0000000001177632

AUTHOR

F. Feinstein

showing 21 related works from this author

The data acquisition system for the ANTARES neutrino telescope

2006

The ANTARES neutrino telescope is being constructed in the Mediterranean Sea. It consists of a large three-dimensional array of photo-multiplier tubes. The data acquisition system of the detector takes care of the digitisation of the photo-multiplier tube signals, data transport, data filtering, and data storage. The detector is operated using a control program interfaced with all elements. The design and the implementation of the data acquisition system are described.

Nuclear and High Energy Physics[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and DetectorsData managementAstrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONFOS: Physical sciencesAstrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Data filteringData acquisition0103 physical sciences14. Life underwaterElectronics010306 general physicsInstrumentationdata acquisition system; neutrino telescopeRemote sensingAstroparticle physicsPhysicsneutrino telescope data acquisition system[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsbusiness.industryDetectorAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for AstrophysicsAstronomyneutrino telescopedata acquisition systemComputer data storageFísica nuclearbusiness
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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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Polarised quark distributions in the nucleon from semi-inclusive spin asymmetries

1998

We present a measurement of semi-inclusive spin asymmetries for positively and negatively charged hadrons from deep inelastic scattering of polarised muons on polarised protons and deuterons in the range $0.003$1 GeV$^2$. Compared to our previous publication on this subject, with the new data the statistical errors have been reduced by nearly a factor of two. From these asymmetries and our inclusive spin asymmetries we determine the polarised quark distributions of valence quarks and non-strange sea quarks at $Q^2$=10 GeV$^2$. The polarised $u$ valence quark distribution, $\Delta u_v(x)$, is positive and the polarisation increases with $x$. The polarised $d$ valence quark distribution, $\De…

QuarkPhysicsNuclear and High Energy PhysicsParticle physicsMuonValence (chemistry)SMCHadronFOS: Physical sciencesSMC; SIDIS; Polarized quark distributionsDeep inelastic scatteringSIDISHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)DeuteriumHigh Energy Physics::ExperimentPolarized quark distributionsNucleonParticle Physics - ExperimentPhysics Letters B
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Spin asymmetries for events with highpThadrons in DIS and an evaluation of the gluon polarization

2004

We present a measurement of the longitudinal spin cross section asymmetry for deep-inelastic muon-nucleon interactions with two high transverse momentum hadrons in the final state. Two methods of event classification are used to increase the contribution of the photon-gluon fusion process to above 30%. The most effective one, based on a neural network approach, provides the asymmetries A(p)lN(-->)lhhX=0.030+/-0.057(stat)+/-0.010(syst) and A(d)lN(-->)lhhX=0.070+/-0.076(stat)+/-0.010(syst). From these values we derive an averaged gluon polarization DeltaG/G=-0.20+/-0.28(stat)+/-0.10(syst) at an average fraction of nucleon momentum carried by gluons =0.07.

PhysicsNuclear and High Energy PhysicsParticle physicsMeson production010308 nuclear & particles physicsmedia_common.quotation_subjectHadronDeep inelastic scatteringPolarization (waves)01 natural sciencesAsymmetryGluonNuclear physics0103 physical sciencesTransverse momentumHigh Energy Physics::ExperimentAstrophysics::Earth and Planetary AstrophysicsNuclear Experiment010306 general physicsNucleonmedia_commonPhysical Review D
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A line-shape analysis for spin-1 NMR signals

1997

An analytic model of the deuteron absorption function has been developed and is compared to experimental NMR signals of deuterated butanol obtained at the SMC experiment in order to determine the deuteron polarization. The absorption function model includes dipolar broadening and a frequency-dependent treatment of the intensity factors. The high-precision TE signal data available are used to adjust the model for Q-meter distortions and dispersion effects. Once the Q-meter adjustment is made, the enhanced polarizations determined by the asymmetry and TE-calibration methods compare well within the accuracy of each method. In analyzing the NMR signals, the quadrupolar coupling constants could …

Coupling constantPhysicsdisNuclear and High Energy PhysicsButanolmedia_common.quotation_subjectsmcpolarized targetQ meterdiPolarization (waves)AsymmetryMolecular physicschemistry.chemical_compoundDipoleNuclear magnetic resonanceDeuteriumchemistrysmc; dis; polarized targetDetectors and Experimental TechniquesInstrumentationShape analysis (digital geometry)media_common
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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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First results of the Instrumentation Line for the deep-sea ANTARES neutrino telescope

