Unifying Einstein and Palatini gravities
- 1. Institute for Theoretical Physics and Spinoza Institute, Leuvenlaan 4, 3584 CE Utrecht (Netherlands)
- 2. Physics Department, University of Helsinki, and Helsinki Institute of Physics, FIN-00014 University of Helsinki (Finland)
- 3. Institut fuer Theoretische Physik, University of Heidelberg, Philosophenweg 16, 69120 Heidelberg (Germany)
Description
We consider a novel class of f(R) gravity theories where the connection is related to the conformally scaled metric gμν=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.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.83.044016;
- arXiv
- arXiv:1010.4776v1;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 83
- Journal Issue
- 4
- Journal Page Range
- p. 044016-044016.14
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 42097471
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- CONSERVATION LAWS; DISTURBANCES; GRAVITATION; LAGRANGIAN FUNCTION; METRICS; NONLINEAR PROBLEMS; PERTURBATION THEORY; SCALING; STABILITY
- Descriptors DEC
- FUNCTIONS
Optional Information
- Notes
- (c) 2011 American Institute of Physics