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宇宙のインフレーション
出典: フリー百科事典『ウィキペディア（Wikipedia）』 (2012/05/18 23:47 UTC 版)
(インフレーション宇宙論 から転送)
宇宙のインフレーション（うちゅうのインフレーション、cosmic inflation）とは、極初期宇宙に宇宙が加速的急膨張を引き起こすことにより、ビッグバン理論のいくつかの問題を一挙に解決する初期宇宙の進化モデルである。- ^ K. Sato, "First-order phase transition of a vacuum and the expansion of the Universe", Monthly Notices of Royal Astronomical Society, 195, 467, (1981).
- ^ A. H. Guth, "The Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems", Phys. Rev. D 23, 347 (1981).
- ^ de Sitter, Willem (1917). “Einstein's theory of gravitation and its astronomical consequences. Third paper”. Monthly Notices of the Royal Astronomical Society 78: 3–28.
- ^ Starobinsky, A. A. - Spectrum Of Relict Gravitational Radiation And The Early State Of The Universe - JETP Lett. 30, 682 (1979) {Pisma Zh. Eksp. Teor. Fiz. 30, 719 (1979)}.
- ^ Starobinsky, Alexei A. (1980). “A new type of isotropic cosmological models without singularity”. Phys. Lett. B91: 99–102.
- ^ Kazanas, D. (1980). “Dynamics of the universe and spontaneous symmetry breaking”. Astrophys. J. 241: L59–63. doi:10.1086/183361.
- ^ Sato, K. (1981). “Cosmological baryon number domain structure and the first order phase transition of a vacuum”. Phys. Lett. B33: 66–70.
- ^ Einhorn, Martin B (1981). “Monopole Production In The Very Early Universe In A First Order Phase Transition”. Nucl. Phys. B180: 385–404. doi:10.1016/0550-3213(81)90057-2.
- ^ A. H. Guth, "The Inflationary Universe", Perseus Books Group, (1998), ISBN 0201328402. ; アラン・H・グース、『なぜビッグバンは起こったか』, 早川書房, (1999), ISBN 4152082283.
- ^ A. 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).
- ^ A. Albrecht and P. J. Steinhardt, "Cosmology For Grand Unified Theories With Radiatively Induced Symmetry Breaking," Phys. Rev. Lett. 48, 1220 (1982).
- ^ J. M. Bardeen, P. J. Steinhardt and M. S. Turner, "Spontaneous Creation Of Almost Scale-Free Density Perturbations In An Inflationary Universe," Phys. Rev. D 28, 679 (1983).
- ^ See Linde (1990) and Mukhanov (2005).
- ^ Mukhanov, Viatcheslav F. (1981). “Quantum fluctuation and "nonsingular" universe”. JETP Lett. 33: 532–5.
- ^ Mukhanov, Viatcheslav F. (1982). “The vacuum energy and large scale structure of the universe”. Sov. Phys. JETP 56: 258–65.
- ^ See Guth (1997) for a popular description of the workshop, or The Very Early Universe, ISBN 0521316774 eds Hawking, Gibbon & Siklos for a more detailed report
- ^ Hawking, S.W. (1982). “The development of irregularities in a single bubble inflationary universe”. Phys.Lett. B115: 295.
- ^ Starobinsky, Alexei A. (1982). “Dynamics of phase transition in the new inflationary universe scenario and generation of perturbations”. Phys. Lett. B117: 175–8.
- ^ Guth, A.H. (1982). “Fluctuations in the new inflationary universe”. Phys. Rev. Lett. 49: 1110–3. doi:10.1103/PhysRevLett.49.1110.
- ^ Bardeen, James M. (1983). “Spontaneous creation Of almost scale-free density perturbations in an inflationary universe”. Phys. Rev. D28: 679.
- ^ A. Linde, "Eternal chaotic inflation", Mod. Phys. Lett., A1, 81, (1986).
- ^ A. Linde, "Eternally existing self-reproducing chaotic inflationary universe", Phys. Lett., B175, 395, (1986).
- ^ A. Borde, A. Guth and A. Vilenkin, "Inflationary space-times are incomplete in past directions", Phys. Rev. Lett., 90, 151301, (2003).
- ^ A. Borde, "Open and closed universes, initial singularities and inflation", Phys. Rev., D50, 3692, (1994).
- ^ A. Borde and A. Vilenkin, "Eternal inflation and the initial singularity", Phys. Rev. Lett., 72, 3305, (1994).
- ^ A. Linde, "Inflation and String Cosmology," eConf C040802 (2004) L024; J.Phys.Conf.Ser. 24 (2005) 151-160 (available from [1].
- ^ Anthony Aguirre, Steven Gratton, "Steady-State Eternal Inflation", Phys.Rev., D65, 083507, (2002). [2]
- ^ http://arxiv.org/abs/hep-ph/0101119
[続きの解説]
「宇宙のインフレーション」の続きの解説一覧
- 1 宇宙のインフレーションとは
- 2 宇宙のインフレーションの概要
- 3 観測
- 4 その後
宇宙のインフレーションに関係した商品
- 宇宙の創成と進化楽天ブックス
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