Search results for " Oscillation"

showing 10 items of 845 documents

Search for a Lorentz-violating sidereal signal with atmospheric neutrinos in IceCube

2010

A search for sidereal modulation in the flux of atmospheric muon neutrinos in IceCube was performed. Such a signal could be an indication of Lorentz-violating physics. Neutrino oscillation models, derivable from extensions to the Standard Model, allow for neutrino oscillations that depend on the neutrino's direction of propagation. No such direction-dependent variation was found. A discrete Fourier transform method was used to constrain the Lorentz and CPT-violating coefficients in one of these models. Due to the unique high energy reach of IceCube, it was possible to improve constraints on certain Lorentz-violating oscillations by three orders of magnitude with respect to limits set by oth…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Nuclear and High Energy PhysicsParticle physicsMuonSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFOS: Physical sciencesSolar neutrino problemHigh Energy Physics - ExperimentStandard ModelHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Sidereal timeMeasurements of neutrino speedddc:530High Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaNeutrino oscillation
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Collective flavor transitions of supernova neutrinos

2009

We give a very brief overview of collective effects in neutrino oscillations in core collapse supernovae where refractive effects of neutrinos on themselves can considerably modify flavor oscillations, with possible repercussions for future supernova neutrino detection. We discuss synchronized and bipolar oscillations, the role of energy and angular neutrino modes, as well as three-flavor effects. We close with a short summary and some open questions.

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFOS: Physical sciencesAtomic and Molecular Physics and OpticsSupernovaHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino detectorHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationAstrophysics - High Energy Astrophysical PhenomenaFlavorParticle Physics - Phenomenology
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Analysis of the 4-year IceCube high-energy starting events

2016

After four years of data taking, the IceCube neutrino telescope has detected 54 high-energy starting events (HESE, or contained-vertex events) with deposited energies above 20TeV. They represent the first ever detection of high-energy extraterrestrial neutrinos and therefore, the first step in neutrino astronomy. In order to study the energy, flavor and isotropy of the astrophysical neutrino flux arriving at Earth, we perform different analyses of two different deposited energy intervals, [10 TeV $-$ 10 PeV] and [60 TeV $-$ 10 PeV]. We first consider an isotropic unbroken power-law spectrum and constrain its shape, normalization and flavor composition. Our results are in agreement with the …

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Particle physics010308 nuclear & particles physicsSolar neutrinomedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSolar neutrino problem01 natural sciencesAsymmetryHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino detector13. Climate action0103 physical sciencesMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyAstrophysics - High Energy Astrophysical Phenomena010306 general physicsNeutrino oscillationmedia_commonPhysical Review D
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CP and T violation in neutrino oscillations

2000

The conditions to induce appreciable CP-and T-odd effects in neutrino oscillations are discussed. The propagation in matter leads to fake CP-and CPT-odd asymmetries, besides a Bohm-Aharonov type modification of the interference pattern. We study the separation of fake and genuine CP violation by means of energy and distance dependence.

PhysicsHigh Energy Physics - PhenomenologyNuclear and High Energy PhysicsParticle physicsHigh Energy Physics - Phenomenology (hep-ph)FísicaCP violationFOS: Physical sciencesHigh Energy Physics::ExperimentNeutrino oscillationAtomic and Molecular Physics and OpticsEnergy (signal processing)
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Master Majorana neutrino mass parametrization

2019

After introducing a master formula for the Majorana neutrino mass matrix, we present a master parametrization for the Yukawa matrices automatically in agreement with neutrino oscillation data. This parametrization can be used for any model that induces Majorana neutrino masses. The application of the master parametrization is also illustrated in an example model, with special focus on its lepton flavor violating phenomenology.

