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Single-field models of inflation might lead to amplified scalar fluctuations on small scales due, for example, to a transient ultra-slow-roll phase.
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2011
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2011
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2013
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M. H. Namjoo, H. Firouzjahi and M. Sasaki, Violation of non-gaussianity consistency relation in a single-field inflationary model , EPL (Europhysics Letters) 101
2013
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H. Motohashi, A. A. Starobinsky and J. Yokoyama, Inflation with a constant rate of roll , JCAP 09
2015
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B. Carr, F. Kuhnel and M. Sandstad, Primordial Black Holes as Dark Matter , Phys. Rev. D 94
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K. Dimopoulos, Ultra slow-roll inflation demystified , Phys. Lett. B 775
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2019
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2021
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M. Taoso and A. Urbano, Non-gaussianities for primordial black hole formation , JCAP 08
2021
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2022
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S.-L. Cheng, D.-S. Lee and K.-W. Ng, Power spectrum of primordial perturbations during ultra-slow-roll inflation with back reaction effects , Physics Letters B 827
2022
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S. Pi and J. Wang, Primordial black hole formation in starobinsky’s linear potential model , Journal of Cosmology and Astroparticle Physics 2023
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