Observational constraints to ricci dark energy model by using: SN, BAO, OHD, fgas data sets

Journal of Cosmology and Astroparticle Physics

Volumn 2010, Issue 6, 2010, Pages

  Xu, Lixin ^a   Wang, Yuting ^a  

^a DALIAN UNIVERSITY OF TECHNOLOGY   (China)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 77953101885     PISSN: 14757516     EISSN: 14757516     Source Type: Journal    
DOI: 10.1088/1475-7516/2010/06/002     Document Type: Article

References (82)

1. Supernova Search Team collaboration, A.G. Riess et al., 1998 Observational evidence from supernovae for an accelerating universe and a cosmological constant, Astron. J. 116 1009 [astro-ph/9805201]
2. Supernova Cosmology Project collaboration, S. Perlmutter et al., 1999 Measurements of Ω and Λ from 42 high-redshift supernovae, Astrophys. J. 517 565 [astro-ph/9812133]
3. WMAP collaboration, D.N. Spergel et al., 2003 First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: determination of cosmological parameters, Astrophys. J. Suppl. 148 175 [astro-ph/0302209]
4. WMAP collaboration, D.N. Spergel et al., 2007 Wilkinson Microwave Anisotropy Probe (WMAP) three year results: implications for cosmology, Astrophys. J. Suppl. 170 377 [astro-ph/0603449]
5. SDSS collaboration, M. Tegmark et al., 2004 Cosmological parameters from SDSS and WMAP, Phys. Rev. D 69 103501 [astro-ph/0310723]
6. SDSS collaboration, M. Tegmark et al., 2004 The 3 D power spectrum of galaxies from the SDSS, Astrophys. J. 606 702 [astro-ph/0310725]
7. H.K. Jassal, J.S. Bagla and T. Padmanabhan, Understanding the origin of CMB constraints on dark energy, [astro-ph/0601389]
8. T.M. Davis et al., 2007 Scrutinizing exotic cosmological models using {ESSENCE} supernova data combined with other cosmological probes, Astrophys. J. 666 716 [astro-ph/0701510]
9. L. Samushia and B. Ratra, 2008 Constraints on dark energy from galaxy cluster gas mass fraction versus redshift data, Astrophys. J. 680 L1 [0803.3775]
10. P.J.E. Peebles and B. Ratra, 1988 Cosmology with a time-variable cosmological 'constant', Astrophys. J. Lett. 325 L17
11. B. Ratra and P.J.E. Peebles, 1988 Cosmological consequences of a rolling homogeneous scalar field, Phys. Rev. D 37 3406
12. I. Zlatev, L.-M. Wang and P.J. Steinhardt, 1999 Quintessence, cosmic coincidence and the cosmological constant, Phys. Rev. Lett. 82 896 [astro-ph/9807002]
13. P.J. Steinhardt, L.-M. Wang and I. Zlatev, 1999 Cosmological tracking solutions, Phys. Rev. D 59 123504 [astro-ph/9812313]
14. M.S. Turner, 2002 Making sense of the new cosmology, Int. J. Mod. Phys. A 17S1 180 [astro-ph/0202008]
15. V. Sahni, 2002 The cosmological constant problem and quintessence, Class. Quant. Grav. 19 3435 [astro-ph/0202076]
16. R.R. Caldwell, M. Kamionkowski and N.N. Weinberg, 2003 Phantom energy and cosmic doomsday, Phys. Rev. Lett. 91 071301 [astro-ph/0302506]
17. B. Feng, X.-L. Wang and X.-M. Zhang, 2005 Dark energy constraints from the cosmic age and supernova, Phys. Lett. B 607 35 [astro-ph/0404224]
18. S.D.H. Hsu, 2004 Entropy bounds and dark energy, Phys. Lett. B 594 13 [hep-th/0403052]
19. M. Li, 2004 A model of holographic dark energy, Phys. Lett. B 603 1 [hep-th/0403127]
20. R.-G. Cai, 2007 A dark energy model characterized by the age of the universe, Phys. Lett. B 657 228 [0707.4049]
