Modified Chaplygin gas as an interacting holographic dark energy model

Science China: Physics, Mechanics and Astronomy

Volumn 53, Issue 4, 2010, Pages 598-606

  Yabo, Wu ^a   Weiqiang, Yang ^a   Cong, Wang ^a   Lei, Wang ^a  

^a LIAONING NORMAL UNIVERSITY   (China)

Author keywords

Geometrical diagnostics; Interacting holographic dark energy; Modified Chaplygin gas

Indexed keywords

CHAPLYGIN GAS; COUPLING CONSTANTS; DARK ENERGY; DARK MATTER; DENSITY PARAMETERS; EQUATION OF STATE; PRESENT VALUE; RED SHIFT;

AEROSPACE VEHICLES; COSMOLOGY; EQUATIONS OF STATE;

ASTROPHYSICS;

EID: 77953161799     PISSN: 16747348     EISSN: None     Source Type: Journal    
DOI: 10.1007/s11433-010-0119-9     Document Type: Article

References (41)

1. Riess A G, Filippenko Al V, Challis P, et al. Observational evidence from supernovae for an accelerating universe and a cosmological constant. Astron J, 1998, 116:1009-1038
2. Spergel D N, Verde L, Peiris H V, et al. First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of cosmological parameters. Astrophys J Suppl, 2003, 148:175-194
3. Tegmark M, Strauss M, Blanton M, et al. Cosmological parameters from SDSS and WMAP. Phys Rev D, 2004, 69:103501
4. Hinshaw G, Weiland J L, Hill R S, et al. Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data processing, sky maps, and basic results. Astrophys J Suppl, 2009, 180:225-245
5. Carroll S M. The cosmological constant. Living Rev Rel, 2001, 4:1
6. Fitch V L, Marlow D R, Dementi M A E. Critical Problems in Physics. Princeton. New Jersey: Princeton University Press, 1997
7. Peebles P J E, Ratra B. The cosmological constant and dark energy. Rev Mod Phys, 2003, 75:559-606
8. Padmanabhan T. Cosmological constant - the weight of the vacuum. Phys Rep, 2003, 380:235-320
9. Caldwell R R. A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state. Phys Lett B, 2002, 545:23-29
10. Chiba T, Okabe T, Yamaguchi M. Kinetically driven quintessence. Phys Rev D, 2000, 62:023511
11. Feng B, Wang X L, Zhang X M. Dark energy constraints from the cosmic age and supernova. Phys Lett B, 2005, 607:35-41
12. Sen A. Tachyon matter. J High Energy Phys, 2002, 0207:065
13. Kamenshchik A, Moschella U, Pasquier V. An alternative to quintessence. Phys Lett B, 2001, 511:265-268
14. Chimento L P. Extended tachyon field, Chaplygin gas and solvable kessence cosmologies. Phys Rev D, 2004, 69:123517
15. Wu Y B, Li S, Lu J B, et al. The modified Chaplygin gas as a unified dark sector model. Modern Phys Lett A, 2007, 22(11):783-790
16. Wu Y B, He J, Wang C, et al. Cosmological Evolution of Modified Chaplygin Gas Interacting with Barotropic Background Fluid. Modern Phys Lett A, 2009, 24(1):63-72
17. Li M. A model of holographic dark energy. Phys Lett B, 2004, 603:1
18. Cohen A G, Kaplan D B, Nelson A E. Effective field theory, black holes, and the cosmological constant. Phys Rev Lett, 1999, 82:4971-4974
19. Zhang X, Wu F Q. Constraints on holographic dark energy from type Ia supernova observations. Phys Rev D, 2005, 72:043524;
20. Constraints on holographic dark energy from the latest supernovae, galaxy clustering, and cosmic microwave background anisotropy observations. Phys Rev D, 2007, 76:023502;
21. Chang Z, Wu F Q, Zhang X. Constraints on holographic dark energy from X-ray gas mass fraction of galaxy clusters. Phys Lett B, 2006, 633:14-18;
22. Li M, Li X D, Wang S, et al. Holographic dark energy models: A comparison from the latest observational data. JCAP, 2009, 0906:036
23. Wang B, Gong Y, Abdalla E. Transition of the dark energy equation of state in an interacting holographic dark energy model. Phys Lett B, 2005, 624:141-146
24. Li M, Lin C S, Wang Y. Some issues concerning holographic dark energy. JCAP, 2008, 0805:023
25. Huang Q G, Li M. The holographic dark energy in a non-flat universe. JCAP, 2004, 0408:013
26. Zhang X. Reconstructing holographic quintessence. Phys Lett B, 2007, 648:1-7;
27. Dynamical vacuum energy, holographic quintom, and the reconstruction of scalar-field dark energy. Phys Rev D, 2006, 74:103505;
28. Holographic Ricci dark energy: Current observational constraints, quintom feature, and the reconstruction of scalar-field dark energy. Phys Rev D, 2009, 79:103509;
29. Zhang J F, Zhang X, Liu H Y. Holographic tachyon model. Phys Lett B, 2007, 651:84-87
30. Cunha J V, Lima J A S. Transition redshift: New kinematic constraints from supernovae. Mon Not Roy Astron Soc, 2008, 390:210-217
31. Sahni V, Saini T D, Starobinsky A A, et al. Statefinder - a new geometrical diagnostic of dark energy. JETP Lett, 2003, 77:201-206
32. Alam U, Sahni V, Saini T D, et al. Exploring the expanding universe and dark energy using the Statefinder Diagnostic. Mon Not Roy Astron Soc, 2003, 344:1057;
33. Zhang X. Statefinder diagnostic for coupled quintessence. Phys Lett B, 2005, 611:1-7;
34. Zhang X, Wu F Q, Zhang J F. New generalized Chaplygin gas as a scheme for unification of dark energy and dark matter. JCAP, 2006, 0601:003
35. Sahni V, Shafieloo A, Starobinsky A A. Two new diagnostics of dark energy. Phys Rev D, 2008, 78:103502
36. Zhang X. Statefinder diagnostic for holographic dark energy model. Int J Mod Phys D, 2005, 14:1597-1606; (Pubitemid 41376745)
37. Zhang J F, Zhang X, Liu H Y. Statefinder diagnosis for the interacting model of holographic dark energy. Phys Lett B, 2008, 659:26-33;
38. Wei H, Cai R G. Statefinder diagnostic and w-w' analysis for the agegraphic dark energy models without and with interaction. Phys Lett B, 2007, 655:1-6
39. Setare M R, Zhang J F, Zhang X. Statefinder diagnosis in a non-flat universe and the holographic model of dark energy. JCAP, 2007, 0703:007
40. Caldwell R R, Linder E V. The limits of quintessence. Phys Rev Lett, 2005, 95:141301
41. Scherrer R J. Dark energy models in the w-w' plane. Phys Rev D, 2006, 73:043502