Abstract
AbstractWe show that the observed primordial perturbations can be entirely sourced by a light spectator scalar field with a quartic potential, akin to the Higgs boson, provided that the field is sufficiently displaced from vacuum during inflation. The framework relies on the indirect modulation of reheating, which is implemented without any direct coupling between the spectator field and the inflaton and does not require non-renormalisable interactions. The scenario gives rise to local non-Gaussianity with $$f_{\mathrm{NL}}\simeq 5$$
f
NL
≃
5
as the typical signal. As an example model where the indirect modulation mechanism is realised for the Higgs boson, we study the Standard Model extended with right-handed neutrinos. For the Standard Model running we find, however, that the scenario analysed does not seem to produce the observed perturbation.
Funder
Eesti Teadusagentuur
European Regional Development Fund
H2020 Marie Sklodowska-Curie Actions
Science and Technology Facilities Council
Institute for Particle Physics Phenomenology, Durham University
Publisher
Springer Science and Business Media LLC
Subject
Physics and Astronomy (miscellaneous),Engineering (miscellaneous)
Cited by
1 articles.
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1. Primordial black holes from spectator field bubbles;Journal of Cosmology and Astroparticle Physics;2022-02-01