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General dissipation coefficient in low-temperature warm inflation

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Original languageEnglish
Article number016
JournalJournal of Cosmology and Astroparticle Physics (JCAP)
Volume2013
Issue numberJanuary
DOIs
Publication statusPublished - 14 Jan 2013

Abstract

In generic particle physics models, the inflaton field is coupled to other bosonic and fermionic fields that acquire large masses during inflation and may decay into light degrees of freedom. This leads to dissipative effects that modify the inflationary dynamics and may generate a nearly-thermal radiation bath, such that inflation occurs in a warm rather than supercooled environment. In this work, we perform a numerical computation and obtain expressions for the associated dissipation coefficient in supersymmetric models, focusing on the regime where the radiation temperature is below the heavy mass threshold. The dissipation coefficient receives contributions from the decay of both on-shell and off-shell degrees of freedom, which are dominant for small and large couplings, respectively, taking into account the light field multiplicities. In particular, we find that the contribution from on-shell decays, although Boltzmann-suppressed, can be much larger than that of virtual modes, which is bounded by the validity of a perturbative analysis. This result opens up new possibilities for realizations of warm inflation in supersymmetric field theories.

    Research areas

  • hep-ph, astro-ph.CO, hep-th, supersymmetry and cosmology, particle physics - cosmology connection, inflation

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