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

We study prospects for detecting extragalactic binary black holes similar toGW150914 by evolved Laser Interferometer Space Antenna (eLISA). We find thatthe majority of detected binary black holes will not merge within reasonableobservation periods of eLISA in any configuration. While long-arm detectors arehighly desired for promoting multiband gravitational-wave astronomy byincreasing the detections of merging binaries, the number of total detectionscan be increased also by improving the acceleration noise. A monochromaticapproximation works well to derive semiquantitative features of observationalprospects for non-merging binaries with clearly indicating the parameterdependence. Our estimate also suggests that the number of galaxies in the errorvolume is so small that the host galaxy may be determined uniquely with highconfidence.

Concise estimate of the expected number of detections for stellar-mass binary black holes by eLISA