Cited by 872Cosmology and Gravitation TheoriesBlack Holes and Theoretical PhysicsNoncommutative and Quantum Gravity Theories

The pre-big bang scenario in string cosmology

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Gasperini, M., Veneziano, G.·2003·Physics Reports

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  • Each of the other cosmological scenarios (pre-Big-Bang, ekpyrotic/cyclic, Aguirre-Gratton, and Bojowald loop quantum gravity) invokes special low-entropy conditions on some Cauchy surface, either asymptotically in the far past or at some moment of minimum size for the universe.

    “To the best of our understanding, each of these proposals invokes special low-entropy conditions on some Cauchy surface, either asymptotically in the far past or at some moment of minimum size for the universe.”

    From Spontaneous inflation and the origin of the arrow of time (2004) · cites this paper as [94]

    For the pre-big-bang scenario, Section 3 (Initial conditions; page unavailable) describes an initially highly entropic state and proposes that gravitational collapse generates the low-entropy region corresponding to our universe. The paper does impose asymptotic-past-triviality in a simplified model, but it does not describe this as a special low-entropy condition on a Cauchy surface. This source does not establish the claim about the other named scenarios. (LLM, conf=0.86)

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Research works printed but not linked: 272

  1. A. Abramovici et al., Science 256, 325 (1992).
  2. E. J. Ahn, M. Cavaglià and A. Olinto, hep-th/0201042. · arXiv
  3. E. J. Ahn and M. Cavaglià, hep-ph/0205168. · arXiv
  4. K. Akama and H. Terazawa, Gen. Relat. Gravit. 15, 201 (1983).
  5. S. O. Alexeyev, A. V. Toporensky and V. O. Ustiansky, Class. Quant. Grav. 17, 2243 (2000).
  6. B. Allen, in Astrophysical Sources of Gravitational waves, Proc. Les Houches School, 1996, eds. J. A. Marck and J. P. Lasota ( University Press, Cambridge, 1997), p. 373.
  7. E. Alvarez and M. Osorio, Int. J. Theor. Phys. 28, 949 (1989).
  8. L. Amendola, Phys. Rev. D 62, 043511 (2000).
  9. L. Amendola and D. Tocchini-Valentini, Phys. Rev. D 64, 043509 (2001).
  10. I. Antoniadis, in Gravitational Waves and Experimental Gravity, Proc. XXXIV Ren- contres de Moriond, Les Arcs, 1999, eds. J. Tran Thanh Van et al. (World Scientific, Singapore, 2000).
  11. A. Ashtekar and R. Geroch, Rep. Prog. Phys. 37, 1211 (1974).
  12. P. Astone, in Proc. Second Edoardo Amaldi Conference on Gravitational Waves, CERN, 1997, eds. E. Coccia et al. (World Scientific, Singapore, 1998), p. 192.
  13. P. Astone et al., Astron. Astrophys. 351, 811 (1999).
  14. P. Astone et al., in Proc. Second Edoardo Amaldi Conference on Gravitational Waves, CERN, 1997, eds. E. Coccia et al. (World Scientific, Singapore, 1998), p. 551.
  15. P. Astone, J. Lobo and B. Schutz, Classical Quant. Grav. 11, 2093 (1994).
  16. P. Astone, G. Pallottino and G. Pizzella, Classical Quant. Grav. 14, 2019 (1997).
  17. D. Babusci, S. Foffa, G. Losurdo, M. Maggiore, G. Matone and R. Sturani, in Gravi- tational Waves, Proc. SIGRAV School, Centre A. Volta, Como, 1999, eds. I. Ciufolini et al. (IOP Publishing, Bristol, 2001), p. 179.
