Search results for "Measurements"

showing 10 items of 720 documents

A neutron spectrometer for studying giant resonances with (p, n) reactions in inverse kinematics

2014

A neutron spectrometer, the European Low-Energy Neutron Spectrometer (ELENS), has been constructed to study exotic nuclei in inverse-kinematics experiments. The spectrometer, which consists of plastic scintillator bars, can be operated in the neutron energy range of 100 keV to 10 MeV. The neutron energy is determined using the time-of-flight technique, while the position of the neutron detection is deduced from the time-difference information from photomultipliers attached to both ends of each bar. A novel wrapping method has been developed for the plastic scintillators. The array has a larger than 25% detection efficiency for neutrons of approximately 500 keV in kinetic energy and an angul…

Nuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsELENSPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryFOS: Physical sciencesScintillator01 natural sciences7. Clean energyNeutron time-of-flight scatteringNuclear physicsDETECTOR ARRAYVM2000 wrappingSCINTILLATORS0103 physical sciencesNeutron detectionNeutronNeutron time-of-flight measurementsNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentInstrumentationNuclear ExperimentLow-energy neutron spectrometerPhysicsBonner sphereSpectrometer010308 nuclear & particles physicsCOUNTERSInstrumentation and Detectors (physics.ins-det)Neutron temperature3. Good healthScintillation counterFísica nuclear
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Measurements of the T2K neutrino beam properties using the INGRID on-axis near detector

2012

Precise measurement of neutrino beam direction and intensity was achieved based on a new concept with modularized neutrino detectors. INGRID (Interactive Neutrino GRID) is an on-axis near detector for the T2K long baseline neutrino oscillation experiment. INGRID consists of 16 identical modules arranged in horizontal and vertical arrays around the beam center. The module has a sandwich structure of iron target plates and scintillator trackers. INGRID directly monitors the muon neutrino beam profile center and intensity using the number of observed neutrino events in each module. The neutrino beam direction is measured with accuracy better than 0.4 mrad from the measured profile center. The …

Nuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsNeutrino oscillationPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical Phenomenaon-axis near detectorFOS: Physical sciencesddc:500.201 natural sciences7. Clean energyNeutrino oscillation; on-axis near detectorneutrino oscillation; neutrino detector; wavelength shifting fiber; t2k; extruded scintillator; neutrino beamNeutrino detectorNuclear physicsNeutrino beamneutrino beam0103 physical sciencesExtruded scintillatorMuon neutrinoneutrino oscillation[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationInstrumentationT2KPhysicst2k010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyNeutrino oscillation; T2K; Neutrino beam; Neutrino detector; Extruded scintillator; Wavelength shifting fiberT2K experimentextruded scintillatorFísicaInstrumentation and Detectors (physics.ins-det)Neutrino detectorneutrino detectorWavelength shiftingfiberMeasurements of neutrino speedPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNeutrinoBeam (structure)Leptonwavelength shifting fiber
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Energy calibration of the NEXT-White detector with 1% resolution near Q ββ of 136Xe

2019

Excellent energy resolution is one of the primary advantages of electroluminescent high pressure xenon TPCs, and searches for rare physics events such as neutrinoless double-beta decay ($\beta\beta0\nu$) require precise energy measurements. Using the NEXT-White detector, developed by the NEXT (Neutrino Experiment with a Xenon TPC) collaboration, we show for the first time that an energy resolution of 1% FWHM can be achieved at 2.6 MeV, establishing the present technology as the one with the best energy resolution of all xenon detectors for $\beta\beta0\nu$ searches.

Nuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsPhysical measurementsPhysics::Instrumentation and DetectorsDark Matter and Double Beta DecayFísica -- Mesuramentschemistry.chemical_elementBioengineeringAtomic01 natural sciencesMathematical SciencesNuclear physicsParticle and Plasma PhysicsXenonAffordable and Clean Energy0103 physical sciencesDark Matter and Double Beta Decay (experiments)CalibrationNuclearlcsh:Nuclear and particle physics. Atomic energy. RadioactivityCalibratge010306 general physicsMathematical PhysicsPhysicsQuantum Physics010308 nuclear & particles physicsDetectorResolution (electron density)MolecularDetectorsNuclear & Particles PhysicsFull width at half maximumchemistryBeta (plasma physics)Physical SciencesCalibrationlcsh:QC770-798High Energy Physics::ExperimentNeutrinoEnergy (signal processing)
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Detecting the upturn of the solar 8B neutrino spectrum with LENA

2014

LENA ( L ow E nergy N eutrino A stronomy) has been proposed as a next generation 50 kt liquid scintillator detector. The large target mass allows a high precision measurement of the solar 8 B neutrino spectrum, with an unprecedented energy threshold of 2 MeV. Hence, it can probe the MSW-LMA prediction for the electron neutrino survival probability in the transition region between vacuum and matter-dominated neutrino oscillations. Based on Monte Carlo simulations of the solar neutrino and the corresponding background spectra, it was found that the predicted upturn of the solar 8 B neutrino spectrum can be detected with 5 σ significance after 5 years.

Nuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsSolar neutrinoSolar neutrinosFOS: Physical sciencesAstrophysicsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Neutrino oscillationInstrumentation and Methods for Astrophysics (astro-ph.IM)Solar and Stellar Astrophysics (astro-ph.SR)PhysicsHigh Energy Physics::PhenomenologyInstrumentation and Detectors (physics.ins-det)Solar neutrino problemlcsh:QC1-999ddc:Neutrino detectorAstrophysics - Solar and Stellar AstrophysicsMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyAstrophysics - Instrumentation and Methods for AstrophysicsElectron neutrinolcsh:PhysicsPhysics Letters B
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Oscillation effects on high-energy neutrino fluxes from astrophysical hidden sources

2006

High-energy neutrinos are expected to be produced in a vareity of astrophysical sources as well as in optically thick hidden sources. We explore the matter-induced oscillation effects on emitted neutrino fluxes of three different flavors from the latter class. We use the ratio of electron and tau induced showers to muon tracks, in upcoming neutrino telescopes, as the principal observable in our analysis. This ratio depends on the neutrino energy, density profile of the sources and on the oscillation parameters. The largely unknown flux normalization drops out of our calculation and only affects the statistics. For the current knowledge of the oscillation parameters we find that the matter-i…

Nuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics01 natural sciences7. Clean energyPartícules (Física nuclear)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationPhysicsMuon010308 nuclear & particles physicsOscillationAstrophysics (astro-ph)Solar neutrino problemHigh Energy Physics - PhenomenologyNeutrino detector13. Climate actionMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino
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Charge radii of neon isotopes across the sd neutron shell

2011

We report on the changes in mean square charge radii of unstable neon nuclei relative to the stable Ne-20, based on the measurement of optical isotope shifts. The studies were carried out using collinear laser spectroscopy on a fast beam of neutral neon atoms. High sensitivity on short-lived isotopes was achieved thanks to nonoptical detection based on optical pumping and state-selective collisional ionization, which was complemented by an accurate determination of the beam kinetic energy. The new results provide information on the structural changes in the sequence of neon isotopes all across the neutron sd shell, ranging from the proton drip line nucleus and halo candidate Ne-17 up to the…

Nuclear and High Energy PhysicsProtonNuclear Theoryquadrupole collectivitychemistry.chemical_elementXXargon isotopesNeonCharge radiusrich nucleiNeutronPhysics::Atomic PhysicsNuclear Experimentcluster statesMagic number (physics)Physicslaser-spectroscopy measurementssodium isotopesIsland of inversionintruder configurationsmean-field theorychemistryIsotopes of neonlight-nucleiAtomic physicsmass shiftNucleon
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If sterile neutrinos exist, how can one determine the total solar neutrino fluxes?

