0000000000050499

AUTHOR

G.v. Russo

showing 22 related works from this author

The data acquisition system for the ANTARES neutrino telescope

2006

The ANTARES neutrino telescope is being constructed in the Mediterranean Sea. It consists of a large three-dimensional array of photo-multiplier tubes. The data acquisition system of the detector takes care of the digitisation of the photo-multiplier tube signals, data transport, data filtering, and data storage. The detector is operated using a control program interfaced with all elements. The design and the implementation of the data acquisition system are described.

Nuclear and High Energy Physics[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and DetectorsData managementAstrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONFOS: Physical sciencesAstrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Data filteringData acquisition0103 physical sciences14. Life underwaterElectronics010306 general physicsInstrumentationdata acquisition system; neutrino telescopeRemote sensingAstroparticle physicsPhysicsneutrino telescope data acquisition system[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsbusiness.industryDetectorAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for AstrophysicsAstronomyneutrino telescopedata acquisition systemComputer data storageFísica nuclearbusiness
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Search for an Invisibly Decaying Z′ Boson at Belle II in e+e−→μ+μ−(e±μ∓) Plus Missing Energy Final States

2020

Theories beyond the standard model often predict the existence of an additional neutral boson, the Z′. Using data collected by the Belle II experiment during 2018 at the SuperKEKB collider, we perform the first searches for the invisible decay of a Z′ in the process e+e-→μ+μ-Z′ and of a lepton-flavor-violating Z′ in e+e-→e±μZ′. We do not find any excess of events and set 90% credibility level upper limits on the cross sections of these processes. We translate the former, in the framework of an Lμ-Lτ theory, into upper limits on the Z′ coupling constant at the level of 5×10-2-1 for MZ′≤6 GeV/c2.

PhysicsCoupling constantParticle physicsMissing energyPhysics beyond the Standard ModelGeneral Physics and Astronomy01 natural scienceslaw.inventionlaw0103 physical sciencesHigh Energy Physics::Experiment010306 general physicsColliderBosonPhysical Review Letters
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The ANTARES optical module

2001

The ANTARES collaboration is building a deep sea neutrino telescope in the Mediterranean Sea. This detector will cover a sensitive area of typically 0.1 km-squared and will be equipped with about 1000 optical modules. Each of these optical modules consists of a large area photomultiplier and its associated electronics housed in a pressure resistant glass sphere. The design of the ANTARES optical module, which is a key element of the detector, has been finalized following extensive R & D studies and is reviewed here in detail.

Nuclear and High Energy PhysicsPhotomultiplierAstrophysics and AstronomyPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeFOS: Physical sciencesAstrophysics01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsOptical Moduleneutrino astronomyHigh Energy Physics - Experiment (hep-ex)deep sea detector; neutrino astronomyMediterranean sea0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]14. Life underwaterElectronicsDetectors and Experimental Techniques010306 general physicsInstrumentationRemote sensingPhysics010308 nuclear & particles physicsDetectorAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for AstrophysicsNeutrino detectordeep sea detectorFísica nuclearNeutrino astronomy
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The ANTARES Optical Beacon System

2007

ANTARES is a neutrino telescope being deployed in the Mediterranean Sea. It consists of a three dimensional array of photomultiplier tubes that can detect the Cherenkov light induced by charged particles produced in the interactions of neutrinos with the surrounding medium. High angular resolution can be achieved, in particular when a muon is produced, provided that the Cherenkov photons are detected with sufficient timing precision. Considerations of the intrinsic time uncertainties stemming from the transit time spread in the photomultiplier tubes and the mechanism of transmission of light in sea water lead to the conclusion that a relative time accuracy of the order of 0.5 ns is desirabl…

Nuclear and High Energy PhysicsPhotomultiplierPhysics::Instrumentation and Detectors[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesneutrino telescope; optical beacon; time calibrationAstrophysics01 natural scienceslaw.inventionTelescope[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Opticslaw0103 physical sciencesCalibrationtime calibrationAngular resolution14. Life underwateroptical beacon010306 general physicsInstrumentationCherenkov radiationPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]neutrino telescope time calibration optical beacon010308 nuclear & particles physicsbusiness.industryDetectorAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for Astrophysicsneutrino telescopeSITEAstronomyBeaconLIGHTFísica nuclearNeutrinobusiness
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First Evidence for cos2β>0 and Resolution of the Cabibbo-Kobayashi-Maskawa Quark-Mixing Unitarity Triangle Ambiguity

