Search results for "Control system"

showing 10 items of 971 documents

Sensitivity recovery for the AX-PET prototype using inter-crystal scattering events

2014

The development of novel detection devices and systems such as the AX-positron emission tomography (PET) demonstrator often introduce or increase the measurement of atypical coincidence events such as inter-crystal scattering (ICS). In more standard systems, ICS events often go undetected and the small measured fraction may be ignored. As the measured quantity of such events in the data increases, so too does the importance of considering them during image reconstruction. Generally, treatment of ICS events will attempt to determine which of the possible candidate lines of response (LoRs) correctly determine the annihilation photon trajectory. However, methods of assessment often have low su…

PhotonsRadiological and Ultrasound TechnologyPhantoms ImagingComputer scienceScatteringIterative reconstructionSensitivity and SpecificityImaging phantomSignal-to-noise ratioPositron-Emission TomographyImage Processing Computer-AssistedScattering RadiationRadiology Nuclear Medicine and imagingTomographySensitivity (control systems)AlgorithmAlgorithmsSimulationPhysics in Medicine and Biology
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EUDAQ $-$ A Data Acquisition Software Framework for Common Beam Telescopes

2019

EUDAQ is a generic data acquisition software developed for use in conjunction with common beam telescopes at charged particle beam lines. Providing high-precision reference tracks for performance studies of new sensors, beam telescopes are essential for the research and development towards future detectors for high-energy physics. As beam time is a highly limited resource, EUDAQ has been designed with reliability and ease-of-use in mind. It enables flexible integration of different independent devices under test via their specific data acquisition systems into a top-level framework. EUDAQ controls all components globally, handles the data flow centrally and synchronises and records the data…

Physics - Instrumentation and DetectorsDetector control systems (detector and experiment monitoring and slow-control systems architecture hardware algorithms databases)data acquisitionData management01 natural sciences7. Clean energyHigh Energy Physics - Experiment030218 nuclear medicine & medical imagingHigh Energy Physics - Experiment (hep-ex)0302 clinical medicineData acquisitionbeam [charged particle]Particle tracking detectors[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]hardwareDetectors and Experimental Techniquesphysics.ins-detInstrumentationMathematical PhysicsData processingData stream miningPhysicsDetectorInstrumentation and Detectors (physics.ins-det)control systemCharged particle beamdatabases)Particle Physics - ExperimentComputer hardwareperformancearchitectureData acquisition system for beam tests [5]FOS: Physical sciencesalgorithmsprogramming03 medical and health sciencesCalorimeterscharged particle: beam0103 physical sciencesddc:530ddc:610[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]hep-ex010308 nuclear & particles physicsbusiness.industryDetector control systems (detector and experiment monitoring and slow-control systemsData acquisition conceptsData flow diagramdata managementbusinessBeam (structure)
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Quantum sensitivity limits of nuclear magnetic resonance experiments searching for new fundamental physics

2021

Nuclear magnetic resonance is a promising experimental approach to search for ultra-light axion-like dark matter. Searches such as the cosmic axion spin-precession experiments (CASPEr) are ultimately limited by quantum-mechanical noise sources, in particular, spin-projection noise. We discuss how such fundamental limits can potentially be reached. We consider a circuit model of a magnetic resonance experiment and quantify three noise sources: spin-projection noise, thermal noise, and amplifier noise. Calculation of the total noise spectrum takes into account the modification of the circuit impedance by the presence of nuclear spins, as well as the circuit back-action on the spin ensemble. S…

Physics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Materials Science (miscellaneous)Dark matterFOS: Physical sciences01 natural sciencesNoise (electronics)010305 fluids & plasmasNuclear magnetic resonanceHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesddc:530Sensitivity (control systems)Electrical and Electronic Engineering010306 general physicsAxionQuantumElectrical impedanceSpin-½PhysicsQuantum PhysicsSpinsInstrumentation and Detectors (physics.ins-det)Atomic and Molecular Physics and OpticsCondensed Matter - Other Condensed MatterHigh Energy Physics - PhenomenologyQuantum Physics (quant-ph)Other Condensed Matter (cond-mat.other)
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The 3 Cavity Prototypes of RADES: An Axion Detector Using Microwave Filters at CAST

2019

The Relic Axion Detector Experimental Setup (RADES) is an axion search project that uses a microwave filter as resonator for Dark Matter conversion. The main focus of this publication is the description of the 3 different cavity prototypes of RADES. The result of the first tests of one of the prototypes is also presented. The filters consist of 5 or 6 stainless steel sub-cavities joined by rectangular irises. The size of the sub-cavities determines the working frequency, the amount of sub-cavities determine the working volume. The first cavity prototype was built in 2017 to work at a frequency of $\sim$ 8.4 GHz and it was placed at the 9 T CAST dipole magnet at CERN. Two more prototypes wer…

Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsFOS: Physical sciences7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)ResonatorOpticsDipole magnet0103 physical sciencesSensitivity (control systems)Detectors and Experimental Techniques010306 general physicsAxionphysics.ins-detPhysicsLarge Hadron Collider010308 nuclear & particles physicsbusiness.industryhep-exDetectorInstrumentation and Detectors (physics.ins-det)Filter (signal processing)Physics::Accelerator PhysicsbusinessMicrowaveParticle Physics - Experiment
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Combined sensitivity to the neutrino mass ordering with JUNO, the IceCube Upgrade, and PINGU

2020

Physical review / D 101(3), 032006 (1-19) (2020). doi:10.1103/PhysRevD.101.032006

Physics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorsantineutrino/e: energy spectrumJoint analysishiukkasfysiikka7. Clean energy01 natural sciencesString (physics)PINGUHigh Energy Physics - ExperimentSubatomär fysikHigh Energy Physics - Experiment (hep-ex)neutrino: atmosphereSubatomic Physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Particle Physics Experimentsneutrino: massphysics.ins-detPhysicsJUNOPhysicsneutriinotoscillation [neutrino]Instrumentation and Detectors (physics.ins-det)massa (fysiikka)atmosphere [neutrino]tensionneutrino: nuclear reactormass difference [neutrino]ddc:UpgradePhysique des particules élémentairesnuclear reactor [neutrino]proposed experimentNeutrinoperformanceParticle physicsAstrophysics::High Energy Astrophysical Phenomenaneutrino: mass differenceFOS: Physical sciencesddc:500.25300103 physical sciencesEnergy spectrumIceCube: upgradeOSCILLATIONSddc:530Sensitivity (control systems)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationenergy spectrum [antineutrino/e]hep-ex010308 nuclear & particles physicssensitivityPhysics and Astronomymass [neutrino]stringupgrade [IceCube]High Energy Physics::ExperimentReactor neutrinoneutrino: oscillationMATTER
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Solar neutrino detection in liquid xenon detectors via charged-current scattering to excited states

2020

We investigate the prospects for real-time detection of solar neutrinos via the charged-current neutrino-nucleus scattering process in liquid xenon time projection chambers. We use a nuclear shell model, benchmarked with experimental data, to calculate the cross sections for populating specific excited states of the caesium nuclei produced by neutrino capture on $^{131}$Xe and $^{136}$Xe. The shell model is further used to compute the decay schemes of the low-lying $1^{+}$ excited states of $^{136}$Cs, for which there is sparse experimental data. We explore the possibility of tagging the characteristic de-excitation $\gamma$-rays/conversion electrons using two techniques: spatial separation…

Physics - Instrumentation and DetectorsSolar neutrinochemistry.chemical_elementFOS: Physical sciencesksenonhiukkasfysiikka7. Clean energy01 natural sciencesnucleus-neutrino interactionsHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)XenonHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesSensitivity (control systems)010306 general physicsPhysics010308 nuclear & particles physicsNuclear shell modelshell modelneutriinotInstrumentation and Detectors (physics.ins-det)nuclear structure and decays3. Good healthProjection (relational algebra)High Energy Physics - PhenomenologychemistryilmaisimetExcited statesolar neutrinosNeutrinoydinfysiikkaEnergy (signal processing)
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The distributed Slow Control System of the XENON100 experiment

2012

The XENON100 experiment, in operation at the Laboratori Nazionali del Gran Sasso (LNGS) in Italy, was designed to search for evidence of dark matter interactions inside a volume of liquid xenon using a dual-phase time projection chamber. This paper describes the Slow Control System (SCS) of the experiment with emphasis on the distributed architecture as well as on its modular and expandable nature. The system software was designed according to the rules of Object-Oriented Programming and coded in Java, thus promoting code reusability and maximum flexibility during commissioning of the experiment. The SCS has been continuously monitoring the XENON100 detector since mid 2008, remotely recordi…

Physics - Instrumentation and Detectorsarchitecture[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]JavaComputer scienceReal-time computingFOS: Physical scienceschemistry.chemical_elementControl and monitor systems online; Control systems; Detector control systems (detector and experiment monitoring and slow-control systems architecture hardware algorithms databases)algorithms01 natural sciencesXenon0103 physical scienceshardwareDETECTOR CONTROL SYSTEMS[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]CONTROL SYSTEMS010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)InstrumentationMathematical Physicscomputer.programming_languageTime projection chamber010308 nuclear & particles physicsbusiness.industryControl and monitor systems onlineDetector control systems (detector and experiment monitoring and slow-control systemsEmphasis (telecommunications)Volume (computing)Instrumentation and Detectors (physics.ins-det)Modular design[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]chemistryControl systemAstrophysics - Instrumentation and Methods for Astrophysicsdatabases)businesscomputerSystem software
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Feasibility and physics potential of detecting $^8$B 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 8B 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 8B 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 …

