Wormhole surgery and cosmology on the brane: The world is not enough

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 62, Issue 6, 2000, Pages 1-4

  Anchordoqui, Luis A ^a   Perez Bergliaffa, Santiago E ^b  

^a NORTHEASTERN UNIVERSITY   (United States)

^b CENTRO BRASILEIRO DE PESQUISAS FÍSICAS   (Brazil)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 4243996747     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

References (34)

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2. This scale emerges from supersymmetry breaking, see, for instance, L. Randall and R. Sundrum, Nucl. Phys. B557, 79 (1999), and references therein.
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5. This confinement might be explained by string and M theory. See P. Hořava and E. Witten, Nucl. Phys. B460, 506 (1996); E. Witten, ibid. B471, 135 (1996); I. Antoniadis, G. D'Appollonio, E. Dudas, and A. Sagnotti, ibid. B553, 133 (1999).
6. This confinement might be explained by string and M theory. See P. Hořava and E. Witten, Nucl. Phys. B460, 506 (1996); E. Witten, ibid. B471, 135 (1996); I. Antoniadis, G. D'Appollonio, E. Dudas, and A. Sagnotti, ibid. B553, 133 (1999).
7. This confinement might be explained by string and M theory. See P. Hořava and E. Witten, Nucl. Phys. B460, 506 (1996); E. Witten, ibid. B471, 135 (1996); I. Antoniadis, G. D'Appollonio, E. Dudas, and A. Sagnotti, ibid. B553, 133 (1999).
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10. Before going on, it is interesting to remark that the gravitational collapse of uncharged nonrotating matter trapped on the brane (with a noncompact fifth dimension) settles down to a steady state with a "naked" singularity. A. Chamblin, S. W. Hawking, and H. S. Reall, Phys. Rev. D 61, 065007 (2000).
11. N. Arkani-Hamed, S. Dimopoulos, N. Kaloper, and J. March Russell, Nucl. Phys. B567, 189 (2000); N. Kaloper, Phys. Rev. D 60, 123506 (1999); C. Csáki, M. Graesser, C. Kolda, and J. Terning, Phys. Lett. B 462, 34 (1999); J. M. Cline, C. Grojean, and G. Servant, Phys. Rev. Lett. 83, 4245 (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); J. Cline, C. Grojean, and G. Servant, ibid. 472, 302 (2000); P. Kraus, J. High Energy Phys. 11, 9912 (1999); S. Nam, hep-th/9911237; N. Arkani-Hamed, S. Dimopoulos, G. Dvali, and N. Kaloper, hep-ph/9911386; C. Csaki, M. Graesser, L. Randall, and J. Terning, Phys. Rev. D (to be published), hep-ph/9911406; D. Ida, gr-qc/9912002; N. Kaloper, Phys. Lett. B 474, 269 (2000); M. Cvetič and J. Wang, Phys. Rev. D 61, 124020 (2000); S. Mukohyama, T. Shiromizu, and K. Maeda, ibid. 62, 024028 (2000).
12. N. Arkani-Hamed, S. Dimopoulos, N. Kaloper, and J. March Russell, Nucl. Phys. B567, 189 (2000); N. Kaloper, Phys. Rev. D 60, 123506 (1999); C. Csáki, M. Graesser, C. Kolda, and J. Terning, Phys. Lett. B 462, 34 (1999); J. M. Cline, C. Grojean, and G. Servant, Phys. Rev. Lett. 83, 4245 (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); J. Cline, C. Grojean, and G. Servant, ibid. 472, 302 (2000); P. Kraus, J. High Energy Phys. 11, 9912 (1999); S. Nam, hep-th/9911237; N. Arkani-Hamed, S. Dimopoulos, G. Dvali, and N. Kaloper, hep-ph/9911386; C. Csaki, M. Graesser, L. Randall, and J. Terning, Phys. Rev. D (to be published), hep-ph/9911406; D. Ida, gr-qc/9912002; N. Kaloper, Phys. Lett. B 474, 269 (2000); M. Cvetič and J. Wang, Phys. Rev. D 61, 124020 (2000); S. Mukohyama, T. Shiromizu, and K. Maeda, ibid. 62, 024028 (2000).
