Hostname: page-component-586b7cd67f-tf8b9 Total loading time: 0 Render date: 2024-11-30T16:18:37.987Z Has data issue: false hasContentIssue false
  • English
  • Français

Monopole Evolution in the Early Universe

Published online by Cambridge University Press:  26 May 2016

Michiyasu Nagasawa
Michiyasu Nagasawa*
Affiliation:
Department of Information Science, Faculty of Science, Kanagawa University, Kanagawa 259-1293, Japan E-Mail: [email protected]

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.

The formation and evolution of monopoles produced at TeV energy scales are considered. They can contribute to the generation of baryon number and may solve the cosmological problem. The dynamics of electroweak defects is completely different from that of conventional grand unification scale defects so that their number density should not be described by the scaling model.

Type
Posters
Information
Symposium - International Astronomical Union , Volume 208: Astrophysical Supercomputing using Particle Simulations , 2003 , pp. 429 - 430
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Kephart, T.W., & Vachaspati, T. 1996, Phys. Lett. B388, 481 Google Scholar
Nagasawa, M., & Yokoyama, J. 1996, Phys. Rev. Lett 77, 2166 CrossRefGoogle Scholar
Brandenberger, R.H., & Davis, A.-C. 1994, Phys. Lett. B332, 305 Google Scholar
Soni, V. 1997, Phys. Lett. B394, 275 Google Scholar
Aulakh, C.S., Nagasawa, M., & Soni, V. 1999, Phys. Lett. B471, 13 Google Scholar