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/

Zendy Plus

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

Zendy Tools

Zendy Open

Highest energy neutrino events (contained) in cubic km ICECUBE detectorresulted in last three years to be as many as $37-2=35$ signals (two of thosehaving been recently discharged); these tens-hundred TeV (32 energetic events)up to rarest (only 3) PeV cascade showers, proved to have an extraterrestrialorigin. The UHE neutrino flavor transition from a $\nu_{\mu}$ atmosphericdominance (over $\nu_{e}$ showers at TeV energy), toward a higher energy showercascade ($\nu_{e}$, $\nu_{\tau}$) events at few tens TeV up to PeV energy is ahint of such a fast extraterrestrial injection. The majority (28 out of 35) ofall these events are spherical cascade; their consequent smeared map isinconclusive. The additional rarest $9-2=7$ muon tracks, while being sharp inarrival directions, did not offer any correlated clustering nor any overlappingwithin known sources. We recently suggested that the highest energy (tens-TeV)crossing muon along the ICECUBE, mostly at horizons or upcoming, are the idealtool able to reveal soon such clustering or even any narrow angle pointing toknown (IR, X, Radio or $\gamma$) sources or self-correlation in rare doublet ortriplet: a last hope for a meaningful and short-time $\nu$ Astronomy. Anycrossing muons clustering along galactic sources or within UHECR arrivals mightalso probe rarest UHECR event made by nuclei or neutrons. Within three years ofICECUBE data all the non-contained crossing highest energy muons above few tensTeV may be several dozens, possibly around $54$ (27 for upward ones), mostlyenhanced along horizontal edges, painting known sources and/or self-correlatingin doublets or rarest triplet (if steady or transient nearby source are atsight). Recent preliminary ICECUBE presentation on crossing muons areconsistent with present preliminary muon rate estimate.

Crossing muons in Icecube at highest energy: Cornerstone to neutrino astronomy