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 Tools annual

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 monthly

Global: Zendy Plus monthly

Presents the access of premium content as premium feature

Premium Content

Global: Zendy Plus annual

Global: Zendy Free Plan

We perform a hierarchical Bayesian inference to investigate the populationproperties of the coalescing compact binaries involving at least one neutronstar (NS). With the current observation data, we can not rule out either of theDouble Gaussian, Single Gaussian and Uniform NS mass distribution models,although the mass distribution of the Galactic NSs is slightly preferred by thegravitational wave (GW) observations. The mass distribution of black holes(BHs) in the neutron star-black hole (NSBH) population is found to be similarto that for the Galactic X-ray binaries. Additionally, the ratio of the mergerrate densities between NSBHs and BNSs is estimated to be about 3 : 7. The spinproperties of the binaries, though constrained relatively poor, play nontrivialrole in reconstructing the mass distribution of NSs and BHs. We find that aperfectly aligned spin distribution can be ruled out, while a purely isotropicdistribution of spin orientation is still allowed.

Population properties of neutron stars in the coalescing compact binaries