Search results for "elementary"

showing 10 items of 863 documents

Expansion cone for the 3-inch PMTs of the KM3NeT optical modules

2013

[EN] Detection of high-energy neutrinos from distant astrophysical sources will open a new window on the Universe. The detection principle exploits the measurement of Cherenkov light emitted by charged particles resulting from neutrino interactions in the matter containing the telescope. A novel multi-PMT digital optical module (DOM) was developed to contain 31 3-inch photomultiplier tubes (PMTs). In order to maximize the detector sensitivity, each PMT will be surrounded by an expansion cone which collects photons that would otherwise miss the photocathode. Results for various angles of incidence with respect to the PMT surface indicate an increase in collection efficiency by 30% on average…

Optical detector readout concepts; Instrument optimisation; Cherenkov detectorsPhotomultiplier[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Instrument optimisationCherenkov detectorPhysics::Instrumentation and Detectors01 natural scienceslarge detector systems for particle and astroparticle physics; optical detector readout concepts; cherenkov detectors; instrument optimization.Photocathodelaw.inventionTelescopeOpticslaw0103 physical sciencesOptical detector readout conceptsNEUTRINO TELESCOPE010306 general physicsInstrumentationMathematical PhysicsCherenkov radiationPhysics010308 nuclear & particles physicsbusiness.industryLarge detector systems for particle and astroparticle physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]DetectorCherenkov detectorsAstrophysics::Instrumentation and Methods for AstrophysicsInstrument optimizationINGENIERIA TELEMATICAOptical detector readout concept[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]KM3NeTLarge detector systems for particle and astroparticle physicNeutrinobusinessPROJECTCherenkov detector85.60.Ha Photomultipliers ; phototubes and photocathodes ; 42.15.Dp Wave fronts and ray tracing ; 98.80.-k Cosmology ; 95.55.Vj Neutrino muon pion and other elementary particle detectors; cosmic ray detectors ; 29.40.Ka Cherenkov detectors
researchProduct

Orientation of199mHg by optical pumping detected by ?-radiation anisotropy

1975

199mHg was produced and mass separated at the ISOLDE facility (CERN). Nuclear orientation achieved by optical pumping via the resonance line 6s21S0→6s6p3P1,λ=2537A was monitored by means of the anisotropy of theγ-radiation emitted in the cascade199mHg(I=13/2+) $${}^{199m}Hg(I = 13/2^ + )\xrightarrow[{M4}]{}{}^{199*}Hg(I = 5/2^ - )\xrightarrow[{E2}]{}{}^{199}Hg(I = 1/2^ - ).$$ 199*Hg(I=5/2−)199Hg(I=1/2−).

Optical pumpingOrientation (vector space)PhysicsNuclear and High Energy Physicsγ radiationIsotopic shiftAnalytical chemistryNuclear fusionElementary particleAtomic physicsAnisotropyResonance lineZeitschrift f�r Physik A Atoms and Nuclei
researchProduct

Acoustic and optical variations during rapid downward motion episodes in the deep north-western Mediterranean Sea

2011

An Acoustic Doppler Current Profiler (ADCP) was moored at the deep-sea site of the ANTARES neutrino telescope near Toulon, France, thus providing a unique opportunity to compare high-resolution acoustic and optical observations between 70 and 170 m above the sea bed at 2475 m. The ADCP measured downward vertical currents of magnitudes up to 0.03 m s-1 in late winter and early spring 2006. In the same period, observations were made of enhanced levels of acoustic reflection, interpreted as suspended particles including zooplankton, by a factor of about 10 and of horizontal currents reaching 0.35 m s-1. These observations coincided with high light levels detected by the telescope, interpreted …

