Search results for "methods"

showing 10 items of 4526 documents

The neutron background of the XENON100 dark matter search experiment

2013

TheXENON100 experiment, installed underground at the LaboratoriNazionali del Gran Sasso, aims to directly detect dark matter in the form of weakly interacting massive particles (WIMPs) via their elastic scattering off xenon nuclei. This paper presents a study on the nuclear recoil background of the experiment, taking into account neutron backgrounds from (alpha, n) reactions and spontaneous fission due to natural radioactivity in the detector and shield materials, as well as muon-induced neutrons. Based on MonteCarlo simulations and using measured radioactive contaminations of all detector components, we predict the nuclear recoil backgrounds for the WIMP search results published by theXENO…

Nuclear and High Energy PhysicsParticle physicsLarge Underground Xenon experimentPhysics::Instrumentation and DetectorsDark matterGeant4Astrophysics::Cosmology and Extragalactic AstrophysicsWIMP Argon Programme01 natural sciencesNuclear physicsWIMPNuclear and High Energy Physics Neutron Background Dark Matter Search XENON TPC0103 physical sciencesNeutron[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNuclear ExperimentGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)ComputingMilieux_MISCELLANEOUSSpontaneous fissionPhysicsElastic scatteringFluxMuons010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsDetectorsWeakly interacting massive particlesHigh Energy Physics::ExperimentSimulation
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Distribution Amplitudes of Heavy-Light Mesons

2019

A symmetry-preserving approach to the continuum bound-state problem in quantum field theory is used to calculate the masses, leptonic decay constants and light-front distribution amplitudes of empirically accessible heavy-light mesons. The inverse moment of the $B$-meson distribution is particularly important in treatments of exclusive $B$-decays using effective field theory and the factorisation formalism; and its value is therefore computed: $\lambda_B(\zeta = 2\,{\rm GeV}) = 0.54(3)\,$GeV. As an example and in anticipation of precision measurements at new-generation $B$-factories, the branching fraction for the rare $B\to \gamma(E_\gamma) \ell \nu_\ell$ radiative decay is also calculated…

Nuclear and High Energy PhysicsParticle physicsMesonNuclear TheoryAstrophysics::High Energy Astrophysical PhenomenaInverseFOS: Physical sciencesHeavy-light mesons01 natural sciencesParton distribution amplitudesNuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)High Energy Physics - Lattice0103 physical sciencesBound stateNonperturbative continuum methods in quantum field theoryEffective field theoryQuantum field theory010306 general physicsNuclear ExperimentQuantum chromodynamicsPhysics010308 nuclear & particles physicsBranching fractionHigh Energy Physics - Lattice (hep-lat)High Energy Physics::PhenomenologyB-meson decayslcsh:QC1-999High Energy Physics - PhenomenologyAmplitudeHigh Energy Physics::Experimentlcsh:PhysicsQuantum chromodynamics
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Neutral baryonic systems with strangeness

2020

We review the status as regards the existence of three- and four-body bound states made of neutrons and $\Lambda$ hyperons. For interesting cases, the coupling to neutral baryonic systems made of charged particles of different strangeness has been addressed. There are strong arguments showing that the $\Lambda nn$ system has no bound states. $\Lambda\Lambda nn$ strong stable states are not favored by our current knowledge of the strangeness $-1$ and $-2$ baryon-baryon interactions. However, a possible $\Xi^- t$ quasibound state decaying to $\Lambda\Lambda nn$ might exist in nature. Similarly, there is a broad agreement about the nonexistence of $\Lambda\Lambda n$ bound states. However, the …

Nuclear and High Energy PhysicsParticle physicsNuclear TheoryNuclear TheoryFOS: Physical sciencesGeneral Physics and AstronomyStrangenessFew-body systems01 natural sciencesNuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesBound stateComputer Science::General LiteratureNeutronNuclear Experiment010306 general physicsPhysics010308 nuclear & particles physicsComputer Science::Information RetrievalAstrophysics::Instrumentation and Methods for AstrophysicsHyperonComputer Science::Computation and Language (Computational Linguistics and Natural Language and Speech Processing)Charge (physics)BaryonHigh Energy Physics - PhenomenologyCoupling (physics)International Journal of Modern Physics E
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An improved method for measuring muon energy using the truncated mean of dE/dx

