Unifying Einstein and Palatini gravities

Luca Amendola, Kari Enqvist, and Tomi Koivisto
Phys. Rev. D 83, 044016 – Published 8 February 2011

Abstract

We consider a novel class of f(R) gravity theories where the connection is related to the conformally scaled metric g^μν=C(R)gμν with a scaling that depends on the scalar curvature R only. We call them C theories and show that the Einstein and Palatini gravities can be obtained as special limits. In addition, C theories include completely new physically distinct gravity theories even when f(R)=R. With nonlinear f(R), C theories interpolate and extrapolate the Einstein and Palatini cases and may avoid some of their conceptual and observational problems. We further show that C theories have a scalar-tensor formulation, which in some special cases reduces to simple Brans-Dicke–type gravity. If matter fields couple to the connection, the conservation laws in C theories are modified. The stability of perturbations about flat space is determined by a simple condition on the Lagrangian.

  • Received 4 November 2010

DOI:https://doi.org/10.1103/PhysRevD.83.044016

© 2011 American Physical Society

Authors & Affiliations

Luca Amendola*

  • Institut für Theoretische Physik, University of Heidelberg, Philosophenweg 16, 69120 Heidelberg, Germany

Kari Enqvist

  • Physics Department, University of Helsinki, and Helsinki Institute of Physics, FIN-00014 University of Helsinki

Tomi Koivisto

  • Institute for Theoretical Physics and Spinoza Institute, Leuvenlaan 4, 3584 CE Utrecht, The Netherlands.

  • *l.amendola@thphys.uni-heidelberg.de
  • kari.enqvist@helsinki.fi
  • t.s.koivisto@uu.nl

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Issue

Vol. 83, Iss. 4 — 15 February 2011

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