Search results for "detectors"

showing 10 items of 2229 documents

The THESEUS space mission concept: science case, design and expected performances

2018

THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and time-domain astrophysics. These goals will be achieved through a unique combination of instruments allowing GRB and X-ray transient detection over a broad field of view (more than 1sr) with 0.5¿1 arcmin localization, an energy band extending from several MeV down to 0.3¿keV and high sensitivity to transient sources in the soft X-ray domain, as well as on-board prompt (few minutes) follow-up with a 0.7¿m class IR telescope with both imaging and spectroscopic capabilities. THESEUS will be perfectly suited for addressing …

IonizationAtmospheric Sciencecosmological modelCherenkov Telescope Array[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]AstronomyDark ageMASSIVE SINGLE STARSStar formation rates Gamma ray01 natural sciencesCosmology: observationlocalizationlaw.inventionAstrophysicEinstein Telescopeobservational cosmologylawObservational cosmologyRe-ionizationCosmology: observations; Dark ages; First stars; Gamma-ray: bursts; Re-ionizationLIGOobservations [Cosmology]Telescope010303 astronomy & astrophysicsHigh sensitivityHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMulti-wavelengthenergy: highsezelegamma-ray burstsCosmology: observationsCosmology: observations; Dark ages; First stars; Gamma-ray: bursts; Re-ionization; Aerospace Engineering; Space and Planetary ScienceAstrophysics::Instrumentation and Methods for Astrophysicsimagingstar: formationburst [Gamma-ray]observatoryGeophysicsDark agesX rays Cosmology: observationAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenasignatureStarTIDAL DISRUPTIONGamma-ray: burstAstrophysics::High Energy Astrophysical PhenomenaSIMILAR-TO 6Socio-culturaleFOS: Physical sciencesAerospace EngineeringGamma-ray: burstsobservation [Cosmology]galaxy: luminosityX-ray astronomy: instrumentation7 CANDIDATE GALAXIESAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burst114 Physical sciencesSettore FIS/03 - Fisica della MateriaTelescopeX-raybursts [Gamma-ray]FIS/05 - ASTRONOMIA E ASTROFISICASettore FIS/05 - Astronomia e AstrofisicaFirst star0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]KAGRAInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics::Galaxy AstrophysicsFirst starsLIGHT CURVESEinstein Telescope010308 nuclear & particles physicsGravitational wavegravitational radiationAstronomyAstronomy and Astrophysics115 Astronomy Space scienceCherenkov Telescope ArrayredshiftsensitivityRedshiftNEUTRON-STAR MERGERmessengerVIRGOelectromagneticLUMINOSITY FUNCTIONSpace and Planetary ScienceBLACK-HOLEGeneral Earth and Planetary SciencesGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Radiation effects on optical frequency domain reflectometry fiber-based sensor

2015

International audience; We investigate the radiation effects on germanosilicate optical fiber acting as the sensing element of optical frequency domain reflectometry devices. Thanks to a new setup permitting to control temperature during irradiation, we evaluate the changes induced by 10 keV x rays on their Rayleigh response up to 1 MGy in a temperature range from −40°C up to 75°C. Irradiation at fixed temperature points out that its measure is reliable during both irradiation and the recovery process. Mixed temperature and radiation measurements show that changing irradiation temperature leads to an error in distributed measurements that depends on the calibration procedure. These results …

Ionizing radiationMaterials scienceOptical fiberPhysics::Instrumentation and Detectors02 engineering and technologyRayleigh scatteringRadiation01 natural scienceslaw.inventionScattering010309 opticssymbols.namesakeOpticslaw0103 physical sciencesRayleighIrradiationElectroniqueRayleigh scatteringReflectometryRadiationbusiness.industryFiber optics sensorsdistributed fiber optics sensorAtmospheric temperature rangeDistributed acoustic sensing021001 nanoscience & nanotechnologyAtomic and Molecular Physics and Optics[SPI.TRON]Engineering Sciences [physics]/ElectronicsFiber optic sensoroptical frequency domain reflectometrysymbols0210 nano-technologybusinesstemperature sensingOptics Letters
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Feasibility and physics potential of detecting 8B solar neutrinos at JUNO

2021

The Jiangmen Underground Neutrino Observatory (JUNO) features a 20 kt multi-purpose underground liquid scintillator sphere as its main detector. Some of JUNO's features make it an excellent location for B-8 solar neutrino measurements, such as its low-energy threshold, high energy resolution compared with water Cherenkov detectors, and much larger target mass compared with previous liquid scintillator detectors. In this paper, we present a comprehensive assessment of JUNO's potential for detecting B solar neutrinos via the neutrino-electron elastic scattering process. A reduced 2 MeV threshold for the recoil electron energy is found to be achievable, assuming that the intrinsic radioactive …

JUNOneutriino-oskillaatiosolar neutrinoPhysics::Instrumentation and DetectorsilmaisimettutkimuslaitteetneutriinotHigh Energy Physics::Experimenthiukkasfysiikkaydinfysiikka
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Inducing Strong Non-Linearities in a Phonon Trapping Quartz Bulk Acoustic Wave Resonator Coupled to a Superconducting Quantum Interference Device

