Search results for " Instrumentation."

showing 10 items of 712 documents

Acoustic transmitters for underwater neutrino telescopes.

2012

In this paper acoustic transmitters that were developed for use in underwater neutrino telescopes are presented. Firstly, an acoustic transceiver has been developed as part of the acoustic positioning system of neutrino telescopes. These infrastructures are not completely rigid and require a positioning system in order to monitor the position of the optical sensors which move due to sea currents. To guarantee a reliable and versatile system, the transceiver has the requirements of reduced cost, low power consumption, high pressure withstanding (up to 500 bars), high intensity for emission, low intrinsic noise, arbitrary signals for emission and the capacity of acquiring and processing recei…

Physics - Instrumentation and DetectorsPositioning systemparametric sourcesFOS: Physical sciencesUnderwater neutrino telescopesacoustic transceiver; sensor array; underwater neutrino telescopes; calibration; positioning systems; parametric sourcessensor arraylcsh:Chemical technology01 natural sciencesBiochemistrySignalArticleAnalytical ChemistryPositioning systemsSensor array0103 physical sciencesAcoustic transceiverElectronic engineeringlcsh:TP1-118514. Life underwaterElectrical and Electronic EngineeringInstrumentation and Methods for Astrophysics (astro-ph.IM)010301 acousticsInstrumentationSensor arrayPhysics010308 nuclear & particles physicsTransmitterParametric sourcespositioning systemsInstrumentation and Detectors (physics.ins-det)calibrationAtomic and Molecular Physics and OpticsNoiseacoustic transceiverNeutrino detectorFISICA APLICADACalibrationNeutrinoAstrophysics - Instrumentation and Methods for Astrophysicsunderwater neutrino telescopesUnderwater acoustic communicationSensors (Basel, Switzerland)
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Comparison of proton shower developments in the BGO calorimeter of the Dark Matter Particle Explorer between GEANT4 and FLUKA simulations

2020

The DArk Matter Particle Explorer (DAMPE) is a satellite-borne detector for high-energy cosmic rays and $\gamma$-rays. To fully understand the detector performance and obtain reliable physical results, extensive simulations of the detector are necessary. The simulations are particularly important for the data analysis of cosmic ray nuclei, which relies closely on the hadronic and nuclear interactions of particles in the detector material. Widely adopted simulation softwares include the GEANT4 and FLUKA, both of which have been implemented for the DAMPE simulation tool. Here we describe the simulation tool of DAMPE and compare the results of proton shower properties in the calorimeter from t…

Physics - Instrumentation and DetectorsProton85Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHadronDark matterS-General Physics and AstronomyFOS: Physical sciencesCosmic rayNuclear physicsSpectral analysisInstrumentation and Methods for Astrophysics (astro-ph.IM)Monte Carlo simulationPhysicsTp9550Calorimeter (particle physics)96DetectorInstrumentation and Detectors (physics.ins-det)5513Cosmic Rays-n-tParticleHigh Energy Physics::ExperimentAstrophysics - Instrumentation and Methods for Astrophysics
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Relative luminosity measurement of the LHC with the ATLAS forward calorimeter

2010

In this paper it is shown that a measurement of the relative luminosity changes at the LHC may be obtained by analysing the currents drawn from the high voltage power supplies of the electromagnetic section of the forward calorimeter of the ATLAS detector. The method was verified with a reproduction of a small section of the ATLAS forward calorimeter using proton beams of known beam energies and variable intensities at the U-70 accelerator at IHEP in Protvino, Russia. The experimental setup and the data taking during a test beam run in April 2008 are described in detail. A comparison of the measured high voltage currents with reference measurements from beam intensity monitors shows a linea…

Physics - Instrumentation and DetectorsProtonPhysics::Instrumentation and DetectorsFOS: Physical sciences01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Atlas (anatomy)0103 physical sciencesmedicineDetectors and Experimental Techniques010306 general physicsInstrumentationMathematical PhysicsPhysicsLarge Hadron ColliderLuminosity (scattering theory)Calorimeter (particle physics)010308 nuclear & particles physicsHigh voltageInstrumentation and Detectors (physics.ins-det)medicine.anatomical_structurePhysics::Accelerator PhysicsBeam (structure)Intensity (heat transfer)
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The pulsed neutron beam EDM experiment

2018

International audience; We report on the Beam EDM experiment, which aims to employ a pulsed cold neutron beam to search for an electric dipole moment instead of the established use of storable ultracold neutrons. We present a brief overview of the basic measurement concept and the current status of our proof-of-principle Ramsey apparatus.

