Reheating constraints on mutated hilltop inflation
arXiv:2401.09806 · doi:10.1142/S0218271824500408
Abstract
Future research studies of cosmic microwave background polarization seems likely to provide a more improved upper bound of on the tensor-to-scalar ratio(r). In our work, we have done the reheating study of mutated hilltop inflation(MHI), a model falling in the broad category of small field inflation. We have parameterized reheating in terms of various parameters like reheating duration , reheating temperature and effective equation of state using observationally viable values of scalar power spectrum amplitude and scalar spectral index . In our study, working over a range of , we found that the MHI potential is well consistent with combined Planck and BK18 observations for within a particular range of model's parameter space and the lower values of the model parameter in MHI generate considerably smaller r compared to normal hilltop potential without any incompatibility of with observational data, making MHI a better choice in accordance to recent and future studies.
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Cited by in corpus (4)
- Reheating study of Mexican-Hat-type Potentials
- Reheating and relic gravitational waves as remedies for degeneracies of non-canonical natural inflation
- Mutated hilltop inflation in light of Planck/ACT observations
- Hamilton-Jacobi analysis of noncanonical inflation in gravity: Constraints from Planck/ACT data, and theoretical bounds