  18. D. Babusci and M. Giovannini, Classical Quant. Grav. 17, 2621 (2000).
  19. D. Bak and S. Rey, Classical Quant. Grav. 17, L1 (2000).
  20. A. Balbi, C. Baccigalupi, S. Matarrese, F. Perrotta and N. Vittorio, Astrophys. J. 547, L89 (2001).
  21. A. J. Banday et al., Astrophys. J. 475, 393 (1997).
  22. T. Banks, W. Fischler and L. Motl, JHEP 9901, 019 (1999).
  23. J. D. Barrow and K. E. Kunze, Chaos, Soliton Frac. 10, 257 (1999).
  24. B. A. Bassett, Phys. Rev. D 56, 3439 (1997).
  25. J. D. Bekenstein, Int. J. Theor. Phys. 28, 967 (1989).
  26. V. A. Belinskii and I. M. Khalatnikov, Sov. Phys. JETP 36, 591 (1973).
  27. V. A. Belinskii, I. M. Khalatnikov and E. M. Lifshitz, Adv. Phys. 19, 525 (1970).
  28. C. L. Bennet et al., Astrophys. J. 430, 423 (1994).
  29. C. L. Bennet et al., Astrophys. J. 464, L1 (1996).
  30. M. G. Bento and O. Bertolami, Classical Quant. Grav. 12, 1919 (1995).
  31. P. Bernard, G. Gemme, R. Parodi and E. Picasso, Rev. Sci. Instrum. 72, 2428 (2001).
  32. M. Bianchi, M. Brunetti, E. Coccia, F. Fucito and J. A. Lobo, Phys. Rev. D 57, 4525 (1998).
  33. M. Bianchi, E. Coccia, C. Colacino, V. Fafone and F. Fucito, Classical Quant. Grav. 13, 2865 (1996).
  34. A. P. Billyard, A. A. Coley and J. E. Lidsey, J. Math. Phys. 40, 5092 (1999).
  35. A. P. Billyard, A. A. Coley and J. E. Lidsey, Classical Quant. Grav. 17, 453 (2000).
  36. N. D. Birrel and P. C. W. Davies, Quantum fields in curved spaces (University Press, Cambridge, 1982).
  37. H. J. Blome and W. Priester, Astron. Astrophys. 250, 43 (1991).
  38. H. Bondi, M. G. J. van der Burg and A. W. K. Metzner, Proc. Roy. Soc. Lond. A269, 21 (1962).
  39. A. Borde, A. Guth and A. Vilenkin, gr-qc/0110012. · arXiv
  40. A. Borde and A. Vilenkin, Phys. Rev. Lett. 72, 3305 (1994).
  41. R. Bousso, JHEP 9906, 028 (1999).
  42. R. Bousso, JHEP 9907, 004 (1999).
  43. M. J. Bowick, L. Smolin and L. C. R. Wijewardhana, Gen. Relat. Gravit. 19, 113 (1987).
  44. V. Bozza, M. Gasperini, M. Giovannini and G. Veneziano, hep-ph/0206131. · arXiv
  45. V. Bozza and G. Veneziano, JHEP 0010, 35 (2000).
  46. R. Brandenberger, APCTP Bulletin 6 (2001).
  47. R. H. Brandenberger, R. Easther and J. Maia, JHEP 9808, 007 (1998).
  48. R. Brandenberger and F. Finelli, JHEP 0111, 056 (2001).
  49. R. Brandenberger, V. F. Mukhanov and T. Prokopec, Phys. Rev. Lett. 69, 3606 (1992).
  50. M. Bruni, G. F. R. Ellis and P. K. S. Dunsby, Classical Quant. Grav. 9, 921 (1992).
  51. R. Brustein, Chaos, Soliton Frac. 10, 283 (1999).
  52. R. Brustein and R. Madden, JHEP 9907, 006 (1999).
  53. R. Brustein and G. Veneziano, Phys. Rev. Lett. 84, 5695 (2000).
  54. A. Buonanno, M. Gasperini, M. Maggiore and C. Ungarelli, Classical Quant. Grav.14, L97 (1997).
