0000000000055554

AUTHOR

Paolo Lombardi

showing 50 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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Solar neutrino physics with Borexino

2018

We present the most recent solar neutrino results from the Borexino experiment at the Gran Sasso underground laboratory. In particular, refined measurements of all neutrinos produced in the {\it pp} fusion chain have been made. It is the first time that the same detector measures the entire range of solar neutrinos at once. These new data weakly favor a high-metallicity Sun. Prospects for measuring CNO solar neutrinos are also discussed.

fusionPhysics - Instrumentation and Detectorsneutrino: solarPhysics::Instrumentation and DetectorsQC1-999Astrophysics::High Energy Astrophysical PhenomenaSolar neutrinoFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesNuclear physics0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Nuclear Experiment (nucl-ex)Nuclear Experiment010303 astronomy & astrophysicsBorexinoPhysicsp p: fusion010308 nuclear & particles physicsPhysicsHigh Energy Physics::PhenomenologyInstrumentation and Detectors (physics.ins-det)Gran Sasso* Automatic Keywords *Physics::Space PhysicsUnderground laboratoryBorexinoHigh Energy Physics::ExperimentAstrophysics::Earth and Planetary AstrophysicsNeutrinoexperimental resultsSciPost Physics Proceedings
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The next-generation liquid-scintillator neutrino observatory LENA

2012

We propose the liquid-scintillator detector LENA (Low Energy Neutrino Astronomy) as a next-generation neutrino observatory on the scale of 50 kt. The outstanding successes of the Borexino and KamLAND experiments demonstrate the large potential of liquid-scintillator detectors in low-energy neutrino physics. LENA's physics objectives comprise the observation of astrophysical and terrestrial neutrino sources as well as the investigation of neutrino oscillations. In the GeV energy range, the search for proton decay and long-baseline neutrino oscillation experiments complement the low-energy program. Based on the considerable expertise present in European and international research groups, the …

Neutrino detectors; Liquid-scintillator detectors; Low-energy neutrinos; Proton decay; Longbaseline neutrino beamsParticle physicsPhysics - Instrumentation and Detectors[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaLongbaseline neutrino beamsFOS: Physical sciencesLow-energy neutrinos7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentNONuclear physicsLiquid-scintillator detectorsHigh Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Neutrino detectorsNeutrino oscillationInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsBorexinoPhysics010308 nuclear & particles physicsFísicaAstronomy and AstrophysicsInstrumentation and Detectors (physics.ins-det)Proton decaySolar neutrino problem[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Neutrino detectorddc:540Measurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyAstrophysics - Instrumentation and Methods for Astrophysics
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Effects of berberine, curcumin, resveratrol alone and in combination with chemotherapeutic drugs and signal transduction inhibitors on cancer cells-P…

2017

Over the past fifty years, society has become aware of the importance of a healthy diet in terms of human fitness and longevity. More recently, the concept of the beneficial effects of certain components of our diet and other compounds, that are consumed often by different cultures in various parts of the world, has become apparent. These “healthy” components of our diet are often referred to as nutraceuticals and they can prevent/suppress: aging, bacterial, fungal and viral infections, diabetes, inflammation, metabolic disorders and cardiovascular diseases and have other health-enhancing effects. Moreover, they are now often being investigated because of their anti-cancer properties/po…

0301 basic medicineCancer ResearchCurcuminBerberinemedia_common.quotation_subjectInflammationAntineoplastic AgentsPharmacologyResveratrol03 medical and health scienceschemistry.chemical_compoundNutraceuticalBerberineGeneticNeoplasmsGeneticsMedicineAnimalsHumansMolecular Biologymedia_commonbusiness.industryLongevityMetforminMetformin030104 developmental biologychemistryCardiovascular DiseasesResveratrolCancer cellDietary SupplementsCurcuminMolecular Medicinemedicine.symptombusinessBerberine; Curcumin; Metformin; Resveratrolmedicine.drugSignal TransductionAdvances in biological regulation
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Recent Borexino results and perspectives of the SOX measurement

2017

International audience; Borexino is a liquid scintillator detector sited underground in the Laboratori Nazionali del Gran Sasso (Italy). Its physics program, until the end of this year, is focussed on the study of solar neutrinos, in particular from the Beryllium, pp, pep and CNO fusion reactions. Knowing the reaction chains in the sun provides insights towards physics disciplines such as astrophysics (star physics, star formation, etc.), astroparticle and particle physics. Phase II started in 2011 and its aim is to improve the phase I results, in particular the measurements of the neutrino fluxes from the pep and CNO processes. By the end of this year, data taking from the sun will be over…

Sterile neutrinoneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoQC1-999scintillation counter: liquidanomaly[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energy01 natural sciencesStandard ModelNuclear physics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear fusion010306 general physicsNeutrino oscillationBorexinoPhysicsgallium010308 nuclear & particles physicsStar formationPhysicsstar: formationstabilityneutrino: sterilesensitivityberylliumGran SassoLSNDelectron: lifetimeHigh Energy Physics::ExperimentBorexinoneutrino: oscillationnuclear reactorNeutrinoneutrino: geophysicstalk: Kolymbari 2017/08/17experimental results
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The measurement of the pp chain solar neutrinos in Borexino

2019

Proton–proton chain reactionPhysicsParticle physicsSolar neutrinoBorexino
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SOX: search for short baseline neutrino oscillations with Borexino

2015

International audience; The Borexino detector has convincingly shown its outstanding performances in the low energy regime through its accomplishments in the observation and study of the solar and geo neutrinos. It is then an ideal tool to perform a state of the art source-based experiment for testing the longstanding hypothesis of a fourth sterile neutrino with ~ eV(2) mass, as suggested by several anomalies accumulated over the past three decades in source, reactor, and accelerator-based experiments. The SOX project aims at successively deploying two intense radioactive sources, made of Cerium (antineutrino) and Chromium (neutrino), respectively, in a dedicated pit located beneath the det…

HistoryParticle physicsSterile neutrinochromium: nuclidePhysics::Instrumentation and DetectorsSolar neutrino[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energyEducationNuclear physicsPhysics and Astronomy (all)0103 physical sciencesddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationBorexinoactivity reportPhysics010308 nuclear & particles physicsHigh Energy Physics::Phenomenologyneutrino: particle sourceSolar neutrino problemneutrino: sterilesensitivityComputer Science ApplicationsNeutrino detector13. Climate actioncerium: nuclideMeasurements of neutrino speedHigh Energy Physics::ExperimentBorexinoneutrino: oscillationNeutrinoantineutrino: particle source
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Short distance neutrino oscillations with Borexino

