Lorentz Chern-Simons理論在Bianchi第三類和第五類空間的穩定性分析

Full metadata record

DC Field	Value	Language
dc.contributor.author	江建廷	en_US
dc.contributor.author	高文芳	en_US
dc.date.accessioned	2014-12-12T01:50:17Z	-
dc.date.available	2014-12-12T01:50:17Z	-
dc.date.issued	2012	en_US
dc.identifier.uri	http://140.113.39.130/cdrfb3/record/nctu/#GT079827528	en_US
dc.identifier.uri	http://hdl.handle.net/11536/47706	-
dc.description.abstract	在Einstein-Hilbert action 中加入Lorentz Chern-Simons交互作用項，深入計算Bianchi type III 和 V 的宇宙時空演化情形，並檢驗No-hair conjecture在此是否成立。	zh_TW
dc.description.abstract	Lorentz Chern-Simons interaction is added to the Einstein-Hilbert action. We will show that the evolution of the universe in Bianchi Type III and V are both consistent with the No-hair conjecture.	en_US
dc.language.iso	zh_TW	en_US
dc.subject	無毛猜想	zh_TW
dc.subject	交互作用項	zh_TW
dc.subject	宇宙時空演化	zh_TW
dc.subject	Lorentz Chern-Simons	en_US
dc.subject	the universe in Bianchi Type III and V	en_US
dc.subject	No-hair conjecture	en_US
dc.title	Lorentz Chern-Simons理論在Bianchi第三類和第五類空間的穩定性分析	zh_TW
dc.title	The stability analysis of Lorentz Chern-Simons theory in Bianchi type III and type V spaces	en_US
dc.type	Thesis	en_US
dc.contributor.department	物理研究所	zh_TW
Appears in Collections:	Thesis