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Bianchi Type-Ⅲ String Cosmological Models with Time Dependent Bulk Viscosity
引用本文:BALI Raj PRADHAN Anirudh. Bianchi Type-Ⅲ String Cosmological Models with Time Dependent Bulk Viscosity[J]. 中国物理快报, 2007, 24(2): 585-588
作者姓名:BALI Raj PRADHAN Anirudh
作者单位:[1]Department of Mathematics, University of Rajasthan, Jaipur-302 004, India [2]Department'of Mathematics, Hindu Post-Graduate College, Zamania-232 331, Ghazipur, India
摘    要:Bianchi type-Ⅲ string cosmological models with bulk viscous fluid for massive string are investigated. To obtain the determinate model of the universe, we assume that the coeffcient of bulk viscosity ξ is inversely proportional to the expansion θ in the model and expansion θ in the model is proportional to the shear g. This leads to B =lC^n, where l and n are constants. Behaviour of the model in the presence and absence of bulk viscosity is discussed. The physical implications of the models are also discussed in detail.

关 键 词:宇宙模型 时间 粘性流体 体积
收稿时间:2006-11-03
修稿时间:2006-11-03

Bianchi Type-III String Cosmological Models with Time Dependent Bulk Viscosity
BALI Raj,PRADHAN Anirudh. Bianchi Type-III String Cosmological Models with Time Dependent Bulk Viscosity[J]. Chinese Physics Letters, 2007, 24(2): 585-588
Authors:BALI Raj  PRADHAN Anirudh
Affiliation:Department of Mathematics, University of Rajasthan, Jaipur-302 004, IndiaDepartment of Mathematics, Hindu Post-Graduate College, Zamania-232 331, Ghazipur, India
Abstract:
Keywords:98.80.Cq  04.20.-q
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