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Primordial black hole formation from self-resonant preheating?

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arxiv 2406.09122 v4 pith:ZOZC7USS submitted 2024-06-13 astro-ph.CO gr-qchep-phhep-th

Primordial black hole formation from self-resonant preheating?

classification astro-ph.CO gr-qchep-phhep-th
keywords blackformationgenericpreheatingprimordialholeholesoutcome
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We revisit the question of how generic is the formation of primordial black holes via self-resonant growth of inflaton fluctuations in the post-inflationary, preheating phase. Using analytical and lattice calculations, we find that primordial black hole production is far from being a generic outcome. Also, in most of the parameter space of viable inflationary models, the metric preheating term is subleading to the anharmonic terms and the approximation of a quadratic potential for describing the resonance dynamics is inadequate. Nonetheless, the anharmonicity of the potential cannot be used to rescue the mechanism: The generic outcome of the non-linear evolution of the scalar field in this case is the formation of metastable transients or oscillons, that do not generically collapse into black holes.

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Cited by 2 Pith papers

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