Cosmological dynamics on the brane

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 62, Issue 8, 2000, Pages 1-14

  Maartens, Roy ^a  

^a UNIVERSITY OF PORTSMOUTH   (United Kingdom)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 16644368000     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.62.084023     Document Type: Article

References (50)

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10. P. Binetruy, C. Deffayet, and D. Langlois, Nucl. Phys. B565, 269 (2000); N. Kaloper, Phys. Rev. D 60, 123506 (1999); T. Nihei, Phys. Lett. B 465, 81 (1999); C. Csaki, M. Graesser, C. Kolda, and J. Terning, ibid. 462, 34 (1999); H. B. Kim and H. D. Kim, Phys. Rev. D 61, 064003 (2000); P. Kanti, I. I. Kogan, K. A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); D. J. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); J. M. Cline, C. Grojean, and G. Servant, Phys. Rev. Lett. 83, 4245 (1999); E. E. Flanagan, S.-H. Tye, and I. Wasserman, Phys. Rev. D 62, 044039 (2000); P. Kraus, J. High Energy Phys. 12, 011 (1999); S. Mukoyama, Phys. Lett. B 473, 241 (2000); D. Ida, gr-qc/9912002; D. N. Vollick, hep-th/9911181; C. Csaki, M. Graesser, L. Randall, and J. Terning, Phys. Rev. D 62, 045015 (2000); C. Csaki, J. Erlich, T. J. Hollowood, and J. Terning, hep-th/0003076; R. N. Mohaptra, A. Perez-Lorenzana, and C. A. Pires, hep-ph/0003328; N. Deruelle and T. Dolezel, Phys. Rev. D (to be published), gr-qc/0004021; C. Barcelo and M. Visser, Phys. Lett. B 482, 183 (2000); J. Lesgourgues, S. Pastor, M. Peloso, and L. Sorbo, hep-ph/0004086; H. Stoica, S.-H. Henry Tye, and I. Wasserman, Phys. Lett. B 482, 205 (2000).
11. P. Binetruy, C. Deffayet, and D. Langlois, Nucl. Phys. B565, 269 (2000); N. Kaloper, Phys. Rev. D 60, 123506 (1999); T. Nihei, Phys. Lett. B 465, 81 (1999); C. Csaki, M. Graesser, C. Kolda, and J. Terning, ibid. 462, 34 (1999); H. B. Kim and H. D. Kim, Phys. Rev. D 61, 064003 (2000); P. Kanti, I. I. Kogan, K. A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); D. J. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); J. M. Cline, C. Grojean, and G. Servant, Phys. Rev. Lett. 83, 4245 (1999); E. E. Flanagan, S.-H. Tye, and I. Wasserman, Phys. Rev. D 62, 044039 (2000); P. Kraus, J. High Energy Phys. 12, 011 (1999); S. Mukoyama, Phys. Lett. B 473, 241 (2000); D. Ida, gr-qc/9912002; D. N. Vollick, hep-th/9911181; C. Csaki, M. Graesser, L. Randall, and J. Terning, Phys. Rev. D 62, 045015 (2000); C. Csaki, J. Erlich, T. J. Hollowood, and J. Terning, hep-th/0003076; R. N. Mohaptra, A. Perez-Lorenzana, and C. A. Pires, hep-ph/0003328; N. Deruelle and T. Dolezel, Phys. Rev. D (to be published), gr-qc/0004021; C. Barcelo and M. Visser, Phys. Lett. B 482, 183 (2000); J. Lesgourgues, S. Pastor, M. Peloso, and L. Sorbo, hep-ph/0004086; H. Stoica, S.-H. Henry Tye, and I. Wasserman, Phys. Lett. B 482, 205 (2000).
