Search results for "neutrino nucleon: interaction"

showing 2 items of 2 documents

Neutrino oscillation studies with IceCube-DeepCore

2016

IceCube, a gigaton-scale neutrino detector located at the South Pole, was primarily designed to search for astrophysical neutrinos with energies of PeV and higher. This goal has been achieved with the detection of the highest energy neutrinos to date. At the other end of the energy spectrum, the DeepCore extension lowers the energy threshold of the detector to approximately 10 GeV and opens the door for oscillation studies using atmospheric neutrinos. An analysis of the disappearance of these neutrinos has been completed, with the results produced being complementary with dedicated oscillation experiments. Following a review of the detector principle and performance, the method used to make…

Physics::Instrumentation and DetectorsSolar neutrinopoleinteraction [neutrino nucleon]PINGU01 natural sciences7. Clean energyneutrino nucleon: interactionIceCubeenergy: thresholdAstronomi astrofysik och kosmologineutrino: atmosphereAstronomy Astrophysics and Cosmologydetector [neutrino]Physicsneutrino: energy spectrumoscillation [neutrino]Astrophysics::Instrumentation and Methods for Astrophysicsatmosphere [neutrino]threshold [energy]mass difference [neutrino]Cosmic neutrino backgroundneutrino: detectorNeutrino detectorPhysique des particules élémentairesMeasurements of neutrino speedNeutrinoperformanceNuclear and High Energy PhysicsParticle physicsAstrophysics::High Energy Astrophysical Phenomenaneutrino: mass differenceddc:500.2530neutrino: energySOUTH-POLE0103 physical sciencesddc:530010306 general physicsNeutrino oscillation010308 nuclear & particles physicsICEenergy spectrum [neutrino]Solar neutrino problemneutrino: mixing anglePhysics and Astronomyenergy [neutrino]High Energy Physics::Experimentneutrino: oscillationNeutrino astronomyMATTERSYSTEMmixing angle [neutrino]experimental results
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The Pros and Cons of Beyond Standard Model Interpretations of ANITA Events

2019

The Antarctic Impulsive Transient Antenna (ANITA) experiment has observed two air shower events with energy $\sim 500~{\rm PeV}$ emerging from the Earth with exit angles $\sim 30^\circ$ above the horizon. As was immediately noted by the ANITA Collaboration, these events (in principle) could originate in the atmospheric decay of an upgoing $\tau$-lepton produced through a charged current interaction of a $\nu_\tau$ inside the Earth. However, the relatively steep arrival angles of these perplexing events create tension with the standard model (SM) neutrino-nucleon interaction cross section. Deepening the conundrum, the IceCube neutrino telescope and the Pierre Auger Observatory with substanti…

airAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesparticle: messengerAstrophysics01 natural scienceshorizonneutrino nucleon: interactioncharged currentIceCubeHigh Energy Physics - Phenomenology (hep-ph)Observatory0103 physical sciences010306 general physicsCharged currentHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger Observatoryneutrino/tauCOSMIC cancer databaseshowers: atmosphere010308 nuclear & particles physicsHorizonANITAAstrophysics::Instrumentation and Methods for AstrophysicstensionsensitivityAugerfluxobservatoryHigh Energy Physics - Phenomenologyneutrino: detectorAir showerNeutrino detector[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Astrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Event (particle physics)Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)
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