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- W3100774924 abstract "The warm inflation scenario in view of the modified Chaplygin gas is studied. We consider the inflationary expansion to be driven by a standard scalar field whose decay ratio $$Gamma $$ has a generic power-law dependence with the scalar field $$phi $$ and the temperature of the thermal bath T. By assuming an exponential power-law dependence in the cosmic time for the scale factor a(t), corresponding to the intermediate inflation model, we solve the background and perturbative dynamics considering our model to evolve according to (1) weak dissipative regime and (2) strong dissipative regime. Specifically, we find explicit expressions for the dissipative coefficient, scalar potential, and the relevant inflationary observables like the scalar power spectrum, scalar spectral index, and tensor-to-scalar ratio. The free parameters characterizing our model are constrained by considering the essential condition for warm inflation, the conditions for the model evolves according to weak or strong dissipative regime, and the 2015 Planck results through the $$n_s$$ –r plane." @default.
- W3100774924 created "2020-11-23" @default.
- W3100774924 creator A5041916789 @default.
- W3100774924 creator A5042058003 @default.
- W3100774924 creator A5045660535 @default.
- W3100774924 creator A5085249966 @default.
- W3100774924 date "2017-10-01" @default.
- W3100774924 modified "2023-10-16" @default.
- W3100774924 title "Impact of generalized dissipative coefficient on warm inflationary dynamics in the light of latest Planck data" @default.
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- W3100774924 doi "https://doi.org/10.1140/epjc/s10052-017-5264-0" @default.