0000000000055567

AUTHOR

Agnese Giaz

showing 17 related works from this author

Nanoseconds Timing System Based on IEEE 1588 FPGA Implementation

2019

Clock synchronization procedures are mandatory in most physical experiments where event fragments are readout by spatially dislocated sensors and must be glued together to reconstruct key parameters (e.g. energy, interaction vertex etc.) of the process under investigation. These distributed data readout topologies rely on an accurate time information available at the frontend, where raw data are acquired and tagged with a precise timestamp prior to data buffering and central data collecting. This makes the network complexity and latency, between frontend and backend electronics, negligible within upper bounds imposed by the frontend data buffer capability. The proposed research work describ…

EthernetFOS: Computer and information sciencesNuclear and High Energy PhysicsEye diagram; field-programmable gate arrays (FPGAs); front-end electronics; hardware; synchronization; timing systemfront-end electronicEye diagramtiming systemSerial communicationData bufferNetwork topology01 natural sciencesClock synchronizationNOComputer Science - Networking and Internet ArchitecturePE2_20103 physical sciencesSynchronization (computer science)hardwareElectrical and Electronic EngineeringNetworking and Internet Architecture (cs.NI)010308 nuclear & particles physicsbusiness.industrySettore FIS/01 - Fisica Sperimentalefront-end electronicsNuclear Energy and Engineeringfield-programmable gate arrays (FPGAs)Precision Time ProtocolbusinesssynchronizationComputer hardwareData link layer
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Response of AGATA segmented HPGe detectors to gamma rays up to 15.1MeV

2013

WOS: 000314826000009

AGATA; Gamma-ray spectroscopy; Gamma-ray tracking; HPGe detectors; Pulse-shape and gamma-ray tracking algorithms; Semiconductor detector performance and simulationsNuclear and High Energy PhysicsPulse-shape and gamma-ray tracking algorithmsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSemiconductor detector performance and simulationsTracking (particle physics)01 natural sciencesNuclear physicsGamma-ray tracking0103 physical sciencesGamma spectroscopyddc:530Gamma-ray spectroscopyNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentInstrumentationNuclear ExperimentDetectors de radiacióPhysicsSpectrometer010308 nuclear & particles physicsDetectorHPGe detectorsGamma ray81V35Semiconductor detectorAGATAFísica nuclearHpge detectorAGATA
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Isomers and high-spin structures in the N=81 isotones Xe135 and Ba137

2017

The high-spin structures of the N = 81 isotones 135Xe and 137Ba are investigated after multinucleontransfer (MNT) and fusion-evaporation reactions. Both nuclei are populated in (i) 136Xe+238U and (ii) 136Xe+208Pb MNT reactions employing the high-resolution Advanced Gamma Tracking Array (AGATA) coupled to the magnetic spectrometer PRISMA, (iii), in the 136Xe+198Pt MNT reaction employing the -ray array GAMMASPHERE in combination with the gas detector array Chico, and (iv) via a 11B+130Te fusion-evaporation reaction. The high-spin level schemes of 135Xe and 137Ba are considerably extended to higher energies. The 2058-keV (19=2 ) state in 135Xe is identified as an isomer, completing the systema…

PhysicsSpectrometer010308 nuclear & particles physics0103 physical sciencesQuadrupoleSHELL modelGammasphereAGATAAtomic physics010306 general physicsSpin (physics)01 natural sciencesPhysical Review C
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Calibration strategy of the JUNO experiment

2021

We present the calibration strategy for the 20 kton liquid scintillator central detector of the Jiangmen Underground Neutrino Observatory (JUNO). By utilizing a comprehensive multiple-source and multiple-positional calibration program, in combination with a novel dual calorimetry technique exploiting two independent photosensors and readout systems, we demonstrate that the JUNO central detector can achieve a better than 1% energy linearity and a 3% effective energy resolution, required by the neutrino mass ordering determination. [Figure not available: see fulltext.]

Nuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorsmeasurement methodsscintillation counter: liquidenergy resolutionFOS: Physical sciencesPhotodetectorScintillator53001 natural sciencesNOHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)hal-03022811PE2_2Optics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Calibrationlcsh:Nuclear and particle physics. Atomic energy. Radioactivityddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsAstrophysiqueJiangmen Underground Neutrino ObservatoryPhysicsJUNOliquid [scintillation counter]010308 nuclear & particles physicsbusiness.industrySettore FIS/01 - Fisica SperimentaleDetectorAstrophysics::Instrumentation and Methods for AstrophysicsLinearityInstrumentation and Detectors (physics.ins-det)calibrationNeutrino Detectors and Telescopes (experiments)lcsh:QC770-798High Energy Physics::ExperimentNeutrinobusinessEnergy (signal processing)Journal of High Energy Physics
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Conceptual design and infrastructure for the installation of the first AGATA sub-array at LNL

2011

WOS: 000295765100014

Nuclear and High Energy PhysicsDANTE Heavy-ion DetectorPhysics::Instrumentation and DetectorsHELENA multiplicity filter01 natural sciences7. Clean energyParticle detectorNuclear physicsPRISMA spectrometerConceptual design0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Nuclear Experiment010306 general physicsGamma detectionInstrumentationTRACE SI detectorPhysicsSpectrometer010308 nuclear & particles physicsbusiness.industrySemiconductor detectorCologne plungerAGATAAGATADANTE heavy-ion-detectorbusinessComputer hardwareNuclear Instruments and Methods in Physics Research
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Charge reconstruction in large-area photomultipliers

2018

Large-area PhotoMultiplier Tubes (PMT) allow to efficiently instrument Liquid Scintillator (LS) neutrino detectors, where large target masses are pivotal to compensate for neutrinos' extremely elusive nature. Depending on the detector light yield, several scintillation photons stemming from the same neutrino interaction are likely to hit a single PMT in a few tens/hundreds of nanoseconds, resulting in several photoelectrons (PEs) to pile-up at the PMT anode. In such scenario, the signal generated by each PE is entangled to the others, and an accurate PMT charge reconstruction becomes challenging. This manuscript describes an experimental method able to address the PMT charge reconstruction …

PhotomultiplierLiquid detectorsvisible and IR photons (vacuum) (photomultipliers HPDs others)Physics - Instrumentation and Detectorsgas and liquid scintillators)Physics::Instrumentation and DetectorsPhoton detectors for UV visible and IR photons (vacuum) (photomultipliers HPDs others)FOS: Physical sciencesvisible and IR photons (vacuum) (photomultipliers HPDsScintillatorvisible and IR photons (vacuum) (photomultipliers01 natural sciencesParticle detectorNOsymbols.namesakeOptics0103 physical sciencesCalorimeter methods010306 general physicsInstrumentationPhoton detectors for UVMathematical PhysicsPhysicsscintillation and light emission processes (solid gas and liquid scintillators)010308 nuclear & particles physicsbusiness.industrySettore FIS/01 - Fisica SperimentaleWiener filterDetectorReconstruction algorithmScintillators scintillation and light emission processes (solid gas and liquid scintillators)Instrumentation and Detectors (physics.ins-det)Scintillatorscintillation and light emission processes (solidCalorimeter methods; Liquid detectors; Photon detectors for UV visible and IR photons (vacuum) (photomultipliers HPDs others); Scintillators scintillation and light emission processes (solid gas and liquid scintillators)Photon detectors for UV visible and IR photons (vacuum) (photomultipliers HPDs others)Neutrino detectorHPDsCalorimeter methodScintillatorsScintillators scintillation and light emission processes (solid gas and liquid scintillators)symbolsLiquid detectorCalorimeter methods; Liquid detectors; Photon detectors for UV visible and IR photons (vacuum) (photomultipliers HPDs others); Scintillators scintillation and light emission processes (solid gas and liquid scintillators)Deconvolutionbusinessothers)scintillation and light emission processes (solid gas and liquid scintillators)
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Radioactivity control strategy for the JUNO detector

2021

JUNO is a massive liquid scintillator detector with a primary scientific goal of determining the neutrino mass ordering by studying the oscillated anti-neutrino flux coming from two nuclear power plants at 53 km distance. The expected signal anti-neutrino interaction rate is only 60 counts per day, therefore a careful control of the background sources due to radioactivity is critical. In particular, natural radioactivity present in all materials and in the environment represents a serious issue that could impair the sensitivity of the experiment if appropriate countermeasures were not foreseen. In this paper we discuss the background reduction strategies undertaken by the JUNO collaboration…

Nuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsNuclear engineeringMonte Carlo methodControl (management)measurement methodsFOS: Physical sciencesQC770-798Scintillator7. Clean energy01 natural sciencesNOPE2_2Nuclear and particle physics. Atomic energy. Radioactivity0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530Sensitivity (control systems)010306 general physicsPhysicsJUNOliquid [scintillation counter]010308 nuclear & particles physicsbusiness.industryDetectorSettore FIS/01 - Fisica Sperimentaleradioactivity [background]suppression [background]Instrumentation and Detectors (physics.ins-det)Monte Carlo [numerical calculations]Nuclear powerthreshold [energy]sensitivityNeutrino Detectors and Telescopes (experiments)GEANTNeutrinobusinessEnergy (signal processing)
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High-spin structures in Xe132 and Xe133 and evidence for isomers along the N=79 isotones

