Hostname: page-component-76fb5796d-vvkck Total loading time: 0 Render date: 2024-04-26T21:02:14.211Z Has data issue: false hasContentIssue false
  • English
  • Français

Is Cosmic String Domination of the Universe Avoidable?

Published online by Cambridge University Press:  03 August 2017

François R. Bouchet  and
David P. Bennett
François R. Bouchet
Affiliation:
Department of Astronomy, U.C. Berkeley IGPP, Lawrence Livermore National Laboratory On leave from Institut d'Astrophysique de Paris
David P. Bennett
Affiliation:
Theoretical Astrophysics Group, Fermilab Astronomy and Astrophysics Center, University of Chicago

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We address, by means of Numerical Simulations, one of the main issues of the Cosmic String Galaxy Formation Scenario, namely the existence of a scaling solution, which is crucial to the very existence of the scenario. After a brief discussion of our numerical technique, we present our results which, though still preliminary, offer the best support to date of this scaling hypothesis.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 130: Large Scale Structures of the Universe , 1988 , pp. 289 - 291
Copyright
Copyright © Reidel 1988 

References

Albrecht, A., and Turok, N., Phys. Rev. Lett. 54, 1868 (1985).CrossRefGoogle Scholar
Bennett, D. P., Phys. Rev. D33, 872, and D34, 3592 (1986).Google Scholar
Kibble, T. W. B., Nucl. Phys. B252, 227 (1985).CrossRefGoogle Scholar
Turok, N., and Bhattacharjee, P., Phys. Rev. D29, 1557 (1984).Google Scholar
Vachaspati, T., and Vilenkin, A., Phys. Rev. D30, 2036 (1984).Google Scholar