0000000001212377

AUTHOR

Patrick Huber

showing 8 related works from this author

Non-standard interactions: Atmospheric versus neutrino factory experiments

2001

We consider the potential of a generic neutrino factory (NUFACT) in probing non-standard neutrino-matter interactions (NSI). We find that the sensitivity to flavour-changing (FC) NSI can be substantially improved with respect to present atmospheric neutrino data, especially at energies higher than approximately 50 GeV, where the effect of the tau mass is small. For example, a 100 GeV NUFACT can probe FC neutrino interactions at the level of few $|\epsilon| < {few} \times 10^{-4}$ at 99 % C.L.

PhysicsParticle physicsAtmospheric neutrinosNuclear and High Energy PhysicsNeutrino mass and mixingNeutrino oscillationsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyNeutrino factoryFOS: Physical sciencesFísicaHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino FactoryHigh Energy Physics::ExperimentSensitivity (control systems)Atmospheric neutrinoNeutrino
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Physics at a future Neutrino Factory and super-beam facility

2009

The conclusions of the Physics Working Group of the international scoping study of a future Neutrino Factory and super-beam facility (the ISS) are presented. The ISS was carried by the international community between NuFact05, (the 7th International Workshop on Neutrino Factories and Superbeams, Laboratori Nazionali di Frascati, Rome, June 21-26, 2005) and NuFact06 (Ivine, California, 24{30 August 2006). The physics case for an extensive experimental programme to understand the properties of the neutrino is presented and the role of high-precision measurements of neutrino oscillations within this programme is discussed in detail. The performance of second generation super-beam experiments, …

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Particle physicsPhysics::Instrumentation and DetectorsMUONIUM-ANTIMUONIUM CONVERSIONFOS: Physical sciencesGeneral Physics and Astronomyddc:500.2LONG-BASE-LINE01 natural sciences7. Clean energyWARM DARK-MATTERNuclear physicsLEPTON-FLAVOR VIOLATIONELECTRIC-DIPOLE MOMENTHigh Energy Physics - Phenomenology (hep-ph)Double beta decay0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]ANOMALOUS MAGNETIC-MOMENT010306 general physicsNeutrino oscillationNeutrino physics; Neutrino factoryParticle Physics - PhenomenologyR-PARITY VIOLATIONPhysicsMuonAnomalous magnetic dipole moment010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]LARGE EXTRA DIMENSIONSDOUBLE-BETA-DECAYNeutrino factoryFísicaMU-E CONVERSIONNeutrino physicsHigh Energy Physics - PhenomenologyExperimental High Energy PhysicsLarge extra dimensionCP violationPhysics::Accelerator PhysicsNeutrino FactoryHigh Energy Physics::ExperimentNeutrino
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NuSTEC White Paper: Status and challenges of neutrino–nucleus scattering

2018

International audience; The precise measurement of neutrino properties is among the highest priorities in fundamental particle physics, involving many experiments worldwide. Since the experiments rely on the interactions of neutrinos with bound nucleons inside atomic nuclei, the planned advances in the scope and precision of these experiments require a commensurate effort in the understanding and modeling of the hadronic and nuclear physics of these interactions, which is incorporated as a nuclear model in neutrino event generators. This model is essential to every phase of experimental analyses and its theoretical uncertainties play an important role in interpreting every result.In this Wh…

electron nucleus: interactionNuclear TheoryElementary particle7. Clean energy01 natural sciencesCROSS-SECTIONSScatteringHigh Energy Physics - Phenomenology (hep-ph)Nuclear Experimentneutrino: interactionCOHERENT PION-PRODUCTIONPhysicsstrong interactionElectroweak interactionModel; Neutrino; Nuclear; Nucleus; Oscillations; Scattering; Nuclear and High Energy PhysicsHigh Energy Physics - PhenomenologyMUON-NEUTRINONeutrinoNucleonnumerical calculations: Monte CarloNuclear and High Energy PhysicsParticle physicsOscillationsFORM-FACTORSProcess (engineering)FOS: Physical sciencesELECTROMAGNETIC RESPONSEnuclear modelNucleusMESON-EXCHANGE CURRENTSNNLO QCD ANALYSISCHARGED-CURRENT INTERACTIONSnuclear physicsdeep inelastic scattering0103 physical sciencesNeutrinoNuclear010306 general physicsneutrino nucleus: scatteringresonance: modelelectroweak interaction010308 nuclear & particles physicsR=SIGMA-L/SIGMA-Tneutrino nucleus: interactionDeep inelastic scatteringPhysics and Astronomy13. Climate actionINELASTIC ELECTRON-SCATTERING[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Atomic nucleusneutrino: oscillationEvent (particle physics)Model
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Antineutrino monitoring of spent nuclear fuel

