Search results for "Instrumentation"

showing 10 items of 4914 documents

Commissioning of the CALIFA Barrel Calorimeter of the R3B Experiment at FAIR

2020

5 pags., 4 figs. -- FAIRNESS2019: FAIR NExt generation ScientistS 20-24 May 2019, Arenzano, Genova, Italy

PhysicsPaperHistoryHigh energyPhysics - Instrumentation and DetectorsCalorimeter (particle physics)business.industryPhysics::Instrumentation and DetectorsDetectorBarrel (horology)FOS: Physical sciencesInstrumentation and Detectors (physics.ins-det)ScintillatorComputer Science ApplicationsEducationddc:OpticsNuclear Experiment (nucl-ex)businessNuclear Experiment
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Rare Z Decays and Neutrino Flavor Universality

2015

We study rare four-body decays of the Z-boson involving at least one neutrino and one charged lepton. Large destructive interferences make these decays very sensitive to the Z couplings to neutrinos. As the identified charged leptons can determine the neutrino flavors, these decays probe the universality of the Z couplings to neutrinos. The rare four-body processes could be accurately measured at future lepton colliders, leading to percent level precision.

PhysicsParticle physics010308 nuclear & particles physicsPhysics::Instrumentation and DetectorsPhysics beyond the Standard ModelSolar neutrinoHigh Energy Physics::PhenomenologyFOS: Physical sciencesSolar neutrino problem01 natural sciencesUniversality (dynamical systems)Nuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesMeasurements of neutrino speedddc:530High Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationLepton
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Flux limits on ultra high energy neutrinos with AMANDA-B10

2005

Abstract Data taken during 1997 with the AMANDA-B10 detector are searched for a diffuse flux of neutrinos of all flavors with energies above 10 16  eV. At these energies the Earth is opaque to neutrinos, and thus neutrino induced events are concentrated at the horizon. The background are large muon bundles from down-going atmospheric air shower events. No excess events above the background expectation are observed and a neutrino flux following E −2 , with an equal mix of all flavors, is limited to E 2 Φ (10 15  eV  E 18  eV) ⩽ 0.99 × 10 −6  GeV cm −2  s −1  sr −1 at 90% confidence level. This is the most restrictive experimental bound placed by any neutrino detector at these energies. Bound…

PhysicsParticle physicsAMANDAMuonPhysics::Instrumentation and DetectorsUHE neutrinosAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoHigh Energy Physics::PhenomenologyFluxAstronomy and AstrophysicsSolar neutrino problemAMANDA; Neutrino astronomy; Neutrino telescopes; UHE neutrinosNeutrino detectorNeutrino astronomyMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyNeutrino telescopes
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Neutrino mass ordering at DUNE: An extra ν bonus

2019

We study the possibility of extracting the neutrino mass ordering at the future Deep Underground Neutrino Experiment using atmospheric neutrinos, which will be available before the muon neutrino beam starts being perational. The large statistics of the atmospheric muon neutrino and antineutrino samples at the far detector, together with the baselines of thousands of kilometers that these atmospheric (anti)neutrinos travel, provide the ideal ingredients to extract the neutrino mass ordering via matter effects in the neutrino propagation through the Earth. Crucially, muon capture by Argon provides excellent charge-tagging, allowing to disentangle the neutrino and antineutrino signature. This …

PhysicsParticle physicsArgonTime projection chamber010308 nuclear & particles physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaDetectorHigh Energy Physics::Phenomenologychemistry.chemical_element01 natural sciences7. Clean energyHigh Energy Physics - ExperimentMuon captureHigh Energy Physics - Phenomenologychemistry13. Climate action0103 physical sciencesDeep Underground Neutrino ExperimentMuon neutrinoHigh Energy Physics::ExperimentNeutrino010306 general physicsBeam (structure)Physical Review D
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The MuPix high voltage monolithic active pixel sensor for the Mu3e experiment

2015

Mu3e is a novel experiment searching for charged lepton flavor violation in the rare decay μ → eee. In order to reduce background by up to 16 orders of magnitude, decay vertex position, decay time and particle momenta have to be measured precisely. A pixel tracker based on 50 μm thin high voltage monolithic active pixel sensors (HV-MAPS) in a magnetic field will deliver precise vertex and momentum information. Test beam results like an excellent efficiency of >99.5% and a time resolution of better than 16.6 ns obtained with the MuPix HV-MAPS chip developed for the Mu3e pixel tracker are presented.

