Holographic interacting dark energy in the braneworld cosmology

Modern Physics Letters A

Volumn 22, Issue 35, 2007, Pages 2631-2645

  Kyoung, Yee Kim ^a   Hyung, Won Lee ^a   Yun, Soo Myung ^a  

^a Inje University   (South Korea)

Author keywords

Brane cosmology; Holographic dark energy

Indexed keywords

EID: 36049043290     PISSN: 02177323     EISSN: None     Source Type: Journal    
DOI: 10.1142/S0217732307025765     Document Type: Article

References (59)

1. A. G. Riess et al., Astron. J. 116, 1009 (1998).
2. S. J. Perlmutter et al., Astrophys. J. 517, 565 (1999).
3. A. G. Riess et al., Astrophys. J. 607, 665 (2004).
4. P. Astier et al., Astron. Astrophys. 447, 31 (2006).
5. SDSS Collab. (M. Tegmark et al.), Phys. Rev. D 69, 103501 (2004).
6. SDSS Collab. (K. Abazajian et al.), Astron. J. 128, 502 (2004).
7. SDSS Collab. (K. Abazajian et al.), Astron. J. 129, 1755 (2005).
8. H. V. Peiris et al., Astrophys. J. Suppl. 148, 213 (2003).
9. C. L. Bennett et al., Astrophys. J. Suppl. 148, 1 (2003).
10. D. N. Spergel et al., Astrophys. J. Suppl. 148, 175 (2003).
11. D. N. Spergel et al., astro-ph/0603449.
12. A. Cohen, D. Kaplan and A. Nelson, Phys. Rev. Lett. 82, 4971 (1999).
13. P. Horava and D. Minic, Phys. Rev. Lett. 85, 1610 (2000).
14. S. Thomas, Phys. Rev. Lett. 89, 081301 (2002).
15. S. D. Hsu, Phys. Lett. B 594, 13 (2004).
16. M. Li, Phys. Lett. B 603, 1 (2004).
17. Q.-C. Huang and Y. Gong, J. Cosmol. Astropart. Phys. 0408, 006 (2004).
18. Y. Gong, Phys. Rev. D 70, 064029 (2004).
19. B. Wang, E. Abdalla and R.-K. Su, hep-th/0404057.
20. K. Enqvist and M. S. Sloth, Phys. Rev. Lett. 93, 221302 (2004).
21. S. Hsu and A. Zee, hep-th/0406142.
22. K. Ke and M. Li, hep-th/0407056.
23. P. F. Gonzalez-Diaz, hep-th/0411070.
24. H. Kim, H. W. Lee and Y. S. Myung, hep-th/0501118.
25. H. Kim, H. W. Lee and Y. S. Myung, Phys. Lett. B 628, 11 (2005).
26. X. Zhang, astro-ph/0504586.
27. X. Zhang and F.-Q. Wu, astro-ph/0506310.
28. H. M. Sadjadi and M. Honardoost, gr-qc/0609076.
29. M. R. Setare, J. Zhang and X. Zhang, gr-qc/0611084.
30. Y. S. Myung, Phys. Lett. B 610, 18 (2005).
31. Y. S. Myung, Mod. Phys. Lett. A 27, 2035 (2005).
32. A. J. M. Medved, hep-th/0501100.
33. D. Pavon and W. Zimdahl, Phys. Lett. B 628, 206 (2005).
34. W. Zimdahl, gr-qc/0505056.
35. M. S. Berger and H. Shojaei, Phys. Rev. D 73, 083528 (2006).
36. R. Horvat, Phys. Rev. D 70, 087301 (2004).
37. M. Szydlowski, Phys. Lett. B 632, 1 (2006).
38. E. J. Copeland, M. Sami and S. Tsujikawa, hep-th/0603057.
39. B. Wang, Y. Gong and E. Abdalla, Phys. Lett. B 624, 141 (2005).
40. H. Kim, H. W. Lee and Y. S. Myung, Phys. Lett. B 632, 605 (2006).
41. Q. G. Huang and M. Li, J. Cosmol. Astropart. Phys. 0408, 013 (2004).
42. B. Wang, C. Y. Lin and E. Abdalla, Phys. Lett. B 637, 357 (2006).
43. M. R. Setare, Phys. Lett. B 642, 1 (2006).
44. K. H. Kim, H. W. Lee and Y. S. Myung, Phys. Lett. B 648, 107 (2007).
45. M. R. Setare and E. C. Vagenas, arXiv: 0704.2070 [hep-th].
46. R. G. Cai, Y. G. Gong and B. Wang, J. Cosmol. Astropart. Phys. 0603, 006 (2006).
47. M. R. Setare, Phys. Lett. B 642, 421 (2006).
48. L. Randall and R. Sundrum, Phys. Rev. Lett. 83, 4690 (1999).
49. P. Binetruy, C. Deffayet and D. Langlois, Nucl. Phys. B 565, 269 (2000).
50. P. Binetruy, C. Deffayet, U. Ellwanger and D. Langlois, Phys. Lett. B 477, 285 (2000).
51. Y. S. Myung and J. Y. Kim, Class. Quantum Grav. 20, L169 (2003).
52. Kiritsis E.,Kofinas G.,Tetradis N.,Tomaras T.N.,Zarikas V.Cosmological evolution with brane-bulk energy exchange.Journal of High Energy Physics 7(2),2003,pp:733-754.
53. N. Tetradis, Phys. Lett. B 569, 1 (2003).
54. W. Zimdahl, D. Pavon and L. P. Cimento, Phys. Lett. B 521, 133 (2001).
55. Y. S. Myung, Phys. Lett. B 626, 1 (2005).
56. W. Zimdahl, D. J. Schwarz, A. B. Balakin and D. Pavon, Phys. Rev. D 64, 063501 (2001).
57. A. B. Balakin, D. Pavon, D. J. Schwarz and W. Zimdahl, New J. Phys. 5, 085 (2003).
58. Q. Wu, Y. Gong, A. Wang and J. S. Alcaniz, arXiv: 0705.1006 [astro-ph].
59. C. Bogdanos, S. Nesseris, L. Perivolaropoulos and K. Tamvakis, arXiv: 0705.3181 [hep-ph].