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Exact Scale-Invariant Background of Gravitational Waves from Cosmic Defects

Daniel G. Figueroa, Mark Hindmarsh, and Jon Urrestilla
Phys. Rev. Lett. 110, 101302 – Published 6 March 2013

Abstract

We demonstrate that any scaling source in the radiation era produces a background of gravitational waves with an exact scale-invariant power spectrum. Cosmic defects, created after a phase transition in the early universe, are such a scaling source. We emphasize that the result is independent of the topology of the cosmic defects, the order of phase transition, and the nature of the symmetry broken, global or gauged. As an example, using large-scale numerical simulations, we calculate the scale-invariant gravitational wave power spectrum generated by the dynamics of a global O(N) scalar theory. The result approaches the large N theoretical prediction as N2, albeit with a large coefficient. The signal from global cosmic strings is O(100) times larger than the large N prediction.

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  • Received 12 January 2013

DOI:https://doi.org/10.1103/PhysRevLett.110.101302

© 2013 American Physical Society

Authors & Affiliations

Daniel G. Figueroa1,2, Mark Hindmarsh2,3, and Jon Urrestilla4,3

  • 1Département de Physique Théorique and Center for Astroparticle Physics, Université de Genève, 24 quai Ernest Ansermet, CH-1211 Genève 4, Switzerland
  • 2Physics Department, University of Helsinki and Helsinki Institute of Physics, P. O. Box 64, FI-00014 Helsinki, Finland
  • 3Department of Physics and Astronomy, University of Sussex, Brighton BN1 9QH, United Kingdom
  • 4Department of Theoretical Physics, University of the Basque Country UPV/EHU, 48080 Bilbao, Spain

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Issue

Vol. 110, Iss. 10 — 8 March 2013

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