Primordial black holes from fifth forces
Primordial black holes can be produced by a long-range attractive fifth force stronger than gravity, mediated by a light scalar field interacting with nonrelativistic “heavy” particles. As soon as the energy fraction of heavy particles reaches a threshold, the fluctuations rapidly become nonlinear....
Gespeichert in:
| Hauptverfasser: | , , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
15 April 2018
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| In: |
Physical review
Year: 2018, Jahrgang: 97, Heft: 8 |
| ISSN: | 2470-0029 |
| DOI: | 10.1103/PhysRevD.97.081302 |
| Online-Zugang: | Verlag, Volltext: http://dx.doi.org/10.1103/PhysRevD.97.081302 Verlag, Volltext: https://link.aps.org/doi/10.1103/PhysRevD.97.081302 
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| Verfasserangaben: | Luca Amendola, Javier Rubio, and Christof Wetterich |
MARC
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| 520 | |a Primordial black holes can be produced by a long-range attractive fifth force stronger than gravity, mediated by a light scalar field interacting with nonrelativistic “heavy” particles. As soon as the energy fraction of heavy particles reaches a threshold, the fluctuations rapidly become nonlinear. The overdensities collapse into black holes or similar screened objects, without the need for any particular feature in the spectrum of primordial density fluctuations generated during inflation. We discuss whether such primordial black holes can constitute the total dark matter component in the Universe. | ||
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