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 Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

High-energy neutrino (HEN) and gravitational wave (GW) can probeastrophysical sources in addition to electromagnetic observations.Multimessenger studies can reveal nature of the sources which may not bediscerned from one type of signal alone. We discuss HEN emission in connectionwith the Advanced Laser Interferometer Gravitational-wave Observatory (ALIGO)event GW150914 which could be associated with a short gamma-ray burst (GRB)detected by the $Fermi$ Gamma-ray Burst Monitor (GBM) 0.4 s after the GW eventand within localization uncertainty of the GW event. We calculate HEN flux fromthis short GRB, GW150914-GBM, and show that non-detection of a high-energystarting event (HESE) by the IceCube Neutrino Observatory can constrain thetotal isotropic-equivalent jet energy of this short burst to be less than$3\times 10^{52}$ erg.

High Energy Neutrinos from the Gravitational Wave event GW150914 possibly associated with a short Gamma-Ray Burst