The coincidence problem and interacting holographic dark energy

Journal of Cosmology and Astroparticle Physics

Volumn 2008, Issue 5, 2008, Pages

  Karwan, Khamphee ^a  

^a CHULALONGKORN UNIVERSITY   (Thailand)

Author keywords

Classical tests of cosmology; Dark energy theory

Indexed keywords

EID: 44449096725     PISSN: 14757516     EISSN: 14757516     Source Type: Journal    
DOI: 10.1088/1475-7516/2008/05/011     Document Type: Article

References (26)

1. Riess A G et al 1998 Observational evidence from supernovae for an accelerating universe and a cosmological constant Astron. J. 116 1009 [astro-ph/9805201]
2. Perlmutter S et al 1999 Measurements of Omega and Lambda from 42 high-redshift supernovae Astrophys. J. 517 565 [astro-ph/9812133]
3. Zimdahl W and Pavón D 2003 Scaling cosmology Gen. Rel. Grav. 35 413 [astro-ph/0210484]
4. del Campo S, Herrera R, Olivares G and Pavón D 2006 Interacting models of soft coincidence Phys. Rev. D 74 023501 [astro-ph/0606520]
5. Sadjadi H M and Alimohammadi M 2006 Cosmological coincidence problem in interacting dark energy models Phys. Rev. D 74 103007 [gr-qc/0610080]
6. Amendola L 2000 Coupled quintessence Phys. Rev. D 62 043511 [astro-ph/9908023]
7. Chimento L P, Jakubi A S, Pavón D and Zimdahl W 2003 Interacting quintessence solution to the coincidence problem Phys. Rev. D 67 083513 [astro-ph/0303145]
8. Cohen A G, Kaplan D B and Nelson A E 1999 Effective field theory, black holes, and the cosmological constant Phys. Rev. Lett. 82 4971 [hep-th/9803132]
9. Li M 2004 A model of holographic dark energy Phys. Lett. B 603 1 [hep-th/0403127]
10. Setare M R and Vagenas E C 2007 The cosmological dynamics of interacting holographic dark energy model Preprint 0704.2070
11. Setare M R 2006 Interacting holographic dark energy model in non-flat universe Phys. Lett. B 642 1 [hep-th/0609069]
12. Setare M R 2006 Bulk-brane interaction and holographic dark energy Phys. Lett. B 642 421 [hep-th/0609104]
13. Setare M R 2007 Interacting holographic phantom Eur. Phys. J. C 50 991 [hep-th/0701085]
14. Elizalde E, Nojiri S, Odintsov S D and Wang P 2005 Dark energy: vacuum fluctuations, the effective phantom phase, and holography Phys. Rev. D 71 103504 [hep-th/0502082]
15. Gong Y, Wang B and Wang A 2007 Thermodynamical properties of dark energy Phys. Rev. D 75 123516 [gr-qc/0611155]
16. Riess A G et al 2006 New Hubble Space Telescope discoveries of type Ia supernovae at z>1: narrowing constraints on the early behavior of dark energy Preprint astro-ph/0611572
17. Wang Y and Mukherjee P 2006 Observational constraints on dark energy and cosmic curvature Astrophys. J. 650 1 [astro-ph/0703780]
18. Eisenstein D J 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]
19. Zhang X and Wu F 2005 Constraints on holographic dark energy from type Ia supernova observations Phys. Rev. D 72 043524 [astro-ph/0506310]
20. Zhang X and Wu F 2007 Constraints on holographic dark energy from latest supernovae, galaxy clustering, and cosmic microwave background anisotropy observations Phys. Rev. D 76 023502 [astro-ph/0701405]
21. Spergel D N et al 2003 First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: determination of cosmological parameters Astrophys. J. Suppl. 148 175 [astro-ph/0302209]
22. Li M, Lin C and Wang Y 2008 Some issues concerning holographic dark energy Preprint 0801.1407
23. Kodama H and Sasaki M 1984 Cosmological perturbation theory Prog. Theor. Phys. Suppl. 78 1
24. Malik K 2001 Cosmological perturbations in an inflationary universe Preprint astro-ph/0101563
25. Doran M 2005 Cmbeasy:: an object oriented code for the cosmic microwave background J. Cosmol. Astropart. Phys. JCAP10(2005)011 [astro-ph/0302138]
26. Spergel D N et al 2007 Wilkinson Microwave Anisotropy Probe (WMAP) three year results: implications for cosmology Astrophys. J. Suppl. 170 377 [astro-ph/0603449]