2014

International audience; The Borexino detector has convincingly shown its outstanding performances in the low energy, sub-MeV regime through its unprecedented accomplishments in the solar and geo-neutrinos detection. These performances make it the ideal tool to accomplish a state-of-the-art experiment able to test unambiguously the long-standing issue of the existence of a sterile neutrino, as suggested by the several anomalous results accumulated over the past two decades, i.e. the outputs of the LSND and Miniboone experiments, the results of the source calibration of the two Gallium solar neutrino experiments, and the recently hinted reactor anomaly. The SOX project will exploit two source…

Particle physicsSterile neutrinoneutrino: solarPhysics::Instrumentation and DetectorsQC1-999Solar neutrinoscintillation counter: liquidanomalyneutrino: beam7. Clean energy01 natural sciencesNuclear physicsMiniBooNEPhysics and Astronomy (all)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsNeutrino oscillationBorexinoenergy: lowPhysicsgallium010308 nuclear & particles physicsantineutrino: beamPhysicsDetectorHigh Energy Physics::Phenomenologytalk: Noto 2014/09/30neutrino: sterilecalibrationneutrino: nuclear reactorceriumLSNDradioactivityHigh Energy Physics::ExperimentBorexinoneutrino: familychromiumneutrino: oscillationNeutrinoAnomaly (physics)performanceexperimental results
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First real–time detection of solar pp neutrinos by Borexino

2014

International audience; Solar neutrinos have been pivotal to the discovery of neutrino flavour oscillations and are a unique tool to probe the reactions that keep the Sun shine. Although most of solar neutrino components have been directly measured, the neutrinos emitted by the keystone pp reaction, in which two protons fuse to make a deuteron, have so far eluded direct detection. The Borexino experiment, an ultra-pure liquid scintillator detector running at the Laboratori Nazionali del Gran Sasso in Italy, has now filled the gap, providing the first direct real time measurement of pp neutrinos and of the solar neutrino luminosity.

deuteronParticle physicsneutrino: solarPhysics::Instrumentation and DetectorsQC1-999Solar neutrinoAstrophysics::High Energy Astrophysical Phenomenascintillation counter: liquidgap7. Clean energy01 natural sciencesNuclear physicsPhysics and Astronomy (all)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530flavor: oscillation010306 general physicsNuclear ExperimentBorexinoPhysicsICARUSp p: fusion010308 nuclear & particles physicsPhysicsHigh Energy Physics::Phenomenologytalk: Noto 2014/09/30Solar neutrino problemGran SassoNeutrino detectorneutrino: flavorMeasurements of neutrino speedCOUNTING TEST FACILITYHigh Energy Physics::Experimentdirect detectionBorexinoneutrino: oscillationNeutrino astronomyNeutrinoexperimental resultsneutrino: luminosity
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A test of electric charge conservation with Borexino

2015

Borexino is a liquid scintillation detector located deep underground at the Laboratori Nazionali del Gran Sasso (LNGS, Italy). Thanks to the unmatched radio-purity of the scintillator, and to the well understood detector response at low energy, a new limit on the stability of the electron for decay into a neutrino and a single mono-energetic photon was obtained. This new bound, tau > 6.6 10**28 yr at 90 % C.L., is two orders of magnitude better than the previous limit.

Particle physicsPhysics - Instrumentation and DetectorsOrders of magnitude (temperature)Physics::Instrumentation and DetectorsGeneral Physics and AstronomyFOS: Physical sciencesElectronScintillatorElectric chargeHigh Energy Physics - ExperimentNuclear physicsPhysics and Astronomy (all)High Energy Physics - Experiment (hep-ex)ddc:550Nuclear ExperimentBorexinoComputingMilieux_MISCELLANEOUSPhysics[PHYS]Physics [physics]Liquid scintillation countingDetectorAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)High Energy Physics::ExperimentNeutrino[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Neutrinos from the primary proton–proton fusion process in the Sun

2014

International audience; In the core of the Sun, energy is released through sequences of nuclear reactions that convert hydrogen into helium. The primary reaction is thought to be the fusion of two protons with the emission of a low-energy neutrino. These so-called pp neutrinos constitute nearly the entirety of the solar neutrino flux, vastly outnumbering those emitted in the reactions that follow. Although solar neutrinos from secondary processes have been observed, proving the nuclear origin of the Sun's energy and contributing to the discovery of neutrino oscillations, those from proton-proton fusion have hitherto eluded direct detection. Here we report spectral observations of pp neutrin…

PhysicsParticle physicsMultidisciplinaryProtonSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaNuclear TheorySolar neutrino problemNuclear physicsNeutrino detectorPhysics::Space PhysicsAstrophysics::Solar and Stellar AstrophysicsMeasurements of neutrino speedAstrophysics::Earth and Planetary AstrophysicsNeutrino astronomyNeutrino[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Nuclear ExperimentBorexino
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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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Search for low-energy neutrinos from astrophysical sources with Borexino

2019

We report on searches for neutrinos and antineutrinos from astrophysical sources performed with the Borexino detector at the Laboratori Nazionali del Gran Sasso in Italy. Electron antineutrinos ($\bar{\nu}_e$) are detected in an organic liquid scintillator through the inverse $\beta$-decay reaction. In the present work we set model-independent upper limits in the energy range 1.8-16.8 MeV on neutrino fluxes from unknown sources that improve our previous results, on average, by a factor 2.5. Using the same data set, we first obtain experimental constraints on the diffuse supernova $\bar{\nu}_e$ fluxes in the previously unexplored region below 8 MeV. A search for $\bar{\nu}_e$ in the solar ne…

antineutrinosPhysics - Instrumentation and Detectorssolar flaresmagnetic field: highneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoscintillation counter: liquidelastic scatteringantineutrino/e: particle identification01 natural sciences7. Clean energyneutrino: fluxlaw.inventionHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)law[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]neutrino: supernova26.65.+t010303 astronomy & astrophysicsBorexinoElastic scatteringPhysicsSolar flareSupernova Relic Neutrinosneutrino: energy spectrumS067EB8neutrinosInstrumentation and Detectors (physics.ins-det)neutrino: magnetic momentDiffuse Supernova Neutrino Background3. Good healthSupernovaHomestakeddc:540neutrino: flavorAntineutrinoBorexinoNeutrino97.60.BwHomestake experimentFlareantineutrino/e: fluxAntineutrinos13.15.+G; 26.65.+T; 29.40.Mc; 97.60.Bw; Antineutrinos; Diffuse supernova neutrino background; Neutrinos; Solar flares; Supernova relic neutrinosAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSupernova relic neutrinosupernova relic neutrinosNONuclear physics13.15.+gPE2_2Antineutrinos; Neutrinos; Diffuse supernova neutrino background; Supernova relic neutrinos; Solar flares0103 physical sciencesNeutrino[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Neutrinosdiffuse supernova neutrino background010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomy and Astrophysicsneutrino: particle source29.40.McGran SassoSolar flareSolar Flares13. Climate actionspectralHigh Energy Physics::Experimentexperimental results
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The $^{144}$Ce source for SOX

