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Original scientific paper

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

Hassan Amirhashchi ; Physics Department, Universiti Putra Malaysia, 43400 UPM, Serdang, Selangor D.E. Malaysia; Physics Department, Mahshahr Islamic Azad University, Mahshahr, Iran
Hishamuddin Zainuddin ; Physics Department, Universiti Putra Malaysia, 43400 UPM, Serdang, Selangor D.E. Malaysia


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Abstract

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 of the fluid, respectively. The physical behavior of these models is also discussed.

Keywords

Bianchi type-III models; stiff fluid; anti-stiff fluid

Hrčak ID:

304595

URI

https://hrcak.srce.hr/304595

Publication date:

2.5.2010.

Article data in other languages: croatian

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