2018

International audience; A quartz Bulk Acoustic Wave resonator is designed to coherently trap phonons in such a way that they are well confined and immune to suspension losses so they exhibit extremely high acoustic Q-factors at low temperature, with Q × f products of order 10¹⁸ Hz. In this work we couple such a resonator to a Superconducting Quantum Interference Device (SQUID) amplifier and investigate effects in the strong signal regime. Both parallel and series connection topologies of the system are investigated. The study reveals significant non-Duffing response that is associated with the nonlinear characteristics of Josephson junctions. The nonlinearity provides quasi-periodic structu…

Josephson effect[SPI.OTHER]Engineering Sciences [physics]/OtherPhysics - Instrumentation and DetectorsPhononphonon trappingFOS: Physical sciences02 engineering and technologySQUID01 natural sciencesSignallcsh:Technologylaw.inventionlcsh:ChemistryResonatorlaw0103 physical sciencesnon-linear couplingMesoscale and Nanoscale Physics (cond-mat.mes-hall)low noise oscillatorGeneral Materials Science010306 general physicsInstrumentationlcsh:QH301-705.5Fluid Flow and Transfer ProcessesPhysicsCondensed matter physicsCondensed Matter - Mesoscale and Nanoscale Physicslcsh:TProcess Chemistry and TechnologyAmplifierGeneral EngineeringInstrumentation and Detectors (physics.ins-det)021001 nanoscience & nanotechnologylcsh:QC1-999Computer Science ApplicationsSQUIDNonlinear systemlcsh:Biology (General)lcsh:QD1-999lcsh:TA1-2040BAW Resonator; SQUID; phonon trapping; low noise oscillator; non-linear couplingBAW Resonator0210 nano-technologylcsh:Engineering (General). Civil engineering (General)Crystal oscillatorlcsh:Physics
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Differential branching fraction and angular analysis of the decay $B^{0} \to K^{*0} \mu^{+}\mu^{-}$

2013

The angular distribution and differential branching fraction of the decay B-0 -> K*(0)mu(+)mu(-) are studied using a data sample, collected by the LHCb experiment in pp collisions at root s = 7 TeV, corresponding to an integrated luminosity of 1.0 fb(-1). Several angular observables are measured in bins of the dimuon invariant mass squared, q(2). A first measurement of the zero-crossing point of the forward-backward asymmetry of the dimuon system is also presented. The zero-crossing point is measured to be q(0)(2) = 4.9 +/- 0.9 GeV2/c(4), where the uncertainty is the sum of statistical and systematic uncertainties. The results are consistent with the Standard Model predictions.

K-ASTERISK-L(+)L(-)12.15.Mm01 natural sciencesB physicsLuminositydecayHigh Energy Physics - ExperimentSettore FIS/04 - Fisica Nucleare e SubnucleareNeutral currentFlavor physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Invariant massQCDetectors de radiaciómedia_commonPhysicsB0 mesonHadron-induced high- and super-high-energy interactions (energy > 10 GeV): Inclusive production with identified hadronObservableCP violationFIS/01 - FISICA SPERIMENTALENuclear countersLeptonic semileptonic and radiative decays of bottom mesonsFísica nuclearLHCB physics; Flavor physics; Flavour Changing Neutral Currents; Hadron-Hadron Scattering; Rare decayParticle Physics - ExperimentParticle physicsNuclear and High Energy Physicsmedia_common.quotation_subject14.40.NdFlavour Changing Neutral CurrentsHadronsAsymmetryPartícules (Física nuclear)Standard ModelB physics; Flavor physics; Flavour Changing Neutral Currents; Hadron-Hadron Scattering; Rare decay; Nuclear and High Energy PhysicsNeutral currentsAngular distributionASYMMETRIES0103 physical sciencesLeptonic semileptonic and radiative decays of bottom mesonLHC flavour physics010306 general physicsHadron-induced high- and super-high-energy interactions (energy > 10 GeV): Inclusive production with identified hadronsB0 meson; decay; LHCb; LHCHadron-Hadron Scattering010308 nuclear & particles physicsBranching fractionCromodinàmica quànticaLHCbRare decay13.20.HeBottom mesons (|B|>0); Leptonic semileptonic and radiative decays of bottom mesons; Hadron-induced high- and super-high-energy interactions (energy > 10 GeV): Inclusive production with identified hadrons; Neutral currents; 14.40.Nd; 13.20.He; 13.85.Ni; 12.15.Mm;Bottom mesons (|B|>0)High Energy Physics::Experiment13.85.NiDifferential (mathematics)FIS/04 - FISICA NUCLEARE E SUBNUCLEAREQuantum chromodynamicsexperimental results
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Deep sea tests of a prototype of the KM3NeT digital optical module

