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 Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

Modified gravitational wave propagation is a smoking gun of modifications ofgravity at cosmological scales, and can be the most promising observable fortesting such theories. The observation of gravitational waves (GW) in recentyears has allowed us to start probing this effect, and here we briefly reviewtwo promising ways of testing it. We will show that, already with the currentnetwork of detectors, it is possible to reach an interesting accuracy in theestimation of the $\Xi_0$ parameter (that characterizes modified gravitationalwave propagation, with $\Xi_{0, {\rm GR}} = 1$) and with next generationfacilities, such as the Einstein Telescope, we can get a sub-percentmeasurement.

Modified gravitational wave propagation: information from strongly lensed binaries and the BNS mass function