Inflation in models with large extra dimension driven by a bulk scalar field

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 62, Issue 10, 2000, Pages 1-6

  Mohapatra, R N ^a   Perez Lorenzana A ^a,b   Pires, C A D S ^a  

^a Bldg 142   (United States)

^b DEPARTAMENTO DE FÍSICA   (Mexico)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 17044423804     PISSN: 05562821     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevD.62.105030     Document Type: Article

References (58)

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47. See for instance P. Binetruy, C. Deffayet, and D. Langlois, Nucl. Phys. B565, 269 (2000); P. Binetruy et al., Phys. Lett. B 477, 285 (2000); J. M. Cline, C. Grojean, and G. Servant, Phys. Rev. Lett. 83, 4245 (1999); P. Kanti et al., Phys. Lett. B 468, 31 (1999); R. N. Mohapatra, A. Pérez-Lorenzana, and C. A. de S. Pires, hep-ph/0003328; C. Barcelo and M. Visser, Phys. Lett. B 482, 183 (2000); V. Barger, T. Han, T. Li, J. D. Lykken, and D. Marfatia, ibid. 488, 97 (2000); P. Kanti, I. I. Kogan, K. A. Olive, and M. Pospelov, ibid. 468, 31 (1999); Phys. Rev. D 61, 106004 (2000); P. Kanti, K. A. Olive, and M. Pospelov, ibid. (to be published), hep-ph/0005146.
48. See for instance P. Binetruy, C. Deffayet, and D. Langlois, Nucl. Phys. B565, 269 (2000); P. Binetruy et al., Phys. Lett. B 477, 285 (2000); J. M. Cline, C. Grojean, and G. Servant, Phys. Rev. Lett. 83, 4245 (1999); P. Kanti et al., Phys. Lett. B 468, 31 (1999); R. N. Mohapatra, A. Pérez-Lorenzana, and C. A. de S. Pires, hep-ph/0003328; C. Barcelo and M. Visser, Phys. Lett. B 482, 183 (2000); V. Barger, T. Han, T. Li, J. D. Lykken, and D. Marfatia, ibid. 488, 97 (2000); P. Kanti, I. I. Kogan, K. A. Olive, and M. Pospelov, ibid. 468, 31 (1999); Phys. Rev. D 61, 106004 (2000); P. Kanti, K. A. Olive, and M. Pospelov, ibid. (to be published), hep-ph/0005146.
49. See for instance P. Binetruy, C. Deffayet, and D. Langlois, Nucl. Phys. B565, 269 (2000); P. Binetruy et al., Phys. Lett. B 477, 285 (2000); J. M. Cline, C. Grojean, and G. Servant, Phys. Rev. Lett. 83, 4245 (1999); P. Kanti et al., Phys. Lett. B 468, 31 (1999); R. N. Mohapatra, A. Pérez-Lorenzana, and C. A. de S. Pires, hep-ph/0003328; C. Barcelo and M. Visser, Phys. Lett. B 482, 183 (2000); V. Barger, T. Han, T. Li, J. D. Lykken, and D. Marfatia, ibid. 488, 97 (2000); P. Kanti, I. I. Kogan, K. A. Olive, and M. Pospelov, ibid. 468, 31 (1999); Phys. Rev. D 61, 106004 (2000); P. Kanti, K. A. Olive, and M. Pospelov, ibid. (to be published), hep-ph/0005146.
50. See for instance P. Binetruy, C. Deffayet, and D. Langlois, Nucl. Phys. B565, 269 (2000); P. Binetruy et al., Phys. Lett. B 477, 285 (2000); J. M. Cline, C. Grojean, and G. Servant, Phys. Rev. Lett. 83, 4245 (1999); P. Kanti et al., Phys. Lett. B 468, 31 (1999); R. N. Mohapatra, A. Pérez-Lorenzana, and C. A. de S. Pires, hep-ph/0003328; C. Barcelo and M. Visser, Phys. Lett. B 482, 183 (2000); V. Barger, T. Han, T. Li, J. D. Lykken, and D. Marfatia, ibid. 488, 97 (2000); P. Kanti, I. I. Kogan, K. A. Olive, and M. Pospelov, ibid. 468, 31 (1999); Phys. Rev. D 61, 106004 (2000); P. Kanti, K. A. Olive, and M. Pospelov, ibid. (to be published), hep-ph/0005146.
51. See for instance P. Binetruy, C. Deffayet, and D. Langlois, Nucl. Phys. B565, 269 (2000); P. Binetruy et al., Phys. Lett. B 477, 285 (2000); J. M. Cline, C. Grojean, and G. Servant, Phys. Rev. Lett. 83, 4245 (1999); P. Kanti et al., Phys. Lett. B 468, 31 (1999); R. N. Mohapatra, A. Pérez-Lorenzana, and C. A. de S. Pires, hep-ph/0003328; C. Barcelo and M. Visser, Phys. Lett. B 482, 183 (2000); V. Barger, T. Han, T. Li, J. D. Lykken, and D. Marfatia, ibid. 488, 97 (2000); P. Kanti, I. I. Kogan, K. A. Olive, and M. Pospelov, ibid. 468, 31 (1999); Phys. Rev. D 61, 106004 (2000); P. Kanti, K. A. Olive, and M. Pospelov, ibid. (to be published), hep-ph/0005146.
52. See for instance P. Binetruy, C. Deffayet, and D. Langlois, Nucl. Phys. B565, 269 (2000); P. Binetruy et al., Phys. Lett. B 477, 285 (2000); J. M. Cline, C. Grojean, and G. Servant, Phys. Rev. Lett. 83, 4245 (1999); P. Kanti et al., Phys. Lett. B 468, 31 (1999); R. N. Mohapatra, A. Pérez-Lorenzana, and C. A. de S. Pires, hep-ph/0003328; C. Barcelo and M. Visser, Phys. Lett. B 482, 183 (2000); V. Barger, T. Han, T. Li, J. D. Lykken, and D. Marfatia, ibid. 488, 97 (2000); P. Kanti, I. I. Kogan, K. A. Olive, and M. Pospelov, ibid. 468, 31 (1999); Phys. Rev. D 61, 106004 (2000); P. Kanti, K. A. Olive, and M. Pospelov, ibid. (to be published), hep-ph/0005146.
53. See for instance P. Binetruy, C. Deffayet, and D. Langlois, Nucl. Phys. B565, 269 (2000); P. Binetruy et al., Phys. Lett. B 477, 285 (2000); J. M. Cline, C. Grojean, and G. Servant, Phys. Rev. Lett. 83, 4245 (1999); P. Kanti et al., Phys. Lett. B 468, 31 (1999); R. N. Mohapatra, A. Pérez-Lorenzana, and C. A. de S. Pires, hep-ph/0003328; C. Barcelo and M. Visser, Phys. Lett. B 482, 183 (2000); V. Barger, T. Han, T. Li, J. D. Lykken, and D. Marfatia, ibid. 488, 97 (2000); P. Kanti, I. I. Kogan, K. A. Olive, and M. Pospelov, ibid. 468, 31 (1999); Phys. Rev. D 61, 106004 (2000); P. Kanti, K. A. Olive, and M. Pospelov, ibid. (to be published), hep-ph/0005146.
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