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

In 2012 the IceCube detector observed the first clear detection of a diffuse astrophysical high energy neutrino flux, however, the sources for these neutrinos have yet to be found. Hadronic interactions around cosmic ray accelerators result in both high energy gamma and neutrino fluxes from the decay of neutral and charged pion respectively. Observing gamma ray sources with neutrinos provides unique evidence of the hadronic nature of these sources. These searches involve looking for a significant clustering of neutrinos from any direction or a correlation with a known source observed by other messengers also expected to emit a neutrino flux. These searches range from stacking populations of similar sources such as active galactic nuclei, to time-dependent searches targeting individual sources when they are in flaring states. We present here the most recent updates in the search for sources of extraterrestrial neutrinos using the latest methods and source information.

A Summary of Recent Updates in the Search for Cosmic Ray Sources using the IceCube Detector