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Such scenarios can be constrained by existing measurements of the high-latitude gamma-ray background and the ultra-high energy cosmic ray spectrum, along with searches for ultra-high energy neutrinos by IceCube and other neutrino telescopes.

Also, we discuss RPV SUSY interpretations of the recent anomalous, upward-going EeV air showers observed at ANITA, in terms of long-lived charged or neutral next-to-lightest SUSY = $$ GeV) dark matter particles decaying in the halo of the Milky Way. Using the ultra-high energy neutrino events observed recently at IceCube, with the fact that for a given power-law flux of astrophysical neutrinos, there is no statistically significant deviation in the current data from the Standard Model expectations, we derive robust upper limits on the RPV couplings as a function of the resonantly-produced squark mass, independent of the other unknown model parameters, as long as the squarks decay dominantly to two-body final states involving leptons and quarks through the RPV couplings. The presence of RPV interactions involving ultra-high energy neutrinos with Earth-matter can lead to resonant production of TeV-scale SUSY partners of the SM quarks and leptons (squarks and sleptons), thereby giving rise to potentially anomalous behavior in the event spectrum observed by large-volume neutrino detectors, such as IceCube, as well as balloon-borne cosmic ray experiments, such as ANITA. We make new theoretical and observational contributions. It was started by the astroparticle physicist Elisa Resconi from the Technical University of Munich in 2017. Here we focus on a new event class for neutrino telescopes: dimuons, two energetic muons from one neutrino interaction. The Pacific Ocean Neutrino Experiment (P-ONE) is an initiative towards constructing a multi-cubic-kilometre neutrino telescope in the Pacific Ocean to expand our observable window of the Universe to the highest energies. Their power is increased when they can isolate different event classes, e.g., by flavor, though that is not the only possibility.

NEUTRINO TELESCOPES DOWNLOAD

We review the prospects of probing $$R$$-parity violating Supersymmetry (RPV SUSY) at neutrino telescopes using some of the highest energy particles given to us by Nature. Neutrino telescopes are powerful probes of high-energy astrophysics and particle physics. Download Citation Neutrino Telescopes This paper addresses the working principle of neutrino telescopes, important detector parameters as well as the layout and performance of current.