13. N. Arkani-Hamed, S. Dimopoulos, N. Kaloper, and J. March Russell, Nucl. Phys. B567, 189 (2000); N. Kaloper, Phys. Rev. D 60, 123506 (1999); C. Csáki, M. Graesser, C. Kolda, and J. Terning, Phys. Lett. B 462, 34 (1999); J. M. Cline, C. Grojean, and G. Servant, Phys. Rev. Lett. 83, 4245 (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); J. Cline, C. Grojean, and G. Servant, ibid. 472, 302 (2000); P. Kraus, J. High Energy Phys. 11, 9912 (1999); S. Nam, hep-th/9911237; N. Arkani-Hamed, S. Dimopoulos, G. Dvali, and N. Kaloper, hep-ph/9911386; C. Csaki, M. Graesser, L. Randall, and J. Terning, Phys. Rev. D (to be published), hep-ph/9911406; D. Ida, gr-qc/9912002; N. Kaloper, Phys. Lett. B 474, 269 (2000); M. Cvetič and J. Wang, Phys. Rev. D 61, 124020 (2000); S. Mukohyama, T. Shiromizu, and K. Maeda, ibid. 62, 024028 (2000).
14. N. Arkani-Hamed, S. Dimopoulos, N. Kaloper, and J. March Russell, Nucl. Phys. B567, 189 (2000); N. Kaloper, Phys. Rev. D 60, 123506 (1999); C. Csáki, M. Graesser, C. Kolda, and J. Terning, Phys. Lett. B 462, 34 (1999); J. M. Cline, C. Grojean, and G. Servant, Phys. Rev. Lett. 83, 4245 (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); J. Cline, C. Grojean, and G. Servant, ibid. 472, 302 (2000); P. Kraus, J. High Energy Phys. 11, 9912 (1999); S. Nam, hep-th/9911237; N. Arkani-Hamed, S. Dimopoulos, G. Dvali, and N. Kaloper, hep-ph/9911386; C. Csaki, M. Graesser, L. Randall, and J. Terning, Phys. Rev. D (to be published), hep-ph/9911406; D. Ida, gr-qc/9912002; N. Kaloper, Phys. Lett. B 474, 269 (2000); M. Cvetič and J. Wang, Phys. Rev. D 61, 124020 (2000); S. Mukohyama, T. Shiromizu, and K. Maeda, ibid. 62, 024028 (2000).
15. N. Arkani-Hamed, S. Dimopoulos, N. Kaloper, and J. March Russell, Nucl. Phys. B567, 189 (2000); N. Kaloper, Phys. Rev. D 60, 123506 (1999); C. Csáki, M. Graesser, C. Kolda, and J. Terning, Phys. Lett. B 462, 34 (1999); J. M. Cline, C. Grojean, and G. Servant, Phys. Rev. Lett. 83, 4245 (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); J. Cline, C. Grojean, and G. Servant, ibid. 472, 302 (2000); P. Kraus, J. High Energy Phys. 11, 9912 (1999); S. Nam, hep-th/9911237; N. Arkani-Hamed, S. Dimopoulos, G. Dvali, and N. Kaloper, hep-ph/9911386; C. Csaki, M. Graesser, L. Randall, and J. Terning, Phys. Rev. D (to be published), hep-ph/9911406; D. Ida, gr-qc/9912002; N. Kaloper, Phys. Lett. B 474, 269 (2000); M. Cvetič and J. Wang, Phys. Rev. D 61, 124020 (2000); S. Mukohyama, T. Shiromizu, and K. Maeda, ibid. 62, 024028 (2000).
16. N. Arkani-Hamed, S. Dimopoulos, N. Kaloper, and J. March Russell, Nucl. Phys. B567, 189 (2000); N. Kaloper, Phys. Rev. D 60, 123506 (1999); C. Csáki, M. Graesser, C. Kolda, and J. Terning, Phys. Lett. B 462, 34 (1999); J. M. Cline, C. Grojean, and G. Servant, Phys. Rev. Lett. 83, 4245 (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); J. Cline, C. Grojean, and G. Servant, ibid. 472, 302 (2000); P. Kraus, J. High Energy Phys. 11, 9912 (1999); S. Nam, hep-th/9911237; N. Arkani-Hamed, S. Dimopoulos, G. Dvali, and N. Kaloper, hep-ph/9911386; C. Csaki, M. Graesser, L. Randall, and J. Terning, Phys. Rev. D (to be published), hep-ph/9911406; D. Ida, gr-qc/9912002; N. Kaloper, Phys. Lett. B 474, 269 (2000); M. Cvetič and J. Wang, Phys. Rev. D 61, 124020 (2000); S. Mukohyama, T. Shiromizu, and K. Maeda, ibid. 62, 024028 (2000).
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