0000000000186243

AUTHOR

J. Salvado

showing 4 related works from this author

High intensity neutrino oscillation facilities in Europe

2013

The EUROnu project has studied three possible options for future, high intensity neutrino oscillation facilities in Europe. The first is a Super Beam, in which the neutrinos come from the decay of pions created by bombarding targets with a 4 MW proton beam from the CERN High Power Superconducting Proton Linac. The far detector for this facility is the 500 kt MEMPHYS water Cherenkov, located in the Frejus tunnel. The second facility is the Neutrino Factory, in which the neutrinos come from the decay of mu(+) and mu(-) beams in a storage ring. The far detector in this case is a 100 kt magnetized iron neutrino detector at a baseline of 2000 km. The third option is a Beta Beam, in which the neu…

Nuclear and High Energy PhysicsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and Detectors[PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph]7. Clean energy01 natural sciencesNuclear physicsneutrino0103 physical sciencesEmmaFysiklcsh:Nuclear and particle physics. Atomic energy. Radioactivityddc:530010306 general physicsNeutrino oscillationQCAstroparticle physicsPhysicsLarge Hadron ColliderBeta-Beam010308 nuclear & particles physicsFísicaSurfaces and InterfacesAccelerators and Storage RingsNeutrino detectorPhysical Scienceslcsh:QC770-798Physics::Accelerator PhysicsNeutrino FactoryHigh Energy Physics::ExperimentNeutrino[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Storage ringLepton
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Fundamental physics with high-energy cosmic neutrinos today and in the future

2019

The astrophysical neutrinos discovered by IceCube have the highest detected neutrino energies --- from TeV to PeV --- and likely travel the longest distances --- up to a few Gpc, the size of the observable Universe. These features make them naturally attractive probes of fundamental particle-physics properties, possibly tiny in size, at energy scales unreachable by any other means. The decades before the IceCube discovery saw many proposals of particle-physics studies in this direction. Today, those proposals have become a reality, in spite of astrophysical unknowns. We will showcase examples of doing fundamental neutrino physics at these scales, including some of the most stringent tests o…

High Energy Astrophysical Phenomena (astro-ph.HE)High Energy Physics - Theoryastro-ph.HEhep-exAstrophysics::High Energy Astrophysical Phenomenahep-thAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical scienceshep-phHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)High Energy Physics::ExperimentAstrophysics - High Energy Astrophysical Phenomena
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Searches for Sterile Neutrinos with the IceCube Detector

2016

The IceCube neutrino telescope at the South Pole has measured the atmospheric muon neutrino spectrum as a function of zenith angle and energy in the approximate 320 GeV to 20 TeV range, to search for the oscillation signatures of light sterile neutrinos. No evidence for anomalous $\nu_\mu$ or $\bar{\nu}_\mu$ disappearance is observed in either of two independently developed analyses, each using one year of atmospheric neutrino data. New exclusion limits are placed on the parameter space of the 3+1 model, in which muon antineutrinos would experience a strong MSW-resonant oscillation. The exclusion limits extend to $\mathrm{sin}^2 2\theta_{24} \leq$ 0.02 at $\Delta m^2 \sim$ 0.3 $\mathrm{eV}^…

Particle physicsSterile neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Physics and Astronomy01 natural sciencesHigh Energy Physics - ExperimentMiniBooNENuclear physicsHigh Energy Physics - Experiment (hep-ex)Physics and Astronomy (all)0103 physical sciencesOSCILLATIONSddc:550Muon neutrino010306 general physicsNeutrino oscillationZenithHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMuon010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyMODELNeutrino detectorPhysics and Astronomy13. Climate actionHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical PhenomenaEnergy (signal processing)SYSTEM
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Testable Baryogenesis in Seesaw Models (NuFact 2016)

2016

We revisit the production of baryon asymmetries in the minimal type I seesaw model with heavy Majorana singlets in the GeV range. We include "washout" effects from scattering processes with gauge bosons, higgs decays and inverse decays, besides the dominant top scatterings. We show that in the minimal model with two singlets, and for an inverted light neutrino ordering, future measurements from SHiP and neutrinoless double beta decay could in principle provide sufficient information to predict the matter-antimatter asymmetry in the universe.

High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics::PhenomenologyFOS: Physical sciencesHigh Energy Physics::Experiment
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