2006

In 2005, the ANTARES Collaboration deployed and operated at a depth of 2500 m a so-called Mini Instrumentation Line equipped with Optical Modules (MILOM) at the ANTARES site. The various data acquired during the continuous operation from April to December 2005 of the MILOM confirm the satisfactory performance of the Optical Modules, their front-end electronics and readout system, as well as the calibration devices of the detector. The in-situ measurement of the Optical Module time response yields a resolution better than 0.5 ns. The performance of the acoustic positioning system, which enables the spatial reconstruction of the ANTARES detector with a precision of about 10 cm, is verified. T…

Photomultiplierneutrino astronomy; photon detection; underwater detectorPositioning systemInstrumentationAstrophysics::High Energy Astrophysical PhenomenaNeutrino astronomy Underwater detector Photon detectionFOS: Physical sciencesAstrophysics01 natural sciencesneutrino astronomy[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciencesCalibrationAngular resolution010306 general physicsRemote sensingAstroparticle physicsPhysicsunderwater detector[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsDetectorAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for AstrophysicsAstronomySITEAstronomy and AstrophysicsLIGHTPHOTON DETECTIONNEUTRINO ASTRONOMYFísica nuclearUNDERWATER DETECTORNeutrino astronomy
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Study of Large Hemispherical Photomultiplier Tubes for the ANTARES Neutrino Telescope

2005

The ANTARES neutrino telescope, to be immersed depth in the Mediterranean Sea, will consist of a 3 dimensional matrix of 900 large area photomultiplier tubes housed in pressure resistant glass spheres. The selection of the optimal photomultiplier was a critical step for the project and required an intensive phase of tests and developments carried out in close collaboration with the main manufacturers worldwide. This paper provides an overview of the tests performed by the collaboration and describes in detail the features of the PMT chosen for ANTARES.

Nuclear and High Energy PhysicsPhotomultiplierPhysics - Instrumentation and DetectorsNeutrino detectionNeutrino telescopeFOS: Physical sciences01 natural scienceslarge area photosensor hemispherical photomultiplier neutrino detectionNuclear physicsOpticsIntensive Phase0103 physical sciences14. Life underwater[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsInstrumentationAstroparticle physicsPhysics010308 nuclear & particles physicsbusiness.industryHemispherical photomultiplierInstrumentation and Detectors (physics.ins-det)Large area photosensorGlass spheresNeutrino detector95.55.Vj; 85.60.HaFísica nuclearbusinesshemispherical photomultiplier; large area photosensor; neutrino detection
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Spin asymmetriesA1of the proton and the deuteron in the lowxand lowQ2region from polarized high energy muon scattering

1999

We present the results of the spin asymmetries (Formula presented) of the proton and the deuteron in the kinematic region extending down to (Formula presented) and (Formula presented) The data were taken with a dedicated low x trigger, which required hadron detection in addition to the scattered muon, so as to reduce the background at low x. The results complement our previous measurements and the two sets are consistent in the overlap region. No significant spin effects are found in the newly explored region. © 1999 The American Physical Society.

PhysicsNuclear physicsNuclear and High Energy PhysicsHigh energyParticle physicsMuonDeuteriumProtonScatteringHadronDeep inelastic scatteringSpin-½Physical Review D
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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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Spin asymmetriesA1and structure functionsg1of the proton and the deuteron from polarized high energy muon scattering

1998

We present the final results of the spin asymmetries A1 and the spin structure functions g1 of the proton and the deuteron in the kinematic range 0.0008<x<0.7 and 0.2<Q2<100 GeV2. For the determination of A1, in addition to the usual method which employs inclusive scattering events and includes a large radiative background at low x, we use a new method which minimizes the radiative background by selecting events with at least one hadron as well as a muon in the final state. We find that this hadron method gives smaller errors for x<0.02, so it is combined with the usual method to provide the optimal set of results.

PhysicsNuclear and High Energy PhysicsParticle physicsRange (particle radiation)MuonProtonScatteringHadronSpin structureNuclear physicsRadiative transferHigh Energy Physics::ExperimentNuclear ExperimentSpin-½Physical Review D
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A large Streamer Chamber muon tracking detector in a high-flux fixed-target application.