2016

Military and civilian applications of nuclear energy have left a significant amount of spent nuclear fuel over the past 70 years. Currently, in many countries world wide, the use of nuclear energy is on the rise. Therefore, the management of highly radioactive nuclear waste is a pressing issue. In this letter, we explore antineutrino detectors as a tool for monitoring and safeguarding nuclear waste material. We compute the flux and spectrum of antineutrinos emitted by spent nuclear fuel elements as a function of time, and we illustrate the usefulness of antineutrino detectors in several benchmark scenarios. In particular, we demonstrate how a measurement of the antineutrino flux can help to…

010308 nuclear & particles physicsNuclear engineeringDetectorGeneral Physics and AstronomyFluxRadioactive wasteFOS: Physical sciences01 natural sciencesSpent nuclear fuel3. Good healthHigh Energy Physics - ExperimentOverburdenHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesElectromagnetic shieldingEnvironmental scienceNeutrinoNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentLeakage (electronics)
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Towards the european strategy for particle physics: The briefing book

2007

This document was prepared as part of the briefing material for the Workshop of the CERN Council Strategy Group, held in DESY Zeuthen from 2nd to 6th May 2006. It gives an overview of the physics issues and of the technological challenges that will shape the future of the field, and incorporates material presented and discussed during the Symposium on the European Strategy for Particle Physics, held in Orsay from 30th January to 2nd February 2006, reflecting the various opinions of the European community as recorded in written submissions to the Strategy Group and in the discussions at the Symposium.

High Energy Physics - TheoryParticle physicsANTIHYDROGENPhysics and Astronomy (miscellaneous)European communityNEUTRINO OSCILLATIONSFOS: Physical sciencesddc:500.2ACCELERATION01 natural sciencesELECTRON-BEAMSHigh Energy Physics - ExperimentENERGYHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]FIELD010306 general physicsEngineering (miscellaneous)Particle Physics - PhenomenologyPhysicsLarge Hadron Collider010308 nuclear & particles physicshep-exLHC LUMINOSITY UPGRADE[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Field (Bourdieu)hep-thFísicaDESYhep-phHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)LASER-PULSES[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]DOUBLE-BETA DECAY
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Can OPERA help in constraining neutrino non-standard interactions?

2008

We study how much the unique ability of the OPERA experiment to directly detect \nu_\tau can help in probing new, non-standard contact interactions of the third family of neutrinos. We perform a combined analysis of future, high-statistics MINOS and OPERA data. For the case of non-standard interactions in \nu_\mu to \nu_e transitions we also include the impact of possible DoubleCHOOZ data. In all cases we find that the \nu_\tau sample of OPERA is too small to be statistically significant, even if one doubles the nominal exposure of OPERA to 4.5E20 pot. OPERA's real benefit for this measurement lies in its very high neutrino energy and hence very different L/E compared to MINOS.

PhysicsNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsOperaHigh Energy Physics::PhenomenologyFísicaFOS: Physical sciencesElementary particleCHOOZNuclear physicsMassless particleHigh Energy Physics - PhenomenologyPhysics::Popular PhysicsHigh Energy Physics - Phenomenology (hep-ph)MINOSHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationParticle Physics - Phenomenology
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Confusing non-standard neutrino interactions with oscillations at a neutrino factory

2002

Most neutrino mass theories contain non-standard interactions (NSI) of neutrinos which can be either non-universal (NU) or flavor-changing (FC). We study the impact of such interactions on the determination of neutrino mixing parameters at a neutrino factory using the so-called ``golden channels'' \pnu{e}\to\pnu{\mu} for the measurement of \theta_{13}. We show that a certain combination of FC interactions in neutrino source and earth matter can give exactly the same signal as oscillations arising due to \theta_{13}. This implies that information about \theta_{13} can only be obtained if bounds on NSI are available. Taking into account the existing bounds on FC interactions, this leads to a …

PhysicsNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsHigh Energy Physics::PhenomenologyFísicaFOS: Physical sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Neutrino FactoryHigh Energy Physics::ExperimentSensitivity (control systems)NeutrinoNeutrino oscillationOrder of magnitudeMixing (physics)
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How sensitive is a neutrino factory to the angle Theta(13)?

2001

We consider the impact of non-standard interactions of neutrinos (NSI) on the determination of neutrino mixing parameters at a neutrino factory using $\pnu{e}\to\pnu{\mu}$ ``golden channels'' for the measurement of $\theta_{13}$. We show how a small residual NSI leads to a drastic loss in sensitivity in $\theta_{13}$, of up to two orders of magnitude. This can be somewhat overcome if two baselines are combined.

High Energy Physics - PhenomenologyFísicaHigh Energy Physics::Experiment
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