Search results for "Particle radiation"

showing 7 items of 677 documents

Search for a diffuse flux of high-energy ¿µ with the ANTARES neutrino telescope

2011

A search for a diffuse flux of astrophysical muon neutrinos, using data collected by the ANTARES neutrino telescope is presented. A $(0.83\times 2\pi)$ sr sky was monitored for a total of 334 days of equivalent live time. The searched signal corresponds to an excess of events, produced by astrophysical sources, over the expected atmospheric neutrino background. The observed number of events is found compatible with the background expectation. Assuming an $E^{-2}$ flux spectrum, a 90% c.l. upper limit on the diffuse $\nu_\mu$ flux of $E^2\Phi_{90%} = 5.3 \times 10^{-8} \ \mathrm{GeV\ cm^{-2}\ s^{-1}\ sr^{-1}} $ in the energy range 20 TeV - 2.5 PeV is obtained. Other signal models with differ…

neutrino telescope; antares; diffuse muon neutrino fluxNuclear and High Energy PhysicsParticle physics[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]media_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeFluxAstrophysicsNeutrino telescope01 natural sciences7. Clean energySpectral lineMUONSLIMITS0103 physical sciencesNeutrins010306 general physicsDETECTORmedia_commonPhysicsRange (particle radiation)MuonsMuonANTARES:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsMuon Collaboration[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsNeutrino astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]MODELDiffuse muon neutrino fluxSky:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]High Energy Physics::ExperimentFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical PhenomenaEnergy (signal processing)
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Measurement of the average shape of longitudinal profiles of cosmic-ray air showers at the Pierre Auger Observatory

2019

The profile of the longitudinal development of showers produced by ultra-high energy cosmic rays carries information related to the interaction properties of the primary particles with atmospheric nuclei. In this work, we present the first measurement of the average shower profile in traversed atmospheric depth at the Pierre Auger Observatory. The shapes of profiles are well reproduced by the Gaisser-Hillas parametrization within the range studied, for E>10 17.8 eV .A detailed analysis of the systematic uncertainties is performed using ten years of data and a full detector simulation. The average shape is quantified using two variables related to the width and asymmetry of the profile, and …

p: showersphoton: Cherenkovinteraction: modelAstronomyHadronpiastro-ph.HE; astro-ph.HE01 natural sciencesnitrogenironParametrization (atmospheric modeling)Monte Carlomedia_commonPhysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Range (particle radiation)photomultiplierSettore FIS/01 - Fisica SperimentaleDetectorAstrophysics::Instrumentation and Methods for AstrophysicsDETETOREScosmic rays detectors; ultra high energy cosmic rays; Astronomy and AstrophysicsAugerobservatorycosmic rays detectorscosmic rays detectors; ultra high energy cosmic raysgeometricalAstrophysics - High Energy Astrophysical PhenomenaasymmetrylongitudinalCherenkov counter: waterairmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayheliumultra high energy cosmic raysnucleus: atmosphereAsymmetry0103 physical sciencesHigh Energy Physicscosmic radiation: UHEcosmic rays detectorFLUORESCENCEAstrophysiquePierre Auger Observatoryelectron positronshowers: atmosphere010308 nuclear & particles physicsbackgrounddetector: surfaceshowers: spatial distributionparametrizationAstronomy and AstrophysicsAstronomieComputational physics13. Climate actiongamma rayExperimental High Energy Physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)Journal of Cosmology and Astroparticle Physics
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The PANDA Endcap Disc DIRC

2018

Journal of Instrumentation 13(02), C02002 - C02002 (2018). doi:10.1088/1748-0221/13/02/C02002

particle identification [K]Physics::Instrumentation and Detectors61001 natural sciencesDIRCK: particle identificationOpticsPionDetection of internally reflected Cherenkov light0103 physical sciencesparticle identification [pi]ddc:610010306 general physicsNuclear ExperimentInstrumentationMathematical PhysicsCherenkov radiationPhysicsCherenkov counter: designRange (particle radiation)010308 nuclear & particles physicsbusiness.industryPANDADetectorSolid angleDESYLight guideTest beamdesign [Cherenkov counter]Radiator (engine cooling)Facility for Antiproton and Ion ResearchHigh Energy Physics::ExperimentPhotonicsbusinesspi: particle identificationperformance
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Single Event Upsets Induced by Direct Ionization from Low-Energy Protons in Floating Gate Cells

