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Primordial Black Holes in Higgs-$R^2$ Inflation as a Whole Dark Matter

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arxiv 1912.12032 v3 pith:ZT72BMPX submitted 2019-12-27 hep-ph astro-ph.COgr-qchep-th

classification hep-phastro-ph.COgr-qchep-th
keywords blackholesprimordialdarkinflationmatterabundanceconsist
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abstract

Primordial black holes are produced in a minimal UV extension to the Higgs inflation with an included $R^2$ term. We show that for parameters consistent with Standard Model measurements and Planck observation results lead to $M_{\rm PBH} \in (10^{-16}, 10^{-15}) M_\odot$ primordial black holes with significant abundance, which may consist the majority of dark matter.

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Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Superhorizon curvature perturbations in hybrid inflation revisited

    astro-ph.CO 2026-06 unverdicted novelty 6.0 of 10

    Hybrid inflation's waterfall tachyonic instability grows isocurvature modes that convert to curvature perturbations at the field-space turn, yielding a k^{3}-peaked spectrum with always-positive f_NL that enhances PBH...

  2. Implication of preheating on gravity assisted baryogenesis in $R^2$-Higgs inflation

    hep-ph 2024-11 conditional novelty 6.0 of 10

    Preheating in R2-Higgs inflation sets the reheating temperature, and matching the observed baryon asymmetry fixes the baryogenesis scale to about 2.1 to 2.8 x 10^-5 M_Planck for xi_H between 1 and 10.

  3. Gravitational waves from a first-order phase transition of the inflaton

    hep-ph 2024-12 conditional novelty 5.0 of 10

    A single non-minimally coupled dark Higgs can drive both inflation and a first-order phase transition whose gravitational waves fall within the reach of planned experiments.

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