Returning back to Mukhanov parametrization of inflationary equation of state

Abstract We have re-examined Mukhanov parametrization for inflationary equation of state, $$1+\omega =\frac{\beta }{({N}+1)^\alpha }$$ 1 + ω = β ( N + 1 ) α , in the light of Planck 2018 results and latest bound of tensor-to-scalar ratio employing Hamilton–Jacobi formalism. We have found that the cu...

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Bibliographic Details
Main Author: Barun Kumar Pal
Format: Article
Language:English
Published: SpringerOpen 2025-05-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-025-14259-x
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