Hamilton-Jacobi analysis of slow-roll inflation with non-Bekenstein-Hawking entropies yields fitted entropy parameters (δ≈1.1-1.2, α∼10^{-14}, K∼10^{-17}) consistent with ns and r data.
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Conformally coupled scalar field of mass order 10 M_pl can drive both inflation and dark energy via its vacuum stress tensor; minimally coupled field cannot.
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Hamilton-Jacobi Approach to Inflationary Scenarios through Extended Entropies: An Observational Perspective
Hamilton-Jacobi analysis of slow-roll inflation with non-Bekenstein-Hawking entropies yields fitted entropy parameters (δ≈1.1-1.2, α∼10^{-14}, K∼10^{-17}) consistent with ns and r data.
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Regularized vacuum stress tensor of a scalar field as the inflaton or dark energy
Conformally coupled scalar field of mass order 10 M_pl can drive both inflation and dark energy via its vacuum stress tensor; minimally coupled field cannot.