PhysicsParticle physicsCMOS sensorElectronic detector readout concepts (solid-state)PixelPhysics::Instrumentation and Detectorsbusiness.industryHigh voltageChipElectronic detector readout concepts (solid-state); Particle tracking detectors (solidstate detectors)Magnetic fieldVertex (geometry)OpticsHigh Energy Physics::Experimentddc:610Electric potentialDetectors and Experimental TechniquesParticle tracking detectors (solidstate detectors)ddc:620businessInstrumentationParticle Physics - ExperimentMathematical PhysicsEngineering & allied operationsLepton
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Neutrino Unification

2000

Present neutrino data are consistent with neutrino masses arising from a common seed at some ``neutrino unification'' scale $M_X$. Such a simple theoretical ansatz naturally leads to quasi-degenerate neutrinos that could lie in the electron-volt range with neutrino mass splittings induced by renormalization effects associated with supersymmetric thresholds. In such a scheme the leptonic analogue of the Cabibbo angle $\theta_{\odot}$ describing solar neutrino oscillations is nearly maximal. Its exact value is correlated with the smallness of $\theta_{reactor}$. These features agree both with latest data on the solar neutrino spectra and with the reactor neutrino data. The two leading mass-ei…

PhysicsParticle physicsCabibbo–Kobayashi–Maskawa matrixPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyGeneral Physics and AstronomyFísicaFOS: Physical sciencesScale (descriptive set theory)530Spectral lineRenormalizationHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Double beta decayHigh Energy Physics::ExperimentNeutrinoAnsatz
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Parameter Degeneracy in Flavor-Dependent Reconstruction of Supernova Neutrino Fluxes

2008

We reexamine the possibility of reconstructing the initial fluxes of supernova neutrinos emitted in a future core-collapse galactic supernova explosion and detected in a Megaton-sized water Cherenkov detector. A novel key element in our method is the inclusion, in addition to the total and the average energies of each neutrino species, of a "pinching" parameter characterizing the width of the distribution as a fit parameter. We uncover in this case a continuous degeneracy in the reconstructed parameters of supernova neutrino fluxes at the neutrinosphere. We analyze in detail the features of this degeneracy and show how it occurs irrespective of the parametrization used for the distribution …

PhysicsParticle physicsCherenkov detectorPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFísicaFOS: Physical sciencesAstronomy and Astrophysicslaw.inventionSupernovaHigh Energy Physics - PhenomenologyDistribution (mathematics)Distribution functionHigh Energy Physics - Phenomenology (hep-ph)lawNeutrinoDegeneracy (mathematics)Parametrization
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Analysis method for detecting topological defect dark matter with a global magnetometer network

2019

Abstract The Global Network of Optical Magnetometers for Exotic physics searches (GNOME) is a network of time-synchronized, geographically separated, optically pumped atomic magnetometers that is being used to search for correlated transient signals heralding exotic physics. GNOME is sensitive to exotic couplings of atomic spins to certain classes of dark matter candidates, such as axions. This work presents a data analysis procedure to search for axion dark matter in the form of topological defects: specifically, walls separating domains of discrete degenerate vacua in the axion field. An axion domain wall crossing the Earth creates a distinctive signal pattern in the network that can be d…

PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Field (physics)Spins010308 nuclear & particles physicsMagnetometerDark matterFOS: Physical sciencesAstronomy and Astrophysics01 natural sciencesTopological defectlaw.inventionDomain wall (string theory)Space and Planetary Sciencelaw0103 physical sciencesAstrophysics - Instrumentation and Methods for Astrophysics010303 astronomy & astrophysicsAxionInstrumentation and Methods for Astrophysics (astro-ph.IM)GnomeAstrophysics - Cosmology and Nongalactic Astrophysics
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Resurrection of large lepton number asymmetries from neutrino flavor oscillations

2016

We numerically solve the evolution equations of neutrino three-flavor density matrices, and show that, even if neutrino oscillations mix neutrino flavors, large lepton number asymmetries are still allowed in certain limits by Big Bang Nucleosynthesis (BBN).

PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics::Instrumentation and Detectors010308 nuclear & particles physicsHigh Energy Physics::LatticeAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFOS: Physical sciences01 natural sciencesLepton numberNuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesis0103 physical sciencesMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationFlavorAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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Neutrino mass in supersymmetry

2009

10 páginas, 8 figuras.-- El PDF es la versión pre-print (arXiv:0911.3103v1).-- Trabajo presentado al SUSY09: 7th International Conference on Supersymmetry and the Unification of Fundamental Interactions.

PhysicsParticle physicsLarge Hadron Collider010308 nuclear & particles physicsPhysics::Instrumentation and DetectorsHigh Energy Physics::PhenomenologyFOS: Physical sciencesContext (language use)Supersymmetry01 natural sciencesHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometryR-parity0103 physical sciencesHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationMixing (physics)
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