An Effective Theory for Higgs Inflation
A. Tronconi, G. Venturi

TL;DR
This paper proposes a Higgs inflation model with quantum corrections that can produce primordial black holes consistent with CMB data, potentially explaining dark matter.
Contribution
It introduces two minimal EFT models where Higgs-driven inflation generates curvature perturbations capable of forming primordial black holes matching observational constraints.
Findings
Models produce curvature perturbations consistent with CMB observations
Primordial black holes formed in the asteroid mass range
Potential explanation for dark matter via primordial black holes
Abstract
The generation of large curvature perturbations associated with the production of primordial black holes is studied in the context of a Higgs inflaton. To enable this amplification, we consider an inflationary model in which the tree-level action for gravity and the Standard Model Higgs is modified by quantum corrections, described by a series of higher-dimension operators. Finally within a minimal EFT framework, we present two viable models in which the spectrum of curvature perturbations generated by the Higgs field is consistent with CMB observations and can lead to the formation of primordial black holes in the asteroid mass range, potentially accounting for the entirety of dark matter.
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Taxonomy
TopicsCosmology and Gravitation Theories · Particle physics theoretical and experimental studies · Black Holes and Theoretical Physics