12. P. Binetruy, C. Deffayet, and D. Langlois, Nucl. Phys. B565, 269 (2000); N. Kaloper, Phys. Rev. D 60, 123506 (1999); T. Nihei, Phys. Lett. B 465, 81 (1999); C. Csaki, M. Graesser, C. Kolda, and J. Terning, ibid. 462, 34 (1999); H. B. Kim and H. D. Kim, Phys. Rev. D 61, 064003 (2000); P. Kanti, I. I. Kogan, K. A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); D. J. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); J. M. Cline, C. Grojean, and G. Servant, Phys. Rev. Lett. 83, 4245 (1999); E. E. Flanagan, S.-H. Tye, and I. Wasserman, Phys. Rev. D 62, 044039 (2000); P. Kraus, J. High Energy Phys. 12, 011 (1999); S. Mukoyama, Phys. Lett. B 473, 241 (2000); D. Ida, gr-qc/9912002; D. N. Vollick, hep-th/9911181; C. Csaki, M. Graesser, L. Randall, and J. Terning, Phys. Rev. D 62, 045015 (2000); C. Csaki, J. Erlich, T. J. Hollowood, and J. Terning, hep-th/0003076; R. N. Mohaptra, A. Perez-Lorenzana, and C. A. Pires, hep-ph/0003328; N. Deruelle and T. Dolezel, Phys. Rev. D (to be published), gr-qc/0004021; C. Barcelo and M. Visser, Phys. Lett. B 482, 183 (2000); J. Lesgourgues, S. Pastor, M. Peloso, and L. Sorbo, hep-ph/0004086; H. Stoica, S.-H. Henry Tye, and I. Wasserman, Phys. Lett. B 482, 205 (2000).
13. P. Binetruy, C. Deffayet, and D. Langlois, Nucl. Phys. B565, 269 (2000); N. Kaloper, Phys. Rev. D 60, 123506 (1999); T. Nihei, Phys. Lett. B 465, 81 (1999); C. Csaki, M. Graesser, C. Kolda, and J. Terning, ibid. 462, 34 (1999); H. B. Kim and H. D. Kim, Phys. Rev. D 61, 064003 (2000); P. Kanti, I. I. Kogan, K. A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); D. J. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); J. M. Cline, C. Grojean, and G. Servant, Phys. Rev. Lett. 83, 4245 (1999); E. E. Flanagan, S.-H. Tye, and I. Wasserman, Phys. Rev. D 62, 044039 (2000); P. Kraus, J. High Energy Phys. 12, 011 (1999); S. Mukoyama, Phys. Lett. B 473, 241 (2000); D. Ida, gr-qc/9912002; D. N. Vollick, hep-th/9911181; C. Csaki, M. Graesser, L. Randall, and J. Terning, Phys. Rev. D 62, 045015 (2000); C. Csaki, J. Erlich, T. J. Hollowood, and J. Terning, hep-th/0003076; R. N. Mohaptra, A. Perez-Lorenzana, and C. A. Pires, hep-ph/0003328; N. Deruelle and T. Dolezel, Phys. Rev. D (to be published), gr-qc/0004021; C. Barcelo and M. Visser, Phys. Lett. B 482, 183 (2000); J. Lesgourgues, S. Pastor, M. Peloso, and L. Sorbo, hep-ph/0004086; H. Stoica, S.-H. Henry Tye, and I. Wasserman, Phys. Lett. B 482, 205 (2000).
14. P. Binetruy, C. Deffayet, and D. Langlois, Nucl. Phys. B565, 269 (2000); N. Kaloper, Phys. Rev. D 60, 123506 (1999); T. Nihei, Phys. Lett. B 465, 81 (1999); C. Csaki, M. Graesser, C. Kolda, and J. Terning, ibid. 462, 34 (1999); H. B. Kim and H. D. Kim, Phys. Rev. D 61, 064003 (2000); P. Kanti, I. I. Kogan, K. A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); D. J. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); J. M. Cline, C. Grojean, and G. Servant, Phys. Rev. Lett. 83, 4245 (1999); E. E. Flanagan, S.-H. Tye, and I. Wasserman, Phys. Rev. D 62, 044039 (2000); P. Kraus, J. High Energy Phys. 12, 011 (1999); S. Mukoyama, Phys. Lett. B 473, 241 (2000); D. Ida, gr-qc/9912002; D. N. Vollick, hep-th/9911181; C. Csaki, M. Graesser, L. Randall, and J. Terning, Phys. Rev. D 62, 045015 (2000); C. Csaki, J. Erlich, T. J. Hollowood, and J. Terning, hep-th/0003076; R. N. Mohaptra, A. Perez-Lorenzana, and C. A. Pires, hep-ph/0003328; N. Deruelle and T. Dolezel, Phys. Rev. D (to be published), gr-qc/0004021; C. Barcelo and M. Visser, Phys. Lett. B 482, 183 (2000); J. Lesgourgues, S. Pastor, M. Peloso, and L. Sorbo, hep-ph/0004086; H. Stoica, S.-H. Henry Tye, and I. Wasserman, Phys. Lett. B 482, 205 (2000).
