Conditions for the cosmological viability of f(R) dark energy models
Abstract
We derive the conditions under which dark energy models whose Lagrangian densities f are written in terms of the Ricci scalar R are cosmologically viable. We show that the cosmological behavior of f(R) models can be understood by a geometrical approach consisting of studying the m(r) curve on the (r,m) plane, where m{identical_to}Rf{sub ,RR}/f{sub ,R} and r{identical_to}Rf{sub ,R}/f with f{sub ,R}{identical_to}df/dR. This allows us to classify the f(R) models into four general classes, depending on the existence of a standard matter epoch and on the final accelerated stage. The existence of a viable matterdominated epoch prior to a latetime acceleration requires that the variable m satisfies the conditions m(r){approx_equal}+0 and dm/dr>1 at r{approx_equal}1. For the existence of a viable latetime acceleration we require instead either (i) m=r1, ({radical}(3)1)/2<m{<=}1 and dm/dr<1 or (ii) 0<m{<=}1 at r=2. These conditions identify two regions in the (r,m) space, one for the matter era and the other for the acceleration. Only models with an m(r) curve that connects these regions and satisfies the requirements above lead to an acceptable cosmology. The models of type f(R)={alpha}R{sup n} and f=R+{alpha}R{sup n} do not satisfy these conditions for any n>0 and n<1 and are thus cosmologically unacceptable. Similarmore »
 Authors:
 INAF/Osservatorio Astronomico di Roma, Via Frascati 33, 00040 Monte Porzio Catone (Rome) (Italy)
 (France)
 (Japan)
 Publication Date:
 OSTI Identifier:
 21020346
 Resource Type:
 Journal Article
 Resource Relation:
 Journal Name: Physical Review. D, Particles Fields; Journal Volume: 75; Journal Issue: 8; Other Information: DOI: 10.1103/PhysRevD.75.083504; (c) 2007 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; ACCELERATION; ATTRACTORS; COSMOLOGY; DENSITY; LAGRANGIAN FUNCTION; NONLUMINOUS MATTER; PHANTOMS; SCALARS
Citation Formats
Amendola, Luca, Gannouji, Radouane, Polarski, David, Tsujikawa, Shinji, LPTA, Universite Montpellier II, CNRS, 34095 Montpellier Cedex 05, and Department of Physics, Gunma National College of Technology, Gunma 3718530. Conditions for the cosmological viability of f(R) dark energy models. United States: N. p., 2007.
Web. doi:10.1103/PHYSREVD.75.083504.
Amendola, Luca, Gannouji, Radouane, Polarski, David, Tsujikawa, Shinji, LPTA, Universite Montpellier II, CNRS, 34095 Montpellier Cedex 05, & Department of Physics, Gunma National College of Technology, Gunma 3718530. Conditions for the cosmological viability of f(R) dark energy models. United States. doi:10.1103/PHYSREVD.75.083504.
Amendola, Luca, Gannouji, Radouane, Polarski, David, Tsujikawa, Shinji, LPTA, Universite Montpellier II, CNRS, 34095 Montpellier Cedex 05, and Department of Physics, Gunma National College of Technology, Gunma 3718530. Sun .
"Conditions for the cosmological viability of f(R) dark energy models". United States.
doi:10.1103/PHYSREVD.75.083504.
@article{osti_21020346,
title = {Conditions for the cosmological viability of f(R) dark energy models},
author = {Amendola, Luca and Gannouji, Radouane and Polarski, David and Tsujikawa, Shinji and LPTA, Universite Montpellier II, CNRS, 34095 Montpellier Cedex 05 and Department of Physics, Gunma National College of Technology, Gunma 3718530},
abstractNote = {We derive the conditions under which dark energy models whose Lagrangian densities f are written in terms of the Ricci scalar R are cosmologically viable. We show that the cosmological behavior of f(R) models can be understood by a geometrical approach consisting of studying the m(r) curve on the (r,m) plane, where m{identical_to}Rf{sub ,RR}/f{sub ,R} and r{identical_to}Rf{sub ,R}/f with f{sub ,R}{identical_to}df/dR. This allows us to classify the f(R) models into four general classes, depending on the existence of a standard matter epoch and on the final accelerated stage. The existence of a viable matterdominated epoch prior to a latetime acceleration requires that the variable m satisfies the conditions m(r){approx_equal}+0 and dm/dr>1 at r{approx_equal}1. For the existence of a viable latetime acceleration we require instead either (i) m=r1, ({radical}(3)1)/2<m{<=}1 and dm/dr<1 or (ii) 0<m{<=}1 at r=2. These conditions identify two regions in the (r,m) space, one for the matter era and the other for the acceleration. Only models with an m(r) curve that connects these regions and satisfies the requirements above lead to an acceptable cosmology. The models of type f(R)={alpha}R{sup n} and f=R+{alpha}R{sup n} do not satisfy these conditions for any n>0 and n<1 and are thus cosmologically unacceptable. Similar conclusions can be reached for many other examples discussed in the text. In most cases the standard matter era is replaced by a cosmic expansion with scale factor a{proportional_to}t{sup 1/2}. We also find that f(R) models can have a strongly phantom attractor but in this case there is no acceptable matter era.},
doi = {10.1103/PHYSREVD.75.083504},
journal = {Physical Review. D, Particles Fields},
number = 8,
volume = 75,
place = {United States},
year = {Sun Apr 15 00:00:00 EDT 2007},
month = {Sun Apr 15 00:00:00 EDT 2007}
}

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