21. H. Wei and R.-G. Cai, 2008 A new model of agegraphic dark energy, Phys. Lett. B 660 113 [0708.0884]
22. C. Gao, X. Chen and Y.-G. Shen, 2009 A holographic dark energy model from Ricci scalar curvature, Phys. Rev. D 79 043511 [0712.1394]
23. L. Xu, W. Li and J. Lu, 2009 Cosmic constraint on Ricci dark energy model, Mod. Phys. Lett. A 24 1355 [0810.4730]
24. ESSENCE collaboration, W.M. Wood-Vasey et al., 2007 Observational constraints on the nature of the dark energy: first cosmological results from the ESSENCE supernova survey, Astrophys. J. 666 694 [astro-ph/0701041]
25. Supernova Search Team collaboration, A.G. Riess et al., 2004 Type Ia supernova discoveries at z > 1 from the Hubble Space Telescope: evidence for past deceleration and constraints on dark energy evolution, Astrophys. J. 607 665 [astro-ph/0402512]
26. Λ and w from the first year data set, Astron. Astrophys. 447 31 [astro-ph/0510447]
27. A.G. Riess et al., 2007 New Hubble Space Telescope discoveries of type Ia supernovae at z > 1: narrowing constraints on the early behavior of dark energy, Astrophys. J. 659 98 [astro-ph/0611572]
28. Y. Wang and P. Mukherjee, 2006 Robust dark energy constraints from supernovae, galaxy clustering and three-year Wilkinson Microwave Anisotropy Probe observations, Astrophys. J. 650 1 [astro-ph/0604051]
29. SDSS collaboration, D.J. Eisenstein et al., 2005 Detection of the baryon acoustic peak in the large-scale correlation function of SDSS luminous red galaxies, Astrophys. J. 633 560 [astro-ph/0501171]
30. X. Zhang, 2009 Holographic Ricci dark energy: current observational constraints, quintom feature and the reconstruction of scalar-field dark energy, Phys. Rev. D 79 103509 [0901.2262]
31. M. Suwa and T. Nihei, 2010 Observational constraints on the interacting Ricci dark energy model, Phys. Rev. D 81 023519 [0911.4810]
32. WMAP collaboration, E. Komatsu et al., 2009 Five-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: cosmological interpretation, Astrophys. J. Suppl. 180 330 [0803.0547]
33. L. Xu, J. Lu and W. Li, 2009 Generalized holographic and Ricci dark energy models, Eur. Phys. J. C 64 89 [0906.0210]
34. W.J. Percival et al., 2007 Measuring the baryon acoustic oscillation scale using the SDSS and 2dFGRS, Mon. Not. Roy. Astron. Soc. 381 1053 [0705.3323]
35. M. Li, X.-D. Li and X. Zhang, Comparison of dark energy models: a perspective from the latest observational data, [0912.3988]
36. M. Hicken et al., 2009 Improved dark energy constraints from ∼ 100 new CfA supernova type Ia light curves, Astrophys. J. 700 1097 [0901.4804]
37. W.J. Percival et al., 2010 Baryon acoustic oscillations in the Sloan digital sky survey data release 7 galaxy sample, Mon. Not. Roy. Astron. Soc. 401 2148 [0907.1660]
38. S.W. Allen et al., 2008 Improved constraints on dark energy from Chandra X-ray observations of the largest relaxed galaxy clusters, Mon. Not. Roy. Astron. Soc. 383 879 [0706.0033]
39. E. Gaztanaga, A. Cabre and L. Hui, 2009 Clustering of luminous red galaxies IV: baryon acoustic peak in the line-of-sight direction and a direct measurement of H(z), Mon. Not. Roy. Astron. Soc. 399 1663 [0807.3551]
40. A.G. Riess et al., 2009 A redetermination of the Hubble constant with the Hubble Space Telescope from a differential distance ladder, Astrophys. J. 699 539 [0905.0695]
