Search results for "background: low"

showing 7 items of 7 documents

Test of the electric charge conservation law with Borexino detector

2015

International audience; The new limit on the electron lifetime is obtained from data of the Borexino experiment. The expected signal from the e → γν decay mode is a 256 keV photon detected in liquid scintillator. Because of the extremely low radioactive background level in the Borexino detector it was possible to improve the previous measurement by two orders of magnitude.

GRAN SASSOelectron --> photon neutrinoHistoryPhysics::Instrumentation and Detectorsscintillation counter: liquidElectronScintillator01 natural sciencesParticle detectorPhysics::GeophysicsEducationNuclear physicsSCINTILLATORPhysics and Astronomy (all)background: low0103 physical sciencescharge: conservation law[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010303 astronomy & astrophysicsBorexinolifetimePhysicsCharge conservationSTABILITY010308 nuclear & particles physicsDetectorEXPERIMENTAL LIMITSComputer Science ApplicationsNeutrino detectorelectron: lifetimeBorexinoNeutrinoDECAYJournal of Physics: Conference Series
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Geo-neutrino results with Borexino

2015

International audience; Borexino is a liquid scintillator detector primary designed to observe solar neutrinos. Due to its low background level as well as its position in a nuclear free country, Italy, Borexino is also sensitive to geo-neutrinos. Borexino is leading this interdisciplinary field of neutrino geoscience by studying electron antineutrinos which are emitted from the decay of radioactive isotopes present in the crust and the mantle of the Earth. With 2056 days of data taken between December 2007 and March 2015, Borexino observed 77 antineutrino candidates. If we assume a chondritic Th/U mass ratio of 3.9, the number of geo-neutrino events is found to be 23.7(+6.5) (-5.7)(stat) (+…

History010504 meteorology & atmospheric sciencesSolar neutrinoscintillation counter: liquidchemistry.chemical_elementScintillator010502 geochemistry & geophysics7. Clean energy01 natural sciencesthoriumEducationuraniumNuclear physicsPhysics and Astronomy (all)background: low[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Borexino0105 earth and related environmental sciencesPhysicsRadionuclideRadiogenic nuclideThoriumMass rationuclide: mass ratioComputer Science Applicationschemistry13. Climate actionradioactivityBorexinoGEOPHYSICSneutrino: geophysicsNeutrinoexperimental resultsJournal of Physics: Conference Series
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Gamma-induced background in the KATRIN main spectrometer

2019

The KATRIN experiment aims to measure the effective electron antineutrino mass $$m_{\overline{\nu }_e}$$ mν¯e with a sensitivity of $${0.2}\,{\hbox {eV}/\hbox {c}^2}$$ 0.2eV/c2 using a gaseous tritium source combined with the MAC-E filter technique. A low background rate is crucial to achieving the proposed sensitivity, and dedicated measurements have been performed to study possible sources of background electrons. In this work, we test the hypothesis that gamma radiation from external radioactive sources significantly increases the rate of background events created in the main spectrometer (MS) and observed in the focal-plane detector. Using detailed simulations of the gamma flux in the e…

Speichertechnik - Abteilung BlaumPhysics - Instrumentation and Detectorsgamma ray: backgroundshieldingshielding: magneticPhysicsFOS: Physical scienceslcsh:AstrophysicsInstrumentation and Detectors (physics.ins-det)electron: secondarysensitivityKATRINbackground: lowlcsh:QB460-466electron: backgroundlcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. Radioactivityddc:530gamma ray: flux[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Electromagnetismonumerical calculationselectrostatic
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Features of W production in p-p, p-Pb and Pb-Pb collisions

2017

We consider the production of inclusive W bosons in variety of high-energy hadronic collisions: p--p, p--$\overline{\rm p}$, p--Pb, and Pb--Pb. In particular, we focus on the resulting distributions of charged leptons from W decay that can be measured with relatively low backgrounds. The leading-order expressions within the collinearly factorized QCD indicate that the center-of-mass energy dependence at forward/backward rapidities should be well approximated by a simple power law. The scaling exponent is related to the small-$x$ behaviour of the quark distributions, which is largely driven by the parton evolution. An interesting consequence is the simple scaling law for the lepton charge as…

heavy ion: scatteringHadronPb-Pb collisionsPartonElementary particle02 engineering and technologycomputer.software_genrePower lawHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)background: lowHigh Energy Physics - Phenomenology (hep-ph)0202 electrical engineering electronic engineering information engineering[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]050107 human factorsBosonQuantum chromodynamicsPhysicsDatabasehigher-order: 0Hadronic collisionsCharge asymmetries05 social sciencesscalinghep-phCharged leptonsHigh Energy Physics - PhenomenologyCERN LHC CollParticle Physics - ExperimentQuarkInelastic scatteringParticle physicssmall-xquark: distribution functionp p: scatteringFOS: Physical sciencesW: decay114 Physical sciencesenergy dependence[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]W: productionquantum chromodynamicsanti-p p: scatteringCollision systems0501 psychology and cognitive sciencesHigh energy physicsp nucleus: scatteringBosonsParticle Physics - Phenomenologyhep-exlepton: charge: asymmetryfactorization: collinearHigh Energy Physics::PhenomenologyElementary particlesScaling exponent Lead alloys020207 software engineeringBinary alloysW bosonsLeading ordersrapidityevolution equation[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph][ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::Experimentcomputerhigh-energy hadronic collisionsLead Center-of-mass energiesLepton
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Solar neutrino spectroscopy in Borexino

