Primordial black holes from no-scale supergravity
Abstract
We calculate the primordial black hole abundance in the context of a Wess-Zumino type no-scale supergravity model. We modify the Kähler potential, by adding an extra exponential term. Using just one parameter in the context of this model, we are able to satisfy the Planck cosmological constraints for the spectral index ns , the tensor-to-scalar ratio r, and to produce up to ~ 20 % of the dark matter of the Universe in the form of primordial black holes.
- Authors:
-
- Texas A & M Univ., College Station, TX (United States); Houston Advanced Research Center (HARC), Woodlands, TX (United States); Academy of Athens (Greece)
- National and Kapodistrian University of Athens (Greece)
- Publication Date:
- Research Org.:
- Texas A & M Univ., College Station, TX (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC); Alexander S. Onassis Public Benefit Foundation; Hellenic Foundation for Research and Innovation
- OSTI Identifier:
- 1851446
- Grant/Contract Number:
- SC0010813; FG02-13ER42020
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review. D.
- Additional Journal Information:
- Journal Volume: 102; 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
Nanopoulos, Dimitri V., Spanos, Vassilis C., and Stamou, Ioanna D. Primordial black holes from no-scale supergravity. United States: N. p., 2020.
Web. doi:10.1103/physrevd.102.083536.
Nanopoulos, Dimitri V., Spanos, Vassilis C., & Stamou, Ioanna D. Primordial black holes from no-scale supergravity. United States. https://doi.org/10.1103/physrevd.102.083536
Nanopoulos, Dimitri V., Spanos, Vassilis C., and Stamou, Ioanna D. Thu .
"Primordial black holes from no-scale supergravity". United States. https://doi.org/10.1103/physrevd.102.083536. https://www.osti.gov/servlets/purl/1851446.
@article{osti_1851446,
title = {Primordial black holes from no-scale supergravity},
author = {Nanopoulos, Dimitri V. and Spanos, Vassilis C. and Stamou, Ioanna D.},
abstractNote = {We calculate the primordial black hole abundance in the context of a Wess-Zumino type no-scale supergravity model. We modify the Kähler potential, by adding an extra exponential term. Using just one parameter in the context of this model, we are able to satisfy the Planck cosmological constraints for the spectral index ns , the tensor-to-scalar ratio r, and to produce up to ~ 20 % of the dark matter of the Universe in the form of primordial black holes.},
doi = {10.1103/physrevd.102.083536},
journal = {Physical Review. D.},
number = 8,
volume = 102,
place = {United States},
year = {Thu Oct 01 00:00:00 EDT 2020},
month = {Thu Oct 01 00:00:00 EDT 2020}
}
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