1999

Arrays of limited streamer tubes of the Iarocci type were deployed in our experiment at CERN as part of a forward muon detector system with provisions for the beam to pass through the center of each panel in the array. A total of 16 4 m x 4 m panels were assembled with inductive readout strips on both sides of each panel. An active feedback system. was deployed to regulate the high voltage to the streamer tubes to insure a constant efficiency for minimum ionizing particles. The arrays were operated in this environment for over five years of data taking. Streamer tube track-reconstruction efficiencies and tube replacement rates are reported. (C) 1999 Elsevier Science B.V. All rights reserved.

PhysicsDISNuclear and High Energy PhysicsLarge Hadron ColliderSMCPhysics::Instrumentation and Detectorsbusiness.industryDetectorHigh voltageSTRIPSTracking (particle physics)law.inventionNuclear physicsOpticsSMC; DIS; Large area detectorslawTube (fluid conveyance)Detectors and Experimental TechniquesbusinessLarge area detectorsInstrumentationBeam (structure)Electronic circuit
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The spin-dependent structure function g1(x) of the proton from polarized deep-inelastic muon scattering

1997

We present a new measurement of the virtual photon proton asymmetry $A_1^{\rm p}$ from deep inelastic scattering of polarized muons on polarized protons in the kinematic range $0.0008 1$ GeV$^{2}$. A perturbative QCD evolution in next-to-leading order is used to determine $g_1^{\rm p}(x)$ at a constant $Q^2$. At $Q^{2} = 10$ GeV$^{2}$ we find, in the measured range, $\int_{0.003}^{0.7} g_{1}^{\rm p}(x){\rm d}x = 0.139 \pm 0.006~({\rm stat})\pm 0.008~({\rm syst)} \pm 0.006~({\rm evol})$. The value of the first moment $\Gamma_{1}^{\rm p} = \int_{0}^{1} g_{1}^{\rm p}(x){\rm d}x$ of $g_{1}^{\rm p}$ depends on the approach used to describe the behaviour of $g_{1}^{\rm p}$ at low $x$. We find tha…

PhysicsQuantum chromodynamicsDISNuclear and High Energy PhysicsParticle physicsMuonProtonSMCScatteringg1 structure functionSMC; DIS; g1 structure functionPerturbative QCDDeep inelastic scatteringNuclear physicsSum rule in quantum mechanicsNucleonParticle Physics - ExperimentPhysics Letters B
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A new measurement of the spin-dependent structure function $g_{1}(x)$ of the deuteron

1995

Abstract We present a new measurement of the spin-dependent structure function g 1 d of the deuteron in deep inelastic scattering of 190 GeV polarised muons on polarised deuterons, in the kinematic range 0.003 x 2 Q 2 2 . This structure function is found to be negative at small x . The first moment Γ 1 d =∫ 0 1 g 1 d d x evaluated at Q 0 2 = 10 GeV 2 is 0.034 ± 0.009 (stat.) ± 0.006 (syst.). This value is below the Ellis-Jaffe sum rule prediction by three standard deviations. Using our earlier determination of Γ 1 p , we obtain Γ 1 p − Γ 1 n = 0.199 ± 0.038 which agrees with the Bjorken sum rule.

PhysicsNuclear and High Energy PhysicsParticle physicsRange (particle radiation)MuonStructure functionDeep inelastic scatteringdeep inelastic scattering; spin sum rule; SMC experimentStandard deviationNuclear physicsspin sum ruleDeuteriumdeep inelastic scatteringSum rule in quantum mechanicsSMC experimentParticle Physics - ExperimentSpin-½
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The polarized double cell target of the SMC

1999

The polarized target of the Spin Muon Collaboration at CERN was used for deep inelastic muon scattering experiments during 1993-1996 with a polarized muon beam to investigate the spin structure of the nucleon. Most of the experiments were carried out with longitudinal target polarization and 190 GeV muons, and some were done with transverse polarization and 100 GeV muons. Protons as well as deuterons were polarized by dynamic nuclear polarization (DNP) in three kinds of solid materials - butanol, ammonia, and deuterated butanol - with maximum degrees of polarization of 94%, 91% and 60%, respectively. Considerable attention was paid to the accuracies of the NMR polarization measurements and …

PhysicsNuclear and High Energy PhysicsDISLarge Hadron ColliderMuonanalysisScatteringSMCPolarized targetSpin structurepolarized protons and deuteronsPolarization (waves)Deep inelastic scatteringNMRdynamic nuclear polarizationSMC; DIS; Polarized targetNuclear physicsDeuteriumPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentDetectors and Experimental TechniquesNuclear ExperimentNucleonInstrumentation
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Measurement of the SMC muon beam polarisation using the asymmetry in the elastic scattering off polarised electrons

