Chaotic inflation in F(R) supergravity

Research School of High-Energy Physics

Research output: Contribution to journal › Article

Abstract

The bosonic f(R) gravity function is derived from a chiral F(R) supergravity model for the first time. We find the existence of the upper limit (or AdS bound) on the scalar curvature, as well as a solution with the vanishing cosmological constant. We compare our simple model of F(R) supergravity to the well-known Starobinsky model of chaotic inflation.

Original language	English
Pages (from-to)	272-276
Number of pages	5
Journal	Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Volume	692
Issue number	4
DOIs	https://doi.org/10.1016/j.physletb.2010.07.045
Publication status	Published - Sep 2010

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Keywords

Inflation
Supergravity

ASJC Scopus subject areas

Nuclear and High Energy Physics

Cite this

Ketov, S. V. (2010). Chaotic inflation in F(R) supergravity. Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, 692(4), 272-276. https://doi.org/10.1016/j.physletb.2010.07.045

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Access to Document

10.1016/j.physletb.2010.07.045