2015

International audience; The SOX (Short distance neutrino Oscillations with BoreXino) project aims at testing the light sterile neutrino hypothesis. To do so, two artificials sources of antineutrinos and neutrinos respectively will be consecutively deployed at the Laboratori Nazionali del Gran Sasso (LNGS) in close vicinity to Borexino, a large liquid scintillator detector. This document reports on the source production and transportation. The source should exhibit a long lifetime and a high decay energy, a requirement fullfilled by the (144)Ce-(144)Pr pair at secular equilibrium. It will be produced at FSUE “Mayak” PA using spent nuclear fuel. It will then be shielded and packed according t…

HistorySterile neutrinoParticle physicsenergy: decay[PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph]Scintillator01 natural sciences7. Clean energyEducationNuclear physicsPhysics and Astronomy (all)0103 physical sciencesddc:530010306 general physicsNeutrino oscillationparticle sourceBorexinoPhysicslifetimenucleusSecular equilibriumneutrino: sterileantineutrinosensitivitySpent nuclear fuelComputer Science ApplicationsGran SassoceriumDecay energyradioactivityBorexinoneutrino: oscillationproductionNeutrino
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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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Seasonal Modulation of the $^7$Be Solar Neutrino Rate in Borexino

2017

We detected the seasonal modulation of the $^7$Be neutrino interaction rate with the Borexino detector at the Laboratori Nazionali del Gran Sasso in Italy. The period, amplitude, and phase of the observed time evolution of the signal are consistent with its solar origin, and the absence of an annual modulation is rejected at 99.99\% C.L. The data are analyzed using three methods: the sinusoidal fit, the Lomb-Scargle and the Empirical Mode Decomposition techniques, which all yield results in excellent agreement.

liquid scintillators detectorsPhysics - Instrumentation and Detectorsexperimental methodsneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinolow background detectorsSolar neutrinos01 natural sciencesflux: time dependenceneutrino: fluxHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Liquid scintillators detectors; Low background detectors; Neutrino oscillations; Solar neutrinos; Astronomy and Astrophysics[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Borexinoneutrino: interactionMSW effectPhysicsNeutrino oscillationsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)neutrino electron: elastic scatteringmodulationAmplitudeModulationsolar neutrinosBorexinoNeutrinoLiquid scintillators detectorFLUXLow background detectordata analysis methodNeutrino oscillationFOS: Physical sciencesSolar neutrinoNuclear physicsTIME-SERIES ANALYSIS[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]Low background detectorsLiquid scintillators detectorsSEARCH0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]SPACED DATA010306 general physicsNeutrino oscillationbackground: radioactivityneutrino oscillations010308 nuclear & particles physicsAstronomy and AstrophysicsEMPIRICAL MODE DECOMPOSITIONberylliumGran SassoHigh Energy Physics::Experimentneutrino: oscillationEvent (particle physics)experimental results
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CNO and pep solar neutrino measurements and perspectives in Borexino

2015

International audience; The detection of neutrinos emitted in the CNO reactions in the Sun is one of the ambitious goals of Borexino Phase-II. A measurement of CNO neutrinos would be a milestone in astrophysics, and would allow to solve serious issues in current solar models. A precise measurement of the rate of neutrinos from the pep reaction would allow to investigate neutrino oscillations in the MSW transition region. The pep and CNO solar neutrino physics, the measurement in Borexino Phase-I and the perspectives for the new phase are reviewed in this proceeding.

model: solarHistoryneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical Phenomena7. Clean energy01 natural sciencesEducationNuclear physicsPhysics and Astronomy (all)talk: Moscow 2015/10/050103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Astrophysics::Solar and Stellar Astrophysicsddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationBorexinoMSW effectPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologySolar neutrino problemComputer Science ApplicationsMassless particleNeutrino detector13. Climate actionHigh Energy Physics::ExperimentBorexinoneutrino: oscillationNeutrinoLeptonexperimental results
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Perspectives for CNO neutrino detection in Borexino

2018

International audience; Borexino measured with unprecedented accuracy the fluxes of solar neutrinos emitted at all the steps of the pp fusion chain. Still missing is the measurement of the flux of neutrinos produced in the CNO cycle. A positive measurement of the CNO neutrino flux is of fundamental importance for understanding the evolution of stars and addressing the unresolved controversy on the solar abundances. The measurement of the CNO neutrino flux in Borexino is challenging because of the low intensity of this component (CNO cycle accounts for about 1% of the energy emitted by Sun), the lack of prominent spectral features and the presence of background sources. The main background c…

CNO cycleexperimental methodsneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical Phenomenascintillation counter: liquidSolar neutrinosbismuth: admixtureAstrophysics[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energySolar neutrinoCNO-cycleneutrino: fluxAstrophysics::Solar and Stellar Astrophysics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Stellar evolutionBorexinoliquid scintillatorAstrophysics::Galaxy AstrophysicsPhysicsEnergy distributiondetectorbackgroundbismuth: nuclideCNO cycleNeutrino detector13. Climate actionBorexinoExperimental methodsNeutrino
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Overview and accomplishments of the Borexino experiment

2015

International audience; The Borexino experiment is running at the Laboratori del Gran Sasso in Italy since 2007. Its technical distinctive feature is the unprecedented ultralow background of the inner scintillating core, which is the basis of the outstanding achievements accumulated by the experiment. In this talk, after recalling the main features of the detector, the impressive solar data gathered so far by the experiment will be summarized, with special emphasis to the most recent and prominent result concerning the detection of the fundamental pp solar neutrino flux, which is the direct probe of the engine mechanism powering our star. Such a milestone measurement puts Borexino in the un…

Historyneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoreview[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energy01 natural sciencesneutrino: fluxEducationNuclear physicsPhysics and Astronomy (all)energy: solarstar0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicsddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsBorexinoPhysicsSolar energetic particlesbusiness.industrybackgroundAstronomyoscillationSolar energyComputer Science ApplicationsGran SassoMassless particleNEUTRINOSNeutrino detectorPhysics::Space PhysicsBorexinoNeutrinobusinessLepton
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Introduction of WT-TP53 into pancreatic cancer cells alters sensitivity to chemotherapeutic drugs, targeted therapeutics and nutraceuticals