2000

A muon beam polarimeter was built for the SMC experiment at the CERN SPS, for beam energies of 100 and 190 GeV. The beam polarisation is determined from the asymmetry in the elastic scattering off the polarised electrons of a ferromagnetic target whose magnetisation is periodically reversed. At muon energies of 100 and 190 GeV the measured polarisation is P-mu = -0.80 +/- 0.03 (stat.) +/- 0.02 (syst.) and P-mu = - 0.797 +/- 0.011 (stat.) +/- 0.012 (syst.), respectively. These results agree with measurements of the beam polarisation using a shape analysis of the decay positron energy spectrum. (C) 2000 Elsevier Science B.V. All rights reserved.

electronNuclear and High Energy PhysicsSMC; DIS; muon polarimetermedia_common.quotation_subjectmuon beamElectronAsymmetryNuclear physicsMagnetizationpolarisation measurementDetectors and Experimental TechniquesNuclear ExperimentInstrumentationmedia_commonPhysicsElastic scatteringDISLarge Hadron ColliderMuonpolarised scatteringSMCmagnetised targetPolarimeterpolarised muonPolarization (waves)muon polarimeterPhysics::Accelerator PhysicsHigh Energy Physics::Experimentpolarised
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The spin-dependent structure function g1(x) of the deuteron from polarized deep-inelastic muon scattering

1997

We present a new measurement of the spin-dependent structure function $g_{1}^{\rm d}$ of the deuteron from deep inelastic scattering of 190 GeV polarized muons on polarized deuterons. The results are combined with our previous measurements of $g_{1}^{\rm d}$. A perturbative QCD evolution in next-to-leading order is used to compute $g_{1}^{\rm d}(x)$ at a constant $Q^{2}$. At $Q^{2} = 10$ GeV$^{2}$, we obtain a first moment $\Gamma_{1}^{\rm d} = \int_{0}^{1} g_{1}^{\rm d}{\rm d}x = 0.041 \pm 0.008$, a flavour-singlet axial charge of the nucleon $a_{0} = 0.30 \pm 0.08$, and an axial charge of the strange quark $a_{s} = -0.09 \pm 0.03$. Using our earlier determination of $\Gamma_{1}^{\rm p}$, …

PhysicsDISNuclear and High Energy PhysicsStrange quarkMuonSMCScatteringg1 structure functionSMC; DIS; g1 structure functionPerturbative QCDDeep inelastic scatteringNuclear physicsHigh Energy Physics::ExperimentSum rule in quantum mechanicsNucleonParticle Physics - ExperimentSpin-½Physics Letters B
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Measurement of the spin-dependent structure function g1(x) of the deuteron

1993

We report on the first measurement of the spin-dependent structure function g1d of the deuteron in the deep inelastic scattering of polarised muons off polarised deuterons, in the kinematical range 0.006&lt;x&lt;0.6, 1 GeV2&lt;Q2&lt;30 GeV2. The first moment, Γ1d=sh{phonetic}01 g1d dx=0.023±0.020 (stat.) ± 0.015 (syst.), is smaller than the prediction of the Ellis-Jaffe sum rules. Using earlier measurements of g1p, we infer the first moment of the spin-dependent neutron structure function g1n. The difference Γ1p-Γ1n=0.20 ±0.05 (stat.) ± 0.04 (syst.) agrees with the prediction of the Bjorken sum rule, Γ1p-Γ1n=0.191 ±0.002.

deuteron: polarized targetNuclear and High Energy PhysicsINELASTIC E-P; POLARIZED PROTONS; SUM-RULE; SCATTERING; ELECTROPRODUCTION; ASYMMETRYINELASTIC E-PProtonpolarized target: deuterondeep inelastic scattering: muon deuteronstructure function: spinmuon deuteron: deep inelastic scatteringSUM-RULE530Nuclear physicsINELASTIC E-P; POLARIZED PROTONS; SUM-RULE; SCATTERING; ELECTROPRODUCTION; ASYMMETRY; MODELTheoryofComputation_ANALYSISOFALGORITHMSANDPROBLEMCOMPLEXITYSCATTERINGNeutronpolarized beam: muonSpin-½PhysicsQuantum chromodynamicsspin: structure functionMuonScatteringdeuteron: structure functionELECTROPRODUCTIONnucleon: structure functionCERN SPSDeep inelastic scatteringmomentmagnetic spectrometer: experimental resultsPOLARIZED PROTONSapprox. 100 GeVASYMMETRYSum rule in quantum mechanicsmuon: polarized beamParticle Physics - ExperimentPhysics Letters B
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Measurement of proton and nitrogen polarization in ammonia and a test of equal spin temperature

