Contents Previous

REFERENCES

  1. A. H. Guth, "The inflationary universe: A possible solution to the horizon and flatness problems," Phys. Rev. D 23, 347 (1981).
  2. A. D. Linde, "A new inflationary universe scenario: A possible solution of the horizon, flatness, homogeneity, isotropy and primordial monopole problems," Phys. Lett. B 108, 389 (1982).
  3. A. Albrecht, P. J. Steinhardt, "Cosmology for grand unified theories with radiatively induced symmetry breaking," Phys. Rev. Lett. 48, 1220 (1982).
  4. A. D. Linde, Particle Physics and Inflationary Cosmology (Harwood, Philadelphia, 1990).
  5. E. W. Kolb, M. S. Turner, The Early Universe (Addison-Wesley, Reading, MA, 1990).
  6. A. R. Liddle, D. H. Lyth, Cosmological Inflation and Large-Scale Structure (Cambridge Univ. Press, New York, 2000).
  7. A. H. Guth, The Inflationary Universe: The Quest for a New Theory of Cosmic Origins (Addison-Wesley, Reading, MA, 1997).
  8. R. C. Tolman, "Possibilities in relativistic thermodynamics for irreversible processes without exhaustion of free energy," Phys. Rev. 39, 320 (1932).
  9. D. H. Lyth, A. Riotto, "Particle physics models of inflation and the cosmological density perturbation," Phys. Rep. 314, 1 (1999) [arXiv: hep-ph/9807278].
  10. M. Tegmark et al., "Cosmological parameters from SDSS and WMAP," Phys. Rev. D 69, 103501 (2004) [arXiv: astro-ph/0310723].
  11. D. J. Fixsen et al., "The cosmic microwave background spectrum from the full COBE FIRAS data set," Astrophys. J. 473, 576 (1996) [arXiv: astro-ph/9605054].
  12. D. N. Spergel et al., "First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Determination of cosmological parameters," Astrophys. J. Suppl. 148, 175 (2003) [arXiv: astro-ph/0302209].
  13. For a review, see V. F. Mukhanov, H. A. Feldman, R. H. Brandenberger, "Theory of cosmological perturbations," Phys. Rep. 215, 203 (1992) and also [6].
  14. For a review, see R. P. Kirshner, "Throwing light on dark energy," Science 300, 1914 (2003).
  15. A. Vilenkin, E. P. S. Shellard, Cosmic Strings and other Topological Defects (Cambridge Univ. Press, New York, 1994).
  16. U.-L. Pen, U. Seljak, N. Turok, "Power spectra in global defect theories of cosmic structure formation," Phys. Rev. Lett. 79, 1611 (1997) [arXiv: astro-ph/9704165].
  17. For a review, see J. Polchinski, "Introduction to cosmic F- and D-strings," arXiv: hep-th/0412244.
  18. We thank Max Tegmark for providing this graph, which shows the most precise data points for each range of ell from recent observations, as summarized in [10]. The cosmic string prediction is taken from [16]. The other curves were all calculated for ns = 1, Omegabaryon = 0.05, and H = 70 km s-1 Mpc-1, with the remaining parameters fixed as follows. "Inflation with Lambda": OmegaDM(dark matter) = 0.23, OmegaLambda = 0.72, and optical depth parameter tau = 0.17; "Inflation without Lambda": OmegaDM = 0.95, OmegaLambda = 0, tau = 0.06; "Open universe": OmegaDM = 0.25, OmegaLambda = 0, tau = 0.06. The 1-SD error bars include both observational uncertainty and "cosmic variance," the intrinsic quantum uncertainty in the predictions, as calculated from the "Inflation with Lambda" model. With our current ignorance of the underlying physics, none of these theories predicts the overall amplitude of the fluctuations; the "Inflation with Lambda" curve was normalized for a best fit, and the others were normalized arbitrarily.
  19. P. J. Steinhardt, "Natural inflation", in The Very Early Universe, G. W. Gibbons, S. W. Hawking, S. T. C. Siklos, Eds. (Cambridge Univ. Press, New York, 1983), p. 251.
  20. A. Vilenkin, "The birth of inflationary universes," Phys. Rev. D 27, 2848 (1983).
  21. A. D. Linde, "Eternally existing self-reproducing chaotic inflationary universe," Phys. Lett. B 175, 395 (1986).
  22. For a review, see A. H. Guth, "Inflation and eternal inflation," Phys. Rep. 333-334, 555 (2000) [arXiv: astro-ph/0002156].
  23. A. Borde, A. H. Guth, A. Vilenkin, "Inflationary space-times are incomplete in past directions," Phys. Rev. Lett. 90, 151301 (2003) [arXiv: gr-qc/0110012].
  24. L. A. Kofman, A. D. Linde, A. A. Starobinsky, "Reheating after inflation," Phys. Rev. Lett. 73, 3195 (1994) [arXiv: hep-th/9405187].