2018

Abstract Pancreatic ductal adenocarcinoma (PDAC) is an aggressive, highly metastatic malignancy and accounts for 85% of pancreatic cancers. PDAC patients have poor prognosis with a five-year survival of only 5–10%. Mutations at the TP53 gene are readily detected in pancreatic tumors isolated from PDAC patients. We have investigated the effects of restoration of wild-type (WT) TP53 activity on the sensitivity of pancreatic cancer cells to: chemotherapy, targeted therapy, as well as, nutraceuticals. Upon introduction of the WT-TP53 gene into the MIA-PaCa-2 pancreatic cancer cell line, the sensitivity to drugs used to treat pancreatic cancer cells such as: gemcitabine, fluorouracil (5FU), cisp…

0301 basic medicineCancer ResearchPaclitaxelendocrine system diseasesmedicine.medical_treatmentTargeted therapeuticIrinotecanDeoxycytidineTargeted therapyGlycogen Synthase Kinase 303 medical and health scienceschemistry.chemical_compound0302 clinical medicineCell Line TumorPancreatic cancerGeneticsmedicineHumansDoxorubicinTP53Signal transduction inhibitorneoplasmsMolecular BiologyCell ProliferationCisplatinChemotherapybusiness.industryPancreatic Neoplasmmedicine.diseaseGemcitabinedigestive system diseasesGemcitabinePancreatic NeoplasmsOxaliplatin030104 developmental biologyPaclitaxelchemistryFluorouracil030220 oncology & carcinogenesisCancer researchMolecular MedicineFluorouracilCisplatinbusinessDrug sensitivityHumanSignal Transductionmedicine.drug
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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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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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CeSOX: An experimental test of the sterile neutrino hypothesis with Borexino

2017

International audience; The third phase of the Borexino experiment that’s referred to as SOX is devoted to test the hypothesis of the existence of one (or more) sterile neutrinos at a short baseline (~5–10m). The experimental measurement will be made with artificial sources namely with a 144Ce–144Pr antineutrino source at the first stage (CeSOX) and possibly with a 51Cr neutrino source at the second one. The fixed 144Ce–144Pr sample will be placed beneath the detector in a special pit and the initial activity will be about 100 – 150 kCi. The start of data taking is scheduled for April 2018. The article gives a short description of the preparation for the first stage and shows the expected s…

Physicsneutrino: sterile: search forHistorySterile neutrinoParticle physics010308 nuclear & particles physicsInitial activitysensitivity01 natural sciencesComputer Science ApplicationsEducationPHYSICSPhysics and Astronomy (all)cesium0103 physical sciencesOSCILLATIONS[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530Borexinoproposed experimentNeutrino010306 general physicsantineutrino: particle sourceBorexinotalk: Moscow 2017/10/02
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Effects of the MDM-2 inhibitor Nutlin-3a on PDAC cells containing and lacking WT-TP53 on sensitivity to chemotherapy, signal transduction inhibitors …

2019

Abstract Mutations at the TP53 gene are readily detected (approximately 50–75%) in pancreatic ductal adenocarcinoma (PDAC) patients. TP53 was previously thought to be a difficult target as it is often mutated, deleted or inactivated on both chromosomes in certain cancers. In the following study, the effects of restoration of wild-type (WT) TP53 activity on the sensitivities of MIA-PaCa-2 pancreatic cancer cells to the MDM2 inhibitor nutlin-3a in combination with chemotherapy, targeted therapy, as well as, nutraceuticals were examined. Upon introduction of the WT-TP53 gene into MIA-PaCa-2 cells, which contain a TP53 gain of function (GOF) mutation, the sensitivity to the MDM2 inhibitor incre…

0301 basic medicineCancer ResearchNutlin-3aSettore MED/09 - Medicina Internaendocrine system diseasesmedicine.medical_treatmentmedicine.disease_causePiperazinesTargeted therapy0302 clinical medicineTP53MutationbiologyChemistryImidazolesProto-Oncogene Proteins c-mdm2OxaliplatinTargeted TherapeuticsDrug sensitivity; Nutlin-3a; Nutraceuticals; Targeted therapeutics; TP53030220 oncology & carcinogenesisMolecular MedicineMdm2NutraceuticalNutraceuticalsSignal transductionCarcinoma Pancreatic DuctalSignal Transductionmedicine.drugDrug sensitivityAntineoplastic AgentsIrinotecan03 medical and health sciencesCell Line TumorPancreatic cancerGeneticsmedicineHumansMolecular BiologyneoplasmsChemotherapymedicine.diseasedigestive system diseasesOxaliplatinPancreatic Neoplasms030104 developmental biologyCell cultureDietary Supplementsbiology.proteinCancer researchTERAPÊUTICA MÉDICATumor Suppressor Protein p53
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Recent results from Borexino and the first real time measure of solar pp neutrinos

2014

International audience; The Borexino detector was built starting from 1996 in the underground hall C of Gran Sasso National Laboratory (LNGS) in Italy under about 1400 m of rock (3800 m.w.e) and it is mostly aimed to the study in real-time of the low-energy solar neutrinos.Since the beginning of data taking, in May 2007, the unprecedented detector radio-purity made the performances of the detector unique: a milestone has been very recently achieved with the measurement of solar pp neutrino flux, providing the first direct observation in real time of the key fusion reaction powering the Sun.In this contribution the most important Borexino achievements to the fields of solar, geo-neutrino and…

geo-neutrinosNuclear and High Energy PhysicsParticle physicsNeutrino oscillationneutrino: solarPhysics::Instrumentation and DetectorsGeo-neutrinos; Neutrino oscillations; Solar neutrinos; Nuclear and High Energy PhysicsSolar neutrinotalk: Valencia 2014/07/02Solar neutrinosSolar neutrino01 natural sciences7. Clean energyPhysics::Geophysics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530010306 general physicsNeutrino oscillationBorexinoPhysicsneutrino oscillations010308 nuclear & particles physicsNeutrino oscillationsSolar neutrino problemGran SassoNeutrino detectorGeo-neutrinosolar neutrinosMeasurements of neutrino speedBorexinoHigh Energy Physics::Experimentneutrino: oscillationneutrino: geophysicsNeutrino astronomyNeutrinoexperimental resultsGeo-neutrinosNuclear and Particle Physics Proceedings
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Recent Borexino results and prospects for the near future

2015

The Borexino experiment, located in the Gran Sasso National Laboratory, is an organic liquid scintillator detector conceived for the real time spectroscopy of low energy solar neutrinos. The data taking campaign phase I (2007 - 2010) has allowed the first independent measurements of 7Be, 8B and pep fluxes as well as the first measurement of anti-neutrinos from the earth. After a purification of the scintillator, Borexino is now in phase II since 2011. We review here the recent results achieved during 2013, concerning the seasonal modulation in the 7Be signal, the study of cosmogenic backgrounds and the updated measurement of geo-neutrinos. We also review the upcoming measurements from phase…

