The Analysis of the Bianchi Type I Anisotropically
碩士 === 國立交通大學 === 物理研究所 === 98 === Inflation in the early universe is a scenario that could be induced by the scalar field model and/or the high derivative gravity model. Moreover, initial conditions of the space time may affect the evolution of the large-scale isotropic and homogeneous universe we...
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| Format: | Others |
| Language: | zh-TW |
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2010
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| Online Access: | http://ndltd.ncl.edu.tw/handle/91581582882753547704 |
| Summary: | 碩士 === 國立交通大學 === 物理研究所 === 98 === Inflation in the early universe is a scenario that could be induced by the scalar field model and/or the high derivative gravity model. Moreover, initial conditions of the space time may affect the evolution of the large-scale isotropic and homogeneous universe we observed today. Therefore, we will focus on the evolution of the Bianchi type I anisotropically inflating universe under the influence of a high derivative pure gravity model. Systematic method in finding the solutions of the equation of motion will be presented in this thesis. We will also try to find out whether these solutions are stable or not.
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