Phantom with Born-Infeld-type Lagrangian

Physical Review D

Volumn 68, Issue 4, 2003, Pages

  Hao, Jian Gang ^a   Li, Xin Zhou ^a  

^a SHANGHAI NORMAL UNIVERSITY   (China)

Author keywords

[No Author keywords available]

Indexed keywords

ANALYTIC METHOD; ARTICLE; ASTRONOMY; COSMOS; ELECTRIC POTENTIAL; ENERGY; KINETICS; PHANTOM;

EID: 0141768360     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.68.043501     Document Type: Article

References (81)

1. P. de Bernardis et al., Nature (London) 404, 955 (2000);
2. S. Hanany et al., Astrophys. J. 545, 1 (2000);
3. N. Bahcall, J.P. Ostriker, S. Perlmutter, and P.J. Steinhardt, Science 284, 1481 (1999);
4. S. Perlmutter et al., Astrophys. J. 517, 565 (1999);
5. A.G. Riess et al., Astron. J. 116, 1009 (1998).
6. B. Ratra and P.J. Peebles, Phys. Rev. D 37, 3406 (1988);
7. R.R. Caldwell, R. Dave, and P.J. Steinhardt, Phys. Rev. Lett. 80, 1582 (1998);
8. P.J. Steinhardt, L. Wang, and I. Zlatev, Phys. Rev. D 59, 123504 (1999);
9. I. Zlatev, L. Wang, and P.J. Steinhardt, Phys. Rev. Lett. 82, 896 (1999);
10. K. Coble, S. Dodelson, and J. Frieman, Phys. Rev. D 55, 1851 (1997);
11. X.Z. Li, J.G. Hao, and D.J. Liu, Class. Quantum Grav. 19, 6049 (2002).
12. A: Melchiorri, L. Mersini, C.J. Odmann, and M. Trodden, Phys. Rev. D (to be published), astro-ph/0211522.
13. J.L. Tonry et al., astro-ph/0305008.
14. R.R. Caldwell, Phys. Lett. B 545, 23 (2002).
15. V. Sahni and A.A. Starobinsky, Int. J. Mod. Phys. D 9, 373 (2002).
16. L. Parker and A. Raval, Phys. Rev. D 60, 063512 (1999).
17. T. Chiba, T. Okabe, and M. Yamaguchi, Phys. Rev. D 62, 023511 (2000).
18. B. Boisseau, G. Esposito-Farese, D. Polarski, and A.A. Starobinsky, Phys. Rev. Lett. 85, 2236 (2000).
19. A.E. Schulz and M. White, Phys. Rev. D 64, 043514 (2001).
20. V. Faraoni, Int. J. Mod. Phys. D 11, 471 (2002).
21. I. Maor, R. Brustein, J. McMahon, and P.J. Steinhardt, Phys. Rev. D 65, 123003 (2002).
22. V.K. Onemli and R.P. Woodard, Class. Quantum Grav. 19, 4607 (2002).
23. D.F. Torres, Phys. Rev. D 66, 043522 (2002).
24. S. M. Carroll, M. Hoffman, and M. Trodden, Phys. Rev. D 68, 023509 (2003).
25. P.H. Frampton, hep-th/0302007.
26. J.G. Hao and X.Z. Li, Phys. Rev. D 67, 107303 (2003);
27. X.Z. Li and J.G. Hao, hep-th/0303093.
28. R.R. Caldwell, M. Kamionkowski, and N.N. Weinberg, astro-ph/0302506.
29. G.W. Gibbons, hep-th/0302199.
30. A. Feinstein and S. Jhingan, hep-th/0304069;
31. L. P. Chimento and A. Feinstein, astro-ph/0305007;
32. P. Singh, M. Sami, and N. Dadhich, Phys. Rev. D (to be published), hep-tn/0305110.
33. A. Sen, J. High Energy Phys. 04, 048 (2002);
34. A. Sen, J. High Energy Phys. 07, 065 (2002);
35. G.W. Gibbons, Phys. Lett. B 537, l (2002);
36. A. Sen, J. Math. Phys. 42, 2844 (2001);
37. G.W. Gibbons, K. Hori, and P. Yi, Nucl. Phys. B596, 136 (2001);
