English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

The merger rate of black hole binaries inferred from the detections in thefirst Advanced LIGO science run, implies that a stochastic background producedby a cosmological population of mergers will likely mask the primordialgravitational-wave background. Here we demonstrate that the next generation ofground-based detectors, such as the Einstein Telescope and Cosmic Explorer,will be able to observe binary black hole mergers throughout the universe withsufficient efficiency that the confusion background can potentially besubtracted to observe the primordial background at the level of$\Omega_{\mathrm{GW}} \simeq 10^{-13}$ after five years of observation.

Digging deeper: Observing primordial gravitational waves below the binary black hole produced stochastic background