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• W2559405922 abstract "The merger rate of black hole binaries inferred from the recent LIGO detections implies that a stochastic background produced by a cosmological population of mergers will likely mask the primordial gravitational-wave background. Here we demonstrate that the next generation of ground-based detectors, such as the Einstein Telescope and Cosmic Explorer, will be able to observe binary black hole mergers throughout the universe with sufficient efficiency that the confusion background can be subtracted to observe the primordial background at the level of $Omega_{mathrm{GW}} simeq 10^{-13}$ after five years of observation." @default.
• W2559405922 created "2016-12-08" @default.
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• W2559405922 date "2016-11-28" @default.
• W2559405922 modified "2023-09-27" @default.
• W2559405922 title "Digging deeper: Observing primordial gravitational waves below black hole binary confusion noise" @default.
• W2559405922 hasPublicationYear "2016" @default.
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