Skip to main content
Log in

A neutrino universe with viscosity

  • General Relativity
  • Published:
Pramana Aims and scope Submit manuscript

Abstract

A solution of the Einstein field equation corresponding to a distribution of fluid with equation of stateρ = 3p but with a nonvanishing shear viscosity is presented. The solution is spherical symmetric and the flow lines are geodetic.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  • Ellis G F R 1971General relativity and cosmology (ed.) R K Sachs (New York: Academic Press)

    Google Scholar 

  • Landau L D and Lifshitz E M 1971Classical theory of fields (Oxford: Pergamon Press)

    Google Scholar 

  • Raychaudhuri A K 1979Theoretical cosmology (Oxford: University Press)

    MATH  Google Scholar 

  • Tolman R C 1934Relativity, thermodynamics and cosmology (Oxford: University Press)

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Modak, B. A neutrino universe with viscosity. Pramana - J Phys 23, 809–814 (1984). https://doi.org/10.1007/BF02894772

Download citation

  • Received:

  • Revised:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF02894772

Keywords

PACS No.

Navigation