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dc.contributor.author黃宣翰en_US
dc.contributor.authorHuang, Hsuan-Hanen_US
dc.contributor.author高文芳en_US
dc.contributor.authorKao, Win-Funen_US
dc.date.accessioned2014-12-12T01:31:04Z-
dc.date.available2014-12-12T01:31:04Z-
dc.date.issued2009en_US
dc.identifier.urihttp://140.113.39.130/cdrfb3/record/nctu/#GT079627525en_US
dc.identifier.urihttp://hdl.handle.net/11536/42705-
dc.description.abstract觀測的證據顯示我們的宇宙正在膨脹,宇宙學家隨即引入帶有膨脹解的宇宙模型。根據無毛定理的猜想:只有均向膨脹的 de sitter宇宙才是穩定的時空,因此所有非均向膨脹解必然都不穩定。在早期宇宙的研究中,宇宙模型須考慮高階修正項,修正後卻可能得到不一樣的非均向膨脹解。本論文將呈現一些已知的 Bianchi type I 膨脹解,並介紹這些非均向膨脹解是不穩定的證明,這樣的結論說明這些模型符合無毛定理預期的結果。zh_TW
dc.description.abstractAccording to the observation evidences, our universe is an expanding de Sitter space. As a result, many different models have been studied as a natural source of the expanding universe. In particular, higher order corrections terms may be important in the evolution of the early universe. In addition, Gibbons and Hawking come up with the No Hair theorem claiming that the de Sitter solution is the only stable expanding solution. Review on the anisotropically expanding solutions in the Bianchi type I space will be presented in this thesis along with the presentation of the proof of the instability of these expanding solutions. Hence , the result agrees with the conjecture of the no-hair theorem.en_US
dc.language.isozh_TWen_US
dc.subject無毛定理zh_TW
dc.subject均向膨脹zh_TW
dc.subject宇宙模型zh_TW
dc.subject早期宇宙zh_TW
dc.subject非均向膨脹zh_TW
dc.subjectno-hair theoremen_US
dc.subjectisotropically expandingen_US
dc.subjectanisotropically expandingen_US
dc.subjectearly universeen_US
dc.subjectde Sitter spaceen_US
dc.subjectBianchi type Ien_US
dc.subjectde Sitter solutionen_US
dc.titleBianchi type I 宇宙模型的穩定性分析zh_TW
dc.titleStability analysis of the Bianchi type I Model Universeen_US
dc.typeThesisen_US
dc.contributor.department物理研究所zh_TW
Appears in Collections:Thesis


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