1998

The 1996 data taking of the SMC experiment used polarized protons to measure the spin-dependent structure function g(1) of the proton. Three liters of solid granular ammonia were irradiated at the Bonn electron linac in order to create the paramagnetic radicals which are needed for polarizing the protons. Proton polarizations of +/- (90 +/- 2.5)% were routinely reached. An analysis based on a theoretical line shape for spin-1. systems with large quadrupolar broadening was developed which allowed the nitrogen polarization in the ammonia to be determined with a 10% relative error. The measured quadrupolar coupling constant of N-14 agrees well with earlier extrapolated values. The polarization…

Nuclear and High Energy Physicsspin resonanceProtonp polarized targetNuclear Theorychemistry.chemical_elementAmmoniachemistry.chemical_compoundParamagnetismIrradiationDetectors and Experimental TechniquesNuclear ExperimentInstrumentationPhysicsCoupling constantpolarizationquadrupolar interactionsPolarization (waves)Nitrogennitrogen polarized targetdynamic nuclearnuclear magnetic resonancechemistryDeuteriump polarized target; nitrogen polarized target; spin resonanceAtomic physics
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Background light in potential sites for the ANTARES undersea neutrino telescope

2000

The ANTARES collaboration has performed a series of {\em in situ} measurements to study the background light for a planned undersea neutrino telescope. Such background can be caused by $^{40}$K decays or by biological activity. We report on measurements at two sites in the Mediterranean Sea at depths of 2400~m and 2700~m, respectively. Three photomultiplier tubes were used to measure single counting rates and coincidence rates for pairs of tubes at various distances. The background rate is seen to consist of three components: a constant rate due to $^{40}$K decays, a continuum rate that varies on a time scale of several hours simultaneously over distances up to at least 40~m, and random bur…

PhotomultiplierTrigger rateContinuum (design consultancy)Neutrino telescopeFOS: Physical sciencesAstrophysicsAstrophysics01 natural sciencesCoincidenceHigh Energy Physics - Experiment[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]High Energy Physics - Experiment (hep-ex)0103 physical sciencesMetre14. Life underwater010306 general physicsPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsAstrophysics (astro-ph)AstronomyAstronomy and AstrophysicsConstant rate13. Climate actionFísica nuclearBackground lightAstroparticle Physics
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ANTARES: The first undersea neutrino telescope

2011

The ANTARES Neutrino Telescope was completed in May 2008 and is the first operational Neutrino Telescope in the Mediterranean Sea. The main purpose of the detector is to perform neutrino astronomy and the apparatus also offers facilities for marine and Earth sciences. This paper describes the design, the construction and the installation of the telescope in the deep sea, offshore from Toulon in France. An illustration of the detector performance is given. © 2011 Elsevier B.V. All rights reserved.

Optical telescopesPhysics::Instrumentation and DetectorsAstronomyMarine engineeringSubmarine cablesAstrophysics01 natural scienceslaw.inventionAstroparticlelaw010303 astronomy & astrophysicsInstrumentationPhysicsDense wavelength division multiplexingDetectorAstrophysics::Instrumentation and Methods for AstrophysicsDetectorsSubmarine cableDeep seaNeutrino astronomyFísica nuclearNeutrinoMarine technologyAstrophysics - Instrumentation and Methods for AstrophysicsNuclear and High Energy Physics[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Wet mateable connectorAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesLINEOptical telescopePhysics::GeophysicsTelescopePhotomultiplier tube0103 physical sciencesNeutrinoDWDM14. Life underwaterDeep sea detectorInstrumentation and Methods for Astrophysics (astro-ph.IM)DETECTORAstroparticle physics010308 nuclear & particles physicswet mateable connector.Marine technologyAstronomyElementary particles[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]PhotomultipliersKM3NeTFISICA APLICADAEarth (planet)High Energy Physics::ExperimentNeutrino astronomyastroparticle; neutrino astronomy; marine technology; dwdm; photomultiplier tube; deep sea detector; submarine cable; wet mateable connector; neutrinoSYSTEMTelescopes
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