  25. Y. Shtanov, J. H. Traschen, R. H. Brandenberger, "Universe reheating after inflation," Phys. Rev. D 51, 5438 (1995) [arXiv: hep-ph/9407247].
  26. D. Boyanovsky, H. J. de Vega, R. Holman, D. S. Lee, A. Singh, "Dissipation via particle production in scalar field theories", Phys. Rev. D 51, 4419 (1995) [arXiv: hep-ph/9408214].
  27. D. I. Kaiser, "Post-inflation reheating in an expanding universe," Phys. Rev. D 53, 1776 (1996) [arXiv: astro-ph/9507108].
  28. For a review, see L. A. Kofman, "Preheating after inflation", in COSMO-97: Proceedings, L. Roszkowski, Ed. (World Scientific, Singapore, 1998), pp. 312-321 [arXiv: astro-ph/9802221].
  29. B. A. Bassett, D. I. Kaiser, R. Maartens, "General relativistic effects in preheating," Phys. Lett. B 455, 84 (1999) [arXiv: hep-ph/9808404].
  30. Clifford Will, Theory and Experiment in Gravitational Physics (Cambridge Univ. Press, New York, ed. 2, 1993).
  31. C. D. Hoyle et al., "Sub-millimeter tests of the gravitational inverse-square law," Phys. Rev. D 70, 042004 (2004) [arXiv: hep-ph/0405262].
  32. See, for example, J. Polchinski, String Theory (Cambridge Univ. Press, New York, 1998), vol. 1.
  33. N. Arkani-Hamed, S. Dimopoulos, G. Dvali, "The hierarchy problem and new dimensions at a millimeter," Phys. Lett. B 429, 263 (1998) [arXiv: hep-ph/9803315].
  34. L. Randall, R. Sundrum, "An alternative to compactification," Phys. Rev. Lett. 83, 4690 (1999) [arXiv: hep-th/9906064].
  35. For a review, see L. Randall, "Extra dimensions and warped geometries," Science 296, 1422 (2002).
  36. J. Garriga, T. Tanaka, "Gravity in the Randall-Sundrum brane world," Phys. Rev. Lett. 84, 2778 (2000) [arXiv: hep-th/9911055].
  37. S. B. Giddings, E. Katz, L. Randall, "Linearized gravity in brane backgrounds," J. High Energy Phys. 3, 23 (2000) [arXiv: hep-th/0002091].
  38. P. Binetruy, C. Deffayet, D. Langlois, "Non-conventional cosmology from a brane universe," Nucl. Phys. B 565, 269 (2000) [arXiv: hep-th/9905012].
  39. R. Maartens, D. Wands, B. A. Bassett, I. P. C. Heard, "Chaotic inflation on the brane," Phys. Rev. D 62, 041301 (2000) [arXiv: hep-ph/9912464].
  40. For a review, see D. Langlois, "Gravitation and cosmology in brane-worlds," arXiv: gr-qc/0410129.
  41. F. Quevedo, "Lectures on string/brane cosmology," Class. Quant. Grav. 19, 5721 (2002) [arXiv: hep-th/0210292].
  42. A. D. Linde, "Prospects of inflation," arXiv: hep-th/0402051.
  43. C. P. Burgess, "Inflationary string theory?," Pramana 63, 1269 (2004) [arXiv: hep-th/0408037].
  44. G. R. Dvali, S.-H. H. Tye, "Brane inflation," Phys. Lett. B 450, 72 (1999) [arXiv: hep-ph/9812483].
  45. S. Kachru, R. Kallosh, A. Linde, S. P. Trivedi, "De Sitter vacua in string theory," Phys. Rev. D 68, 046005 (2003) [arXiv: hep-th/0301240].
  46. S. Kachru, R. Kallosh, A. Linde, J. Maldacena, L. McAllister, and S. P. Trivedi, "Towards inflation in string theory," J. Cosmol. Astropart. Phys. 10, 013 (2003) [arXiv: hep-th/0308055].
  47. N. Iizuka, S. P. Trivedi, "An inflationary model in string theory," Phys. Rev. D 70, 043519 (2004) [arXiv: hep-th/0403203].
  48. R. Bousso, J. Polchinski, "Quantization of four-form fluxes and dynamical neutralization of the cosmological constant," J. High Energy Phys. 0006, 006 (2000) [arXiv: hep-th/0004134].
  49. L. Susskind, "The anthropic landscape of string theory," arXiv: hep-th/0302219.
  50. R. Bousso, J. Polchinski, "The string theory landscape," Sci. Am. 291, 60 (Sept. 2004).
  51. A. D. Linde, D. Linde, A. Mezhlumian, "Do we live in the center of the world?," Phys. Lett. B 345, 203-210 (1995) [arXiv: hep-th/9411111].
  52. See, for example, J. Garriga, A. Vilenkin, "A prescription for probabilities in eternal inflation," Phys. Rev. D 64, 023507 (2001) [arXiv: gr-qc/0102090], and also [53].
  53. M. Tegmark, "What does inflation really predict?" arXiv: astro-ph/0410281.
  54. S. Weinberg, "Anthropic bound on the cosmological constant," Phys. Rev. Lett. 59, 2607 (1987).
  55. T. Banks, M. Dine, E. Gorbatov, "Is there a string theory landscape?" J. High Energy Phys. 0408, 058 (2004) [arXiv: hep-th/0309170].
  56. For a review, see J. P. Ostriker, P. Steinhardt, "New light on dark matter," Science 300, 1909 (2003) [arXiv: astro-ph/0306402].

Contents Previous