41. D. Stern, R. Jimenez, L. Verde, M. Kamionkowski and S.A. Stanford, 2010 Cosmic chronometers: constraining the equation of state of dark energy. I: H(z) measurements J. Cosmol. Astropart. Phys. JCAP02(2010)008 [0907.3149]
42. A. Lewis and S. Bridle, 2002 Cosmological parameters from CMB and other data: a Monte-Carlo approach, Phys. Rev. D 66 103511 [astro-ph/0205436]
43. Cosmological Monte-Carlo homepage, http://cosmologist.info/cosmomc/
44. D. Rapetti, S.W. Allen and J. Weller, 2005 Constraining dark energy with X-ray galaxy clusters, supernovae and the Cosmic Microwave Background, Mon. Not. Roy. Astron. Soc. 360 555 [astro-ph/0409574]
45. Module for CosmoMC to include the [X-ray cluster gas mass fraction] fgas experiment, http://www.stanford.edu/∼drapetti/fgas-module
46. S. Burles, K.M. Nollett and M.S. Turner, 2001 Big-bang nucleosynthesis predictions for precision cosmology, Astrophys. J. 552 L1 [astro-ph/0010171]
47. M. Biesiada, 2007 Information-theoretic model selection applied to supernovae data J. Cosmol. Astropart. Phys. JCAP02(2007)003 [astro-ph/0701721]
48. A.R. Liddle, 2004 How many cosmological parameters?, Mon. Not. Roy. Astron. Soc. 351 L49 [astro-ph/0401198]
49. W. Godlowski and M. Szydlowski, 2005 Which cosmological model with dark energy - phantom or ΛCDM, Phys. Lett. B 623 10 [astro-ph/0507322]
50. W. Godlowski and M. Szydlowski, 2006 Which cosmological models - with dark energy or modified FRW dynamics?, Phys. Lett. B 633 427 [astro-ph/0509415]
51. M. Szydlowski, A. Kurek and A. Krawiec, 2006 Top ten accelerating cosmological models, Phys. Lett. B 642 171 [astro-ph/0604327]
52. M. Szydlowski and A. Kurek, 2006 Testing and selection cosmological models with dark energy, AIP Conf. Proc. 861 1031 [astro-ph/0603538]
53. L.X. Xu, C.W. Zhang and H.Y. Liu, 2007 Cosmological constant or variable dark energy?, Chin. Phys. Lett. 24 2459.
54. S. Nesseris and L. Perivolaropoulos, 2007 Crossing the phantom divide: theoretical implications and observational status J. Cosmol. Astropart. Phys. JCAP01(2007)018 [astro-ph/0610092]
55. Supernova Cosmology Project collaboration, M. Kowalski et al., 2008 Improved cosmological constraints from new, old and combined supernova datasets, Astrophys. J. 686 749 [0804.4142]
56. J. Guy, P. Astier, S. Nobili, N. Regnault and R. Pain, 2005 SALT: a Spectral Adaptive Light curve Template for type Ia supernovae, Astron. Astrophys. 443 781 [astro-ph/0506583]
57. E. Garcia-Berro, E. Gaztanaga, J. Isern, O. Benvenuto and L. Althaus, On the evolution of cosmological type Ia supernovae and the gravitational constant, [astro-ph/9907440]
58. A. Riazuelo and J.-P. Uzan, 2002 Cosmological observations in scalar-tensor quintessence, Phys. Rev. D 66 023525 [astro-ph/0107386]
59. V. Acquaviva and L. Verde, 2007 Observational signatures of Jordan-Brans-Dicke theories of gravity J. Cosmol. Astropart. Phys. JCAP12(2007)001 [0709.0082]
60. R. Gannouji and D. Polarski, 2008 The growth of matter perturbations in some scalar-tensor DE models J. Cosmol. Astropart. Phys. JCAP05(2008)018 [0802.4196]
61. S. Nesseris and L. Perivolaropoulos, 2005 Comparison of the legacy and gold SnIa dataset constraints on dark energy models, Phys. Rev. D 72 123519 [astro-ph/0511040]
62. L. Perivolaropoulos, 2005 Constraints on linear-negative potentials in quintessence and phantom models from recent supernova data, Phys. Rev. D 71 063503 [astro-ph/0412308]
