Search results for " Detectors"

showing 10 items of 2027 documents

Mass number scaling in ultra-relativistic nuclear collisions from a hydrodynamical approach

1998

We study the different nucleus-nucleus collisions, O+Au, S+S, S+Ag, S+Au and Pb+Pb, at the CERN-SPS energy in a one-fluid hydrodynamical approach using a parametrization based on baryon stopping in terms of the thickness of colliding nuclei. Good agreement with measured particle spectra is achieved. We deduce the mass number scaling behaviour of the initial energy density. We find that the equilibration time is nearly independent of the size of the colliding nuclei.

PhysicsMass numberNuclear TheoryPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsNuclear TheoryFOS: Physical sciencesSpectral lineNuclear Theory (nucl-th)Nuclear physicsBaryonBaryon densityEnergy densityParticleHigh Energy Physics::ExperimentAtomic physicsNuclear ExperimentEngineering (miscellaneous)ParametrizationScalingThe European Physical Journal C
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Observables sensitive to absolute neutrino masses. II

2008

In this followup to Phys. Rev. D 75, 053001 (2007) [arXiv:hep-ph/0608060] we report updated constraints on neutrino mass-mixing parameters, in light of recent neutrino oscillation data (KamLAND, SNO, and MINOS) and cosmological observations (WMAP 5-year and other data). We discuss their interplay with the final 0nu2beta decay results in 76-Ge claimed by part of the Heidelberg-Moscow Collaboration, using recent evaluations of the corresponding nuclear matrix elements, and their uncertainties. We also comment on the 0nu2beta limits in 130-Te recently set by Cuoricino, and on prospective limits or signals from the KATRIN experiment.

PhysicsMass numberNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsAstrophysics (astro-ph)Cosmic background radiationFOS: Physical sciencesAstrophysicsCMB cold spotHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)MINOSDouble beta decayHigh Energy Physics::ExperimentSensitivity (control systems)Nuclear Experiment (nucl-ex)NeutrinoNeutrino oscillationNuclear ExperimentPhysical Review D
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Possible pulsed gamma ray emission above 50 MeV from the Crab pulsar.

1970

A SEARCH for pulsed gamma ray emission from NP 0532 has been carried out with a balloon-borne experiment using a spark chamber as the central detector. This pulsar, situated in the Crab Nebula, is already known to pulsate in the radio, optical and X-ray range1–5.

PhysicsMultidisciplinaryPhysics::Instrumentation and DetectorsCrab PulsarAstrophysics::High Energy Astrophysical PhenomenaDetectorAstrophysics::Instrumentation and Methods for AstrophysicsGamma rayAstronomyAstrophysicsCrab NebulaPulsarSpark chamberGamma detectionNature
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Lepton mass effects for beam-normal single-spin asymmetry in elastic muon-proton scattering

2019

We estimate the beam-normal single-spin asymmetry in elastic lepton-proton scattering without employing the ultrarelativistic approximation. Our calculation is relevant for analyses of muon scattering at energies of few hundred MeV and below -- when effects of the muon mass become essential. At such energies, the transverse polarization of the muon beam is expected to contribute significantly to the systematic uncertainty of precision measurements of elastic muon-proton scattering. We evaluate such systematics using an example of the MUSE experiment at PSI. The muon asymmetry is estimated at about 0.1\% in kinematics of MUSE and it is the largest for scattering into a backward hemisphere.

PhysicsMuon010308 nuclear & particles physicsScatteringPhysics::Instrumentation and Detectorsmedia_common.quotation_subjectFOS: Physical sciencesKinematicsPolarization (waves)01 natural sciencesAsymmetryNuclear physicsTransverse planeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Proton scattering0103 physical sciencesPhysics::Accelerator PhysicsHigh Energy Physics::Experiment010306 general physicsNuclear ExperimentLeptonmedia_common
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The muon magnetic moment

1981

Muon mass and muon magnetic moment are not calculabIe within the theory of Quantum Eiectrodynamics; they rather define the reference acaie in which masses and energies should be determined when muons are used to test QED or to search for anomalous muon coupiings which couid provide the "raison d'@tre" for the muon. Oniy the anomaious part of the muon magnetic moment experimentaily determined with remarkable precision I), can be oaIculated 2~" Theory and experiment agree preciseiy once corrections being appiied for hadronic and weak processes which poiiute the immaculated fieid of QED at high momentum transfers. Muon mass and muon magnetic moment are, in particular, needed for the interpreta…

PhysicsMuonAnomalous magnetic dipole momentNeutron magnetic momentPhysics::Instrumentation and DetectorsMuoniumMuon spin spectroscopyElectron magnetic dipole momentSpin magnetic momentNuclear physicsNuclear magnetic momentPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentPhysics::Atomic Physics
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High-multiplicity neutron events registered by NEMESIS experiment

