English

Unifying Einstein and Palatini gravities

General Relativity and Quantum Cosmology 2011-02-18 v1 Cosmology and Nongalactic Astrophysics

Abstract

We consider a novel class of f(R)f(\R) gravity theories where the connection is related to the conformally scaled metric g^μν=C(R)gμν\hat g_{\mu\nu}=C(\R)g_{\mu\nu} with a scaling that depends on the scalar curvature R\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)=Rf(\R)=\R. With nonlinear f(R)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.

Keywords

Cite

@article{arxiv.1010.4776,
  title  = {Unifying Einstein and Palatini gravities},
  author = {Luca Amendola and Kari Enqvist and Tomi Koivisto},
  journal= {arXiv preprint arXiv:1010.4776},
  year   = {2011}
}

Comments

17 pages, no figures

R2 v1 2026-06-21T16:32:56.788Z