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Bianchi Type-I cosmological mesonic stiff fluid models in Lyra’s geometry

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Abstract

Bianchi Type-I cosmological models in Lyra’s geometry are obtained when the source of gravitational field is a perfect fluid coupled with massless mesonic scalar field. Some physical and kinematical properties of the models are also discussed.

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Authors and Affiliations

  1. PGTD of Mathematics, Rajsthan Aryan Mahavidyalaya, Washim, 444 505, India

    S. D. Katore

  2. Department of Mathematics, Babasaheb Naik College of Engineering, Pusad, 445 215, India

    S. V. Thakare

  3. PGTD of Mathematics, Sant Gadge Baba Amravati University, Amravati, 444 602, India

    K. S. Adhao

Authors
  1. S. D. Katore
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  2. S. V. Thakare
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  3. K. S. Adhao
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Correspondence to S. D. Katore.

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Katore, S.D., Thakare, S.V. & Adhao, K.S. Bianchi Type-I cosmological mesonic stiff fluid models in Lyra’s geometry. Pramana - J Phys 71, 15–22 (2008). https://doi.org/10.1007/s12043-008-0137-6

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  • DOI: https://doi.org/10.1007/s12043-008-0137-6

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