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Parametrically amplified super-radiance towards hot big bang universe

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arxiv 2408.08605 v2 pith:N2MIWBMP submitted 2024-08-16 hep-ph astro-ph.COgr-qchep-th

classification hep-phastro-ph.COgr-qchep-th
keywords producedsuper-radianceuniverseamplifiedbangfieldhubbleinflation
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We propose a mechanism of preheating stage after inflation, using a new idea of parametrically amplified super-radiance. Highly coherent state, characterized by macro-coherence of scalar field coupled to produced massless particle in pairs, is created by parametric resonance effects associated with field oscillation around its potential minimum, within a Hubble volume. The state is described effectively by the simple Dicke-type of super-radiance model, and super-radiant pulse is emitted within a Hubble time, justifying neglect of cosmic expansion. Produced particles are shown to interact to change their energy and momentum distribution to realize thermal hot big bang universe. A long standing problem of heating after inflation may thus be solved. A new dark matter candidate produced at the emergence of thermalized universe is suggested as well.

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    Null results from the MICROSCOPE fifth-force experiment bound the Yukawa conformal coupling in a proposed scalar-tensor gravity to either less than about 3e-6 or greater than about 0.0026, assuming the model's dark-en...

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