PhysicsHistoryParticle physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyYukawa potentialFOS: Physical sciencesMass matrix01 natural sciencesComputer Science ApplicationsEducationHigh Energy Physics - PhenomenologyMAJORANAHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationPhenomenology (particle physics)ParametrizationLeptonJournal of Physics: Conference Series
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Links between CP violation in leptogenesis and low energy supersymmetry

2008

The seesaw mechanism makes leptogenesis a very attractive solution to the baryon asymmetry problem. If the baryon asymmetry of the Universe (BAU) was made via leptogenesis, any observation of CP violation in the lepton sector, for instance CP violation in neutrino oscillations, would support leptogenesis by demonstrating that CP is not a symmetry of leptons. The question is whether a stronger link exists between CP violation at low energies and leptogenesis. In our work we address this question, in the framework of a supersymmetric scenario where new constraints given by the low energy footprints of the high energy theory can be imposed, namely the current experimental bounds on lepton flav…

PhysicsHistoryParticle physicsHigh Energy Physics::PhenomenologySupersymmetrySymmetry (physics)Computer Science ApplicationsEducationBaryon asymmetrySeesaw mechanismLeptogenesisCP violationHigh Energy Physics::ExperimentNeutrino oscillationLeptonJournal of Physics: Conference Series
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The Capabilities of monochromatic EC neutrino beams with the SPS upgrade

2007

The goal for future neutrino facilities is the determination of the U(e3) mixing and CP violation in neutrino oscillations. This will require precision experiments with a very intense neutrino source and energy control. With this objective in mind, the creation of monochromatic neutrino beams from the electron capture decay of boosted ions by the SPS of CERN has been proposed. We discuss the capabilities of such a facility as a function of the energy of the boost and the baseline for the detector. We conclude that the SPS upgrade to 1000 GeV is crucial to reach a better sensitivity to CP violation iff it is accompanied by a longer baseline. We compare the physics potential for two different…

PhysicsHistoryParticle physicsLarge Hadron ColliderElectron capturePhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaDetectorFOS: Physical sciencesFísicaComputer Science ApplicationsEducationHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)UpgradeCP violationHigh Energy Physics::ExperimentMonochromatic colorNeutrinoNeutrino oscillation
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Implications of new generations on neutrino masses

2011

We explore the possible implications that new families, that are being searched for at the LHC, would have on neutrino masses. In particular, we have explored the possibility that the smallness of the observed neutrino masses is naturally understood in a modified version of the Standard Model (SM) with complete extra generations of fermions, i.e., that have right-handed neutrinos, in which neutrino masses are generated at two loops. With one extra family it is not possible to fit the observed spectrum of masses and mixings. However, the radiative mass generated provides an important constraint in these kind of models, so the neutrino masses do not exceed their cosmological bound. Within the…

PhysicsHistoryParticle physicsLarge Hadron ColliderPhysics::Instrumentation and DetectorsHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaContext (language use)FermionParameter spacePartícules (Física nuclear)Computer Science ApplicationsEducationStandard ModelHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Measurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillation
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Three-flavor neutrino oscillations and beyond

2020

Abstract In this work we summarize the current status of global neutrino oscillation analyses in the three-neutrino framework. We first describe the different data samples included in the global fit, emphasizing the role of each of them in constraining a given set of parameters. Next, we discuss the main improvements obtained thanks to the consideration of the latest experimental data. The status of the yet-unknown parameters, such as the true neutrino mass ordering, the Dirac CP-violating phase and the octant of the atmospheric mixing angle is also commented. Finally, we discuss some scenarios where the measurement of the reactor mixing angle or the CP violation phase could be significantl…

PhysicsHistoryParticle physicsNeutrino oscillationFlavorComputer Science ApplicationsEducationJournal of Physics: Conference Series
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Neutrino physics overview

2006

Seesaw-type and low-scale models of neutrino masses are reviewed, along with the corresponding structure of the lepton mixing matrix. The status of neutrino oscillation parameters as of June 2006 is given, including recent fluxes, as well as latest SNO, K2K and MINOS results. Some prospects for the next generation of experiments are given. This writeup updates the material presented in my lectures at the Corfu Summer Institute on Elementary Particle Physics in September 2005.

PhysicsHistoryParticle physicsPhysics::Instrumentation and DetectorsHigh Energy Physics::PhenomenologyPontecorvo–Maki–Nakagawa–Sakata matrixFOS: Physical sciencesFísicaComputer Science ApplicationsEducationElementary particle physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)MINOSHigh Energy Physics::ExperimentNeutrinoNeutrino oscillation
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