English

Primordial black hole formation from self-resonant preheating?

Cosmology and Nongalactic Astrophysics 2025-06-25 v4 General Relativity and Quantum Cosmology High Energy Physics - Phenomenology High Energy Physics - Theory

Abstract

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.

Keywords

Cite

@article{arxiv.2406.09122,
  title  = {Primordial black hole formation from self-resonant preheating?},
  author = {Guillermo Ballesteros and Joaquim Iguaz Juan and Paquale D. Serpico and Marco Taoso},
  journal= {arXiv preprint arXiv:2406.09122},
  year   = {2025}
}

Comments

20 pages, 6 figures. Clarifications added, results unchanged; matches published version in PRD