Izvorni znanstveni članak
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
Sažetak
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.
Ključne riječi
Bianchi type-III models; stiff fluid; anti-stiff fluid
Hrčak ID:
304595
URI
Datum izdavanja:
2.5.2010.
Posjeta: 384 *