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/

Zendy Open

Presents the pdf analysis as premium feature

PDF Analysis

Insights

Presents the summarisation as premium feature

Summarisation

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the zaia usage as premium feature

ZAIA

Zendy Tools

Zendy Plus

Presents the access of premium content as premium feature

Premium Content

Accretion of dark energy onto black holes will take place when dark energy isnot a cosmological constant. It has been proposed that the time evolution ofthe mass of the black holes in binary systems due to dark energy accretioncould be detectable by gravitational radiation. This would make it possible touse observations of black hole binaries to measure local dark energyproperties, e.g., to determine the sign of 1+w where w is the dark energyequation of state. In this Letter we show that such measurements are unfeasibledue to the low accretion rates.

On the use of black hole binaries as probes of local dark energy properties