Bianchi type-III string cosmological models for stiff and anti-stiff fluid in general relativity

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Bianchi type-III string cosmological models for stiff and anti-stiff fluid in general relativity

Bianchi type-III string cosmological models in the presence of stiff and anti-stiff fluids are studied. The scalar expansion is assumed to be proportional to the shear. In the present study, we consider two cases (i)p+ρ= 0 and (ii) p−ρ= 0, where ρ and p are the rest energy density and the pressure...

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Bibliographic Details
Main Authors:	Amirhashchi, Hassan, Zainuddin, Hishamuddin
Format:	Article
Language:	English
Published:	Hrvatsko Fizikalno Drustvo,Croatian Physical Society 2010
Online Access:	http://psasir.upm.edu.my/id/eprint/13390/ http://psasir.upm.edu.my/id/eprint/13390/1/Bianchi%20type.pdf

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