  55. A. Buonanno, K. A. Meissner, C. Ungarelli and G. Veneziano, JHEP 9801, 004 (1998).
  56. E. R. Caianiello, M. Gasperini and G. Scarpetta, Classical Quant. Grav. 8, 659 (1991).
  57. R. R. Caldwell, R. Dave and P. J. Steinhardt, Phys. Rev. Lett. 80, 582 (1998).
  58. B. Caron et al., Classical Quant. Grav. 14, 1461 (1997).
  59. B. J. Carr, Astrophys. J. 201, 1 (1975).
  60. B. J. Carr and S. W. Hawking, Mon. Not. Roy. Astron. Soc. 168, 399 (1974).
  61. C. Cartier, E. J. Copeland and R. Madden, JHEP 0001, 035 (2000).
  62. M. Cavaglià, Classical Quant. Grav. 18, 1355 (2001).
  63. M. Cavaglià and V. De Alfaro, Gen. Relat. Gravit. 29, 773 (1997).
  64. M. Cavaglià and P. V. Moniz, Classical Quant. Grav. 18, 95 (2001).
  65. M. Cavaglià and C. Ungarelli, Classical Quant. Grav. 16, 1401 (1999).
  66. M. Cavaglià and C. Ungarelli, Nucl. Phys. Proc. Suppl. B88, 355 (2000).
  67. M. Cerdonio, L. Conti, J.A. Lobo, A. Ortolan and J. P. Zendri, Phys. Rev. Lett. 87, 031101 (2001).
  68. G. V. Chibisov and V. N. Mukhanov, Mon. Not. Roy. Astron. Soc. 200, 535 (1982)
  69. A. Chincarini, G. Gemme, R. Parodi, P. Bernard and E. Picasso, gr-qc/0203024. · arXiv
  70. M. W. Choptuik, Phys. Rev. Lett. 70, 9 (1993).
  71. D. Christodoulou, Commun. Math. Phys. 105, 337 (1986).
  72. D. Christodoulou, Commun. Math. Phys. 109, 613 (1987).
  73. D. Christodoulou, Commun. Pure Appl. Math. 44, 339 (1991).
  74. D. Christodoulou, Commun. Pure Appl. Math. 46, 11331 (1993).
  75. D. Clancy, J. E. Lidsey and R. Tavakol, Classical Quant. Grav. 15, 257 (1998).
  76. E. Coccia, V. Fafone and I. Modena, Rev. Sci. Instrum. 63, 5432 (1992).
  77. E. J. Copeland, A. R. Liddle, J. E. Lidsey and D. Wands, Gen. Relat. Gravit. 30, 1711 (1998).
  78. A. M. Cruise, Classical Quant. Grav. 17, 2525 (2000).
  79. E. Cuoco, G. Curci and E. Beccaria, in Proc. Second Edoardo Amaldi Conference on Gravitational Waves, CERN, 1997, eds. E. Coccia et al. (World Scientific, Singapore, 1998), p. 524.
  80. T. Damour and M. Henneaux, Phys. Rev. Lett. 85, 920 (2000).
  81. T. Damour and M. Henneaux, Gen. Relat. Gravit. 32, 2339 (2000).
  82. T. Damour and M. Henneaux, Phys. Rev. Lett. 86, 4749 (2001).
  83. T. Damour, F. Piazza and G. Veneziano, gr-qc/0204094. · arXiv
  84. T. Damour, F. Piazza and G. Veneziano, hep-th/0205111. · arXiv
  85. T. Damour and A. M. Polyakov, Gen. Relat. Gravit. 26, 1171 (1994).
  86. T. Damour and A. Vilenkin, Phys. Rev. Lett. 78, 2288 (1997).
  87. P. de Bernardis et al., Nature 404, 955 (2000).
  88. P. de Bernardis et al., Astrophys. J. 564, 559 (2002).
  89. M. Demianski, in Proc. It. Conf. on General Relativity and Gravitational Physics, Capri, 1990, eds. R. Cianci et al. (World Scientific, Singapore, 1991), p. 19.
