Self-accelerating universe in modified gravity with dynamical torsion

V. Nikiforova, S. Randjbar-Daemi, and V. Rubakov
Phys. Rev. D 95, 024013 – Published 11 January 2017

Abstract

We consider a model belonging to the class of gravities with dynamical torsion. The model is free of ghosts and gradient instabilities about Minkowski and torsionless Einstein backgrounds. We find that at zero cosmological constant, the model admits a self-accelerating solution with a non-Riemannian connection. Small value of the effective cosmological constant is obtained at the expense of the hierarchy between the dimensionless couplings.

  • Received 1 September 2016

DOI:https://doi.org/10.1103/PhysRevD.95.024013

© 2017 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

V. Nikiforova*

  • Institute for Nuclear Research of the Russian Academy of Sciences, 60th October Anniversary Prospect 7a, 117312 Moscow, Russia

S. Randjbar-Daemi

  • The Abdus Salam International Centre for Theoretical Physics, Strada Costiera 11 34014 Trieste, Italy

V. Rubakov

  • Institute for Nuclear Research of the Russian Academy of Sciences, 60th October Anniversary Prospect 7a, 117312 Moscow, Russia and Department of Particle Physics and Cosmology, Physics Faculty, Moscow State University Vorobjevy Gory, 119991 Moscow, Russia

  • *nikiforova@ms2.inr.ac.ru
  • seif@ictp.trieste.it
  • rubakov@ms2.inr.ac.ru

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Issue

Vol. 95, Iss. 2 — 15 January 2017

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