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arxiv: 1711.09915 · v2 · submitted 2017-11-27 · 🌌 astro-ph.CO · gr-qc· hep-th

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Primordial black holes from fifth forces

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classification 🌌 astro-ph.CO gr-qchep-th
keywords blackholesprimordialfifthfluctuationsheavyparticlesattractive
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Primordial black holes can be produced by a long range attractive fifth force stronger than gravity, mediated by a light scalar field interacting with nonrelativistic "heavy" particles. As soon as the energy fraction of heavy particles reaches a threshold, the fluctuations rapidly become nonlinear. The overdensities collapse into black holes or similar screened objects, without the need for any particular feature in the spectrum of primordial density fluctuations generated during inflation. We discuss whether such primordial black holes can constitute the total dark matter component in the Universe.

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Cited by 2 Pith papers

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

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    astro-ph.CO 2026-01 accept novelty 7.0

    Tachyonic instabilities from post-inflation curvature reorganization via quadratic Gauss-Bonnet coupling produce the observed dark matter relic density across wide mass and scale ranges, backed by lattice simulations ...

  2. Primordial Black Hole Hotspots Beyond Flat Spacetime

    hep-ph 2026-05 unverdicted novelty 6.0

    Hotspots around light primordial black holes cool faster in an expanding universe following T_plt ∝ t^{-11/15} and vanish completely in finite time, unlike everlasting hotspots in flat spacetime.