15. P. Binetruy, C. Deffayet, and D. Langlois, Nucl. Phys. B565, 269 (2000); N. Kaloper, Phys. Rev. D 60, 123506 (1999); T. Nihei, Phys. Lett. B 465, 81 (1999); C. Csaki, M. Graesser, C. Kolda, and J. Terning, ibid. 462, 34 (1999); H. B. Kim and H. D. Kim, Phys. Rev. D 61, 064003 (2000); P. Kanti, I. I. Kogan, K. A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); D. J. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); J. M. Cline, C. Grojean, and G. Servant, Phys. Rev. Lett. 83, 4245 (1999); E. E. Flanagan, S.-H. Tye, and I. Wasserman, Phys. Rev. D 62, 044039 (2000); P. Kraus, J. High Energy Phys. 12, 011 (1999); S. Mukoyama, Phys. Lett. B 473, 241 (2000); D. Ida, gr-qc/9912002; D. N. Vollick, hep-th/9911181; C. Csaki, M. Graesser, L. Randall, and J. Terning, Phys. Rev. D 62, 045015 (2000); C. Csaki, J. Erlich, T. J. Hollowood, and J. Terning, hep-th/0003076; R. N. Mohaptra, A. Perez-Lorenzana, and C. A. Pires, hep-ph/0003328; N. Deruelle and T. Dolezel, Phys. Rev. D (to be published), gr-qc/0004021; C. Barcelo and M. Visser, Phys. Lett. B 482, 183 (2000); J. Lesgourgues, S. Pastor, M. Peloso, and L. Sorbo, hep-ph/0004086; H. Stoica, S.-H. Henry Tye, and I. Wasserman, Phys. Lett. B 482, 205 (2000).
16. P. Binetruy, C. Deffayet, and D. Langlois, Nucl. Phys. B565, 269 (2000); N. Kaloper, Phys. Rev. D 60, 123506 (1999); T. Nihei, Phys. Lett. B 465, 81 (1999); C. Csaki, M. Graesser, C. Kolda, and J. Terning, ibid. 462, 34 (1999); H. B. Kim and H. D. Kim, Phys. Rev. D 61, 064003 (2000); P. Kanti, I. I. Kogan, K. A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); D. J. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); J. M. Cline, C. Grojean, and G. Servant, Phys. Rev. Lett. 83, 4245 (1999); E. E. Flanagan, S.-H. Tye, and I. Wasserman, Phys. Rev. D 62, 044039 (2000); P. Kraus, J. High Energy Phys. 12, 011 (1999); S. Mukoyama, Phys. Lett. B 473, 241 (2000); D. Ida, gr-qc/9912002; D. N. Vollick, hep-th/9911181; C. Csaki, M. Graesser, L. Randall, and J. Terning, Phys. Rev. D 62, 045015 (2000); C. Csaki, J. Erlich, T. J. Hollowood, and J. Terning, hep-th/0003076; R. N. Mohaptra, A. Perez-Lorenzana, and C. A. Pires, hep-ph/0003328; N. Deruelle and T. Dolezel, Phys. Rev. D (to be published), gr-qc/0004021; C. Barcelo and M. Visser, Phys. Lett. B 482, 183 (2000); J. Lesgourgues, S. Pastor, M. Peloso, and L. Sorbo, hep-ph/0004086; H. Stoica, S.-H. Henry Tye, and I. Wasserman, Phys. Lett. B 482, 205 (2000).
17. P. Binetruy, C. Deffayet, and D. Langlois, Nucl. Phys. B565, 269 (2000); N. Kaloper, Phys. Rev. D 60, 123506 (1999); T. Nihei, Phys. Lett. B 465, 81 (1999); C. Csaki, M. Graesser, C. Kolda, and J. Terning, ibid. 462, 34 (1999); H. B. Kim and H. D. Kim, Phys. Rev. D 61, 064003 (2000); P. Kanti, I. I. Kogan, K. A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); D. J. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); J. M. Cline, C. Grojean, and G. Servant, Phys. Rev. Lett. 83, 4245 (1999); E. E. Flanagan, S.-H. Tye, and I. Wasserman, Phys. Rev. D 62, 044039 (2000); P. Kraus, J. High Energy Phys. 12, 011 (1999); S. Mukoyama, Phys. Lett. B 473, 241 (2000); D. Ida, gr-qc/9912002; D. N. Vollick, hep-th/9911181; C. Csaki, M. Graesser, L. Randall, and J. Terning, Phys. Rev. D 62, 045015 (2000); C. Csaki, J. Erlich, T. J. Hollowood, and J. Terning, hep-th/0003076; R. N. Mohaptra, A. Perez-Lorenzana, and C. A. Pires, hep-ph/0003328; N. Deruelle and T. Dolezel, Phys. Rev. D (to be published), gr-qc/0004021; C. Barcelo and M. Visser, Phys. Lett. B 482, 183 (2000); J. Lesgourgues, S. Pastor, M. Peloso, and L. Sorbo, hep-ph/0004086; H. Stoica, S.-H. Henry Tye, and I. Wasserman, Phys. Lett. B 482, 205 (2000).
