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Magnetized Bianchi Type III Massive String Cosmological Models in General Relativity

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Abstract

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.

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Authors and Affiliations

  1. Physics Department, Mahshahr Islamic Azad University, Mahshahr, Iran

    Hassan Amirhashchi

  2. Physics Department, Universiti Putra Malaysia, 43400 UPM, Serdang, Selangor D.E, Malaysia

    Hassan Amirhashchi

  3. Laboratory of Computational Sciences and Informatics, Institute for Mathematical Research, Universiti Putra Malaysia, 43400 UPM, Serdang, Selangor D.E, Malaysia

    Hishamuddin Zainuddin

  4. Physics Department, Universiti Putra Malaysia, 43400 UPM, Serdang, Selangor D.E, Malaysia

    Hishamuddin Zainuddin

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  1. Hassan Amirhashchi
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  2. Hishamuddin Zainuddin
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Correspondence to Hassan Amirhashchi.

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Amirhashchi, H., Zainuddin, H. Magnetized Bianchi Type III Massive String Cosmological Models in General Relativity. Int J Theor Phys 49, 2815–2828 (2010). https://doi.org/10.1007/s10773-010-0474-3

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  • DOI: https://doi.org/10.1007/s10773-010-0474-3

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