Search results for " Detectors"

showing 10 items of 2027 documents

Implications of a dark matter-neutrino coupling at hyper-kamiokande

2018

Dark matter and neutrinos provide the two most compelling pieces of evidence for new physics beyond the Standard Model of Particle Physics but they are often treated as two different sectors. In this paper, we consider how neutrino observables can be used to constrain the parameter space of different models where active neutrinos interact with DM via mediators of different spins. We study for the first time the sensitivity of the Hyper-Kamiokande detector to neutrinos produced from MeV Dark Matter annihilation. In particular, we find that thermally produced DM candidates with masses between 15-30 MeV could be fully excluded.

High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Physics::Instrumentation and DetectorsHigh Energy Physics::PhenomenologyFOS: Physical sciencesHigh Energy Physics::Experiment
researchProduct

Neutrinos: Fast & Curious

2016

The Standard Model has been effective way beyond expectations in foreseeing the result of almost all the experimental tests done up so far. In it, neutrinos are massless. Nonetheless, in recent years we have collected solid proofs indicating little but non zero masses for the neutrinos (when contrasted with those of the charged leptons). These masses permit neutrinos to change their flavor and oscillate, indeed a unique treat. In these lectures, I discuss the properties and the amazing potential of neutrinos in and beyond the Standard Model.

High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Physics::Instrumentation and DetectorsHigh Energy Physics::PhenomenologyFOS: Physical sciencesHigh Energy Physics::ExperimentParticle Physics - Phenomenology
researchProduct

N-Delta(1232) axial form factors from weak pion production

2010

The N Delta axial form factors are determined from neutrino induced pion production ANL and BNL data by using a theoretical model that accounts both for background mechanisms and deuteron effects. We find violations of the off-diagonal Goldberger-Treiman relation at the level of 2 sigma which might have an impact in background calculations for T2K and MiniBooNE low energy neutrino oscillation precision experiments.

High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Physics::Instrumentation and DetectorsNuclear TheoryFOS: Physical sciencesFísicaHigh Energy Physics::ExperimentNuclear Experiment
researchProduct

Measuring Leptonic CP Violation with a Water Cerenkov

2006

In this talk, we present the physics case for a megaton Water Cerenkov detector in addressing some of the still pending questions in neutrino oscillations physics, particularly the measurement of leptonic CP violation. We compare different future beams that could profit from a water detector and analyse, for the case $\theta_{13} \approx 3^\circ$ (the limit that can be reached by under-construction experiments), the signal-to-background rate for a $\beta$-beam setup with the radioactive ions accelerated to $\gamma = 350$.

High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Physics::Instrumentation and DetectorsPhysics::Accelerator PhysicsFOS: Physical sciencesHigh Energy Physics::Experiment
researchProduct

Measuring anomalous couplings in H -> WW* decays at the International Linear Collider

2010

The measurement of the Higgs coupling to W bosons is an important test of our understanding of the electroweak symmetry-breaking mechanism. We study the sensitivity of the International Linear Collider (ILC) to the presence of anomalous HW+W- couplings using ZH -> nu(nu) over bar WW* -> nu(nu) over bar 4j events. Using an effective Lagrangian approach, we calculate the differential decay rates of the Higgs boson including the effects of new dimension-five operators. We present a Monte Carlo simulation of events at the ILC, using a full detector simulation based on GEANT4 and a real event reconstruction chain. Expected constraints on the anomalous couplings are given.

High Energy Physics - PhenomenologyPhysics::Instrumentation and DetectorsHigh Energy Physics::PhenomenologyHiggs-bosonFísicaHigh Energy Physics::ExperimentLHCHigh Energy Physics - Experiment
researchProduct

Searching for neutrino oscillation parameters in long baseline experiments

2016

Vihonen, Sampsa "Searching for neutrino oscillation parameters in long baseline experiments" in Proceedings, Magellan Workshop: Connecting Neutrino Physics and Astronomy / Dahmke, Stefan K.G., Meyer, Mikko, Vanhoefer, Laura (eds.), Deutsches Elektronen-Synchrotron, DESY : 2016 ; Magellan Workshop, 2016-03-17 - 2016-03-18, Hamburg Magellan Workshop, Hamburg, Germany, 17 Mar 2016 - 18 Mar 2016 ; DESY-PROC 65-70(2016). doi:10.3204/DESY-PROC-2016-05/8