  90. B. S. De Witt, Phys. Rev. 160, 1113 (1967).
  91. S. Dimopoulos et al., Astrophys. J. 330, 545 (1988).
  92. M. R. Douglas, in Nonperturbative Aspects of Strings, Branes and Supersymmetry, Proc. ICTP Spring School, Trieste, 1998 (World Scientific, Singapore, 1999), p. 131.
  93. R. Durrer, Fundams. Cosm. Phys., 15, 209 (1994).
  94. R. Durrer, J. Phys. Stud. 5, 177 (2001).
  95. R. Durrer and J. Laukenmann, Classical Quant. Grav. 13, 1069 (1996).
  96. R. Durrer and F. Vernizzi, hep-ph/0203275. · arXiv
  97. D. M. Eardley and S. B. Giddings, gr-qc/0201034. · arXiv
  98. D. Easson, hep-th/0111055, in Proc. of the COSMO-01 Workshop, Rovaniemi, 2001. · arXiv
  99. D. A. Easson and R. Brandenberger, JHEP 9909, 003 (1999).
  100. R. Easther and D. A. Lowe, Phys. Rev. Lett. 82, 4967 (1999).
  101. A. Erdelyi, W. Magnus, F. Oberhettinger and F. G. Tricomi, Higher transcendental functions (MacGraw-Hill, New York, 1955), Vol. 3.
  102. A. Feinstein, gr-qc/0106001, in Fourth Mexican School on Gravity and Mathematical Physics, Huatulco, 2000. · arXiv
  103. A. Feinstein, K. E. Kunze and M. A. Vázquez-Mozo, Classical Quant. Grav. 17, 3599 (2000).
  104. E. Fischbach and C. Talmadge, Nature 356, 207 (1992).
  105. W. Fischler and L. Susskind, hep-th/9806039. · arXiv
  106. M. Galluccio, F. Litterio and F. Occhionero, Phys. Rev. Lett. 79, 970 (1997).
  107. M. Gasperini, Phys. Rev. Lett. 56, 2873 (1986).
  108. M. Gasperini, in Proc. Advances in Theoretical Physics, Vietri, 1990, ed.
  109. E. R. Ca- ianiello (World Scientific, Singapore 1991), p. 77.
  110. M. Gasperini, Gen. Relat. Gravit. 24, 219 (1992).
  111. M. Gasperini, in Proc. Second Paris Cosmology Colloquium, Observatoire de Paris, 1994, eds. H. J. de Vega and N. Sanchez (World Scientific, Singapore, 1995), p. 429.
  112. M. Gasperini, in Proc. Birth of the Universe and Fundamental Physics, Rome, 1994, ed. F. Occhionero (Springer, New York, 1995), p. 71.
  113. M. Gasperini, in Proc. Third Paris Cosmology Colloquium, Observatoire de Paris, 1995, eds. H. J. de Vega and N. Sanchez (World Scientific, Singapore, 1996), p. 253.
  114. M. Gasperini, in String Gravity and Physics at the Planck Energy Scale, Proc. Erice School, 1995, eds. N. Sanchez and A. Zichichi (Kluwer Acad. Publ., Dordrecht, 1996), p. 305.
  115. M. Gasperini, in Proc. It. Conf. on General Relativity and Gravitational Physics, Rome, 1996, eds. M. Bassan et al. (World Scientific, Singapore, 1997), p. 181.
  116. M. Gasperini, in String theory in curved space times, ed. N. Sanchez (World Scientific, Singapore 1998), p. 333.
  117. M. Gasperini, in Proc. Fourth Paris Cosmology Colloquium, Observatoire de Paris, 1997, eds. H. J. de Vega and N. Sanchez (World Scientific, Singapore, 1998), p. 85.
