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      Binary Cosmic Strings

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          Abstract

          The properties of cosmic strings have been investigated in detail for their implications in early-universe cosmology. Although many variations of the basic structure have been discovered, with implications for both the microscopic and macroscopic properties of cosmic strings, the cylindrical symmetry of the short-distance structure of the string is generally unaffected. In this paper we describe some mechanisms leading to an asymmetric structure of the string core, giving the defects a quasi-two-dimensional character. We also begin to investigate the consequences of this internal structure for the microscopic and macroscopic physics.

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          Vortex-line models for dual strings

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            Superconducting strings

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              Cosmological Density Fluctuations Produced by Vacuum Strings

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                Author and article information

                Journal
                14 July 1995
                Article
                10.1103/PhysRevD.53.1827
                hep-th/9507082
                bc57d5e1-44eb-4af5-8b29-56e45e1e0032
                History
                Custom metadata
                Phys.Rev. D53 (1996) 1827-1834
                19 pages; uses harvmac (not included)
                hep-th

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