Primordial black holes as dark matter in supergravity inflation models
Abstract
We present here a novel scenario to produce abundant primordial black holes (PBHs) in new inflation which is a second phase of a double inflation in the supergravity framework. In our model, some preinflation phase before the new inflation is assumed and it would be responsible for the primordial curvature perturbations on the cosmic microwave background scale, while the new inflation produces only the small scale perturbations. Our new inflation model has linear, quadratic, and cubic terms in its potential and PBH production corresponds with its flat inflection point. The linear term could be interpreted to come from a supersymmetry-breaking sector, and with this assumption, the vanishing cosmological constant condition after inflation and the flatness condition for the inflection point can be consistently satisfied.
- Authors:
-
- Univ. of Tokyo (Japan). Inst. for Cosmic Ray Research; Univ. of Tokyo (Japan). Kavli Institute for the Physics and Mathematics of the Universe (WPI)
- Univ. of California, Los Angeles, CA (United States). Dept. of Physics and Astronomy; Univ. of Tokyo (Japan). Kavli Institute for the Physics and Mathematics of the Universe (WPI)
- Univ. of Tokyo (Japan). Kavli Institute for the Physics and Mathematics of the Universe (WPI)
- Publication Date:
- Research Org.:
- Univ. of California, Los Angeles, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- OSTI Identifier:
- 1609077
- Alternate Identifier(s):
- OSTI ID: 1330127
- Grant/Contract Number:
- SC0009937
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review D
- Additional Journal Information:
- Journal Volume: 94; Journal Issue: 8; Journal ID: ISSN 2470-0010
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS
Citation Formats
Kawasaki, Masahiro, Kusenko, Alexander, Tada, Yuichiro, and Yanagida, Tsutomu T. Primordial black holes as dark matter in supergravity inflation models. United States: N. p., 2016.
Web. doi:10.1103/PhysRevD.94.083523.
Kawasaki, Masahiro, Kusenko, Alexander, Tada, Yuichiro, & Yanagida, Tsutomu T. Primordial black holes as dark matter in supergravity inflation models. United States. https://doi.org/10.1103/PhysRevD.94.083523
Kawasaki, Masahiro, Kusenko, Alexander, Tada, Yuichiro, and Yanagida, Tsutomu T. Wed .
"Primordial black holes as dark matter in supergravity inflation models". United States. https://doi.org/10.1103/PhysRevD.94.083523. https://www.osti.gov/servlets/purl/1609077.
@article{osti_1609077,
title = {Primordial black holes as dark matter in supergravity inflation models},
author = {Kawasaki, Masahiro and Kusenko, Alexander and Tada, Yuichiro and Yanagida, Tsutomu T.},
abstractNote = {We present here a novel scenario to produce abundant primordial black holes (PBHs) in new inflation which is a second phase of a double inflation in the supergravity framework. In our model, some preinflation phase before the new inflation is assumed and it would be responsible for the primordial curvature perturbations on the cosmic microwave background scale, while the new inflation produces only the small scale perturbations. Our new inflation model has linear, quadratic, and cubic terms in its potential and PBH production corresponds with its flat inflection point. The linear term could be interpreted to come from a supersymmetry-breaking sector, and with this assumption, the vanishing cosmological constant condition after inflation and the flatness condition for the inflection point can be consistently satisfied.},
doi = {10.1103/PhysRevD.94.083523},
journal = {Physical Review D},
number = 8,
volume = 94,
place = {United States},
year = {Wed Oct 26 00:00:00 EDT 2016},
month = {Wed Oct 26 00:00:00 EDT 2016}
}
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