Sterile neutrinoPhysics - Instrumentation and Detectorsneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoQC1-999Astrophysics::High Energy Astrophysical Phenomenascintillation counter: liquidFOS: Physical sciencesScintillator53001 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Physics and Astronomy (all)Low energy[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciences[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]010306 general physics[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]BorexinoPhysics010308 nuclear & particles physicsneutrino: energy: lowgeophysicsbackgroundPhysicsDetectorneutrino: flux: measuredHigh Energy Physics::PhenomenologyInstrumentation and Detectors (physics.ins-det)neutrino: particle sourceneutrino: sterileantineutrinoGran SassoNEUTRINOS13. Climate actionBorexinoHigh Energy Physics::ExperimentNeutrinoNational laboratory
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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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Measurement of Solar pp-neutrino flux with Borexino: results and implications

2015

International audience; Measurement of the Solar pp-neutrino flux completed the measurement of Solar neutrino fluxes from the pp-chain of reactions in Borexino experiment. The result is in agreement with the prediction of the Standard Solar Model and the MSW/LMA oscillation scenario. A comparison of the total neutrino flux from the Sun with Solar luminosity in photons provides a test of the stability of the Sun on the 10(5) years time scale, and sets a strong limit on the power production by the unknown energy sources in the Sun.

model: solarHistoryneutrino: solarSolar neutrinoAstrophysics::High Energy Astrophysical Phenomenaluminosity: solarSolar luminosity[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energyneutrino: fluxEducationLuminosityNuclear physicsPhysics and Astronomy (all)SEARCH0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Astrophysics::Solar and Stellar Astrophysicsddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsDETECTORBorexinoMSW effectPhysicsStandard solar modelSolar energetic particles010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyphotonAstronomySolar neutrino problemstabilityoscillationComputer Science Applicationsp p13. Climate actionPhysics::Space PhysicsBorexinoAstrophysics::Earth and Planetary AstrophysicsNeutrinoexperimental results
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Borexino’s search for low-energy neutrino and antineutrino signals correlated with gamma-ray bursts

2017

International audience; A search for neutrino and antineutrino events correlated with 2350 gamma-ray bursts (GRBs) is performed with Borexino data collected between December 2007 and November 2015. No statistically significant excess over background is observed. We look for electron antineutrinos ( ν¯e ) that inverse beta decay on protons with energies from 1.8  MeV to 15  MeV and set the best limit on the neutrino fluence from GRBs below 8  MeV. The signals from neutrinos and antineutrinos from GRBs that scatter on electrons are also searched for, a detection channel made possible by the particularly radio-pure scintillator of Borexino. We obtain currently the best limits on the neutrino f…

antineutrinoselectronAntineutrinosneutrino: solarPhysics::Instrumentation and Detectorsdata acquisitionSolar neutrino[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Astrophysics::High Energy Astrophysical Phenomenalow energy/MeV neutrinosElectrongamma ray: burst01 natural sciencesNuclear physicsLow energy/MeV neutrino0103 physical sciencesNeutrinoLow energy/MeV neutrinosNeutrinosNuclear Experiment010303 astronomy & astrophysicsGamma-ray burstBorexinoscintillation counterPhysicsflavor010308 nuclear & particles physicsbackgroundgamma-ray burstsneutrinosAntineutrinos; Gamma-ray bursts; Low energy/MeV neutrinos; Neutrinos; Astronomy and AstrophysicsAstronomy and Astrophysicssemileptonic decayantineutrinocorrelation: timeNeutrino detectorInverse beta decayddc:540Scintillation counterreadoutHigh Energy Physics::ExperimentBorexinoGamma-ray burstsNeutrinoGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Understanding the detector behavior through Montecarlo and calibration studies in view of the SOX measurement

2015

International audience; Borexino is an unsegmented neutrino detector operating at LNGS in central Italy. The experiment has shown its performances through its unprecedented accomplishments in the solar and geoneutrino detection. These performances make it an ideal tool to accomplish a state- of-the-art experiment able to test the existence of sterile neutrinos (SOX experiment). For both the solar and the SOX analysis, a good understanding of the detector response is fundamental. Consequently, calibration campaigns with radioactive sources have been performed over the years. The calibration data are of extreme importance to develop an accurate Monte Carlo code. This code is used in all the n…

HistoryGeoneutrinoCalibration (statistics)Physics::Instrumentation and DetectorsNuclear engineeringMonte Carlo method01 natural sciencesprogrammingParticle detectorEducationPhysics and Astronomy (all)0103 physical sciencesddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsSimulationBorexinoPhysics010308 nuclear & particles physicsDetectorneutrino: sterilecalibrationComputer Science::Computers and SocietyComputer Science ApplicationsNeutrino detectorBorexinoHigh Energy Physics::ExperimentNeutrinonumerical calculations: Monte Carloperformance
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Abilities of berberine and chemically modified berberines to interact with metformin and inhibit proliferation of pancreatic cancer cells.

2019

Abstract Pancreatic cancer is devastating cancer worldwide with few if any truly effective therapies. Pancreatic cancer has an increasing incidence and may become the second leading cause of death from cancer. Novel, more effective therapeutic approaches are needed as pancreatic cancer patients usually survive for less than a year after being diagnosed. Control of blood sugar levels by the prescription drug metformin in diseases such as diabetes mellitus has been examined in association with pancreatic cancer. While the clinical trials remain inconclusive, there is hope that certain diets and medications may affect positively the outcomes of patients with pancreatic and other cancers. Other…

0301 basic medicineCancer ResearchSettore MED/09 - Medicina Internaendocrine system diseasesBerberineSignal transduction inhibitorsBlood sugarPharmacologyAMP-Activated Protein KinasesBerberine; PDAC; Signal transduction inhibitors; TP5303 medical and health scienceschemistry.chemical_compound0302 clinical medicineBerberineMETFORMINAPancreatic cancerDiabetes mellitusGeneticsmedicineHumansTP53Signal transduction inhibitorMolecular BiologyCell Proliferationbusiness.industryPDACCancerAMPKmedicine.diseaseMetforminMetforminNeoplasm ProteinsPancreatic Neoplasms030104 developmental biologychemistry030220 oncology & carcinogenesisCancer cellMolecular Medicinebusinessmedicine.drugAdvances in biological regulation
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Limiting neutrino magnetic moments with Borexino Phase-II solar neutrino data