  118. M. Gasperini, in Proc. Second Edoardo Amaldi Conference on Gravitational Waves, CERN, 1997, eds. E. Coccia et al. (World Scientific, Singapore, 1998), p. 62.
  119. M. Gasperini, Gen. Relat. Gravit. 30, 1703 (1998).
  120. M. Gasperini, in Proc. Fifth Paris Cosmology Colloquium, Observatoire de Paris, 1998, eds. H. J. de Vega and N. Sanchez (Publications Observatoire de Paris, 1999), p. 317.
  121. M. Gasperini, Classical Quant. Grav. 17, R1 (2000).
  122. M. Gasperini, in Gravitational Waves, Proc. SIGRAV School, Centre A. Volta, Como, 1999), eds. I. Ciufolini et al. (IOP Publishing, Bristol, 2001), p. 280.
  123. M. Gasperini, in Proc. IX Marcel Grossmann Meeting, Rome, 2000, eds. V. G. Gurzadyan, R. Jantzen and R. Ruffini (World Scientific, Singapore, 2002), in press.
  124. M. Gasperini and M. Giovannini, Classical Quant. Grav. 9, L137 (1992).
  125. M. Gasperini and M. Giovannini, Classical Quant. Grav. 10, L133 (1993).
  126. M. Gasperini and M. Giovannini, Classical Quant. Grav. 14, 735 (1997).
  127. M. Gasperini and M. Giovannini, in String theory in curved space times, ed. N. Sanchez (World Scientific, Singapore, 1998), p. 249.
  128. M. Gasperini, M. Giovannini, K. A. Meissner and G. Veneziano, Nucl. Phys. (Proc. Suppl.) B49, 70 (1996).
  129. M. Gasperini, M. Giovannini, K. A. Meissner and G. Veneziano, in String theory in curved space times, ed. N. Sanchez (World Scientific, Singapore, 1998), p. 49.
  130. M. Gasperini, M. Giovannini and G. Veneziano, Phys. Rev. Lett. 75, 3796 (1995).
  131. M. Gasperini and R. Ricci, Classical Quant. Grav. 12, 677 (1995).
  132. M. Gasperini, N. Sanchez and G. Veneziano, Nucl. Phys. B 364, 365 (1991).
  133. M. Gasperini and G. Veneziano, Astropart. Phys. 1, 317 (1993).
  134. M. Gasperini and G. Veneziano, Gen. Rel. Grav. 28, 1301 (1996).
  135. U. Gen, A. Ishibashi and T. Tanaka, hep-th/0110286. · arXiv
  136. M. Giovannini, Teoria quantistica delle perturbazioni in cosmologia di stringa, PhD Thesis (unpublished), University of Turin (1995).
  137. M. Giovannini, H. Kurki-Suonio and E. Sihvola, astro-ph/0203430. · arXiv
  138. A. Giveon, M. Porrati and E. Rabinovici, Phys. Rep. 244, 77 (1994).
  139. M. B. Green, J. Schwartz and E. Witten, Superstring theory (University Press, Cam- bridge, 1987).
  140. L. P. Grishchuk, Sov. Phys. JETP 40, 409 (1975).
  141. L. P. Grishchuk, Sov. Phys. Usp. 31, 490 (1988).
  142. L. P. Grishchuk, Sov. Sci. Rev. E. Astrophys. Space Phys. 7, 267 (1988).
  143. L. P. Grishchuk, in Squeezed states and uncertainty relations, eds. D. Han et al. (NASA Conf. Pub. N. 31353, 1992), p. 329.
  144. L. P. Grishchuk, in Proc. 6th Marcel Grossmann Meeting, Kyoto, 1991, ed.
  145. H. Sato (World Scientific, Singapore, 1992).
  146. L. P. Grishchuk, in Gravitational Waves and Experimental Gravity, Proc. XXXIV Rencontres de Moriond, Les Arcs, 1999, eds. J. Tran Thanh Van et al. (World Scien- tific, Singapore, 2000).
