0000000000826485

AUTHOR

Manuel Masip

showing 2 related works from this author

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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Heavy sterile neutrinos in stellar core-collapse

2018

We perform spherically symmetric simulations of the core collapse of a single progenitor star of zero age main sequence mass $M_{\rm ZAMS} = 15 \, M_{\odot}$ with two models of heavy sterile neutrinos in the mass range of hundred MeV$/c^2$. According to both models, these hypothetical particles are copiously produced in the center, stream outwards a subsequently decay releasing energy into final states (including neutrinos) of the Standard Model. We find that they can lead to a successful explosion in otherwise non-exploding progenitors. Depending on their unknown parameters (e.g., mass and coupling constants with matter), we obtain either no explosion or an explosion of one of two types, i…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSterile neutrino010308 nuclear & particles physicsStar (game theory)Astrophysics::High Energy Astrophysical PhenomenaCenter (category theory)FOS: Physical sciencesAstrophysicsType (model theory)01 natural sciences7. Clean energyStandard ModelSupernovaHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Astrophysics - Solar and Stellar Astrophysics0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsNeutrinoAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Energy (signal processing)Astrophysics::Galaxy Astrophysics
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