Cosmological constant in F(R) supergravity

Sergei V. Ketov, Natsuki Watanabe

Research output: Contribution to journalArticle

7 Citations (Scopus)

Abstract

A cosmological constant in the regime of low space-time curvature is calculated in the recently proposed version of F(R) supergravity with a generic cubic function F. The F(R) supergravity is the N= 1 supersymmetric extension of f(R) gravity. The cubic model is known to successfully describe a chaotic (slow-roll) inflation in the regime of high space-time curvature. We find that a simple extension of the same model allows a positive cosmological constant in the regime of low space-time curvature. The inflaton superfield in F(R) supergravity (like inflaton in f(R) gravity) violates the Strong Energy Condition and thus breaks the restriction of the standard supergravity (with usual matter) that can only have either a negative or vanishing cosmological constant.

Original languageEnglish
Pages (from-to)410-413
Number of pages4
JournalPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Volume705
Issue number4
DOIs
Publication statusPublished - 17 Nov 2011
Externally publishedYes

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supergravity
curvature
gravitation
constrictions
energy

ASJC Scopus subject areas

  • Nuclear and High Energy Physics

Cite this

Cosmological constant in F(R) supergravity. / Ketov, Sergei V.; Watanabe, Natsuki.

In: Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, Vol. 705, No. 4, 17.11.2011, p. 410-413.

Research output: Contribution to journalArticle

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