2002

The 8B solar neutrino flux inferred from a global analysis of solar neutrino experiments is within 11% (1 sigma) of the predicted standard solar model value if only active neutrinos exist, but could be as large as 1.7 times the standard prediction if sterile neutrinos exist. We show that the total 8B neutrino flux (active plus sterile neutrinos) can be determined experimentally to about 10% (1 sigma) by combining charged current measurements made with the KamLAND reactor experiment and with the SNO CC solar neutrino experiment, provided the LMA neutrino oscillation solution is correct and the simulated performance of KamLAND is valid. Including also SNO NC data, the sterile component of the…

Nuclear and High Energy PhysicsSterile neutrinoParticle physicsAstrofísica nuclearNuclear TheoryPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinosFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energyHigh Energy Physics - ExperimentPhysics::GeophysicsNuclear Theory (nucl-th)Nuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Neutrins solars0103 physical sciencesNuclear Experiment (nucl-ex)010306 general physicsNeutrino oscillationNuclear ExperimentBorexinoPhysics010308 nuclear & particles physicsAstrophysics (astro-ph)High Energy Physics::PhenomenologyFísicaSolar neutrino problemHigh Energy Physics - PhenomenologyNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNuclear astrophysicsNeutrino
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Heavy neutrino searches at the lhc with displaced vertices

2013

Sterile neutrinos with masses in the range (1-100) GeV, have been searched for in a variety of experiments. Here, we discuss the prospects to search for sterile neutrinos at the LHC using displaced vertices. Two different cases are discussed: (i) the standard model extended with sterile neutrinos and (ii) right-handed neutrinos in a left-right symmetric extension of the standard model. A dedicated displaced vertex search will allow to probe parts of the parameter space not accessible to other searches, but will require large luminosity in both cases.

Nuclear and High Energy PhysicsSterile neutrinoParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesParameter space01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationPhysicsLarge Hadron Collider010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaVertex (geometry)High Energy Physics - PhenomenologyMeasurements of neutrino speedHigh Energy Physics::ExperimentHeavy neutrinoNeutrino
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High-precision electron-capture Q value measurement of 111In for electron-neutrino mass determination

2022

A precise determination of the ground state $^{111}$In ($9/2^+$) electron capture to ground state of $^{111}$Cd ($1/2^+$) $Q$ value has been performed utilizing the double Penning trap mass spectrometer, JYFLTRAP. A value of 857.63(17) keV was obtained, which is nearly a factor of 20 more precise than the value extracted from the Atomic Mass Evaluation 2020 (AME2020). The high-precision electron-capture $Q$ value measurement along with the nuclear energy level data of 866.60(6) keV, 864.8(3) keV, 855.6(10) keV, and 853.94(7) keV for $^{111}$Cd was used to determine whether the four states are energetically allowed for a potential ultra-low $Q$-value $\beta^{}$ decay or electron-capture deca…

Nuclear and High Energy PhysicsmassaspektrometriaNeutrino massUltra-low Q valueAstrophysics::High Energy Astrophysical PhenomenaPenning trapneutriinotFOS: Physical sciencesNuclear Experiment (nucl-ex)ydinfysiikkaNuclear ExperimentMass measurementsElectron capturePhysics Letters B
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Isosinglet-neutral heavy-lepton production in Z-decays and neutrino mass

1990

Abstract The possible existence of NHLs is often related to neutrino mass. As a result their production cross section may be correspondingly constrained by observational limits on neutrino masses. We analyze the discovery potential of isosinglet NHLs within various models taking also into account cosmological limits on relic neutrino abundances.

Nuclear physicsPhysicsNuclear and High Energy PhysicsCross section (physics)Particle physicsHigh Energy Physics::PhenomenologyMeasurements of neutrino speedHigh Energy Physics::ExperimentSolar neutrino problemNeutrinoNeutrino oscillationLeptonNuclear Physics B
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