Formation and evolution of cosmic strings

Tammay Vachaspati, Alexander Vilenkin

Research output: Contribution to journalArticle

295 Scopus citations

Abstract

Statistical properties of the system of strings produced at a phase transition in the early universe are studied using a Monte Carlo simulation. The fractal dimension of the strings and the size distribution of closed loops are determined, and it is shown that infinite strings contribute about 80% to the total length of strings in the universe. The results are used to analyze the cosmological evolution of strings. Formation of domain walls and of walls bounded by strings is also discussed, and it is shown that in both cases the system is dominated by one infinite cluster of very complicated topology. The results of the simulations may also be of interest in condensed-matter systems where similar topological defects can be formed.

Original languageEnglish (US)
Pages (from-to)2036-2045
Number of pages10
JournalPhysical Review D
Volume30
Issue number10
DOIs
StatePublished - Jan 1 1984
Externally publishedYes

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ASJC Scopus subject areas

  • Nuclear and High Energy Physics
  • Physics and Astronomy (miscellaneous)

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