Primordial black holes from no-scale supergravity [electronic resource]
Saved in:
Online Access: |
Full Text (via OSTI) |
---|---|
Corporate Author: | |
Format: | Government Document Electronic eBook |
Language: | English |
Published: |
Washington, D.C. : Oak Ridge, Tenn. :
United States. Department of Energy. Office of Science ; Distributed by the Office of Scientific and Technical Information, U.S. Department of Energy,
2020.
|
Subjects: |
Abstract: | We calculate the primordial black hole abundance in the context of a Wess-Zumino type no-scale supergravity model. We modify the Kh̃ler 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 n<sub>s</sub> , 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. |
---|---|
Item Description: | Published through Scitech Connect. 10/01/2020. "Journal ID: ISSN 2470-0010." "PRVDAQ." Nanopoulos, Dimitri V. ; Spanos, Vassilis C. ; Stamou, Ioanna D. ; Texas A & M Univ., College Station, TX (United States) Alexander S. Onassis Public Benefit Foundation. Hellenic Foundation for Research and Innovation. |
Physical Description: | Size: Article No. 083536 : digital, PDF file. |