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Testing modified gravity models with recent cosmological observations

  • Published:2012-11-19 Issue:12 Volume:55 Page:2244-2258
  • ISSN:1674-7348
  • Container-title:Science China Physics, Mechanics and Astronomy
  • language:en
  • Short-container-title:Sci. China Phys. Mech. Astron.

Author:

Zhang WenShuai,Cheng Cheng,Huang QingGuo,Li Miao,Li Song,Li XiaoDong,Wang Shuang

Publisher

Springer Science and Business Media LLC

Subject

General Physics and Astronomy

Reference87 articles.

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2. Peebles P J E, Ratra B. The Cosmological constant and dark energy. Rev Mod Phys, 2003, 75: 559–606; Padmanabhan T. Cosmological constant: The weight of the vacuum. Phys Rep, 2003, 380: 235–320; Copeland E J, Sami M, Tsujikawa S. Dynamics of dark energy. Int J Mod Phys D, 2006, 15: 1753–1936; Albrecht A, Gary B, Robert C, et al. Report of the dark energy task force. arXiv:astro-ph/0609591; Frieman J, Turner M, Huterer D. Dark energy and the accelerating universe. Ann Rev Astron Astrophys, 2008, 46: 385–432; Tsujikawa S. Dark energy: Investigation and modeling. arXiv:1004.1493; Li M, Li X D, Wang S, et al. Dark Energy. Commun Theor Phys, 2011, 56: 525–604

3. Ratra B, Peebles P J E. Cosmological consequences of a rolling homogeneous scalar field. Phys Rev D, 1988, 37: 3406–3427; Peebles P J E, Ratra B. Cosmology with a time variable cosmological constant. Astrophys J, 1988, 325: L17–L20; Wetterich C. Cosmology and the fate of dilatation symmetry. Nucl Phys B, 1988, 302: 668–696; Zlatev I,Wang L, Steinhardt P J. Quintessence, cosmic coincidence, and the cosmological constant. Phys Rev Lett, 1999, 82: 896–899; Rahvar S, Movahed M S. Power-law parameterized quintessence model. Phys Rev D, 2007, 75: 023512

4. Caldwell R R. A phantom menace? Phys Lett B, 2002, 545: 23–29; Carroll S M, Hoffman M, Trodden M. Can the dark energy equationof-state parameter w be less than −1? Phys Rev D, 2003, 68: 023509; Huang T T, Wu P X, Yu H W. Observations favor the crossing of phantom divide lines. Sci China-Phys Mech Astron, 2010, 53(3): 562–566

5. Armendariz-Picon C, Damour T, Mukhanov V. k-inflation. Phys Lett B, 1999, 458: 209–218; Armendariz-Picon C, Mukhanov V, Steinhardt P J. Essentials of k essence. Phys Rev D, 2011, 63: 103510; Chiba T, Okabe T, Yamaguchi M. Kinetically driven quintessence. Phys Rev D, 2000, 62: 023511

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