2012

Nuclear instruments & methods in physics research / A 703, 190 - 198 (2013). doi:10.1016/j.nima.2012.11.081

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsFOS: Physical sciencesddc:500.2Cherenkov; dE/dx; IceCube detector; Muon energy; Neutrino energy; Truncated mean53001 natural sciencesParticle detectorParticle identificationNuclear physicsdE/dx0103 physical sciencesSpecific energyddc:530CherenkovNeutrino energyInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsInstrumentationCherenkov radiationHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMuonTruncated meanMuon energy010308 nuclear & particles physicsDE/dxPhysics - Data Analysis Statistics and ProbabilityScintillation counterHigh Energy Physics::ExperimentNeutrinoIceCube detectorAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsData Analysis Statistics and Probability (physics.data-an)Lepton
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The ANTARES optical module

2001

The ANTARES collaboration is building a deep sea neutrino telescope in the Mediterranean Sea. This detector will cover a sensitive area of typically 0.1 km-squared and will be equipped with about 1000 optical modules. Each of these optical modules consists of a large area photomultiplier and its associated electronics housed in a pressure resistant glass sphere. The design of the ANTARES optical module, which is a key element of the detector, has been finalized following extensive R & D studies and is reviewed here in detail.

Nuclear and High Energy PhysicsPhotomultiplierAstrophysics and AstronomyPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeFOS: Physical sciencesAstrophysics01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsOptical Moduleneutrino astronomyHigh Energy Physics - Experiment (hep-ex)deep sea detector; neutrino astronomyMediterranean sea0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]14. Life underwaterElectronicsDetectors and Experimental Techniques010306 general physicsInstrumentationRemote sensingPhysics010308 nuclear & particles physicsDetectorAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for AstrophysicsNeutrino detectordeep sea detectorFísica nuclearNeutrino astronomy
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First tests of the applicability of gamma-ray imaging for background discrimination in time-of-flight neutron capture measurements

2015

In this work we explore for the first time the applicability of using $\gamma$-ray imaging in neutron capture measurements to identify and suppress spatially localized background. For this aim, a pinhole gamma camera is assembled, tested and characterized in terms of energy and spatial performance. It consists of a monolithic CeBr$_3$ scintillating crystal coupled to a position-sensitive photomultiplier and readout through an integrated circuit AMIC2GR. The pinhole collimator is a massive carven block of lead. A series of dedicated measurements with calibrated sources and with a neutron beam incident on a $^{197}$Au sample have been carried out at n_TOF, achieving an enhancement of a factor…

Nuclear and High Energy PhysicsPhotomultiplierPhysics - Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaNuclear physics01 natural scienceslaw.invention99-00Total energy detectorsOpticsData acquisitionRaigs gammalaw0103 physical sciencesγ-ray imagingmsc:00-01Detectors and Experimental TechniquesFacility n-tof010306 general physicsInstrumentationNuclear ExperimentNeutron capture cross-sectionsGamma cameraPhysicsNeutrons010308 nuclear & particles physicsbusiness.industryAstrophysics::Instrumentation and Methods for AstrophysicsTime-of-flight methodData-acquisition systemNeutron radiationSample (graphics)Pulse-height weighting techniqueNeutron captureTime of flightgamma-ray imagingCernPinhole (optics):Física::Física molecular [Àrees temàtiques de la UPC]Física nuclearbusinessSimulation
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The ANTARES Optical Beacon System

2007

ANTARES is a neutrino telescope being deployed in the Mediterranean Sea. It consists of a three dimensional array of photomultiplier tubes that can detect the Cherenkov light induced by charged particles produced in the interactions of neutrinos with the surrounding medium. High angular resolution can be achieved, in particular when a muon is produced, provided that the Cherenkov photons are detected with sufficient timing precision. Considerations of the intrinsic time uncertainties stemming from the transit time spread in the photomultiplier tubes and the mechanism of transmission of light in sea water lead to the conclusion that a relative time accuracy of the order of 0.5 ns is desirabl…

