完整後設資料紀錄
DC 欄位 | 值 | 語言 |
---|---|---|
dc.contributor.author | 袁珮閎 | en_US |
dc.contributor.author | Yuan, Pei-Hung | en_US |
dc.contributor.author | 高文芳 | en_US |
dc.date.accessioned | 2014-12-12T01:50:16Z | - |
dc.date.available | 2014-12-12T01:50:16Z | - |
dc.date.issued | 2010 | en_US |
dc.identifier.uri | http://140.113.39.130/cdrfb3/record/nctu/#GT079827517 | en_US |
dc.identifier.uri | http://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.abstract | In 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.iso | zh_TW | en_US |
dc.subject | 早期宇宙 | zh_TW |
dc.subject | 暴脹 | zh_TW |
dc.subject | Lorentz Chern-Simons | en_US |
dc.subject | de Sitter | en_US |
dc.title | de Sitter 時空與 Lorentz Chern-Simons 項 | zh_TW |
dc.title | de Sitter space and Lorentz Chern-Simons term | en_US |
dc.type | Thesis | en_US |
dc.contributor.department | 物理研究所 | zh_TW |
顯示於類別: | 畢業論文 |