Optical telescopesDense water formation010504 meteorology & atmospheric sciencesDense watersBoundary currentWave reflectionOptical photo-multiplier observationsSuspended loadWATER FORMATIONOceanography01 natural scienceslaw.inventionPhysics - GeophysicsObservational methodMediterranean sea86-02lawDeep MediteraneanSeabedPhosphorescenceDeep seaCurrent (stream)VARIABILITYOptical methodOceanographyAcoustic variables measurementNorthern boundary currentantares neutrino telescope; deep mediteranean; northern boundary current; acoustic adcp observations; episodic downward current; dense water formation; bioluminescence; optical photo-multiplier observationsFísica nuclearAcoustic Doppler Current ProfilerBioluminescenceAstrophysics - Instrumentation and Methods for AstrophysicsANTARES neutrino telescopeGeology[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Acoustic ADCP observationsCIRCULATIONFOS: Physical sciencesAquatic ScienceLIGURIAN SEAZooplanktonZooplanktonTelescopeAcoustic Doppler current profilerOCEANOPTICAL PHOTO-MULTIPLIERMediterranean Sea14. Life underwaterInstrumentation and Methods for Astrophysics (astro-ph.IM)0105 earth and related environmental sciencesLight reflectionANTARESAcoustic wave010505 oceanographyAdvectionDense waterElementary particlesZOOPLANKTON BIOMASSDoppler effectMARINE RESEARCHESGeophysics (physics.geo-ph)Boundary current[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Boundary currentsCONVECTION13. Climate actionFISICA APLICADAAdvectionEpisodic downward currentMediterranean Sea (Northwest)SYSTEMTelescopes
researchProduct

AMADEUS-The acoustic neutrino detection test system of the ANTARES deep-sea neutrino telescope

2011

The AMADEUS (ANTARES Modules for the Acoustic Detection Under the Sea) system which is described in this article aims at the investigation of techniques for acoustic detection of neutrinos in the deep sea. It is integrated into the ANTARES neutrino telescope in the Mediterranean Sea. Its acoustic sensors, installed at water depths between 2050 and 2300 m, employ piezo-electric elements for the broad-band recording of signals with frequencies ranging up to 125 kHz. The typical sensitivity of the sensors is around - 145 dB re 1 V/mu Pa (including preamplifier). Completed in May 2008, AMADEUS consists of six "acoustic clusters", each comprising six acoustic sensors that are arranged at distanc…

Optical telescopesNuclear and High Energy PhysicsAcoustic devicesNeutrino detectionPreamplifierAmbient noise levelFOS: Physical sciencesLINENeutrino telescope01 natural sciencesOptical telescopeThermo-acoustic modelData acquisition0103 physical sciencesSHOWERSWATERPARTICLE-DETECTION14. Life underwater010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)InstrumentationRemote sensingPhysicsANTARES010308 nuclear & particles physicsSensorsDetectorAstronomyElementary particlesAcoustic waveAMADEUSAcoustic neutrino detectionAcoustic wavesNeutrino detectorAcoustic variables measurementthermo-acoustic model; amadeus; neutrino telescope; acoustic neutrino detection; antaresFISICA APLICADAFísica nuclearNeutrinoNeutrino telescopesComputer hardware description languagesAstrophysics - Instrumentation and Methods for AstrophysicsSignal detection
researchProduct

Time calibration of the ANTARES neutrino telescope

2011

The ANTARES deep-sea neutrino telescope comprises a three-dimensional array of photomultipliers to detect the Cherenkov light induced by upgoing relativistic charged particles originating from neutrino interactions in the vicinity of the detector. The large scattering length of light in the deep sea facilitates an angular resolution of a few tenths of a degree for neutrino energies exceeding 10 TeV. In order to achieve this optimal performance, the time calibration procedures should ensure a relative time calibration between the photomultipliers at the level of ~1 ns. The methods developed to attain this level of precision are described.

Optical telescopesPhysics - Instrumentation and Detectors[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and Detectors01 natural sciencesOptimal performanceHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Calibration procedureDimensional arraysAngular resolution[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutrino energyNEUTRINO TELESCOPE010303 astronomy & astrophysicsPhysicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)Deep seaNeutrino detectorRelative timeCalibrationFísica nuclearNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsTime calibrationPhotomultiplier[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Cherenkov lightAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesScattering lengthNeutrino TelescopesOptical telescopeNuclear physics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Tellurium compounds0103 physical sciencesOptical systemsCalibrationAngular resolution14. Life underwater[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Instrumentation and Methods for Astrophysics (astro-ph.IM)DETECTORCherenkov radiationtime calibration; neutrino telescopes; antaresANTARES010308 nuclear & particles physicsNeutrino interactionsAstronomyElementary particlesAstronomy and AstrophysicsPhotomultipliersFISICA APLICADAHigh Energy Physics::ExperimentUNDERWATER DETECTORNeutrino telescopesSYSTEM
researchProduct

