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Primordial black holes (PBHs) may result from high peaks in a random field of cosmological perturbations.
1903
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M. Shibata and M. Sasaki, “Black hole formation in the Friedmann universe: Formulation and computation in numerical relativity,” Phys. Rev. D 60
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P. Pina Avelino, “Primordial black hole constraints on non-Gaussian inflation models,” Phys. Rev. D 72
2005
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2013
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S. Young and C. T. Byrnes, “Primordial black holes in non-Gaussian regimes,” JCAP 1308
2013
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2015
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2015
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2015
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H. Motohashi, A. A. Starobinsky and J. Yokoyama, “Inflation with a constant rate of roll,” JCAP 1509
2015
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S. Bird, I. Cholis, J. B. Muñoz, Y. Ali-Haïmoud, M. Kamionkowski, E. D. Kovetz, A. Raccanelli and A. G. Riess, · 2016
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2016
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J. Garriga, A. Vilenkin and J. Zhang, “Black holes and the multiverse,” JCAP 1602
2016
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2018
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2018
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2018
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M. Cicoli, V. A. Diaz and F. G. Pedro, “Primordial Black Holes from String Inflation,” JCAP 1806
2018
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2018
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2019
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I. Dalianis, A. Kehagias and G. Tringas, “Primordial black holes from α-attractors,” JCAP 1901
2019
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