High Energy Physics - Phenomenologyneutrino oscillationsHigh Energy Physics - Phenomenology (hep-ph)Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::Phenomenologylong baseline neutrino experimentsFOS: Physical sciencesHigh Energy Physics::Experiment
researchProduct

Ultrahigh-energy neutrino flux as a probe of large extra dimensions

2007

A suppression in the spectrum of ultrahigh-energy (UHE, >= 10^{18} eV) neutrinos will be present in extra-dimensional scenarios, due to enhanced neutrino-antineutrino annihilation processes with the supernova relic neutrinos. In the n>4 scenario, being n the number of extra dimensions, neutrinos can not be responsible for the highest energy events observed in the UHE cosmic ray spectrum. A direct implication of these extra-dimensional interactions would be the absence of UHE neutrinos in ongoing and future neutrino telescopes.

High Energy Physics - TheoryAstrofísicaParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxCosmic rayAstrophysics01 natural sciences7. Clean energyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesUltrahigh energy010306 general physicsPhysicsAnnihilation010308 nuclear & particles physicsAstrophysics (astro-ph)High Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysics3. Good healthHigh Energy Physics - PhenomenologySupernovaExtra dimensionsHigh Energy Physics - Theory (hep-th)13. Climate actionLarge extra dimensionHigh Energy Physics::ExperimentNeutrinoJournal of Cosmology and Astroparticle Physics
researchProduct

Dirac neutrinos from Peccei-Quinn symmetry: a fresh look at the axion

2019

We show that a very simple solution to the strong CP problem naturally leads to Dirac neutrinos. Small effective neutrino masses emerge from a type-I Dirac seesaw mechanism. Neutrino mass limits probe the axion parameters in regions currently inaccessible to conventional searches.

High Energy Physics - TheoryJob creationPhysicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyGeneral Physics and AstronomyLibrary scienceFOS: Physical sciencesAstronomy and Astrophysics01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)0103 physical sciencesChristian ministryHigh Energy Physics::Experiment010306 general physicsAstrophysics - Cosmology and Nongalactic Astrophysics
researchProduct

Reloading the Axion in a 3-3-1 setup

2020

We generalize the idea of the axion to an extended electroweak gauge symmetry setup. We propose a minimal axion extension of the Singer-Valle-Schechter (SVS) theory, in which the standard model fits in $\mathrm{SU(3)_L\otimes U(1)_X}$, the number of families results from anomaly cancellation, and the Peccei-Quinn (PQ) solution to the strong-CP problem is implemented. Neutrino masses arise from a type-I Dirac seesaw mechanism, suppressed by the ratio of SVS and PQ scales, suggesting the existence of new physics at a moderate SVS scale. Novel features include an enhanced axion coupling to photons when compared to the DFSZ axion, as well as flavour-changing axion couplings to quarks.

High Energy Physics - TheoryNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsPhysics beyond the Standard ModelFOS: Physical sciencesStandard ModelHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics::TheoryAxionHigh Energy Physics - Phenomenology (hep-ph)Peccei-Quinn symmetryNeutrinosAxionGauge symmetryPhysicsElectroweak interactionHigh Energy Physics::Phenomenologylcsh:QC1-999High Energy Physics - PhenomenologySeesaw mechanismHigh Energy Physics - Theory (hep-th)Anomaly (physics)Neutrinolcsh:Physics
researchProduct

Decoherent neutrino mixing, dark energy, and matter-antimatter asymmetry

2004

A CPT violating decoherence scenario can easily account for all the experimental evidence in the neutrino sector including LSND. In this work it is argued that this framework can also accommodate the Dark Energy content of the Universe, as well as the observed matter-antimatter asymmetry.

High Energy Physics - TheoryPhysics::General PhysicsNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsCPT symmetrymedia_common.quotation_subjectFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyCosmologyNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)Neutrino oscillationComputer Science::Databasesmedia_commonPhysicsHigh Energy Physics::PhenomenologyFísicaUniverseHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Neutrino detectorAntimatterDark energyHigh Energy Physics::ExperimentNeutrinoPhysical Review D
researchProduct