2017

A search for the solar neutrino effective magnetic moment has been performed using data from 1291.5 days exposure during the second phase of the Borexino experiment. No significant deviations from the expected shape of the electron recoil spectrum from solar neutrinos have been found, and a new upper limit on the effective neutrino magnetic moment of $\mu_{\nu}^{eff}$ $<$ 2.8$\cdot$10$^{-11}$ $\mu_{B}$ at 90\% c.l. has been set using constraints on the sum of the solar neutrino fluxes implied by the radiochemical gallium experiments.Using the limit for the effective neutrino moment, new limits for the magnetic moments of the neutrino flavor states, and for the elements of the neutrino magne…

Physics and Astronomy (miscellaneous)neutrino: solarPhysics::Instrumentation and DetectorsSolar neutrino01 natural sciencesHigh Energy Physics - ExperimentNeutrino detectorHigh Energy Physics - Experiment (hep-ex)SPIN ROTATIONHigh Energy Physics - Phenomenology (hep-ph)electron: recoil[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Astrophysics::Solar and Stellar AstrophysicsBorexinoS066MGMgalliumPhysicsMagnetic momentneutrino: magnetic momentHigh Energy Physics - Phenomenologyneutrino: momentNeutrino detectorneutrino: flavorneutrino: MajoranaMeasurements of neutrino speedBorexinoNeutrinoupper limitParticle physicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSolar neutrinoDECAYSMagnetic momentNuclear physicsstatistical analysis[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciencesddc:530010306 general physicsNeutrino oscillationDETECTORELECTROMAGNETIC PROPERTIES010308 nuclear & particles physicsHigh Energy Physics::PhenomenologySolar neutrino problemMAJORANA NEUTRINOS[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]electron: energy spectrum[ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::Experimentexperimental resultsPhysical Review D
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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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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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Low-energy (anti)neutrino physics with Borexino: Neutrinos from the primary proton-proton fusion process in the Sun

2014

The Sun is fueled by a series of nuclear reactions that produce the energy that makes it shine. The primary reaction is the fusion of two protons into a deuteron, a positron and a neutrino. These neutrinos constitute the vast majority of neutrinos reaching Earth, providing us with key information about what goes on at the core of our star. Several experiments have now confirmed the observation of neutrino oscillations by detecting neutrinos from secondary nuclear processes in the Sun; this is the first direct spectral measurement of the neutrinos from the keystone proton-proton fusion. This observation is a crucial step towards the completion of the spectroscopy of pp-chain neutrinos, as we…

Nuclear reactionPhysics - Instrumentation and DetectorsProtonneutrino: solarPhysics::Instrumentation and Detectors01 natural sciences7. Clean energynuclear reactionHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)PositronstarPrimary (astronomy)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear Experiment (nucl-ex)[ PHYS.NEXP ] Physics [physics]/Nuclear Experiment [nucl-ex]Nuclear ExperimentNuclear Experiment[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]BorexinoPhysicsSPECTROSCOPYInstrumentation and Detectors (physics.ins-det)SOLAR NEUTRINOSAstrophysics - Solar and Stellar AstrophysicsBorexinoNeutrinomodel: solardeuteronGRAN SASSOParticle physicsNuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]talk: Conca Specchiulla 2014/09/07[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationDETECTORSolar and Stellar Astrophysics (astro-ph.SR)neutrino: modelp p: fusion010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyDeuterium13. Climate actionspectralHigh Energy Physics::Experimentneutrino: oscillationexperimental results
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High significance measurement of the terrestrial neutrino flux with the Borexino detector

2015

International audience; We review the geoneutrino measurement with Borexino from 2056 days of data taking.

HistoryParticle physicsSolar neutrinoFlux010502 geochemistry & geophysics01 natural sciencesneutrino: fluxNOEducationNuclear physicstalk: Torino 2015/09/07Physics and Astronomy (all)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530Borexino0105 earth and related environmental sciencesPhysics010308 nuclear & particles physicsDetectorComputer Science ApplicationsNeutrino detectorMeasurements of neutrino speedBorexinoneutrino: geophysicsNeutrinoexperimental results
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The Monte Carlo simulation of the Borexino detector

2017

We describe the Monte Carlo (MC) simulation package of the Borexino detector and discuss the agreement of its output with data. The Borexino MC 'ab initio' simulates the energy loss of particles in all detector components and generates the resulting scintillation photons and their propagation within the liquid scintillator volume. The simulation accounts for absorption, reemission, and scattering of the optical photons and tracks them until they either are absorbed or reach the photocathode of one of the photomultiplier tubes. Photon detection is followed by a comprehensive simulation of the readout electronics response. The algorithm proceeds with a detailed simulation of the electronics c…

Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsSolar neutrinoMonte Carlo methodscintillation counter: liquidSolar neutrinosenergy resolution01 natural sciences7. Clean energyLarge volume liquid scintillator detectorHigh Energy Physics - Experiment[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Large volume liquid scintillator detectorsBorexinoPhysicsphotomultipliertrack data analysisDetectorefficiency: quantumddc:540GEANTBorexinoNeutrinophoton: yieldnumerical calculations: Monte CarloPhotomultiplierdata analysis methodenergy lossScintillatorSolar neutrinoprogrammingphoton: reflectionMonte Carlo simulationsNuclear physics0103 physical sciencesphoton: scattering[INFO]Computer Science [cs][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsbackground: radioactivityMonte Carlo simulationdetector: designScintillation010308 nuclear & particles physicsbibliographyAstronomy and AstrophysicscalibrationLarge volume liquid scintillator detectors; Monte Carlo simulations; Solar neutrinos; Astronomy and Astrophysicsattenuation: lengthpile-upelectronics: readout
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Abilities of berberine and chemically modified berberines to inhibit proliferation of pancreatic cancer cells.