18. P. Binetruy, C. Deffayet, and D. Langlois, Nucl. Phys. B565, 269 (2000); N. Kaloper, Phys. Rev. D 60, 123506 (1999); T. Nihei, Phys. Lett. B 465, 81 (1999); C. Csaki, M. Graesser, C. Kolda, and J. Terning, ibid. 462, 34 (1999); H. B. Kim and H. D. Kim, Phys. Rev. D 61, 064003 (2000); P. Kanti, I. I. Kogan, K. A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); D. J. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); J. M. Cline, C. Grojean, and G. Servant, Phys. Rev. Lett. 83, 4245 (1999); E. E. Flanagan, S.-H. Tye, and I. Wasserman, Phys. Rev. D 62, 044039 (2000); P. Kraus, J. High Energy Phys. 12, 011 (1999); S. Mukoyama, Phys. Lett. B 473, 241 (2000); D. Ida, gr-qc/9912002; D. N. Vollick, hep-th/9911181; C. Csaki, M. Graesser, L. Randall, and J. Terning, Phys. Rev. D 62, 045015 (2000); C. Csaki, J. Erlich, T. J. Hollowood, and J. Terning, hep-th/0003076; R. N. Mohaptra, A. Perez-Lorenzana, and C. A. Pires, hep-ph/0003328; N. Deruelle and T. Dolezel, Phys. Rev. D (to be published), gr-qc/0004021; C. Barcelo and M. Visser, Phys. Lett. B 482, 183 (2000); J. Lesgourgues, S. Pastor, M. Peloso, and L. Sorbo, hep-ph/0004086; H. Stoica, S.-H. Henry Tye, and I. Wasserman, Phys. Lett. B 482, 205 (2000).
19. P. Binetruy, C. Deffayet, and D. Langlois, Nucl. Phys. B565, 269 (2000); N. Kaloper, Phys. Rev. D 60, 123506 (1999); T. Nihei, Phys. Lett. B 465, 81 (1999); C. Csaki, M. Graesser, C. Kolda, and J. Terning, ibid. 462, 34 (1999); H. B. Kim and H. D. Kim, Phys. Rev. D 61, 064003 (2000); P. Kanti, I. I. Kogan, K. A. Olive, and M. Pospelov, Phys. Lett. B 468, 31 (1999); D. J. Chung and K. Freese, Phys. Rev. D 61, 023511 (2000); J. M. Cline, C. Grojean, and G. Servant, Phys. Rev. Lett. 83, 4245 (1999); E. E. Flanagan, S.-H. Tye, and I. Wasserman, Phys. Rev. D 62, 044039 (2000); P. Kraus, J. High Energy Phys. 12, 011 (1999); S. Mukoyama, Phys. Lett. B 473, 241 (2000); D. Ida, gr-qc/9912002; D. N. Vollick, hep-th/9911181; C. Csaki, M. Graesser, L. Randall, and J. Terning, Phys. Rev. D 62, 045015 (2000); C. Csaki, J. Erlich, T. J. Hollowood, and J. Terning, hep-th/0003076; R. N. Mohaptra, A. Perez-Lorenzana, and C. A. Pires, hep-ph/0003328; N. Deruelle and T. Dolezel, Phys. Rev. D (to be published), gr-qc/0004021; C. Barcelo and M. Visser, Phys. Lett. B 482, 183 (2000); J. Lesgourgues, S. Pastor, M. Peloso, and L. Sorbo, hep-ph/0004086; H. Stoica, S.-H. Henry Tye, and I. Wasserman, Phys. Lett. B 482, 205 (2000).
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