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 show that a significant fraction of the energy of a gamma-ray burst(GRB)is probably converted to a burst of 10^{17}-10^{19} eV neutrinos and multipleGeV gammas that follow the GRB by > 10 s . If, as previously suggested, GRB'saccelerate protons to ~10^{20} eV, then both the neutrinos and the gammas maybe detectable.

Neutrino Afterglow from Gamma‐Ray Bursts: ∼1018eV

Neutrino Afterglow from Gamma‐Ray Bursts: ∼10¹⁸eV