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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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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/13390/1/Bianchi%20type.pdf
http://psasir.upm.edu.my/id/eprint/13390/
http://fizika.hfd.hr/fizika_b/bv10/b19p081.htm
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spelling my.upm.eprints.133902015-10-27T08:16:02Z http://psasir.upm.edu.my/id/eprint/13390/ Bianchi type-III string cosmological models for stiff and anti-stiff fluid in general relativity Amirhashchi, Hassan Zainuddin, Hishamuddin 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. Hrvatsko Fizikalno Drustvo,Croatian Physical Society 2010 Article PeerReviewed application/pdf en http://psasir.upm.edu.my/id/eprint/13390/1/Bianchi%20type.pdf Amirhashchi, Hassan and Zainuddin, Hishamuddin (2010) Bianchi type-III string cosmological models for stiff and anti-stiff fluid in general relativity. Fizika B, 19 (2). pp. 81-90. ISSN 1330-0016; ESSN: 333–9133 http://fizika.hfd.hr/fizika_b/bv10/b19p081.htm
institution Universiti Putra Malaysia
building UPM Library
collection Institutional Repository
continent Asia
country Malaysia
content_provider Universiti Putra Malaysia
content_source UPM Institutional Repository
url_provider http://psasir.upm.edu.my/
language English
description 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.
format Article
author Amirhashchi, Hassan
Zainuddin, Hishamuddin
spellingShingle Amirhashchi, Hassan
Zainuddin, Hishamuddin
Bianchi type-III string cosmological models for stiff and anti-stiff fluid in general relativity
author_facet Amirhashchi, Hassan
Zainuddin, Hishamuddin
author_sort Amirhashchi, Hassan
title Bianchi type-III string cosmological models for stiff and anti-stiff fluid in general relativity
title_short Bianchi type-III string cosmological models for stiff and anti-stiff fluid in general relativity
title_full Bianchi type-III string cosmological models for stiff and anti-stiff fluid in general relativity
title_fullStr Bianchi type-III string cosmological models for stiff and anti-stiff fluid in general relativity
title_full_unstemmed Bianchi type-III string cosmological models for stiff and anti-stiff fluid in general relativity
title_sort bianchi type-iii string cosmological models for stiff and anti-stiff fluid in general relativity
publisher Hrvatsko Fizikalno Drustvo,Croatian Physical Society
publishDate 2010
url http://psasir.upm.edu.my/id/eprint/13390/1/Bianchi%20type.pdf
http://psasir.upm.edu.my/id/eprint/13390/
http://fizika.hfd.hr/fizika_b/bv10/b19p081.htm
_version_ 1643825317612093440
score 13.211869

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