Reionization from cosmic string loops

Ken D. Olum and Alexander Vilenkin
Phys. Rev. D 74, 063516 – Published 20 September 2006

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 Gμ must be no more than about 3×108 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.

  • Received 18 May 2006

DOI:https://doi.org/10.1103/PhysRevD.74.063516

©2006 American Physical Society

Authors & Affiliations

Ken D. Olum* and Alexander Vilenkin

  • Institute of Cosmology, Department of Physics and Astronomy, Tufts University, Medford, Massachusetts 02155, USA

  • *Electronic address: kdo@cosmos.phy.tufts.edu
  • Electronic address: vilenkin@cosmos.phy.tufts.edu

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Issue

Vol. 74, Iss. 6 — 15 September 2006

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