宇宙のインフレーション
[Wikipedia|▼Menu]
□記事を途中から表示しています
[最初から表示]

参考文献^ 小松英一郎「小松英一郎が語る 絞られてきたモデル」『日経サイエンス』第47巻第6号、日経サイエンス社、2017年、30頁。 
^ 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).
^Robert H. Brandenberger Challenges for Inflationary Cosmology
^ 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].

次ページ
記事の検索
おまかせリスト
▼オプションを表示
ブックマーク登録
mixiチェック!
Twitterに投稿
オプション/リンク一覧
話題のニュース
列車運行情報
暇つぶしWikipedia

Size:60 KB
出典: フリー百科事典『ウィキペディア(Wikipedia)
担当:undef