  147. L. P. Grishchuk and Y. V. Sidorov, Classical Quant. Grav. 6, L161 (1989).
  148. W. Hamilton, in Proc. Second Edoardo Amaldi Conference on Gravitational Waves, CERN, 1997, eds. E. Coccia et al. (World Scientific, Singapore, 1998), p. 115.
  149. A. Hammesfahr, Classical Quant. Grav. 18, 4045 (2001).
  150. S. Hanany et al., Astrophys. J. 545, L5 (2000).
  151. E. R. Harrison, Phys. Rev. Lett. 30, 188 (1973).
  152. S. W. Hawking, Astrophys. J. 145, 544 (1966).
  153. S. W. Hawking, Commun. Math. Phys. 43, 199 (1975).
  154. S. W. Hawking and G. F. R. Ellis, The large scale structure of spacetime (University Press, Cambridge, 1973).
  155. S. W. Hawking and R. Penrose, Proc. Roy. Soc. Lond. A314, 529 (1970).
  156. A. Hebecker and C. Wetterich, Phys. Rev. Lett. 85, 3339 (2000).
  157. I. Heng, D. Blair, E. Ivanov and M. Tobar, in Proc. Second Edoardo Amaldi Confer- ence on Gravitational Waves, CERN, 1997, eds. E. Coccia et al. (World Scientific, Singapore, 1998), p. 127.
  158. G. 't Hooft, in Abdus Salam Festschrift: A Collection of Talks, eds. A. Ali , J. Ellis and S. Randjbar-Daemi (World Scientific, Singapore, 1993).
  159. K. Hotta, K. Kikkawa and H. Kunitomo, Prog. Theor. Phys. 98, 687 (1997).
  160. J. Hough, in Proc. Second Edoardo Amaldi Conference on Gravitational waves, CERN, 1997, eds. E. Coccia et al. (World Scientific, Singapore, 1998), p. 97.
  161. C. D. Hoyle, U. Schmidt, B. R. Heckel, E. G. Adelberger, J. H. Gundlach, D. J. Kapner and H. E. Swanson, Phys. Rev. Lett. 86, 1418 (2001).
  162. J. H. Hwang, Astrophys. J. 375, 443 (1991).
  163. J. H. Hwang, Astropart. Phys. 8, 201 (1998).
  164. J. H. Hwang and E. T. Vishniac, Astrophys. J. 382, 363 (1991).
  165. W. Johnson and S. Merkowitz, Phys. Rev. Lett. 70, 2367 (1993).
  166. T. Kajita and Y. Totsuka, Rev. Mod. Phys. 73, 85 (2001).
  167. N. Kaloper and K. A. Olive, Astropart. Phys. 1, 185 (1993).
  168. M. Kamionkowski, A. Kosowsky and A. Stebbins, Phys. Rev. Lett. 78, 2058 (1997).
  169. V. Kaplunovsky, Phys. Rev. Lett. 55, 1036 (1985).
  170. V. Kaspi, J. Taylor and M. Ryba, Astrophys. J. 428, 713 (1994).
  171. K. Kawabe and the TAMA collaboration, Classical Quant. Grav. 14, 1477 (1997).
  172. K. Kim, Phys. Rev. Lett. 43, 103 (1979).
  173. E. Kiritsis and C. Kounnas, in Proc. Second Paris Cosmology Colloquium, Observa- toire de Paris, 1994, eds. H. J. De Vega and N. Sanchez (World Scientific, Singapore, 1995), p. 500.