63. E. Di Pietro and J.-F. Claeskens, 2003 Quintessence models faced with future supernovae data, Mon. Not. Roy. Astron. Soc. 341 1299 [astro-ph/0207332]
64. A.C.C. Guimaraes, J.V. Cunha and J.A.S. Lima, 2009 Bayesian analysis and constraints on kinematic models from union SNIa J. Cosmol. Astropart. Phys. JCAP10(2009)010 [0904.3550]
65. L. Xu, W. Li and J. Lu, 2009 Constraints on kinematic model from recent cosmic observations: SN Ia, BAO and observational Hubble data J. Cosmol. Astropart. Phys. JCAP07(2009)031 [0905.4552]
66. T. Okumura et al., 2008 Large-scale anisotropic correlation function of SDSS luminous red galaxies, Astrophys. J. 676 889 [0711.3640]
67. D.J. Eisenstein and W. Hu, 1998 Baryonic features in the matter transfer function, Astrophys. J. 496 605 [astro-ph/9709112]
68. W. Hu and N. Sugiyama, 1995 Anisotropies in the Cosmic Microwave Background: an analytic approach, Astrophys. J. 444 489 [astro-ph/9407093]
69. W. Hu, M. Fukugita, M. Zaldarriaga and M. Tegmark, 2001 CMB observables and their cosmological implications, Astrophys. J. 549 669 [astro-ph/0006436]
70. R.R. Caldwell and M. Doran, 2004 Cosmic Microwave Background and supernova constraints on quintessence: concordance regions and target models, Phys. Rev. D 69 103517 [astro-ph/0305334]
71. J.R. Bond, G. Efstathiou and M. Tegmark, 1997 Forecasting cosmic parameter errors from microwave background anisotropy experiments Mon. Not. Roy. Astron. Soc. 291 L33 [astro-ph/9702100]
72. W. Hu and N. Sugiyama, 1996 Small scale cosmological perturbations: an analytic approach, Astrophys. J. 471 542 [astro-ph/9510117].
73. R. Jimenez and A. Loeb, 2002 Constraining cosmological parameters based on relative galaxy ages, Astrophys. J. 573 37 [astro-ph/0106145]
74. R. Jimenez, L. Verde, T. Treu and D. Stern, 2003 Constraints on the equation of state of dark energy and the Hubble constant from stellar ages and the CMB, Astrophys. J. 593 622 [astro-ph/0302560]
75. J. Simon, L. Verde and R. Jimenez, 2005 Constraints on the redshift dependence of the dark energy potential, Phys. Rev. D 71 123001 [astro-ph/0412269]
76. R.G. Abraham et al., 2004 The Gemini Deep Deep Survey: I. introduction to the survey, catalogs and composite spectra, Astron. J. 127 2455 [astro-ph/0402436]
77. T. Treu, M. Stiavelli, S. Casertano, P. Møller and G. Bertin, 1999 The properties of field elliptical galaxies at intermediate redshift. I: empirical scaling laws, Mon. Not. Roy. Astron. Soc. 308 1037 [astro-ph/9904327]
78. T. Treu, M. Stiavelli, P. Møller, S. Casertano and G. Bertin, 2001 The properties of field elliptical galaxies at intermediate redshift. II: photometry and spectroscopy of an HST selected sample, Mon. Not. Roy. Astron. Soc. 326 221 [astro-ph/0104177]
79. T. Treu, M. Stiavelli, S. Casertano, P. Møller and G. Bertin, 2002 The evolution of field early-type galaxies to z∼ 0.7, Astrophys. J. Lett. 564 L13
80. J. Dunlop et al., 1996 A 3.5-Gyr-old galaxy at redshift 1.55, Nature 381 581
81. H. Spinrad et al., 1997 LBDS 53W091: an old red galaxy at z=1.552, Astrophys. J. 484 581 [astro-ph/9702233]
82. L.A. Nolan, J.S. Dunlop, R. Jimenez and A.F. Heavens, 2003 F stars, metallicity and the ages of red galaxies at z > 1, Mon. Not. Roy. Astron. Soc. 341 464 [astro-ph/0103450]