Astrophysics and Space Science

, Volume 150, Issue 2, pp 309–316 | Cite as

Cosmological viscous fluid models in the presence of electromagnetic field and zero-mass scalar field

  • R. K. Tarachand Singh
  • N. Ibotombi Singh


The problem of electromagnetic field interacting with viscous fluid without and with zero-mass scalar field has been studied. It has been shown that electromagnetic field cannot interact with viscous fluid for spherically-symmetric Robertson-Walker metric. Exact solutions corresponding to the problem of electromagnetic field interactions in presence of viscous fluid and zero-mass scalar field have been obtained subject to various physical conditions. It presents a scope for the study of imperfect fluid FRW models showing the existence of the electromagnetic field due to the presence of zero-mass scalar field.


Physical Condition Exact Solution Electromagnetic Field Scalar Field Viscous Fluid 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.


  1. Charach, C.: 1979,Phys. Rev. D19, 3516.Google Scholar
  2. Charach, C.: 1980,Phys. Rev. D21, 547.Google Scholar
  3. Charach, C. and Malin, S.: 1979,Phys. Rev. D19, 105.Google Scholar
  4. Das, A. and Agarwal, P.: 1974,Gen. Rel. Grav. 5, 95.Google Scholar
  5. Mehra, A. L. and Bohra, M. L.: 1978,Gen. Rel. Grav. 4, 289.Google Scholar
  6. Suszycki, L.: 1978,Acta Cosmologica 7, 147.Google Scholar
  7. Verma, M. N.: 1987, Ph. D. Thesis, I.I.T. Kharagpur, India.Google Scholar

Copyright information

© Kluwer Academic Publishers 1988

Authors and Affiliations

  • R. K. Tarachand Singh
    • 1
  • N. Ibotombi Singh
    • 1
  1. 1.Department of MathematicsManipur UniversityImphalIndia

Personalised recommendations