Disruption of cosmic string wakes by Gaussian fluctuations

Disrael Camargo Neves da Cunha, Robert H. Brandenberger, and Oscar F. Hernández
Phys. Rev. D 93, 123501 – Published 1 June 2016

Abstract

We study the stability of cosmic string wakes against the disruption by the dominant Gaussian fluctuations which are present in cosmological models. We find that for a string tension given by Gμ=107 wakes remain locally stable until a redshift of z=6, and for a value of Gμ=1014 they are stable beyond a redshift of z=20. We study a global stability criterion which shows that wakes created by strings at times after teq are identifiable up to the present time, independent of the value of Gμ. Taking into account our criteria it is possible to develop strategies to search for the distinctive position space signals in cosmological maps which are induced by wakes.

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  • Received 6 November 2015

DOI:https://doi.org/10.1103/PhysRevD.93.123501

© 2016 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Disrael Camargo Neves da Cunha* and Robert H. Brandenberger

  • Department of Physics, McGill University, Montréal, Québec H3A 2T8, Canada

Oscar F. Hernández

  • Department of Physics, McGill University, Montréal, Québec H3A 2T8, Canada and Marianopolis College, 4873 Westmount Avenue, Westmount, Quebec H3Y 1X9, Canada

  • *camargod@physics.mcgill.ca
  • rhb@physics.mcgill.ca
  • oscarh@physics.mcgill.ca

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Issue

Vol. 93, Iss. 12 — 15 June 2016

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