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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| Format: | Article |
| Language: | English English |
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Springer Link
2010
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| Online Access: | http://psasir.upm.edu.my/id/eprint/15503/1/Magnetized%20Bianchi%20type%20III%20massive%20string%20cosmological%20models%20in%20general%20relativity.pdf |
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| author | Amirhashchi, Hassan Zainuddin, Hishamuddin |
| author_facet | Amirhashchi, Hassan Zainuddin, Hishamuddin |
| author_sort | Amirhashchi, Hassan |
| collection | UPM |
| 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. |
| first_indexed | 2024-03-06T07:34:32Z |
| format | Article |
| id | upm.eprints-15503 |
| institution | Universiti Putra Malaysia |
| language | English English |
| last_indexed | 2024-03-06T07:34:32Z |
| publishDate | 2010 |
| publisher | Springer Link |
| record_format | dspace |
| spelling | 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 |
| spellingShingle | Amirhashchi, Hassan Zainuddin, Hishamuddin Magnetized Bianchi type III massive string cosmological models in general relativity. |
| title | 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_short | Magnetized Bianchi type III massive string cosmological models in general relativity. |
| title_sort | magnetized bianchi type iii massive string cosmological models in general relativity |
| url | http://psasir.upm.edu.my/id/eprint/15503/1/Magnetized%20Bianchi%20type%20III%20massive%20string%20cosmological%20models%20in%20general%20relativity.pdf |
| work_keys_str_mv | AT amirhashchihassan magnetizedbianchitypeiiimassivestringcosmologicalmodelsingeneralrelativity AT zainuddinhishamuddin magnetizedbianchitypeiiimassivestringcosmologicalmodelsingeneralrelativity |