Stochastic background from extra-galactic double neutron stars

Abstract

We present Monte Carlo simulations of the extra galactic population of inspiralling double neutron stars, and estimate its contribution to the astrophysical gravitational wave background, in the frequency range of ground based interferometers, corresponding to the last thousand seconds before the last stable orbit when more than 96 percent of the signal is released. We show that sources at redshift z>0.5 contribute to a truly continuous background which may be detected by correlating third generation interferometers.

13 pages, 7 figures - proceeding of a talk given at the 11th GWDAW, to appear in CQG

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Cited by in corpus (20)

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• Stochastic Gravitational Wave Background from Coalescing Binary Black Holes
• Directional limits on persistent gravitational waves from Advanced LIGO's first observing run
• Accessibility of the Gravitational-Wave Background due to Binary Coalescences to Second and Third Generation Gravitational-Wave Detectors
• Directional limits on persistent gravitational waves using LIGO S5 science data
• Imprint of the merger and ring-down on the gravitational wave background from black hole binaries coalescence
• Can we distinguish astrophysical from primordial black holes via the stochastic gravitational wave background?
• Astrophysical Sources of Stochastic Gravitational-Wave Background
• Time-dependence of the astrophysical stochastic gravitational wave background
• Searching for stochastic gravitational waves using data from the two co-located LIGO Hanford detectors
• Prospects of discovering sub-solar primordial black holes using the stochastic gravitational wave background from third-generation detectors
• Inferring the lensing rate of LIGO-Virgo sources from the stochastic gravitational wave background
• Stochastic Gravitational Wave Background from Neutron Star r-mode Instability Revisited
• Stochastic background from extra-galactic double neutron stars
• Fundamental physics using the temporal gravitational wave background
• Stochastic gravitational wave background from magnetic deformation of newly born magnetars
• Stochastic backgrounds of gravitational waves from extragalactic sources
• Stochastic background of gravitational waves from cosmological sources
• The Gravitational Wave Background From Coalescing Compact Binaries: A New Method
• Stochastic Background of Gravitational Waves Generated by Eccentric Neutron Star Binaries