Temperature in warm inflation in non minimal kinetic coupling model

H. Mohseni Sadjadi; Parviz Goodarzi

Temperature in warm inflation in non minimal kinetic coupling model

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arxiv 1409.5119 v2 pith:POPL25O4 submitted 2014-09-17 gr-qc hep-th

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

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Warm inflation in the non minimal derivative coupling model with a general dissipation coefficient is considered. We investigate conditions for the existence of the slow roll approximation and study cosmological perturbations. The spectral index, and the power spectrum are calculated and the temperature of the universe at the end of the slow roll warm inflation is obtained.

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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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