2017

Author(s): Vogt, A; Siciliano, M; Birkenbach, B; Reiter, P; Hadynska-Klȩk, K; Wheldon, C; Valiente-Dobon, JJ; Teruya, E; Yoshinaga, N; Arnswald, K; Bazzacco, D; Blazhev, A; Bracco, A; Bruyneel, B; Chakrawarthy, RS; Chapman, R; Cline, D; Corradi, L; Crespi, FCL; Cromaz, M; De Angelis, G; Eberth, J; Fallon, P; Farnea, E; Fioretto, E; Fransen, C; Freeman, SJ; Fu, B; Gadea, A; Gelletly, W; Giaz, A; Gorgen, A; Gottardo, A; Hayes, AB; Hess, H; Hetzenegger, R; Hirsch, R; Hua, H; John, PR; Jolie, J; Jungclaus, A; Karayonchev, V; Kaya, L; Korten, W; Lee, IY; Leoni, S; Liang, X; Lunardi, S; MacChiavelli, AO; Menegazzo, R; Mengoni, D; Michelagnoli, C; Mijatovic, T; Montagnoli, G; Montanari, D; Muller-…

PhysicsCrystallography010308 nuclear & particles physics0103 physical sciencesGammasphereAGATAAtomic physics010306 general physicsSpin (physics)01 natural sciencesPhysical Review C
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GIGJ: a crustal gravity model of the Guangdong Province for predicting the geoneutrino signal at the JUNO experiment

2019

Gravimetric methods are expected to play a decisive role in geophysical modeling of the regional crustal structure applied to geoneutrino studies. GIGJ (GOCE Inversion for Geoneutrinos at JUNO) is a 3D numerical model constituted by ~46 x 10$^{3}$ voxels of 50 x 50 x 0.1 km, built by inverting gravimetric data over the 6{\deg} x 4{\deg} area centered at the Jiangmen Underground Neutrino Observatory (JUNO) experiment, currently under construction in the Guangdong Province (China). The a-priori modeling is based on the adoption of deep seismic sounding profiles, receiver functions, teleseismic P-wave velocity models and Moho depth maps, according to their own accuracy and spatial resolution. …

010504 meteorology & atmospheric sciencesGeoneutrinogeophysical uncertaintieInverse transform samplingFOS: Physical sciences01 natural sciencesBayesian methodUpper middle and lower crustStandard deviationNOSouth China BlockmiddlePhysics - GeophysicsMonte Carlo stochastic optimizationGOCE data gravimetric inversionGeophysical uncertaintiesGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)Bayesian method; geophysical uncertainties; GOCE data gravimetric inversion; Monte Carlo stochastic optimization; South China Block; upper middle and lower crustImage resolution0105 earth and related environmental sciencesSubdivisionJiangmen Underground Neutrino Observatoryupper and middle and lower crustbusiness.industrySettore FIS/01 - Fisica SperimentaleCrustupperGeodesy[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]Geophysics (physics.geo-ph)and lower crustDepth soundingGeophysics13. Climate actionSpace and Planetary SciencebusinessGeologyBayesian method geophysical uncertainties GOCE data gravimetric inversion Monte Carlo stochastic optimization South China Blockupper and middle and lower crust
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Study of the γ decay of high-lying states in 208Pb via inelastic scattering of 17O ions

2014

A measurement of the high-lying states in 208Pb has been made using 17O beams at 20 MeV/u. The gamma decay following inelastic excitation was measured with the detector system AGATA Demonstrator based on segmented HPGe detectors, coupled to an array of large volume LaBr3:Ce scintillators and to an array of Si detectors. Preliminary results in comparison with (γ,γ’) data, for states in the 5-8 MeV energy interval, are presented.