2017

Floating gate cells in advanced NAND Flash memories, with single-level and multi-level cell architecture, were exposed to low-energy proton beams. The first experimental evidence of single event upsets by proton direct ionization in floating gate cells is reported. The dependence of the error rate versus proton energy is analyzed in a wide energy range. Proton direct ionization events are studied and energy loss in the overlayers is discussed. The threshold LET for floating gate errors in multi-level and single-level cell devices is modeled and technology scaling trends are analyzed, also discussing the impact of the particle track size. peerReviewed

protonitNuclear and High Energy PhysicsProtonfloating gate devicesNAND gateFlash memories01 natural sciencesComputer Science::Hardware ArchitectureIonizationFlash memories; floating gate devices; protons; single event effects; Nuclear and High Energy Physics; Nuclear Energy and Engineering; Electrical and Electronic Engineering0103 physical sciencesHardware_ARITHMETICANDLOGICSTRUCTURESElectrical and Electronic Engineeringflash-muistit010302 applied physicsPhysicsRange (particle radiation)ta114ta213protons010308 nuclear & particles physicsbusiness.industryElectrical engineeringsingle event effectsNon-volatile memoryNuclear Energy and EngineeringLogic gateAtomic physicsbusinessEvent (particle physics)Energy (signal processing)IEEE Transactions on Nuclear Science
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Long-range spin accumulation from heat injection in mesoscopic superconductors with Zeeman splitting

2015

Under the terms of the Creative Commons Attribution License 3.0 (CC-BY).

ta221General Physics and Astronomy02 engineering and technologyZero field splittingengineering.materialsuperconductorsspin7. Clean energy01 natural sciencessymbols.namesake0103 physical sciencesheat injection010306 general physicsta218Spin-½PhysicsSuperconductivityRange (particle radiation)Mesoscopic physicsZeeman effectta214Condensed matter physicsta114Superconducting wire021001 nanoscience & nanotechnologyThermalisationengineeringsymbols0210 nano-technology
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Thermoluminescence response of sodalime glass irradiated with photon and electron beams in the 1-20 Gy range

2011

Abstract The thermoluminescence response of a watch commercial glass was studied after irradiation with photons and electrons, in the range 1–20 Gy, of interest in accidental dosimetry; a linear response was obtained with both beams. This result, together with the satisfactory time stability of the thermoluminescence signal, indicates this glass as a potential material for retrospective dosimetry applications.

thermoluminecence watch glass photons electronsRange (particle radiation)RadiationPhotonMaterials sciencebusiness.industryRadiochemistryElectronThermoluminescenceOpticsDosimetryIrradiationbusinessInstrumentation
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Underground investigation of extensive air showers spectra at high energy range of cosmic rays and other research in the Pyhäsalmi mine

2020

Abstract High energy particles reaching the Earth’s atmosphere are known as cosmic rays. As a result of interactions with nuclei of air molecules, cosmic rays induce showers of secondary particles, which can be divided into 3 components: electromagnetic, hadronic and muonic components. The Experiment with Multi Muon Array (EMMA), located at the depth of 75 m in the Pyhäsalmi mine in Finland, investigates the muonic component of the Extensive Air Showers (EAS) to deduce the direction, energy, and the mass of the primary cosmic ray particles. In this paper we give a concise description and methodology used by EMMA followed by a brief review of the C14 experiment. Finally, we review the feasib…

ғарыш сәулелеріPhysics::Instrumentation and DetectorsastrofysiikkaAstrophysics::High Energy Astrophysical PhenomenaBoreholekneeOcean EngineeringCosmic rayhiukkasfysiikkaSpectral lineAtmosphereNuclear physicsnuclear and elementary particle physicscosmic rayshigh-energy muonжоғары энергиялы мюонPhysicsтізе аймағыtheoretical physicsRange (particle radiation)Muonastrophysicsкең ауқымды нөсер (КАН)Neutrino detectorilmaisimetExtensive Air Shower (EAS)EMMANeutrinokosminen säteily
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