Inflation from tachyon condensation, large N effects

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 69, Issue 10, 2004, Pages

  Majumdar, Mahbub ^a   Davis, Anne Christine ^b  

^a IMPERIAL COLLEGE LONDON   (United Kingdom)

^b UNIVERSITY OF CAMBRIDGE   (United Kingdom)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 3142602951     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.69.103504     Document Type: Article

References (69)

1. J. Polchinski, Phys. Rev. Lett. 75, 4724 (1995).
2. E. Gava, K.S. Narain, and M.H. Sarmadi, Nucl. Phys. B504, 214 (1997).
3. A. Sen, J. High Energy Phys. 06, 007 (1998)
4. J. High Energy Phys.A. Sen08, 010 (1998)
5. J. High Energy Phys.A. Sen08, 012 (1998)
6. A. SenPhys. Lett. B 441, 133 (1998)
7. A. SenJ. High Energy Phys. 09, 023 (1998)
8. A. Senand for reviews see Class. Quantum Grav. 17, 1251 (2000)
9. J.H. Schwarz, “Non-BPS D-Brane Systems,” hep-th/9908144
10. A. Lerda and R. Russo, Int. J. Mod. Phys. A 15, 771 (2000).
11. D. Choudhury, D. Ghoshal, D.P. Jatkar, and S. Panda, Phys. Lett. B 544, 231 (2002)
12. Phys. Lett. BM. Fairbairn and M.H. Tytgat, 546, 1 (2002)
13. Phys. Lett. BG.W. Gibbons, 537, 1 (2002)
14. Phys. Lett. BG. Shiu and I. Wasserman, 541, 6 (2002)
15. Phys. Lett. BA. Frolove, L. Kofman, and A. Starobinsky, 545, 8 (2002)
16. L. Kofman and A. Linde, J. High Energy Phys. 07, 004 (2002)
17. M.C. Bento, O. Bertolami, and A.A. Sen, Phys. Rev. D 67, 063511 (2003)
18. Phys. Rev. DY. Piao, R. Cai, X. Zhang, and Y. Zhang, 66, 121301(R) (2002)
19. Y. Piao, Q. Huang, X. Zhang, and Y. Zhang, Phys. Lett. B 570, 1 (2003)
20. M. Sami, P. Chingangbam, and T. Qureshi, Phys. Rev. D 66, 043530 (2002)
21. M. Sami, hep-th/0301140
22. H.A. Feldman and R.H. Brandenberger, Phys. Lett. B 227, 359 (1989)
23. G.N. Felder, A. Frolov, L. Kofman, and A. Linde, Phys. Rev. D 66, 023507 (2002)
24. Phys. Rev. DZ.K. Guo, Y.S. Piao, R.G. Cai, and Y.Z. Zhang, 68, 043508 (2003).
25. U.H. Danielsson, A. Guijosa, and M. Kruczenski, J. High Energy Phys. 09, 011 (2001).
26. M. Majumdar and A.C. Davis, J. High Energy Phys. 03, 056 (2002).
27. D.H. Lyth, C. Ungarelli, and D. Wands, Phys. Rev. D 67, 023503 (2003).
28. C.B. Netterfield, Astrophys. J. 571, 604 (2002)
29. Astrophys. J.C. Pryke, 568, 46 (2002)
30. R. Stompor, Astrophys. J. Lett. 561, L7 (2001).
31. A. Mazumdar, S. Panda, and A. Perez-Lorenzana, Nucl. Phys. B614, 101 (2001).
32. K. Ohmori, “A Review on Tachyon Condensation in Open String Field Theories,” hep-th/0102085.
33. M.R. Douglas, H. Liu, G. Moore, and B. Zwiebach, J. High Energy Phys. 04, 022 (2002).
34. A. Sen, Int. J. Mod. Phys. A 18, 4869 (2003)
35. A. SenJ. High Energy Phys. 10, 003 (2002)
36. A. SenMod. Phys. Lett. A 17, 1797 (2002)
37. A. SenJ. High Energy Phys. 07, 065 (2002)
38. J. High Energy Phys.A. Sen04, 048 (2002).
39. A.R. Liddle, A. Mazumdar, and F.E. Schunck, Phys. Rev. D 58, 061301 (1998)
40. Phys. Rev. DE.J. Copeland, A. Mazumdar, and N.J. Nunes, 60, 083506 (1999)
41. A. Mazumdar, S. Panda, and A. Perez-Lorenzana, Nucl. Phys. B614, 101 (2001)
42. P. Kanti and K.A. Olive, Phys. Rev. D 60, 043502 (1999)
43. P. KantiK.A. OlivePhys. Lett. B 464, 192 (1999).
44. See, for example, E.P. Shellard and A. Vilenkin, Cosmic Strings and Other Topological Defects (Cambridge University Press, Cambridge, England, 1994)
45. M.B. Hindmarsh and T.W. Kibble, Rep. Prog. Phys. 58, 477 (1995).
46. D. Wands, “Primordial Perturbations from Inflation,” astro-ph/0201541
47. C. Gordon, D. Wands, B.A. Bassett, and R. Maartens, Phys. Rev. D 63, 023506 (2001).
48. A. Frolov, L. Kofman, and A. Starobinsky, Phys. Lett. B 545, 8 (2002)
49. L. Kofman and A. Linde, J. High Energy Phys. 07, 004 (2002)
50. M. Fairbairn and M.H.G. Tytgat, Phys. Lett. B 546, 1 (2002)
51. Phys. Lett. BG. Shiu and I. Wasserman, 541, 6 (2002)
52. G. Felder, L. Kofman, and A. Starobinsky, J. High Energy Phys. 09, 026 (2002)
53. J. High Energy Phys.J. Cline, H. Firouzjahl, and P. Martineau, 11, 041 (2002)
54. C. Kim, H.B. Kim, and Y. Kim, Phys. Lett. B 552, 111 (2003).
55. Y.S. Piao, R.G. Cai, X.M. Zhang, and Y.Z. Zhang, Phys. Rev. D 66, 121301(R) (2002)
56. Phys. Rev. DM. Sami, P. Chingangbam, and T. Qureshi, 66, 043530 (2002)
57. M. Sami, Mod. Phys. Lett. A 18, 691 (2003).
58. A.A. Gerasimov and S.L. Shatashvili, J. High Energy Phys. 10, 034 (2000)
59. J. High Energy Phys.D. Kutasov, M. Marino, and G.W. Moore, 10, 045 (2000)
60. D. KutasovM. MarinoG.W. Moore“Remarks on Tachyon Condensation in Superstring Field Theory,” hep-th/0010108
61. D. Ghoshal and A. Sen, J. High Energy Phys. 11, 021 (2000)
62. J. High Energy Phys.T. Takayanagi, S. Terashima, and T. Uesugi, 03, 019 (2001)
63. P. Kraus and F. Larsen, Phys. Rev. D 63, 106004 (2001)
64. and, for a review, K. Ohmori, “A Review on Tachyon Condensation in Open String Field Theories,” hep-th/0102085.
65. J.A. Minahan and B. Zwiebach, J. High Energy Phys. 03, 038 (2001).
66. S.A. Abel, J.L. Barbon, I.I. Kogan, and E. Rabinovici, J. High Energy Phys. 04, 015 (1999).
67. M. Majumdar and A.C. Davis, J. High Energy Phys. 12, 012 (2003).
68. R. Easther, B.R. Greene, and M.G. Jackson, Phys. Rev. D 66, 023502 (2002).
69. In another vein, see, for example, A. Adams, J. Polchinski, and E. Silverstein, J. High Energy Phys. 10, 029 (2001).