  174. E. Kohlprath and G. Veneziano, gr-qc/0203093. · arXiv
  175. E. W. Kolb and M. S. Turner, The Early Universe (Addison-Wesley, Redwood City, CA, 1990).
  176. L. M. Krauss and M. White, Phys. Rev. Lett. 69, 869 (1992).
  177. K. E. Kunze, Classical Quant. Grav. 16, 3795 (1999).
  178. K. E. Kunze and R. Durrer, Classical Quant. Grav. 17, 2597 (2000).
  179. L. Landau and E. Lifshitz, The classical theory of fields (Pergamon Press, Oxford, 1962).
  180. A. Lawrence and E. Martinec, Classical Quant. Grav. 13, 63 (1996).
  181. J. Lesgourgues, D. Polarski, S. Prunet and A. A. Starobinski, Astron. Astrophys. 359, 414 (2000).
  182. A. R. Liddle and D. H. Lyth, Phys. Rep. 231, 1 (1993).
  183. J. E. Lidsey, Classical Quant. Grav. 15, L77 (1999).
  184. J. E. Lidsey, D. Wands and E. J. Copeland, Phys. Rep. 337, 343 (2000).
  185. E. M. Lifchitz and I. M. Kalatnikov, Adv. Phys. 12, 185 (1963).
  186. A. D. Linde, Sov. Phys. JETP 60, 211 (1984).
  187. H. Luck and the GEO600 Team, Classical Quant. Grav. 14, 1741 (1997).
  188. V. N. Lukash, Sov. Phys. JETP 52, 807 (1980).
  189. R. Madden, JHEP 0101, 23 (2001).
  190. M. Maggiore, Phys. Rep. 331, 283 (2000).
  191. J. Maharana, E. Onofri and G. Veneziano, JHEP 9804, 004 (1998).
  192. X. Martin and A. Vilenkin, Phys. Rev. Lett. 77, 2879 (1996).
  193. J. Marto and P. V. Moniz, in Proc. IX Marcel Grossmann Meeting, Rome, 2000, eds.
  194. V. G. Gurzadyan, R. Jantzen and R. Ruffini (World Scientific, Singapore, 2002), in press.
  195. P. Mauskopf et al., Astrophys. J. 536, L59 (2000).
  196. A. Melchiorri, F. Vernizzi, R. Durrer and G. Veneziano, Phys. Rev. Lett. 83, 4464 (1999).
  197. A. D. Miller et al., Astrophys. J. 524, L1 (1999).
  198. A. G. Mirzabekian and G. A. Vilkovisky, Classical Quant. Grav. 12, 2173 (1995).
  199. T. Moroi and T. Takahashi, hep-ph/0206026. · arXiv
  200. V. F. Mukhanov, Sov. Phys. JETP 67, 1297 (1988).

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Authors
Gasperini, M., & Veneziano, G.
Affiliations
  • Istituto Nazionale di Fisica Nucleare, Sezione di Bari (IT)
  • European Organization for Nuclear Research (CH)
Corresponding author
Veneziano, G.
Venue
Physics Reports
Publisher
Elsevier BV
Published
2003-01
Volume
373
Issue
1-2
Pages
1-212
ISSN
0370-1573 (ISSN-L)
OpenAlex
W2159692634
Cited by
872
References
16
Citations by year
2026: 16 · 2025: 46 · 2024: 29 · 2023: 23 · 2022: 23 · 2021: 26 · 2020: 33 · 2019: 45 · 2018: 44 · 2017: 23 · 2016: 39 · 2015: 21 · 2014: 41 · 2013: 32 · 2012: 30
FWCI
27.51
Type
journal article
Language
en
Open access
Locations
  • Physics Reports (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • CERN Document Server (European Organization for Nuclear Research) (submittedVersion)
  • CINECA IRIS Institutional Research Information System (University of Bari Aldo Moro) (submittedVersion)
  • arXiv (Cornell University)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
  • Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Black Holes and Theoretical Physics
  • Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Noncommutative and Quantum Gravity Theories
Keywords
pre-big bang scenario, string cosmology, superstring cosmology, early universe, phenomenological consequences, open problems

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