Natural inflation in Palatini F(R,X)

IF 5.3 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
N. Bostan, R.H. Dejrah, C. Dioguardi and A. Racioppi
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引用次数: 0

Abstract

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.
Palatini F(R,X)的自然通货膨胀
在Palatini引力的背景下,F(R+X)模型,其中X为暴胀动力学项,具有产生渐近平坦暴胀势的吸引人的性质,就像更常见的Palatini F(R)模型一样,但没有爱因斯坦框架中非规范暴胀动力学项的复杂性。本文研究了一类正有界的约当框架势,即自然膨胀。我们计算了CMB的可观测值,并证明了对于广泛的F(R + X)理论,包括二次型理论,自然暴胀仍然是可行的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Journal of Cosmology and Astroparticle Physics
Journal of Cosmology and Astroparticle Physics 地学天文-天文与天体物理
CiteScore
10.20
自引率
23.40%
发文量
632
审稿时长
1 months
期刊介绍: Journal of Cosmology and Astroparticle Physics (JCAP) encompasses theoretical, observational and experimental areas as well as computation and simulation. The journal covers the latest developments in the theory of all fundamental interactions and their cosmological implications (e.g. M-theory and cosmology, brane cosmology). JCAP''s coverage also includes topics such as formation, dynamics and clustering of galaxies, pre-galactic star formation, x-ray astronomy, radio astronomy, gravitational lensing, active galactic nuclei, intergalactic and interstellar matter.
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