2018

Berberine (BBR) is a common nutraceutical consumed by millions worldwide. BBR has many different effects on human health, e.g., diabetes, diarrhea, inflammation and now more recently it has been proposed to have potent anti-cancer effects. BBR has been shown to suppress the growth of cancer cells more than normal cells. BBR has been proposed to exert its growth-inhibitory effects by many different biochemical mechanisms including: suppression of cell cycle progression, induction of reactive oxygen species, induction of apoptosis and autophagy and interactions with DNA potentially leading to DNA damage, and altered gene expression. Pancreatic cancer is a leading cancer worldwide associated w…

Male0301 basic medicineCancer ResearchSettore MED/09 - Medicina InternaBerberineDNA damagePopulationSignal transduction inhibitorsApoptosisInflammation03 medical and health sciences0302 clinical medicineCell Line TumorPancreatic cancerGeneticsmedicineHumanseducationChemotherapeutic drugMolecular BiologySignal transduction inhibitorAgededucation.field_of_studybusiness.industryCell CycleAutophagyCancerPDACDNA Neoplasmmedicine.diseaseGene Expression Regulation NeoplasticPancreatic Neoplasms030104 developmental biologyApoptosis030220 oncology & carcinogenesisCancer cellCancer researchMolecular MedicineChemotherapeutic drugsmedicine.symptombusinessDNA DamageSignal Transduction
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Neutrino Physics with JUNO

2016

The Jiangmen Underground Neutrino Observatory (JUNO), a 20 kton multi-purpose underground liquid scintillator detector, was proposed with the determination of the neutrino mass hierarchy as a primary physics goal. It is also capable of observing neutrinos from terrestrial and extra-terrestrial sources, including supernova burst neutrinos, diffuse supernova neutrino background, geoneutrinos, atmospheric neutrinos, solar neutrinos, as well as exotic searches such as nucleon decays, dark matter, sterile neutrinos, etc. We present the physics motivations and the anticipated performance of the JUNO detector for various proposed measurements. By detecting reactor antineutrinos from two power plan…

Particle physicsSterile neutrinoNuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsGeoneutrinoreactor neutrino experimentPhysics::Instrumentation and DetectorsSolar neutrinomedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciences7. Clean energy01 natural sciencesNOHigh Energy Physics - Experimentneutrino astronomyHigh Energy Physics - Experiment (hep-ex)neutrino physics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530neutrino mass hierarchy reactor liquid scintillator010306 general physicsJiangmen Underground Neutrino Observatorymedia_commonPhysics010308 nuclear & particles physicsHigh Energy Physics::Phenomenologyneutrino physicInstrumentation and Detectors (physics.ins-det)Universereactor neutrino experimentslarge scintillator detectors; neutrino astronomy; neutrino physics; reactor neutrino experiments; Nuclear and High Energy PhysicsSupernovalarge scintillator detectors13. Climate actionPhysics::Space Physicslarge scintillator detectorHigh Energy Physics::ExperimentNeutrinoreactor neutrino experiments; large scintillator detectors; neutrino physics; neutrino astronomy
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Recent results from Borexino

2016

Journal of Physics Conference Series. - 798, International Conference on Particle Physics and Astrophysics : 10-14 October 2016, Moscow, Russian Federation / proceedings editors: 1. issue: cosmic rays: Arkady Galper (MEPhI, Moscow, Russia) [und 7 andere] 2nd International Conference on Particle Physics and Astrophysics, ICPPA 2016, Moscow, Russia, 11 Oct 2016 - 14 Oct 2016; Bristol : IOP Publ., Journal of Physics Conference Series, 798, 012114 pp. (2017). doi:10.1088/1742-6596/798/1/012114

HistoryParticle physicsneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoContext (language use)53001 natural sciencesneutrino: fluxEducationPhysics::GeophysicsNuclear physicsPhysics and Astronomy (all)Low energyenergy: solar0103 physical sciencesEnergy spectrumddc:530010306 general physicsBorexinoscintillation counterPhysicsCharge conservationMultidisciplinary010308 nuclear & particles physicsstabilityComputer Science ApplicationsGran Sassoenergy: productionPhysics::Space PhysicsHigh Energy Physics::ExperimentBorexinoneutrino: geophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Absence of a day-night asymmetry in the7Be solar neutrino rate in Borexino

2012

We report on a search for the day-night asymmetry of the Be-7 solar neutrino rate measured by Borexino at the Laboratori Nazionali del Gran Sasso (LNGS), Italy. The measured value, Adn=0.001 +- 0.012 (stat) +- 0.007 (syst), shows the absence of a significant asymmetry. This result alone rejects the so-called LOW solution at more than 8.5 sigma. Combined with the other solar neutrino data, it isolates the Large Mixing Angle (LMA) -- MSW solution at DeltaChi2 > 190 without relying on the assumption of CPT symmetry in the neutrino sector. We also show that including the day-night asymmetry, data from Borexino alone restricts the MSW neutrino oscillations to the LMA solution at 90% confidence l…

Particle physicsNuclear and High Energy PhysicsNeutrino oscillationPhysics::Instrumentation and Detectorsmedia_common.quotation_subjectSolar neutrino01 natural sciencesAsymmetrySolar neutrinoNuclear physicsDay-night effect0103 physical sciences010306 general physicsNeutrino oscillationNuclear Experimentday–night effectBorexinomedia_commonPhysicsneutrino oscillations010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaSolar neutrino problemNeutrino detectorsolar neutrinosMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoCPT violation
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Effects of the MDM2 inhibitor Nutlin-3a on sensitivity of pancreatic cancer cells to berberine and modified berberines in the presence and absence of…

2021

Abstract Approaches to improve pancreatic cancer therapy are essential as this disease has a very bleak outcome. Approximately 80% of pancreatic cancers are pancreatic ductal adenocarcinomas (PDAC). A key regulatory gene frequently mutated (∼75%) in PDAC is the TP53 tumor suppressor gene which controls the transcription of multiple genes involved in cell cycle progression, apoptosis, cancer progression and other growth regulatory processes. The mouse double minute 2 homolog (MDM2) gene product is a nuclear-localized E3 ubiquitin ligase and negatively regulates the TP53 protein which results in its proteasomal degradation. Various MDM2 inhibitors have been isolated and examined in clinical t…

Nutlin-3aCancer ResearchBerberineendocrine system diseasesTumor suppressor geneNAX compoundsApoptosisPiperazinesTargeted therapyGene productCell Line TumorPancreatic cancerGeneticsmedicineHumansTP53neoplasmsMolecular BiologyRegulator geneNAX compundsbiologyChemistryImidazolesPDACCancerProto-Oncogene Proteins c-mdm2PDCAmedicine.diseaseUbiquitin ligasePancreatic NeoplasmsCell culturebiology.proteinCancer researchNAX compoundMolecular MedicineMdm2Tumor Suppressor Protein p53Signal TransductionAdvances in Biological Regulation
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SOX : short distance neutrino oscillations with Borexino

2014

Abstract The Borexino detector has convincingly shown its outstanding performance in the in the sub-MeV regime through its unprecedented accomplishments in the solar and geo-neutrinos detection, which make it the ideal tool to unambiguously test the long-standing issue of the existence of a sterile neutrino, as suggested by several anomalies: the outputs of the LSND and Miniboone experiments, the results of the source calibration of the two Gallium solar ν experiments, and the recently hinted reactor anomaly. The SOX project will exploit two sources, based on chromium and cerium, which deployed under the experiment will emit two intense beams of ν e (Cr) and ν e ‾ (Ce). Interacting in the a…