2014

SIRE(opens in a new window)|View at Publisher| Export | Download | Add to List | More... European Physical Journal C Volume 74, Issue 9, 1 September 2014, 8p Deep sea tests of a prototype of the KM3NeT digital optical module: KM3NeT Collaboration (Article) Adrián-Martínez, S.a, Ageron, M.b, Aharonian, F.c, Aiello, S.d, Albert, A.e, Ameli, F.f, Anassontzis, E.G.g, Anghinolfi, M.h, Anton, G.i, Anvar, S.j, Ardid, M.a, de Asmundis, R.k, Balasi, K.l, Band, H.m, Barbarino, G.kn, Barbarito, E.o, Barbato, F.kn, Baret, B.p, Baron, S.p, Belias, A.lq, Berbee, E.m, van den Berg, A.M.r, Berkien, A.m, Bertin, V.b, Beurthey, S.b, van Beveren, V.m, Beverini, N.st, Biagi, S.uv, Bianucci, S.t, Billault, M.b,…

KM3NeT; digital optical modulePhysics - Instrumentation and Detectors[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics and Astronomy (miscellaneous)TELESCOPEPhysics::Instrumentation and Detectorsdigital optical moduleFOS: Physical sciencesNeutrino Telescopesneutrino astrophysics; Cherenkov detector; Neutrino TelescopesKM3NeT; Cherenkov; UnderwaterDESIGNCherenkov[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Instrumentation and Methods for Astrophysics (astro-ph.IM)KM3NeTEngineering (miscellaneous)Astrophysics::Instrumentation and Methods for Astrophysicsneutrino telescopeDATA-ACQUISITIONInstrumentation and Detectors (physics.ins-det)READOUTneutrino astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]NEUTRINOSUnderwaterAstrophysics - Instrumentation and Methods for AstrophysicsSYSTEMCherenkov detector
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Low-energy Neutrino Astronomy in LENA

2015

LENA (Low Energy Neutrino Astronomy) is a proposed next-generation neutrino detector based on 50 kilotons of liquid scintillator. The low detection threshold, good energy resolution and excellent background rejection inherent to the liquid-scintillator detectors make LENA a versatile observatory for low-energy neutrinos from astrophysical and terrestrial sources. In the framework of the European LAGUNA-LBNO design study, LENA is also considered as far detector for a very-long baseline neutrino beam from CERN to Pyhasalmi ¨ (Finland). The present contribution gives an overview LENA’s broad research program, highlighting the unique capabilities of liquid scintillator for the detection of low-…

LENAPhysicsParticle physicsta114Physics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologySolar neutrino problemPhysics and Astronomy(all)astroparticle physics. underground physicsNuclear physicslow-energy neutrino astronomyNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoNeutrino oscillationElectron neutrinoPhysics Procedia
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Investigation of LaBr3(Ce) detectors at the RITU focal plane

2015

The aims of this master thesis were to determine the absolute detection efficiency of the LaBr3(Ce) detectors installed at the RITU focal plane, to study the effect of planar Ge-detector on the LaBr3(Ce) efficiency and to investigate the possibility of half-life measurements with the detectors in a coincidence setup having distributed recoil ions produced by the RITU separator. Time spectra were collected by moving a point radioactive source from one edge of the implantation detector to the other to imitate the ion distribution from the RITU separator. Simulations have been exploited to explore the time spectra obtained from various ion distribution shapes and for different half-lives. A po…

LaBr3(Ce) detectorsPhysics::Instrumentation and Detectorsfast-timingRITU separatorgamma detection
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Performance of ATLAS tracking detector

2012

The track and vertex reconstruction algorithms of the ATLAS Inner Detector have demonstrated excellent performance in the early data from the LHC. However, the rapidly increas- ing number of interactions per bunch crossing introduces new challenges both in computational aspects and physics performance. The combination of both silicon and gas based detectors provides high precision impact parameter and momentum measurement of charged particles, with high efficiency and small fake rate. Vertex reconstruction is used to identify with high efficiency the hard scattering process and to measure the amount of pile-up interactions, both aspects are cru- cial for many physics analyses. The performan…

Large Hadron ColliderAtlas (topology)Computer scienceDetectorScattering processImpact parameterDetectors and Experimental TechniquesImage resolutionCharged particleComputational science
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An FPGA based Topological Processor Prototype for the ATLAS Level-1 Trigger Upgrade

2012

By 2014 the LHC will collide proton bunches at 14TeV with an increased instantaneous luminosity up to 3·10³⁴cm⁻²s⁻¹. The resulting higher event rate will challenge the existing ATLAS trigger system. A reduction on the trigger rate can be achieved by selecting interesting channels based on their expected decay topology and thus reducing background. This will be achieved by introducing of a new FPGA based module in the Level-1 trigger: the Topological Processor L1Topo. With L1Topo it will be possible for the first time to concentrate detailed information from the entire calorimeters and the muon detector into a single module. L1Topo will receive a total aggregate bandwidth of 1Tb/s. The data …

Large Hadron ColliderBandwidth (signal processing)TopologyLinear particle acceleratorComputer Science::Hardware ArchitectureData acquisitionBunchesUpgradePhysics::Accelerator PhysicsTransceiverDetectors and Experimental TechniquesField-programmable gate arrayInstrumentationMathematical Physics
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