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

Ultralight bosons are promising dark matter candidates and can triggersuperradiant instabilities of spinning black holes (BHs), resulting inlong-lived rotating "bosonic clouds" around the BHs and dissipating theirenergy through the emission of monochromatic gravitational waves (GWs). Wefocus on the scalar bosons minimally coupled with both isolated stellar-originBHs (SBH) and their binary merger remnants, and perform Bayesian data analysisto search for the stochastic GW background from all the unstable modes that cantrigger the superradiant instabilities using the data of Advanced LIGO andAdvanced Virgo's first three observing runs. We find no evidence for suchsignal, and hence rule out the scalar bosons within the mass range $[1.5,16]\times10^{-13}$ eV, $[1.9, 8.3]\times10^{-13}$ eV and $[1.3,17]\times10^{-13}$ eV at $95\%$ confidence level for isolated SBHs having auniform dimensionless spin distribution in $[0,1]$, $[0,0.5]$ and $[0.5,1]$,respectively.

physical review. d/physical review. d.

Constraints on the ultralight scalar boson from Advanced LIGO and  Advanced Virgo's first three observing runs using the stochastic  gravitational-wave background