The f(R) gravity function of the Linde quintessence

Sergei V. Ketov, Natsuki Watanabe

Research output: Contribution to journalArticlepeer-review

10 Citations (Scopus)


We calculate the f(R) gravity function in the dual gravity description of the quintessence model with a quadratic (Linde) scalar potential and a positive cosmological constant. We find that in the large curvature regime relevant to chaotic inflation in Early Universe, the dual f(R) gravity is well approximated by the (matter) loop-corrected Starobinsky inflationary model. In the small curvature regime relevant to dark energy in the Present Universe, the f(R) gravity function reduces to the Einstein-Hilbert one with a positive cosmological constant.

Original languageEnglish
Pages (from-to)242-245
Number of pages4
JournalPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Publication statusPublished - 4 Feb 2015

ASJC Scopus subject areas

  • Nuclear and High Energy Physics

Fingerprint Dive into the research topics of 'The f(R) gravity function of the Linde quintessence'. Together they form a unique fingerprint.

Cite this