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Magnetized Bianchi type III massive string cosmological models in general relativity.

The present study deals with Bianchi type III string cosmological models with magnetic field. The magnetic field is assumed to be along z direction. Therefore F 12 is only the non-vanishing component of electromagnetic field tensor F ij . The expansion (θ) in the model is assumed to be proportional...

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Main Authors: Amirhashchi, Hassan, Zainuddin, Hishamuddin
Format: Article
Language:English
English
Published: Springer Link 2010
Online Access:http://psasir.upm.edu.my/id/eprint/15503/1/Magnetized%20Bianchi%20type%20III%20massive%20string%20cosmological%20models%20in%20general%20relativity.pdf
http://psasir.upm.edu.my/id/eprint/15503/
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spelling my.upm.eprints.155032015-11-02T04:33:58Z http://psasir.upm.edu.my/id/eprint/15503/ Magnetized Bianchi type III massive string cosmological models in general relativity. Amirhashchi, Hassan Zainuddin, Hishamuddin The present study deals with Bianchi type III string cosmological models with magnetic field. The magnetic field is assumed to be along z direction. Therefore F 12 is only the non-vanishing component of electromagnetic field tensor F ij . The expansion (θ) in the model is assumed to be proportional to the shear (σ). To get determinate solution in term of cosmic time, we have solved the fields equations in two cases (i) Reddy and (ii) Nambu string. The physical and geometrical behaviour of these models is discussed. Springer Link 2010 Article PeerReviewed application/pdf en http://psasir.upm.edu.my/id/eprint/15503/1/Magnetized%20Bianchi%20type%20III%20massive%20string%20cosmological%20models%20in%20general%20relativity.pdf Amirhashchi, Hassan and Zainuddin, Hishamuddin (2010) Magnetized Bianchi type III massive string cosmological models in general relativity. International Journal of Theoretical Physics, 49 (11). pp. 2815-2828. ISSN 0020-7748 10.1007/s10773-010-0474-3 English
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
English
description The present study deals with Bianchi type III string cosmological models with magnetic field. The magnetic field is assumed to be along z direction. Therefore F 12 is only the non-vanishing component of electromagnetic field tensor F ij . The expansion (θ) in the model is assumed to be proportional to the shear (σ). To get determinate solution in term of cosmic time, we have solved the fields equations in two cases (i) Reddy and (ii) Nambu string. The physical and geometrical behaviour of these models is discussed.
format Article
author Amirhashchi, Hassan
Zainuddin, Hishamuddin
spellingShingle Amirhashchi, Hassan
Zainuddin, Hishamuddin
Magnetized Bianchi type III massive string cosmological models in general relativity.
author_facet Amirhashchi, Hassan
Zainuddin, Hishamuddin
author_sort Amirhashchi, Hassan
title Magnetized Bianchi type III massive string cosmological models in general relativity.
title_short Magnetized Bianchi type III massive string cosmological models in general relativity.
title_full Magnetized Bianchi type III massive string cosmological models in general relativity.
title_fullStr Magnetized Bianchi type III massive string cosmological models in general relativity.
title_full_unstemmed Magnetized Bianchi type III massive string cosmological models in general relativity.
title_sort magnetized bianchi type iii massive string cosmological models in general relativity.
publisher Springer Link
publishDate 2010
url http://psasir.upm.edu.my/id/eprint/15503/1/Magnetized%20Bianchi%20type%20III%20massive%20string%20cosmological%20models%20in%20general%20relativity.pdf
http://psasir.upm.edu.my/id/eprint/15503/
_version_ 1643825949374939136
score 13.18916

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