2018

International audience; In more than ten years of operation, Borexino has performed a precision measurement of the solar neutrino spectrum, resolving almost all spectral components originating from the proton-proton fusion chain. The presentation will review the results recently released for the second data taking phase 2012–2016 during which the detector excelled by its unprecedentedly low background levels. New results on the rate of pp, 7Be, pep and 8B neutrinos as well as their implications for solar neutrino oscillations and metallicity are discussed.

neutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoMetallicityNuclear physicsbackground: lowneutrino: spectrum[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutrino oscillationSpectroscopyBorexinoPhysicsProton–proton chain reactionpp-chainp p: fusionprecision measurementDetector* Automatic Keywords *13. Climate actionsolar neutrinosspectralHigh Energy Physics::ExperimentBorexinoneutrino: oscillationNeutrino[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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The XENON1T Dark Matter Experiment

2017

The XENON1T experiment at the Laboratori Nazionali del Gran Sasso (LNGS) is the first WIMP dark matter detector operating with a liquid xenon target mass above the ton-scale. Out of its 3.2 t liquid xenon inventory, 2.0 t constitute the active target of the dual-phase time projection chamber. The scintillation and ionization signals from particle interactions are detected with low-background photomultipliers. This article describes the XENON1T instrument and its subsystems as well as strategies to achieve an unprecedented low background level. First results on the detector response and the performance of the subsystems are also presented. © 2017, The Author(s).

xenon: targetPhotomultiplierCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)WIMP[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Dark matterchemistry.chemical_elementFOS: Physical scienceslcsh:Astrophysics01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)XENONXenonbackground: lowWIMP[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]Ionization0103 physical scienceslcsh:QB460-466[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Dark Matterlcsh:Nuclear and particle physics. Atomic energy. Radioactivity[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsEngineering (miscellaneous)Instrumentation and Methods for Astrophysics (astro-ph.IM)[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]AstrophysiquePhysicsScintillationxenon: liquidTime projection chamberphotomultiplier010308 nuclear & particles physicsDetectorInstrumentation and Detectors (physics.ins-det)dark matter: detectortime projection chamberchemistrylcsh:QC770-798TPCAstrophysics - Instrumentation and Methods for Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]performanceAstrophysics - Cosmology and Nongalactic AstrophysicsEuropean Physical Journal C
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Excess electronic recoil events in XENON1T

2020

We report results from searches for new physics with low-energy electronic recoil data recorded with the XENON1T detector. With an exposure of 0.65 t-y and an unprecedentedly low background rate of $76\pm2$ events/(t y keV) between 1 and 30 keV, the data enables sensitive searches for solar axions, an enhanced neutrino magnetic moment, and bosonic dark matter. An excess over known backgrounds is observed at low energies and most prominent between 2 and 3 keV. The solar axion model has a 3.4$\sigma$ significance, and a 3D 90% confidence surface is reported for axion couplings to electrons, photons, and nucleons. This surface is inscribed in the cuboid defined by $g_{ae}<3.8 \times 10^{-12}$,…

xenon: targetaxionssolar axionmagnetic momentdimension: 3neutrino: solarPhysics beyond the Standard ModelSolar neutrinodark matter: direct detection01 natural sciences7. Clean energyHigh Energy Physics - ExperimentDark matter direct detection axionHigh Energy Physics - Experiment (hep-ex)neutrinoXENONHigh Energy Physics - Phenomenology (hep-ph)background: lowRecoilelectron: recoil[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]beta-raysParticle Physics Experimentscoupling: (axion 2electron)multi-purpose particle detectornuclear instrumentationComputingMilieux_MISCELLANEOUSinstrumentationPhysicsxenon: liquidboson: dark matteraxion 2nucleontritiumnew physics: search forsemileptonic decayboson: vectortensionneutrino: magnetic momentHigh Energy Physics - Phenomenologyaxion 2photonlow backgroundbosonNeutrinoionizing radiationNucleonAstrophysics - Cosmology and Nongalactic AstrophysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)dark matter detectorelectronic recoilElectron captureXENON1T detectorDark matterlow-energy electronic recoil dataFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]dark matterNONuclear physicsPE2_2PE2_1tritium: semileptonic decay0103 physical sciencessolar axion modelsurface[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]axion: couplingPE2_4010306 general physicspseudoscalarAxiondark matter: vectordark matter XENON1T detector electronic recoilsolar neutrinodetectorDark Matter Axions Beta Decay Liquid Xenon TPC010308 nuclear & particles physicsaxion 2electroncoupling: (axion 2nucleon)dark matter: detectormodel: axionGran Sassometrology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]axionstellar constraintscoupling: (axion 2photon)High Energy Physics::Experimentparticle dark matterdirect detectionbeta decayaxion: solar[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]experimental results
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