Can Primordial Black Holes form in the Standard Model ?
Ioanna Stamou, Sebastien Clesse

TL;DR
This paper examines whether primordial black holes could form within the Standard Model through Higgs field fluctuations, concluding that standard scenarios are unlikely but alternative gravity formulations might allow PBH formation.
Contribution
It demonstrates that standard Higgs field fluctuations in the SM cannot produce PBHs without conflicting with CMB constraints, but Palatini gravity offers a potential alternative.
Findings
Standard Higgs fluctuations produce too large curvature on cosmological scales.
PBH formation in the SM requires fine-tuning of the top-quark mass.
Palatini gravity may enable PBH formation without CMB conflicts.
Abstract
We investigate the viability of primordial black hole (PBH) formation in the Standard Model (SM) in a scenario that does not rely on specific inflationary features or any exotic physics such as phase transitions or non-minimal coupling to gravity. If the Brout-Englert-Higgs (BEH) field lies exactly at the transition between metastability and stability, its potential exhibits an inflexion point due to radiative corrections. The BEH can act like a stochastic curvaton field, leading to a non-Gaussian tail of large curvature fluctuations that later collapse into PBHs when they re-enter inside the horizon. This scenario would require a precise value of the top-quark mas to ensure the Higgs stability, which is disfavored but still consistent with the most recent measurements. However, we also find that large curvature fluctuations are also generated on cosmological scales that are…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Geophysics and Gravity Measurements
