_index.relatively | 8 |
| abstract_inverted_index.structures | 55 |
| abstract_inverted_index.ultra-slow | 102 |
| abstract_inverted_index.usefulness | 164 |
| abstract_inverted_index.J.C.Hidalgo | 65 |
| abstract_inverted_index.Phys.Rev.D, | 68 |
| abstract_inverted_index.abundances. | 156 |
| abstract_inverted_index.constraints | 145 |
| abstract_inverted_index.hereinafter | 73 |
| abstract_inverted_index.oscillating | 23 |
| abstract_inverted_index.potential). | 113 |
| abstract_inverted_index.structures. | 44 |
| abstract_inverted_index.considerable | 81 |
| abstract_inverted_index.cosmological | 37 |
| abstract_inverted_index.illustration | 161 |
| abstract_inverted_index.inflationary | 112, 121 |
| abstract_inverted_index.single-field | 98 |
| abstract_inverted_index.[L.E.Padilla, | 64 |
| abstract_inverted_index.overdensities | 48 |
| abstract_inverted_index.perturbations | 30 |
| abstract_inverted_index.\textit{inflaton} | 43 |
| abstract_inverted_index.nearly-inflection | 108, 126 |
| cited_by_percentile_year | |
| countries_distinct_count | 0 |
| institutions_distinct_count | 3 |
| citation_normalized_percentile |