Abstract

There has been notable effort in recent years to obtain inflationary models from string theory. In the most well-studied scenario, brane inflation, the inflationary phase typically ends with a phase transition leading to the production of a network of cosmic (super)strings. These have different properties than ordinary cosmic strings and thus provide a potential probe to the physics of the early universe. In this letter we review recent work on the cosmological evolution of such string networks. Focusing on analytic velocity-dependent evolution models, we discuss the phenomenology of cosmic (super)string networks and obtain constraints for brane-inflation models.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.