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
researchProduct

Search for doubly charged higgs bosons with lepton-rlavor-violating decays involving τ leptons

2008

We search for pair production of doubly charged Higgs particles (H(+/-+/-)) followed by decays into electron-tau (e tau) and muon-tau (mu tau) pairs using data (350 pb(-1)) collected from (p) over barp collisions at root s = 1.96 TeV by the CDF II experiment. We search separately for cases where three or four final-state leptons are detected, and combine results for exclusive decays to left-handed e tau (mu tau) pairs. We set an H(+/-+/-) lower mass limit of 114(112) GeV/c(2) at the 95% confidence level. RI Ruiz, Alberto/E-4473-2011; Robson, Aidan/G-1087-2011; De Cecco, Sandro/B-1016-2012; Prokoshin, Fedor/E-2795-2012; Azzi, Patrizia/H-5404-2012

Pair productionParticle physicsGeneral Physics and AstronomyFOS: Physical sciencesElementary particleddc:500.201 natural sciencesHigh Energy Physics - ExperimentNuclear physicsTellurium compoundsParticle decayHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesHiggs particles010306 general physicsBosonsBosonPhysicsHiggs bosonsMuon010308 nuclear & particles physicsBranching fractionPhysicsHigh Energy Physics::PhenomenologyPair productionConfidence levelHiggs boson_High Energy Physics::ExperimentLepton
researchProduct

Parental autonomy vs. ability : attendance in a low-income elementary school

2018

The overall aim of this study is to examine the perceptions of low-income elementary school parents with outstanding attendance concerns. This analysis makes salient the need for more complex treatment of the term parental agency in current U.S. educational scholarship by using a cross-disciplinary frame-work. Parental data subjects were collected within the context of a San Diegan NGO’s attendance initiative at a low-income elementary school in San Diego Unified School District. As an “Every Student Every Day” attendance intern, at-risk students with outstanding attendance concerns were added to my case-load at the start of the 2017-2018 school year. Ethnographic data in the form of case n…

ParentsattendanceSan Diegoeducationagencyelementarylow-income
researchProduct

Commutators of second-class axial currents with normal weak currents and consequences for particle decays

1981

Second-class weak axial currents are studied in the framework of normal weak and electromagnetic currents. Equal time commutators between normal and abnormal axial currents and the isoscalar electromagnetic current are postulated and their consequences are worked out. A number of predictions for masses, coupling constants and decay properties are derived and are compared to available data.

Particle accelerationPhysicsCoupling constantPhysics and Astronomy (miscellaneous)Quantum electrodynamicsIsoscalarParticleVertex functionElementary particleField theory (psychology)Quantum field theoryEngineering (miscellaneous)Zeitschrift für Physik C Particles and Fields
researchProduct

Measurement of Wγ and Zγ production in proton-proton collisions at √s =7 TeV with the ATLAS detector

2011

Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer lugar, el nombre del grupo de colaboración, si le hubiere, y los autores pertenecientes a la UAM

Particle physics:Mathematics and natural science: 400::Physics: 430 [VDP]Nuclear and High Energy PhysicsProtonAtlas detectorFOS: Physical sciencesddc:500.2:Mathematics and natural science: 400::Physics: 430::Nuclear and elementary particle physics: 431 [VDP]Hadron-hadron scattering01 natural sciences7. Clean energy530High Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Atlas (anatomy)0103 physical sciencesmedicine[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530High Energy Physics010306 general physicsPhysicsW BOSONHadron-Hadron Scattering010308 nuclear & particles physicsATLAS experimentHigh Energy Physics::PhenomenologyFísicaATLASHigh energy photonmedicine.anatomical_structureZ BOSONW and Z bosonsHADRON-HADRON COLLISIONSFísica nuclearHigh Energy Physics::ExperimentLHCParticle Physics - Experiment
researchProduct