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dc.contributor.author袁珮閎en_US
dc.contributor.authorYuan, Pei-Hungen_US
dc.contributor.author高文芳en_US
dc.date.accessioned2014-12-12T01:50:16Z-
dc.date.available2014-12-12T01:50:16Z-
dc.date.issued2010en_US
dc.identifier.urihttp://140.113.39.130/cdrfb3/record/nctu/#GT079827517en_US
dc.identifier.urihttp://hdl.handle.net/11536/47696-
dc.description.abstract在本篇論文裡,除了考慮以往的幾何項和宇宙常數之外,更加入了超弦與超重力裡的 Kalb-Romand field 和 Chern-Simons terms ,藉由這樣的有效模型而嘗試去探討在極早期宇宙的現象。我們將深入的探討 Lorentz-Chern-Simons 交互作用項對 de Sitter 宇宙演化的影響,首先我們要求在de Sitter度規之下必須要是有解而且穩定存在的,論文中也仔細研究 LCS 作用項在 Bianchi type I 宇宙演化中所扮演的角色,並在論文中檢驗宇宙無毛定理的有效性。zh_TW
dc.description.abstractIn this thesis, not only considering the geometric term with cosmological constant, but added the Kalb-Romand field and Chern-Simons terms. By using this effectively action model to realize the very early universe. The cosmological evolution of the de Sitter space in the presence of the Lorentz-Chern-Simons terms is studied in details. We also try to study the effect of the LCS terms in the Bianchi type I space. No-hair conjecture is also checked carefully in this thesis.en_US
dc.language.isozh_TWen_US
dc.subject早期宇宙zh_TW
dc.subject暴脹zh_TW
dc.subjectLorentz Chern-Simonsen_US
dc.subjectde Sitteren_US
dc.titlede Sitter 時空與 Lorentz Chern-Simons 項zh_TW
dc.titlede Sitter space and Lorentz Chern-Simons termen_US
dc.typeThesisen_US
dc.contributor.department物理研究所zh_TW
Appears in Collections:Thesis