PhysicsScatteringPhysics::Instrumentation and DetectorsPhysicsQC1-999Gamma rayInelastic scatteringParticle detectorSemiconductor detectorIonNuclear physicsPhysics and Astronomy (all)AGATAHigh Energy Physics::ExperimentNuclear ExperimentRadioactive decayEPJ Web of Conferences
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Relativistic Coulomb excitation of Kr 88

2016

International audience; To investigate the systematics of mixed-symmetry states in N=52 isotones, a relativistic Coulomb excitation experiment was performed during the PreSPEC campaign at the GSI Helmholtzzentrum für Schwerionenforschung to determine E2 transition strengths to 2+ states of the radioactive nucleus $^{88}$Kr. Absolute transition rates could be measured towards the first and third 2+ states. For the latter a mixed-symmetry character is suggested on the basis of the indication for a strong M1 transition to the fully symmetric 21+ state, extending the knowledge of the N=52 isotones below Z=40. A comparison with the proton-neutron interacting boson model and shell-model predictio…

PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsNuclear TheoryNuclear structureState (functional analysis)Coulomb excitation[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesNuclear physicsgamma-ray spectroscopySubatomic Physicsrelativistic Coulomb excitationnuclear structure0103 physical sciencesGamma spectroscopyAtomic physicsInteracting boson modelNuclear Experiment010306 general physics
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High-spin structure of Xe134

2016

A. Vogt et al. ; 12 págs.; 9 figs.; 1 tab.

PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsFissionNuclear structureAnalytical chemistryMolecularSpin structure[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Kinetic energy01 natural sciences7. Clean energyAtomicNuclear & Particles PhysicsSubatomär fysikParticle and Plasma Physics0103 physical sciencesSubatomic PhysicsHeavy ionGammasphereAGATANuclear010306 general physicsSpin (physics)Nuclear Experiment
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High-spin structure in the transitional nucleus Xe131 : Competitive neutron and proton alignment in the vicinity of the N=82 shell closure

2018

The transitional nucleus 131Xe is investigated after multinucleon transfer (MNT) in the 136Xe+208Pb and 136Xe+238U reactions employing the high-resolution Advanced GAmma Tracking Array (AGATA) coupled to the magnetic spectrometer PRISMA at the Laboratori Nazionali di Legnaro, Italy and as an elusive reaction product in the fusion-evaporation reaction 124Sn(11B,p3n) 131Xe employing the HORUS γ-ray array coupled to a double-sided silicon strip detector (DSSSD) at the University of Cologne, Germany. The level scheme of 131Xe is extended to 5 MeV. A pronounced backbending is observed at ~ω ≈ 0.4 MeV along the negative-parity one-quasiparticle νh11/2(α = −1/2) band. The results are compared to t…

PhysicsSpectrometerIsotopeProton010308 nuclear & particles physicsShell (structure)Nuclear structureSpin structure01 natural sciencesNuclear physics0103 physical sciencesNeutronAGATA010306 general physicsPhysical Review C
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AGATA-Advanced GAmma Tracking Array

2012

WOS: 000300864200005

Nuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsPulse-shape and gamma-ray tracking algorithmsFOS: Physical sciencesSemiconductor detector performance and simulationsIntegrated circuit[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Tracking (particle physics)gamma-Ray tracking01 natural sciencesPulse-shape and γ-ray tracking algorithmslaw.inventionData acquisitionlaw0103 physical sciencesddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Nuclear Experiment (nucl-ex)010306 general physicsγ-Ray spectroscopyNuclear ExperimentInstrumentationDigital signal processingEvent reconstructiongamma-Ray spectroscopyPhysicssezeleSpectrometerSpectrometers010308 nuclear & particles physicsbusiness.industryDetectorAGATA Digital signals HPGe detectors Pulse-shape Ray trackingHPGe detectorsAlgorithms Crystals Germanium Semiconductor detectors Signal processing Spectrometry Tracking (position)γ-Ray trackingInstrumentation and Detectors (physics.ins-det)Digital signal processingAGATAFísica nuclearbusinessAGATAComputer hardware
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Distillation and stripping pilot plants for the JUNO neutrino detector: Design, operations and reliability

2019

Abstract This paper describes the design, construction principles and operations of the distillation and stripping pilot plants tested at the Daya Bay Neutrino Laboratory, with the perspective to adapt these processes, system cleanliness and leak-tightness standards to the final full scale plants to be used for the purification of the liquid scintillator of the JUNO neutrino detector. The main goal of these plants is to remove radio impurities from the liquid scintillator while increasing its optical attenuation length. Purification of liquid scintillator will be performed with a system combining alumina oxide, distillation, water extraction and steam (or N 2 gas) stripping. Such a combined…