Physics - Instrumentation and Detectorsneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoscintillation counter: liquidhigh [energy resolution]01 natural sciences7. Clean energymass [target]High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)JUNO; Neutrino oscillation; Solar neutrinoelastic scattering [neutrino electron]KamLAND[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]flavor [transformation]neutrino oscillationInstrumentationJiangmen Underground Neutrino ObservatoryPhysicsElastic scatteringJUNOliquid [scintillation counter]neutrino oscillation solar neutrino JUNOSettore FIS/01 - Fisica Sperimentaleoscillation [neutrino]Instrumentation and Detectors (physics.ins-det)Monte Carlo [numerical calculations]neutrino electron: elastic scatteringtensionmass difference [neutrino]ddc:nuclear reactor [antineutrino]observatoryHigh Energy Physics - PhenomenologyPhysics::Space Physicsneutrino: flavorsolar [neutrino]target: massNeutrinonumerical calculations: Monte CarloNuclear and High Energy PhysicsParticle physicsNeutrino oscillationmatter: solarCherenkov counter: waterneutrino: mass differenceFOS: Physical sciencesSolar neutrinoNOtransformation: flavoruraniumPE2_20103 physical scienceselectron: recoil: energyantineutrino: nuclear reactorsolar [matter]ddc:530ddc:610Sensitivity (control systems)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationbackground: radioactivityCherenkov radiationAstrophysiquesolar neutrino010308 nuclear & particles physicswater [Cherenkov counter]radioactivity [background]flavor [neutrino]Astronomy and Astrophysicssensitivityneutrino: mixing anglerecoil: energy [electron]energy spectrum [electron]electron: energy spectrumHigh Energy Physics::Experimentsphereneutrino: oscillationenergy resolution: highEnergy (signal processing)mixing angle [neutrino]
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Correlation based networks of equity returns sampled at different time horizons

2006

We investigate the planar maximally filtered graphs of the portfolio of the 300 most capitalized stocks traded at the New York Stock Exchange during the time period 2001-2003. Topological properties such as the average length of shortest paths, the betweenness and the degree are computed on different planar maximally filtered graphs generated by sampling the returns at different time horizons ranging from 5 min up to one trading day. This analysis confirms that the selected stocks compose a hierarchical system progressively structuring as the sampling time horizon increases. Finally, a cluster formation, associated to economic sectors, is quantitatively investigated.

Physics - Physics and Societynetworks of equity different time horizonsStatistical Finance (q-fin.ST)Equity (finance)Quantitative Finance - Statistical FinanceFOS: Physical sciencesRangingPhysics and Society (physics.soc-ph)Condensed Matter PhysicsElectronic Optical and Magnetic MaterialsCorrelationFOS: Economics and businessBetweenness centralityStock exchangePhysics - Data Analysis Statistics and ProbabilityStatisticsHierarchical control systemPortfolioSampling timeData Analysis Statistics and Probability (physics.data-an)Mathematics
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Nuclear Charge Radius ofBe12

2012

The nuclear charge radius of $^{12}\mathrm{Be}$ was precisely determined using the technique of collinear laser spectroscopy on the $2{s}_{1/2}\ensuremath{\rightarrow}2{p}_{1/2,3/2}$ transition in the ${\mathrm{Be}}^{+}$ ion. The mean square charge radius increases from $^{10}\mathrm{Be}$ to $^{12}\mathrm{Be}$ by $\ensuremath{\delta}⟨{r}_{c}^{2}{⟩}^{10,12}=0.69(5)\text{ }\text{ }{\mathrm{fm}}^{2}$ compared to $\ensuremath{\delta}⟨{r}_{c}^{2}{⟩}^{10,11}=0.49(5)\text{ }\text{ }{\mathrm{fm}}^{2}$ for the one-neutron halo isotope $^{11}\mathrm{Be}$. Calculations in the fermionic molecular dynamics approach show a strong sensitivity of the charge radius to the structure of $^{12}\mathrm{Be}$. Th…

Physics010308 nuclear & particles physicsGeneral Physics and AstronomyCharge densityRadius7. Clean energy01 natural sciencesEffective nuclear charge3. Good healthIonAtomic radiusCharge radius0103 physical sciencesSensitivity (control systems)Atomic physics010306 general physicsSpectroscopyPhysical Review Letters
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