2021

Neutron-induced interactions contribute to the signal-mimicking background in deep-underground searches for exotic phenomena such as Dark Matter, neutrino-less double beta decay, proton decay, etc. Apart from radioactive decay, the primary source of neutrons underground are high-energy muons from cosmic showers. While the maximum number of fission neutrons is around six and energies around one MeV, muon-induced interactions may generate hundreds of neutrons, also with high energies. Furthermore, these processes are not yet reproduced in numerical simulations with sufficient reliability. The main goal of the NEMESIS experiment is to improve our knowledge and understanding of cosmic muon-indu…

PhysicsMuonCOSMIC cancer databaseProton decayPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaDark matterNuclear TheoryneutronithiukkasfysiikkaHigh multiplicityNuclear physicsDouble beta decayNeutronHigh Energy Physics::Experimentfysiikkaradioaktiivinen säteilyydinfysiikkaNuclear ExperimentRadioactive decay
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Magnetic order and local field distribution in the hybrid magnets [FeCp*(2)][MnCr(ox)(3)] and [CoCp*(2)][FeFe(ox)(3)]: a muon spin relaxation study

2016

Zero-field muon spin relaxation (μ+SR) measurements on materials from the series [ZIIICp*2][M IIMIII(ox)3] show precession signals at several frequencies, characteristic of quasistatic magnetic fields at up to three distinct muon sites.

PhysicsMuonCondensed matter physicsPhysics::Instrumentation and DetectorsMagnetRelaxation (NMR)Materials ChemistryPrecessionGeneral ChemistryMuon spin spectroscopyLocal fieldQuasistatic processMagnetic field
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The ATLAS level-1 trigger: Status of the system and experience from commissioning with cosmic ray muons

2007

The detector at CERN's large hadron collider (LHC) was exposed to proton-proton collisions from beams crossing at 40 MHz. A three-level trigger system will select potentially interesting events in order to reduce this rate to 100- 200 Hz. A trigger decision is made by the Level-1 central trigger processor (CTP) reducing the incoming rate to less than 100 kHz. The Level-1 decision is based on calorimeter information and hits in dedicated muon trigger detectors. The final Level-1 trigger system is currently being installed in the experiment with completion expected in autumn 2007. Cosmic ray data are regularly recorded as an increasing fraction of the trigger system comes online. We present a…

PhysicsMuonLarge Hadron ColliderCalorimeter (particle physics)Physics::Instrumentation and DetectorsReal-time computingDetectorCosmic rayNuclear physicsmedicine.anatomical_structureAtlas (anatomy)Nuclear electronicsSystems architecturemedicinePhysics::Accelerator Physics2007 IEEE Nuclear Science Symposium Conference Record
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Measurement of Azimuthal Anisotropy of Muons from Charm and Bottom Hadrons in pp Collisions at s=13  TeV with the ATLAS Detector

2020

The elliptic flow of muons from the decay of charm and bottom hadrons is measured in pp collisions at sqrt[s]=13  TeV using a data sample with an integrated luminosity of 150  pb^{-1} recorded by the ATLAS detector at the LHC. The muons from heavy-flavor decay are separated from light-hadron decay muons using momentum imbalance between the tracking and muon spectrometers. The heavy-flavor decay muons are further separated into those from charm decay and those from bottom decay using the distance-of-closest-approach to the collision vertex. The measurement is performed for muons in the transverse momentum range 4-7 GeV and pseudorapidity range |η|<2.4. A significant nonzero elliptic anisotro…

PhysicsMuonLarge Hadron ColliderPhysics::Instrumentation and DetectorsHigh Energy Physics::PhenomenologyElliptic flowHadronGeneral Physics and Astronomy01 natural sciencesNuclear physicsPseudorapidity0103 physical sciencesQuark–gluon plasmaPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentRapidityImpact parameterNuclear Experiment010306 general physicsPhysical Review Letters
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Optical response of highly reflective film used in the water Cherenkov muon veto of the XENON1T dark matter experiment

2017

The XENON1T experiment is the most recent stage of the XENON Dark Matter Search, aiming for the direct detection of Weakly Interacting Massive Particles (WIMPs). To reach its projected sensitivity, the background has to be reduced by two orders of magnitude compared to its predecessor XENON100. This requires a water Cherenkov muon veto surrounding the XENON1T TPC, both to shield external backgrounds and to tag muon-induced energetic neutrons through detection of a passing muon or the secondary shower induced by a muon interacting in the surrounding rock. The muon veto is instrumented with $84$ $8"$ PMTs with high quantum efficiency (QE) in the Cherenkov regime and the walls of the watertank…

PhysicsMuonPhysics - Instrumentation and Detectors010308 nuclear & particles physicsPhysics::Instrumentation and DetectorsDark matterVetoFOS: Physical sciencesInstrumentation and Detectors (physics.ins-det)01 natural sciencesNuclear physics0103 physical sciencesAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsInstrumentationMathematical PhysicsCherenkov radiation
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