Nuclear and High Energy PhysicsPhotomultiplierPhysics::Instrumentation and Detectors[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesneutrino telescope; optical beacon; time calibrationAstrophysics01 natural scienceslaw.inventionTelescope[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Opticslaw0103 physical sciencesCalibrationtime calibrationAngular resolution14. Life underwateroptical beacon010306 general physicsInstrumentationCherenkov radiationPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]neutrino telescope time calibration optical beacon010308 nuclear & particles physicsbusiness.industryDetectorAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for Astrophysicsneutrino telescopeSITEAstronomyBeaconLIGHTFísica nuclearNeutrinobusiness
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Calibration and Characterization of the IceCube Photomultiplier Tube

2010

Over 5,000 PMTs are being deployed at the South Pole to compose the IceCube neutrino observatory. Many are placed deep in the ice to detect Cherenkov light emitted by the products of high-energy neutrino interactions, and others are frozen into tanks on the surface to detect particles from atmospheric cosmic ray showers. IceCube is using the 10-inch diameter R7081-02 made by Hamamatsu Photonics. This paper describes the laboratory characterization and calibration of these PMTs before deployment. PMTs were illuminated with pulses ranging from single photons to saturation level. Parameterizations are given for the single photoelectron charge spectrum and the saturation behavior. Time resoluti…

Nuclear and High Energy PhysicsPhotomultiplier[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhotonPhysics::Instrumentation and Detectors[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayContext (language use)AstrophysicsAetiology screening and detection [ONCOL 5]01 natural sciencesIceCube Neutrino Observatory[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Optics0103 physical sciencesNeutrinoCherenkovddc:530Instrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsInstrumentationCosmic raysCherenkov radiationPhysicsCherenkov; Cosmic rays; Ice; Neutrino; PMT010308 nuclear & particles physicsbusiness.industry[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]IceAstrophysics::Instrumentation and Methods for AstrophysicsPMTNeutrinoPhotonicsAstrophysics - Instrumentation and Methods for Astrophysicsbusiness
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Performance of the front-end electronics of the ANTARES neutrino telescope

2010

ANTARES is a high-energy neutrino telescope installed in the Mediterranean Sea at a depth of 2475 m. It consists of a three-dimensional array of optical modules, each containing a large photomultiplier tube. A total of 2700 front-end ASICs named Analogue Ring Samplers (ARS) process the phototube signals, measure their arrival time, amplitude and shape as well as perform monitoring and calibration tasks. The ARS chip processes the analogue signals from the optical modules and converts information into digital data. All the information is transmitted to shore through further multiplexing electronics and an optical link. This paper describes the performance of the ARS chip; results from the fu…

Nuclear and High Energy PhysicsPhotomultiplier[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics::Instrumentation and DetectorsOptical linkDigital dataFOS: Physical sciencesAnalog-to-digital converterNeutrino telescope01 natural sciencesMultiplexinglaw.inventionPhototubeApplication-specific integrated circuitPhotomultiplier tubelawASICs0103 physical sciences14. Life underwater010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)InstrumentationPhysics010308 nuclear & particles physicsbusiness.industryASICAstrophysics::Instrumentation and Methods for AstrophysicsElectrical engineeringCIRCUITFront-end electronicsChip[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Física nuclearUNDERWATER DETECTORasic; front-end electronics; neutrino telescope; photomultiplier tubeAstrophysics - Instrumentation and Methods for AstrophysicsbusinessSYSTEMNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Observation and applications of single-electron charge signals in the XENON100 experiment

2014

The XENON100 dark matter experiment uses liquid xenon in a time projection chamber (TPC) to measure xenon nuclear recoils resulting from the scattering of dark matter Weakly Interacting Massive Particles (WIMPs). In this paper, we report the observation of single-electron charge signals which are not related to WIMP interactions. These signals, which show the excellent sensitivity of the detector to small charge signals, are explained as being due to the photoionization of impurities in the liquid xenon and of the metal components inside the TPC. They are used as a unique calibration source to characterize the detector. We explain how we can infer crucial parameters for the XENON100 experim…

Nuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsDrift velocity[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics::Instrumentation and DetectorsDark matterchemistry.chemical_elementFOS: Physical sciencesdouble phase TPC01 natural sciencesdark matterHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)XenonWIMPdouble phase TPC; photoionization; single electron; xenon0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsphotoionizationInstrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsTime projection chamber010308 nuclear & particles physicsScatteringDetectorAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)single electron3. Good health[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]xenonchemistryWeakly interacting massive particlesAtomic physicsAstrophysics - Instrumentation and Methods for AstrophysicsJ. Phys.
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