Physics - Instrumentation and DetectorsQC1-999measurement methodsFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesbeam: pulsedPhysics::Atomic Physics010306 general physicsNuclear Experimentactivity reportPhysicsn: electric moment010308 nuclear & particles physicsPhysicsInstrumentation and Detectors (physics.ins-det)Neutron radiationElectric dipole momentn: beam[PHYS.PHYS.PHYS-INS-DET] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Ultracold neutronsPhysics::Accelerator PhysicsCurrent (fluid)Beam (structure)
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The DArk Matter Particle Explorer mission

2017

The DArk Matter Particle Explorer (DAMPE), one of the four scientific space science missions within the framework of the Strategic Pioneer Program on Space Science of the Chinese Academy of Sciences, is a general purpose high energy cosmic-ray and gamma-ray observatory, which was successfully launched on December 17th, 2015 from the Jiuquan Satellite Launch Center. The DAMPE scientific objectives include the study of galactic cosmic rays up to $\sim 10$ TeV and hundreds of TeV for electrons/gammas and nuclei respectively, and the search for dark matter signatures in their spectra. In this paper we illustrate the layout of the DAMPE instrument, and discuss the results of beam tests and calib…

Physics - Instrumentation and DetectorsSatellite launchesGamma ray observatoriesAstrophysicsGalactic cosmic rays01 natural sciencesCosmologyHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)ObservatoryDetectors and Experimental TechniquesCosmic rays dark matter space experiments010303 astronomy & astrophysicsphysics.ins-detSpace science missionsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)CosmologyCosmology Galaxies Gamma rays Tellurium compounds Chinese Academy of Sciences Dark matter particles Explorer missions Galactic cosmic rays Gamma ray observatories Satellite launches Scientific objectives Space science missions Cosmic raysSpace ScienceAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaParticle Physics - ExperimentAstrophysics and AstronomyAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesCosmic raydark matterTellurium compounds0103 physical sciencesCosmic raysInstrumentation and Methods for Astrophysics (astro-ph.IM)010308 nuclear & particles physicshep-exGamma raysAstronomyAstronomy and AstrophysicsGalaxiesChinese academy of sciencesGalaxyScientific objectivesDark matter particlesChinese Academy of SciencesSatellitespace experimentsExplorer missionsastro-ph.IM
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New opportunities for kaonic atoms measurements from CdZnTe detectors

2023

We present the tests performed by the SIDDHARTA-2 collaboration at the DA{\Phi}NE collider with a quasi-hemispherical CdZnTe detector. The very good room-temperature energy resolution and efficiency in a wide energy range show that this detector technology is ideal for studying radiative transitions in intermediate and heavy-mass kaonic atoms. The CdZnTe detector was installed for the first time in an accelerator environment to perform tests on the background rejection capabilities, which were achieved by exploiting the SIDDHARTA-2 Luminosity Monitor. A spectrum with an $^{241}Am$ source has been acquired, with beams circulating in the main rings, and peak resolutions of 6% at 60 keV and of…

Physics - Instrumentation and DetectorsSettore FIS/01 - Fisica SperimentaleFOS: Physical sciencesInstrumentation and Detectors (physics.ins-det)CZT detectorkaonic atomsSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)
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Solar neutrino detection in liquid xenon detectors via charged-current scattering to excited states

2020

We investigate the prospects for real-time detection of solar neutrinos via the charged-current neutrino-nucleus scattering process in liquid xenon time projection chambers. We use a nuclear shell model, benchmarked with experimental data, to calculate the cross sections for populating specific excited states of the caesium nuclei produced by neutrino capture on $^{131}$Xe and $^{136}$Xe. The shell model is further used to compute the decay schemes of the low-lying $1^{+}$ excited states of $^{136}$Cs, for which there is sparse experimental data. We explore the possibility of tagging the characteristic de-excitation $\gamma$-rays/conversion electrons using two techniques: spatial separation…

Physics - Instrumentation and DetectorsSolar neutrinochemistry.chemical_elementFOS: Physical sciencesksenonhiukkasfysiikka7. Clean energy01 natural sciencesnucleus-neutrino interactionsHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)XenonHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesSensitivity (control systems)010306 general physicsPhysics010308 nuclear & particles physicsNuclear shell modelshell modelneutriinotInstrumentation and Detectors (physics.ins-det)nuclear structure and decays3. Good healthProjection (relational algebra)High Energy Physics - PhenomenologychemistryilmaisimetExcited statesolar neutrinosNeutrinoydinfysiikkaEnergy (signal processing)
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NEXT, high-pressure xenon gas experiments for ultimate sensitivity to Majorana neutrinos

