Exponential gravity

被引:199
作者
Linder, Eric V. [1 ,2 ,3 ]
机构
[1] Berkeley Lab, Berkeley, CA 94720 USA
[2] Univ Calif Berkeley, Berkeley, CA 94720 USA
[3] Ewha Womans Univ, Inst Early Universe, Seoul, South Korea
来源
PHYSICAL REVIEW D | 2009年 / 80卷 / 12期
关键词
D O I
10.1103/PhysRevD.80.123528
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigate a f(R) modification of gravity that is exponential in the Ricci scalar R to explain cosmic acceleration. The steepness of this dependence provides extra freedom to satisfy solar system and other curvature regime constraints. With a parameter to alleviate the usual fine-tuning of having the modification strengthen near the present, the total number of parameters is only one more than Lambda CDM. The resulting class of solutions asymptotes to w=-1 but has no cosmological constant. We calculate the dynamics in detail, examine the effect on the matter power spectrum, and provide a simple fitting form relating the two.
引用
收藏
页数:6
相关论文
共 15 条
  • [1] Do consistent F(R) models mimic general relativity plus Λ?
    Appleby, Stephen A.
    Battye, Richard A.
    [J]. PHYSICS LETTERS B, 2007, 654 (1-2) : 7 - 12
  • [2] Field flows of dark energy
    Cahn, Robert N.
    de Putter, Roland
    Linder, Eric V.
    [J]. JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2008, (11):
  • [3] Limits of quintessence
    Caldwell, RR
    Linder, EV
    [J]. PHYSICAL REVIEW LETTERS, 2005, 95 (14)
  • [4] CALDWELL RR, ANN REV AST IN PRESS, P64035
  • [5] Solar System constraints to general f(R) gravity
    Chiba, Takeshi
    Smith, Tristan L.
    Erickcek, Adrienne L.
    [J]. PHYSICAL REVIEW D, 2007, 75 (12):
  • [6] Class of viable modified f(R) gravities describing inflation and the onset of accelerated expansion
    Cognola, G.
    Elizalde, E.
    Nojiri, S.
    Odintsov, S. D.
    Sebastiani, L.
    Zerbini, S.
    [J]. PHYSICAL REVIEW D, 2008, 77 (04):
  • [7] DURRER R, ARXIV08114132
  • [8] Models of f(R) cosmic acceleration that evade solar system tests
    Hu, Wayne
    Sawicki, Ignacy
    [J]. PHYSICAL REVIEW D, 2007, 76 (06)
  • [9] Khoury J, 2004, PHYS REV D, V69, DOI 10.1103/PhysRevD.69.044026
  • [10] Nonlinear evolution of f(R) cosmologies. II. Power spectrum
    Oyaizu, Hiroaki
    Lima, Marcos
    Hu, Wayne
    [J]. PHYSICAL REVIEW D, 2008, 78 (12):