Skip to main content
Log in

A scalar field theory with a variable cosmological term

  • Research Articles
  • Published:
General Relativity and Gravitation Aims and scope Submit manuscript

Abstract

From the standpoint of cosmology, we investigate the relationship between the Brans-Dicke scalar field ø and the scalar field in particle physics (hereafter abbreviated as p.p.) on the assumption that ø is an arbitrary function ofr, but not oft. And also we see whether the cosmological term A which was originally introduced into cosmology without a relationship to p.p. can be related to the symmetry-breaking term in p.p., supposing a dependence of A upon ø.

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

  1. Endo, M., and Fukui, T. (1977).Gen. Rel. Grav.,8, 833.

    Google Scholar 

  2. Linde, A. D. (1974).JETP Lett.,19, 183.

    Google Scholar 

  3. Cho, T. M., and Freund, P. G. O. (1975).Phys. Rev. D,12, 1588.

    Google Scholar 

  4. Dreitlein, J. (1974).Phys. Rev. Lett.,33, 1243.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Endo, M., Fukui, T. A scalar field theory with a variable cosmological term. Gen Relat Gravit 14, 769–772 (1982). https://doi.org/10.1007/BF00756088

Download citation

  • Received:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00756088

Keywords

Navigation