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General Relativity and Gravitation

, Volume 19, Issue 6, pp 537–543 | Cite as

Scalar and spinor fields in the very early universe

  • Sushil K. Srivastava
Research Articles

Abstract

Here it is shown how the vacuum energy may dominate the energy density of the very early universe even when the Higg's field in the Coleman-Weinberg potential is confined near the origin at extremely high temperature and the inflationary scenario may start. Also it is shown that supersymmetry breaking may be responsible for this phenomenon. Thus it provides another support for the hypothesis of primordial inflation proposed by Ellis et al. [4],

Keywords

Energy Density Differential Geometry Supersymmetry Breaking Early Universe Vacuum Energy 
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.

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References

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    Guth, A. H. (1981).Phys. Rev.,D23, 347; (1983).The Very Early Universe, G. W. Gibbons, S. W. Hawking, and S, Siklos, eds. (Cambridge University Press, Cambridge).Google Scholar
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    Linde, A. D. (1982).Phys. Lett.,B108, 384; (1982).Phys. Lett.,B114, 431.Google Scholar
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    Albrecht, A., and Steinhardt, P. J. (1982).Phys. Rev. Lett.,48, 1220.Google Scholar
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    Ellis, J., Nanopoulos, D. V., Olive, K. A., and Tamvakis, K. (1982).Phys. Lett.,B118, 335; (1983).Nucl. Phys.,B221, 524–548.Google Scholar

Copyright information

© Plenum Publishing Corporation 1987

Authors and Affiliations

  • Sushil K. Srivastava
    • 1
  1. 1.Department of MathematicsNorth Eastern Hill UniversityShillongIndia

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