Cosmological expansion and the uniqueness of the gravitational action
Abstract
Modified theories of gravity have recently been studied by several authors as possibly viable alternatives to the cosmological concordance model. Such theories attempt to explain the accelerating expansion of the universe by changing the theory of gravity, instead of introducing dark energy. In particular, a class of models based on higher order curvature invariants, socalled f(R) gravity models, has drawn attention. In this letter we show that within this framework, the expansion history of the universe does not uniquely determine the form of the gravitational action and it can be radically different from the standard EinsteinHilbert action. We demonstrate that for any fluid with a barotropic equation state, there always exists a class of f(R) models that will have exactly the same expansion history as that arising from the EinsteinHilbert action. This also holds for multicomponent systems that allow an effective fluid description. Consequently, any f(R) model that leads to a given expansion history can always be generalized to a class of models that have exactly the same expansion history as a solution. We explicitly show how one can extend the EinsteinHilbert action by constructing a f(R) theory that is equivalent on the classical level. As a result, we findmore »
 Authors:
 NORDITA, Blegdamsvej 17, DK2100 Copenhagen (Denmark)
 (Finland)
 Department of Physics, University of Turku, FIN20014 Turku (Finland)
 Publication Date:
 OSTI Identifier:
 20795735
 Resource Type:
 Journal Article
 Resource Relation:
 Journal Name: Physical Review. D, Particles Fields; Journal Volume: 73; Journal Issue: 2; Other Information: DOI: 10.1103/PhysRevD.73.024018; (c) 2006 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA)
 Country of Publication:
 United States
 Language:
 English
 Subject:
 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; COSMOLOGICAL CONSTANT; COSMOLOGY; EXPANSION; GENERAL RELATIVITY THEORY; GRAVITATION; MATHEMATICAL SOLUTIONS; NONLUMINOUS MATTER; SCALAR FIELDS; SCALARS; SPACETIME; TENSORS; UNIVERSE
Citation Formats
Multamaeki, T., Department of Physics, University of Turku, FIN20014 Turku, and Vilja, I. Cosmological expansion and the uniqueness of the gravitational action. United States: N. p., 2006.
Web. doi:10.1103/PHYSREVD.73.0.
Multamaeki, T., Department of Physics, University of Turku, FIN20014 Turku, & Vilja, I. Cosmological expansion and the uniqueness of the gravitational action. United States. doi:10.1103/PHYSREVD.73.0.
Multamaeki, T., Department of Physics, University of Turku, FIN20014 Turku, and Vilja, I. Sun .
"Cosmological expansion and the uniqueness of the gravitational action". United States.
doi:10.1103/PHYSREVD.73.0.
@article{osti_20795735,
title = {Cosmological expansion and the uniqueness of the gravitational action},
author = {Multamaeki, T. and Department of Physics, University of Turku, FIN20014 Turku and Vilja, I.},
abstractNote = {Modified theories of gravity have recently been studied by several authors as possibly viable alternatives to the cosmological concordance model. Such theories attempt to explain the accelerating expansion of the universe by changing the theory of gravity, instead of introducing dark energy. In particular, a class of models based on higher order curvature invariants, socalled f(R) gravity models, has drawn attention. In this letter we show that within this framework, the expansion history of the universe does not uniquely determine the form of the gravitational action and it can be radically different from the standard EinsteinHilbert action. We demonstrate that for any fluid with a barotropic equation state, there always exists a class of f(R) models that will have exactly the same expansion history as that arising from the EinsteinHilbert action. This also holds for multicomponent systems that allow an effective fluid description. Consequently, any f(R) model that leads to a given expansion history can always be generalized to a class of models that have exactly the same expansion history as a solution. We explicitly show how one can extend the EinsteinHilbert action by constructing a f(R) theory that is equivalent on the classical level. As a result, we find that one cannot mimic {lambda}CDM type expansion exactly by a matter only universe by any choice of f(R) without introducing an explicit cosmological constant. Because of the classical equivalence between f(R) theories and EinsteinHilbert gravity with an extra scalar field, one can also hence construct equivalent scalartensor theories with standard expansion.},
doi = {10.1103/PHYSREVD.73.0},
journal = {Physical Review. D, Particles Fields},
number = 2,
volume = 73,
place = {United States},
year = {Sun Jan 15 00:00:00 EST 2006},
month = {Sun Jan 15 00:00:00 EST 2006}
}

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