Reheating in a modified teleparallel model of inflation

H. Mohseni Sadjadi; P. Goodarzi

Reheating in a modified teleparallel model of inflation

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arxiv 1808.01225 v3 pith:2N6JDMME submitted 2018-07-30 physics.gen-ph gr-qchep-th

P. Goodarzi , H. Mohseni Sadjadi This is my paper · ORCID

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keywords reheatinginflationcosmologicalduringmodelteleparallelassumedcalculate

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We study the cosmological inflation and reheating in a teleparallel model of gravity. Reheating is assumed to be due to the decay of a scalar field to radiation during its rapid oscillation. By using cosmological perturbations during inflation, and subsequent evolutions of the Universe, we calculate the reheating temperature as a function of the spectral index and the power spectrum.

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End of the constant-roll inflation, and the reheating temperature
gr-qc 2019-08 reject novelty 5.0 of 10

A modified potential can terminate constant-roll inflation and produce an oscillatory reheating phase, yielding a reheating temperature within a few orders of magnitude of the GUT scale.

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