Large-scale experimentNuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsLiquid scintillatorAttenuation length; LAB; Large-scale experiments; Light yield; Liquid scintillator; Nitrogen purging; Radiopurity; Scintillator transparency; Nuclear and High Energy Physics; Instrumentationscintillation counter: liquidMixing (process engineering)Full scaleFOS: Physical sciencesRadiopurityfabricationScintillator01 natural sciences7. Clean energyStripping (fiber)law.inventionNOlaw0103 physical sciencesthorium: admixtureAttenuation length; LAB; Large-scale experiments; Light yield; Liquid scintillator; Nitrogen purging; Radiopurity; Scintillator transparency[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsProcess engineeringDistillationInstrumentationbackground: radioactivityNuclear and High Energy PhysicPhysicsLABJUNOLarge-scale experiments010308 nuclear & particles physicsbusiness.industryuranium: admixtureSettore FIS/01 - Fisica SperimentaleAttenuation lengthInstrumentation and Detectors (physics.ins-det)Attenuation lengthNitrogen purgingNeutrino detectorScintillator transparencyNeutrinobusinessaluminum: oxygenLight yield
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The Design and Sensitivity of JUNO's scintillator radiopurity pre-detector OSIRIS

2021

The European physical journal / C 81(11), 973 (2021). doi:10.1140/epjc/s10052-021-09544-4

Liquid scintillatorPhysics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and Detectorsscintillation counter: liquidmeasurement methodsQC770-798Astrophysics01 natural sciencesthorium: nuclidedesign [detector]neutrinoRadioactive purityPhysicsLow energy neutrinoJUNOliquid [scintillation counter]biologySettore FIS/01 - Fisica SperimentaleDetectorInstrumentation and Detectors (physics.ins-det)3. Good healthQB460-466Physics::Space Physicsnuclide [uranium]FOS: Physical sciencesScintillatornuclide [thorium]530NONuclear physicsPE2_2uranium: nuclideNuclear and particle physics. Atomic energy. Radioactivity0103 physical sciencesddc:530Sensitivity (control systems)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsJUNO neutrino physics liquid scintillatorEngineering (miscellaneous)background: radioactivitydetector: designMeasurement method010308 nuclear & particles physicsradioactivity [background]biology.organism_classificationsensitivityHigh Energy Physics::ExperimentReactor neutrinoOsiris
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JUNO sensitivity to low energy atmospheric neutrino spectra

2021

Atmospheric neutrinos are one of the most relevant natural neutrino sources that can be exploited to infer properties about cosmic rays and neutrino oscillations. The Jiangmen Underground Neutrino Observatory (JUNO) experiment, a 20 kton liquid scintillator detector with excellent energy resolution is currently under construction in China. JUNO will be able to detect several atmospheric neutrinos per day given the large volume. A study on the JUNO detection and reconstruction capabilities of atmospheric $\nu_e$ and $\nu_\mu$ fluxes is presented in this paper. In this study, a sample of atmospheric neutrino Monte Carlo events has been generated, starting from theoretical models, and then pro…

Physics and Astronomy (miscellaneous)Physics::Instrumentation and Detectorsscintillation counter: liquidenergy resolutionAtmospheric neutrinoQC770-798Astrophysics7. Clean energy01 natural sciencesneutrino: fluxHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)particle source [neutrino]neutrinoneutrino: atmosphere[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Cherenkovneutrino/e: particle identificationenergy: low [neutrino]Jiangmen Underground Neutrino ObservatoryPhysicsJUNOphotomultiplierliquid [scintillation counter]primary [neutrino]neutrino: energy spectrumDetectoroscillation [neutrino]neutrinosMonte Carlo [numerical calculations]atmosphere [neutrino]QB460-466observatorycosmic radiationComputer Science::Mathematical Softwareproposed experimentNeutrinonumerical calculations: Monte CarloComputer Science::Machine LearningParticle physicsdata analysis methodAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayScintillatorComputer Science::Digital LibrariesNOStatistics::Machine LearningPE2_2neutrino: primaryneutrino: spectrumNuclear and particle physics. Atomic energy. Radioactivity0103 physical sciencesddc:530structure010306 general physicsNeutrino oscillationEngineering (miscellaneous)Cherenkov radiationparticle identification [neutrino/mu]Scintillationneutrino/mu: particle identificationflavordetectorparticle identification [neutrino/e]010308 nuclear & particles physicsneutrino: energy: lowHigh Energy Physics::Phenomenologyspectrum [neutrino]resolutionenergy spectrum [neutrino]flux [neutrino]neutrino: particle source13. Climate actionHigh Energy Physics::Experimentneutrino: oscillationneutrino detector
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