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Bulk Viscus Fluid Plane Symmetric String Dust Magnetised Cosmological Model in General Relativity

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Abstract

In this paper we have investigated bulk viscous fluid plane symmetric dust magnetized string cosmological model. To get a deterministic model, it is assumed that ε=λ, and a relation between metric potential B=RA n. The behaviour of the model in the presence and absence of magnetic field together with physical and geometrical aspects of the model are also discussed.

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Authors and Affiliations

  1. Department of Mathematics, Govt. Vidarbha Institute of Science and Humanities, Amravati, 444 604, India

    D. D. Pawar & A. G. Deshmukh

  2. Department of Mathematics, R.L.T. Science College, Akola, 444 001, India

    S. W. Bhaware

Authors
  1. D. D. Pawar
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  2. S. W. Bhaware
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  3. A. G. Deshmukh
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Correspondence to D. D. Pawar.

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Pawar, D.D., Bhaware, S.W. & Deshmukh, A.G. Bulk Viscus Fluid Plane Symmetric String Dust Magnetised Cosmological Model in General Relativity. Int J Theor Phys 47, 599–605 (2008). https://doi.org/10.1007/s10773-007-9483-2

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  • DOI: https://doi.org/10.1007/s10773-007-9483-2

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