Collisions of cosmic F- and D-strings

Details Collisions of cosmic F- and D-strings Collisions of cosmic F- and D-strings

Nov 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004crphy...5.1011j&link_type=abstract

Comptes Rendus - Physique, Volume 5, Issue 9-10, p. 1011-1020.

Physics

String Theory Models, Brane Anti-Brane Models, Cosmic String Interactions, Théorie Des Cordes, Modèles Branaires Et Anti-Branaires, Interactions Entre Cordes Cosmiques

Scientific paper

Recent theoretical advances and upcoming experimental measurements make the testing of generic predictions of string theory models of cosmology feasible. Brane anti-brane models of inflation within superstring theory are promising as string theory descriptions of the physics of the early universe. While varied in their construction, these models can have the generic and observable consequence that cosmic strings will be abundant in the early universe. This leads to possible detectable effects in the cosmic microwave background, gravitational wave physics and gravitational lensing. Detailed calculations of cosmic string interactions within string theory are presented, in order to distinguish these cosmic strings from those in more conventional theories; these interaction probabilities can be very different from conventional 4D strings, providing the possibility of experimental tests of string theory. To cite this article: N. Jones, C. R. Physique 5 (2004).

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