Sterile neutrinoPhysics::Instrumentation and Detectorsscintillation counter: liquidtalk: Valencia 2014/07/027. Clean energy01 natural sciences[SPI]Engineering Sciences [physics][PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]BorexinoSterile neutrinogalliumPhysicsOscillationneutrino: sterilesolarceriumBorexinochromiumchromium-51neutrino: geophysicsNeutrinoperformanceNuclear and High Energy PhysicsParticle physicsAnomalous oscillations; Borexino; Cerium-144; Chromium-51; SOX; Sterile neutrinosanomalyneutrino/e: beamScintillatorcerium-144Anomalous oscillations; Borexino; Cerium-144; Chromium-51; SOX; Sterile neutrinos; Nuclear and High Energy PhysicsMiniBooNEsterile neutrinos0103 physical sciences010306 general physicsNeutrino oscillation010308 nuclear & particles physicschromium-51cerium-144calibrationGran SassoLSNDAnomalous oscillationSOXneutrino: familyHigh Energy Physics::Experimentnuclear reactorneutrino: oscillationAnomaly (physics)anomalous oscillationsexperimental resultsneutrino/e: oscillation
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Solar neutrino detectors as sterile neutrino hunters

2016

International audience; The large size and the very low radioactive background of solar neutrino detectors such as Borexino at the Gran Sasso Laboratory in Italy offer a unique opportunity to probe the existence of neutrino oscillations into new sterile components by means of carefully designed and well calibrated anti-neutrino and neutrino artificial sources. In this paper we briefly summarise the key elements of the SOX experiment, a program for the search of sterile neutrinos (and other short distance effects) by means of a (144)Ce-(144)Pr anti-neutrino source and, possibly in the medium term future, with a (51)Cr neutrino source.

HistorySterile neutrinoParticle physicsneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical Phenomena01 natural sciences7. Clean energyEducationPhysics and Astronomy (all)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationnuclideBorexinoPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologySolar neutrino problemneutrino: sterileComputer Science ApplicationspraseodymiumGran Sassoneutrino: detectorNeutrino detectorcerium: nuclideHigh Energy Physics::Experimentneutrino: oscillationNeutrino astronomyNeutrinoantineutrino: particle source[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Effects of resveratrol, curcumin, berberine and other nutraceuticals on aging, cancer development, cancer stem cells and microRNAs

2017

Natural products or nutraceuticals have been shown to elicit anti-aging, anti-cancer and other health-enhancing effects. A key target of the effects of natural products may be the regulation of microRNA (miR) expression which results in cell death or prevents aging, diabetes, cardiovascular and other diseases. This review will focus on a few natural products, especially on resveratrol (RES), curcumin (CUR) and berberine (BBR). RES is obtained from the skins of grapes and other fruits and berries. RES may extend human lifespan by activating the sirtuins and SIRT1 molecules. CUR is isolated from the root of turmeric (Curcuma longa). CUR is currently used in the tutreatment of many disorders, …

0301 basic medicineAgingCurcuminMiRReviewResveratrolPharmacologyCSCNatural productCell LineNOMiRs03 medical and health scienceschemistry.chemical_compound0302 clinical medicineBerberineNutraceuticalCancer stem cellCell Line TumorNeoplasmsmicroRNAHumansMedicineSIRTGene methylationCurcumaNatural productsTumorCSCs Curcumin Gene methylation MiRs Natural products Resveratrol SIRTbiologybusiness.industryCell BiologyCoptis chinensisbiology.organism_classificationCSCs; Curcumin; Gene methylation; MiRs; Natural products; Resveratrol; SIRT; Aging; Cell Line Tumor; Humans; Neoplasms; Neoplastic Stem Cells; Dietary Supplements030104 developmental biologychemistryResveratrol030220 oncology & carcinogenesisDietary SupplementsNeoplastic Stem CellsCurcuminCSCsbusinessAging
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Metformin influences drug sensitivity in pancreatic cancer cells

2018

Abstract Pancreatic ductal adenocarcinoma (PDAC) is an aggressive, highly metastatic malignancy and accounts for 85% of pancreatic cancers. PDAC patients have poor prognosis with a five-year survival of only 5–10% after diagnosis and treatment. Pancreatic cancer has been associated with type II diabetes as the frequency of recently diagnosed diabetics that develop pancreatic cancer within a 10-year period of initial diagnosis of diabetes in increased in comparison to non-diabetic patients. Metformin is a very frequently prescribed drug used to treat type II diabetes. Metformin acts in part by stimulating AMP-kinase (AMPK) and results in the suppression of mTORC1 activity and the induction o…

AMPK0301 basic medicineCancer Researchendocrine system diseases03 medical and health sciencesPancreatic cancerGeneticsMedicineAnimalsHumansDoxorubicinDrug InteractionsRapamycinSignal transduction inhibitormTORC1Molecular BiologyCisplatinSirolimusAnimalbusiness.industryPancreatic NeoplasmCancermedicine.diseaseGemcitabineMetforminMetforminPancreatic Neoplasms030104 developmental biologyDrug InteractionDocetaxelDiabetes Mellitus Type 2SirolimusCancer researchMolecular MedicinebusinessHumanmedicine.drugCarcinoma Pancreatic DuctalSignal Transduction
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The high precision measurement of the 144Ce activity in the SOX experiment

2015

International audience; In order to perform a resolutive measurement to clarify the neutrino anomalies and to observe possible short distance neutrino oscillations, the SOX (Short distance neutrino Oscillations with BoreXino) experiment is under construction. In the first phase, a 100 kCi (144)Ce-(144)Pr antineutrino source will be placed under the Borexino detector at the Laboratori Nazionali del Gran Sasso (LNGS), in center of Italy, and the rate measurement of the antineutrino events, observed by the very low radioactive background Borexino detector, will be compared with the high precision (< 1%) activity measurement performed by two calorimeters. The source will be embedded in a 19 mm …

HistoryParticle physicsWater flowPhysics::Instrumentation and Detectorstungstenwater[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesParticle detectorEducationPhysics::GeophysicsthermalNuclear physicsPhysics and Astronomy (all)alloy0103 physical sciencesddc:530010306 general physicsNeutrino oscillationNuclear Experimentbackground: radioactivityBorexinoPhysics010308 nuclear & particles physicsprecision measurementcalorimeter: designDetectorantineutrinoComputer Science ApplicationsGran SassoceriumflowMeasuring instrumentHigh Energy Physics::ExperimentBorexinoneutrino: oscillationNeutrinoLepton
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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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