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arXiv · 1907.05042

Primordial Black Holes from Inflation with Nonminimal Derivative Coupling

Chengjie Fu·Puxun Wu·Hongwei Yu
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Abstract

We propose a novel enhancement mechanism of the curvature perturbations in the nonminimal derivative coupling inflation model with a coupling parameter related to the inflaton field. By considering a special form of the coupling parameter as a function of the inflaton, a period of ultra-slow-roll inflation can be realized due to the gravitationally enhanced friction, and the resulting power spectrum of the curvature perturbations has a sharp peak, which is large enough to produce the primordial black holes. Under this mechanism, we can easily obtain a sharp mass spectrum of primordial black holes around specific masses such as $\mathcal{O}(10)M_\odot$, $\mathcal{O}(10^{-5})M_\odot$, and $\mathcal{O}(10^{-12})M_\odot$, which can explain the LIGO events, the ultrashort-timescale microlensing events in OGLE data, and the most of dark matter, respectively.

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Chengjie Fu, Puxun Wu, Hongwei Yu. 2019-09-25. Primordial Black Holes from Inflation with Nonminimal Derivative Coupling. https://doi.org/10.1103/physrevd.100.063532

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