Stability conditions for the Bianchi type I anisotropically inflating universe

碩士 === 國立交通大學 === 物理研究所 === 98 === The evolution detail of an anisotropically expanding universe is an interesting research focus lately. The no hair conjecture, proved partially by Robert Wald, states that all anisotropically expanding universes will tend to an isotropic de Sitter space....

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Main Authors: Lee, Chuan-Ruei, 李傳睿
Other Authors: Kao, Win-Fun
Format: Others
Language:zh-TW
Published: 2010
Online Access:http://ndltd.ncl.edu.tw/handle/35763109408408449033
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spelling ndltd-TW-098NCTU51980142016-04-18T04:21:48Z http://ndltd.ncl.edu.tw/handle/35763109408408449033 Stability conditions for the Bianchi type I anisotropically inflating universe 不均向膨脹宇宙 Bianchi type I 的空間穩定性研究 Lee, Chuan-Ruei 李傳睿 碩士 國立交通大學 物理研究所 98 The evolution detail of an anisotropically expanding universe is an interesting research focus lately. The no hair conjecture, proved partially by Robert Wald, states that all anisotropically expanding universes will tend to an isotropic de Sitter space. A class of anisotropically expanding solutions are found in ref. [1] for a gravity model with second-order correction terms derived from all possible combinations of the Ricci curvature tensor and Ricci scalar. We will present the correct expanding solutions in this paper. These solutions can be shown to be unstable by perturbing the field equations. Conventional approach by dynamical system analysis used in ref. [1] will be reviewed carefully and compared with the perturbation method mentioned earlier in this paper. Kao, Win-Fun 高文芳 2010 學位論文 ; thesis 95 zh-TW
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description 碩士 === 國立交通大學 === 物理研究所 === 98 === The evolution detail of an anisotropically expanding universe is an interesting research focus lately. The no hair conjecture, proved partially by Robert Wald, states that all anisotropically expanding universes will tend to an isotropic de Sitter space. A class of anisotropically expanding solutions are found in ref. [1] for a gravity model with second-order correction terms derived from all possible combinations of the Ricci curvature tensor and Ricci scalar. We will present the correct expanding solutions in this paper. These solutions can be shown to be unstable by perturbing the field equations. Conventional approach by dynamical system analysis used in ref. [1] will be reviewed carefully and compared with the perturbation method mentioned earlier in this paper.
author2 Kao, Win-Fun
author_facet Kao, Win-Fun
Lee, Chuan-Ruei
李傳睿
author Lee, Chuan-Ruei
李傳睿
spellingShingle Lee, Chuan-Ruei
李傳睿
Stability conditions for the Bianchi type I anisotropically inflating universe
author_sort Lee, Chuan-Ruei
title Stability conditions for the Bianchi type I anisotropically inflating universe
title_short Stability conditions for the Bianchi type I anisotropically inflating universe
title_full Stability conditions for the Bianchi type I anisotropically inflating universe
title_fullStr Stability conditions for the Bianchi type I anisotropically inflating universe
title_full_unstemmed Stability conditions for the Bianchi type I anisotropically inflating universe
title_sort stability conditions for the bianchi type i anisotropically inflating universe
publishDate 2010
url http://ndltd.ncl.edu.tw/handle/35763109408408449033
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