Natural inflation in Palatini $F(R,X)$

Fuente: arXiv
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Auteurs principaux: Bostan, N., Dejrah, R. H., Dioguardi, C., Racioppi, A.
Format: Preprint
Publié: 2025
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author Bostan, N.
Dejrah, R. H.
Dioguardi, C.
Racioppi, A.
author_facet Bostan, N.
Dejrah, R. H.
Dioguardi, C.
Racioppi, A.
contents In the context of Palatini gravity, $F(R+X)$ models, with X the inflaton kinetic term, are characterized by the appealing property of generating asymptotically flat inflaton potentials, exactly like the more commonly studied Palatini $F(R)$ models, but without the complication of non-canonical inflaton kinetic terms in the Einstein frame. In this paper, we study the case of a Jordan frame potential which is positive and bounded, specifically, natural inflation. We compute the CMB observables and show that for a wide class of $F(R + X)$ theories, including the quadratic one, natural inflation is still viable.
format Preprint
id arxiv_https___arxiv_org_abs_2503_16324
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Natural inflation in Palatini $F(R,X)$
Bostan, N.
Dejrah, R. H.
Dioguardi, C.
Racioppi, A.
General Relativity and Quantum Cosmology
In the context of Palatini gravity, $F(R+X)$ models, with X the inflaton kinetic term, are characterized by the appealing property of generating asymptotically flat inflaton potentials, exactly like the more commonly studied Palatini $F(R)$ models, but without the complication of non-canonical inflaton kinetic terms in the Einstein frame. In this paper, we study the case of a Jordan frame potential which is positive and bounded, specifically, natural inflation. We compute the CMB observables and show that for a wide class of $F(R + X)$ theories, including the quadratic one, natural inflation is still viable.
title Natural inflation in Palatini $F(R,X)$
topic General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2503.16324