General properties of the gravitational wave spectrum from phase transitions

Chiara Caprini, Ruth Durrer, Thomas Konstandin, and Géraldine Servant
Phys. Rev. D 79, 083519 – Published 16 April 2009

Abstract

In this paper we discuss some general aspects of the gravitational wave background arising from postinflationary short-lasting cosmological events such as phase transitions. We concentrate on the physics which determines the shape and the peak frequency of the gravitational wave spectrum. We then apply our general findings to the case of bubble collisions during a first order phase transition and compare different results in the recent literature.

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  • Received 3 February 2009

DOI:https://doi.org/10.1103/PhysRevD.79.083519

©2009 American Physical Society

Authors & Affiliations

Chiara Caprini1,*, Ruth Durrer2,†, Thomas Konstandin3,‡, and Géraldine Servant4,§

  • 1CEA, IPhT, and CNRS, URA 2306, F-91191 Gif-sur-Yvette, France
  • 2Département de Physique Théorique, Université de Genève, 24 quai Ernest Ansermet, CH-1211 Genève 4, Switzerland
  • 3IFAE, Universitat Autònoma de Barcelona, 08193 Bellaterra, Barcelona, Spain
  • 4CERN Physics Department, Theory Division, CH-1211 Geneva 23, Switzerland

  • *chiara.caprini@cea.fr
  • ruth.durrer@unige.ch
  • konstand@ifae.es
  • §geraldine.servant@cern.ch

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Vol. 79, Iss. 8 — 15 April 2009

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