Improved Model of Primordial Black Hole Formation after Starobinsky Inflation
Abstract
:1. Introduction
2. The New Model
3. Inflaton Potential and Slow-Roll
4. Power Spectrum of Scalar Perturbations and PBH Masses
5. Conclusions
Author Contributions
Funding
Data Availability Statement
Acknowledgments
Conflicts of Interest
1 | Accordingly, we changed the notation for the AB-parameter denoted by in Ref. [20] to . |
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r | , g | ||||||
---|---|---|---|---|---|---|---|
6.36 | 0.964959 | 0.0359 | 26 | 47 | 21 | ||
6.70 | 0.964905 | 0.0182 | 34 | 54 | 20 | ||
7.01 | 0.964944 | 0.0095 | 43 | 65 | 22 | ||
7.07 | 0.964917 | 0.0083 | 45 | 64 | 19 | ||
7.12 | 0.964925 | 0.0074 | 47 | 65 | 18 | ||
7.15 | 0.964908 | 0.0070 | 49 | 66 | 17 | ||
7.20 | 0.964961 | 0.0062 | 51 | 64 | 13 |
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Saburov, S.; Ketov, S.V. Improved Model of Primordial Black Hole Formation after Starobinsky Inflation. Universe 2023, 9, 323. https://doi.org/10.3390/universe9070323
Saburov S, Ketov SV. Improved Model of Primordial Black Hole Formation after Starobinsky Inflation. Universe. 2023; 9(7):323. https://doi.org/10.3390/universe9070323
Chicago/Turabian StyleSaburov, Sultan, and Sergei V. Ketov. 2023. "Improved Model of Primordial Black Hole Formation after Starobinsky Inflation" Universe 9, no. 7: 323. https://doi.org/10.3390/universe9070323
APA StyleSaburov, S., & Ketov, S. V. (2023). Improved Model of Primordial Black Hole Formation after Starobinsky Inflation. Universe, 9(7), 323. https://doi.org/10.3390/universe9070323