38. A. Sen, hep-th/0303057;
39. J.G. Hao and X.Z. Li, Phys. Rev. D 66, 087301 (2002);
40. X.Z. Li and X.H. Zhai, Phys. Rev. D ibid. 67, 067501 (2003);
41. A. Frolov, L. Kofman, and A. Starobinsky, Phys. Lett. B 545, 8 (2002);
42. S. Mukohyama, Phys. Rev. D 66, 024009 (2002);
43. T. Padmanabhan, Phys. Rev. D ibid. 66, 021301(R) (2002);
44. M. Sami and T. Padmanabhan, Phys. Rev. D ibid. 67, 083509 (2003);
45. G. Shiu and I. Wasserman, Phys. Lett. B 541, 6 (2002);
46. L. Kofman and A. Linde, J. High Energy Phys. 07, 004 (2002);
47. H. B. Benaoum, hep-th/0205140;
48. A. Ishida and S. Uehara, Phys. Lett. B 544, 353 (2002);
49. T. Chiba, Phys. Rev. D 66, 063514 (2002);
50. T. Mehen and B. Wecht, J. High Energy Phys. 02, 058 (2003);
51. A. Sen, J. High Energy Phys. ibid. 10, 003 (2002);
52. N. Moeller and B. Zwiebach, J. High Energy Phys. ibid. 10, 034 (2002);
53. J.M. Cline, H. Firouzjahi, and P. Martineau, J. High Energy Phys. ibid. 11, 041 (2002);
54. S. Mukohyama, Phys. Rev. D 66, 123512 (2002);
55. P. Mukhopadhyay and A. Sen, J. High Energy Phys. 11, 047 (2002);
56. T. Okuda and S. Sugimoto, Nucl. Phys. B647, 101 (2002);
57. G. Gibbons, K. Hashimoto, and P. Yi, J. High Energy Phys. 09, 061 (2002);
58. M.R. Garousi, Nucl. Phys. B647, 117 (2002);
59. A. Sen, hep-th/0209122;
60. B. Chen, M. Li, and F. Lin, J. High Energy Phys. 11, 050 (2002);
61. J. Kluson, hep-th/0209255;
62. C. Kim, H.B. Kim, Y. Kim, and O.K. Kwon, hep-th/0301142;
63. X.Z. Li, D.J. Liu, and J.G. Hao, hep-th/0207146;
64. G. Felder, L. Kofman, and A. Starobinsky, J. High Energy Phys. 09, 026 (2002);
65. S. Mukohyama, Phys. Rev. D 66, 123512 (2002);
66. G.A. Diamandis, B.C. Georgalas, N.E. Mavromatos, and E. Papantonopoulos, Int. J. Mod. Phys. A 17, 4567 (2002);
67. G.A. Diamandis, B.C. Georgalas, N.E. Mavromatos, and E. Papantonopoulos, Int. J. Mod. Phys. A 17, 2241 (2002);
68. M.C. Bento, O. Bertolami, and A. Sen, Phys. Rev. D 67, 063511 (2003);
69. M.C. Bento, O. Bertolami, and A. Sen, Phys. Rev. D 67, 023504 (2003);
70. C. Kim, H.B. Kim, and Y. Kim, Phys. Lett. B 552, 111 (2003);
71. C. Kim, Y. Kim, O.K. Kwon, and C. Oh Lee, hep-th/0305092;
72. H. Lee and W.S. I'Yi, hep-th/0210221;
73. J.S. Bagla, H.K. Jassal, and T. Padmanabhan, Phys. Rev. D 67, 063504 (2003);
74. F. Leblond and A.W. Peet, hep-th/0303035; hep-th/0305059;
75. T. Matsuda, Phys. Rev. D 67, 083519 (2003); hep-ph/0302078;
76. A. Das and A. DeBenedictis, gr-qc/0304017;
77. M. Majumdar and A. Davis, hep-th/0304226.
78. X. Z. Li, J. G. Hao, and D. J. Liu, Chin. Phys. Lett. 19, 1584 (2002).
79. G.W. Gibbons, Class. Quantum Grav. 20, S321 (2003).
80. D. Kutasov, M. Marino, and G. W. Moore, J. High Energy Phys. 10, 045 (2000).
81. J.K. Erickson et al., Phys. Rev. Lett. 88, 121301 (2002).