2012

In this paper we describe an innovative type of Time Projection Chamber (TPC), which uses high-pressure xenon gas (HPXe) and electroluminescence amplification of the ionization charge as the basis of an apparatus capable of fully reconstructing the energy and topological signature of rare events. We will discuss a specific design of such HPXe TPC, the NEXT-100 detector, that will search for neutrinoless double beta decay events using 100-150 kg of xenon enriched in the isotope Xe-136. NEXT-100 is currently under construction, after completion of an accelerated and very successful R&D period. It will be installed at the Laboratorio Subterr��neo de Canfranc (LSC), in Spain. The commission…

Physics - Instrumentation and DetectorsTime projection chamber010308 nuclear & particles physicschemistry.chemical_elementFOS: Physical sciencesInstrumentation and Detectors (physics.ins-det)7. Clean energy01 natural sciencesParticle detectorHigh Energy Physics - ExperimentMassless particleNuclear physicsHigh Energy Physics - PhenomenologyMAJORANAHigh Energy Physics - Experiment (hep-ex)XenonHigh Energy Physics - Phenomenology (hep-ph)chemistry0103 physical sciencesIsotopes of xenonNeutrino010306 general physicsInstrumentationMathematical PhysicsLepton
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The Next White (NEW) detector

2018

[EN] Conceived to host 5 kg of xenón at a pressure of 15 bar in the ¿ducial volume,the NEXTWhite (NEW)apparatus is currently the largest high pressure xenon gas TPC using electroluminescent ampli¿cation in the world. It is also a 1:2 scale model of the NEXT-100 detector scheduled to start searching for ßß0¿ decays in 136Xe in 2019. Both detectors measure the energy of the event using a plane of photomultipliers located behind a transparent cathode. They can also reconstruct the trajectories of charged tracks in the dense gas of the TPC with the help of a plane of silicon photomultipliers located behind the anode. A sophisticated gas system, common to both detectors, allows the high gas puri…

Physics - Instrumentation and DetectorsXenon010308 nuclear & particles physicsEuropean researchLibrary scienceFOS: Physical sciencesInstrumentation and Detectors (physics.ins-det)7. Clean energy01 natural sciencesHigh-pressure xenon chambersTECNOLOGIA ELECTRONICATime Projection Chamber (TPC)Political science0103 physical sciencesmedia_common.cataloged_instanceEuropean unionNeutrinoless double beta decay010306 general physicsInstrumentationMathematical Physicsmedia_commonNEXT-100 experiment
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Search for WIMP Inelastic Scattering off Xenon Nuclei with XENON100

2017

We present the first constraints on the spin-dependent, inelastic scattering cross section of weakly interacting massive particles (WIMPs) on nucleons from XENON100 data with an exposure of 7.64 ×103 kg .days . XENON100 is a dual-phase xenon time projection chamber with 62 kg of active mass, operated at the Laboratori Nazionali del Gran Sasso (LNGS) in Italy and designed to search for nuclear recoils from WIMP-nucleus interactions. Here we explore inelastic scattering, where a transition to a low-lying excited nuclear state of Xe 129 is induced. The experimental signature is a nuclear recoil observed together with the prompt deexcitation photon. We see no evidence for such inelastic WIMP-Xe…

Physics - Instrumentation and DetectorsXenonPhysics and Astronomy (miscellaneous)Physics::Instrumentation and Detectors[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)XenonRecoilWIMP[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Dark MatterNuclear Experiment[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]nucleus: recoilPhysicsTime projection chamberAstrophysics::Instrumentation and Methods for AstrophysicsWIMP nucleon: cross sectionInstrumentation and Detectors (physics.ins-det)Excited stateWeakly interacting massive particlesTPCNucleonchannel cross section: measuredsignatureAstrophysics - Cosmology and Nongalactic AstrophysicsParticle physicsdata analysis methodCosmology and Nongalactic Astrophysics (astro-ph.CO)WIMPchemistry.chemical_elementFOS: Physical sciencesInelastic scatteringspin: dependenceNuclear physicsstatistical analysis[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]photon: emission0103 physical sciencescross section: inelastic scattering[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsWIMP nucleon: inelastic scattering010308 nuclear & particles physicsS030DP2WIMP nucleus: interactionGran SassochemistryDirect Searchtime projection chamber: xenonHigh Energy Physics::Experiment[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]experimental results
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