English

Reionization from cosmic string loops

Astrophysics 2009-11-11 v1 High Energy Physics - Theory

Abstract

Loops formed from a cosmic string network at early times would act as seeds for early formation of halos, which would form galaxies and lead to early reionization. With reasonable guesses about astrophysical and string parameters, the cosmic string scale GμG\mu must be no more than about 3×1083\times 10^{-8} to avoid conflict with the reionization redshift found by WMAP. The bound is much stronger for superstring models with a small string reconnection probability. For values near the bound, cosmic string loops may explain the discrepancy between the WMAP value and theoretical expectations.

Keywords

Cite

@article{arxiv.astro-ph/0605465,
  title  = {Reionization from cosmic string loops},
  author = {Ken D. Olum and Alexander Vilenkin},
  journal= {arXiv preprint arXiv:astro-ph/0605465},
  year   = {2009}
}

Comments

7 pp., RevTeX, no figures