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...
| Main Authors: | , |
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| Format: | Article |
| Language: | English English |
| Published: |
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 |