2018

We present first evidence that the cosine of the CP-violating weak phase 2β is positive, and hence exclude trigonometric multifold solutions of the Cabibbo-Kobayashi-Maskawa (CKM) Unitarity Triangle using a time-dependent Dalitz plot analysis of B^{0}→D^{(*)}h^{0} with D→K_{S}^{0}π^{+}π^{-} decays, where h^{0}∈{π^{0},η,ω} denotes a light unflavored and neutral hadron. The measurement is performed combining the final data sets of the BABAR and Belle experiments collected at the ϒ(4S) resonance at the asymmetric-energy B factories PEP-II at SLAC and KEKB at KEK, respectively. The data samples contain (471±3)×10^{6}BB[over ¯] pairs recorded by the BABAR detector and (772±11)×10^{6}BB[over ¯] p…

QuarkPhysicsParticle physicsUnitarity010308 nuclear & particles physicsElectron–positron annihilationHadronGeneral Physics and AstronomyDalitz plot01 natural sciencesB-factoryKEKB0103 physical sciencesCP violation010306 general physicsPhysical Review Letters
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Study of Large Hemispherical Photomultiplier Tubes for the ANTARES Neutrino Telescope

2005

The ANTARES neutrino telescope, to be immersed depth in the Mediterranean Sea, will consist of a 3 dimensional matrix of 900 large area photomultiplier tubes housed in pressure resistant glass spheres. The selection of the optimal photomultiplier was a critical step for the project and required an intensive phase of tests and developments carried out in close collaboration with the main manufacturers worldwide. This paper provides an overview of the tests performed by the collaboration and describes in detail the features of the PMT chosen for ANTARES.

Nuclear and High Energy PhysicsPhotomultiplierPhysics - Instrumentation and DetectorsNeutrino detectionNeutrino telescopeFOS: Physical sciences01 natural scienceslarge area photosensor hemispherical photomultiplier neutrino detectionNuclear physicsOpticsIntensive Phase0103 physical sciences14. Life underwater[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsInstrumentationAstroparticle physicsPhysics010308 nuclear & particles physicsbusiness.industryHemispherical photomultiplierInstrumentation and Detectors (physics.ins-det)Large area photosensorGlass spheresNeutrino detector95.55.Vj; 85.60.HaFísica nuclearbusinesshemispherical photomultiplier; large area photosensor; neutrino detection
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Performance of the front-end electronics of the ANTARES neutrino telescope

2010

ANTARES is a high-energy neutrino telescope installed in the Mediterranean Sea at a depth of 2475 m. It consists of a three-dimensional array of optical modules, each containing a large photomultiplier tube. A total of 2700 front-end ASICs named Analogue Ring Samplers (ARS) process the phototube signals, measure their arrival time, amplitude and shape as well as perform monitoring and calibration tasks. The ARS chip processes the analogue signals from the optical modules and converts information into digital data. All the information is transmitted to shore through further multiplexing electronics and an optical link. This paper describes the performance of the ARS chip; results from the fu…

Nuclear and High Energy PhysicsPhotomultiplier[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics::Instrumentation and DetectorsOptical linkDigital dataFOS: Physical sciencesAnalog-to-digital converterNeutrino telescope01 natural sciencesMultiplexinglaw.inventionPhototubeApplication-specific integrated circuitPhotomultiplier tubelawASICs0103 physical sciences14. Life underwater010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)InstrumentationPhysics010308 nuclear & particles physicsbusiness.industryASICAstrophysics::Instrumentation and Methods for AstrophysicsElectrical engineeringCIRCUITFront-end electronicsChip[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Física nuclearUNDERWATER DETECTORasic; front-end electronics; neutrino telescope; photomultiplier tubeAstrophysics - Instrumentation and Methods for AstrophysicsbusinessSYSTEMNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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New Results from the NUMEN Project

2018

International audience; NUMEN aims at accessing experimentally driven information on Nuclear Matrix Elements (NME) involved in the half-life of the neutrinoless double beta decay (0νββ), by high-accuracy measurements of the cross sections of Heavy Ion (HI) induced Double Charge Exchange (DCE) reactions. First evidence about the possibility to get quantitative information about NME from experiments is found for the (^18O,^18Ne) and (^20Ne,^20O) reactions. Moreover, to infer the neutrino average masses from the possible measurement of the half-life of 0νββ decay, the knowledge of the NME is a crucial aspect. The key tools for this project are the high resolution Superconducting Cyclotron beam…

Semileptonic decayheavy ion: scatteringCyclotronContext (language use)[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energy01 natural scienceslaw.inventionNuclear physicsdouble-beta decay: (0neutrino)lawDouble beta decay0103 physical sciencescyclotron010306 general physicsPhysicsnucleus: semileptonic decaySpectrometer010308 nuclear & particles physicsresolutioncross section: measuredmagnetic spectrometercharge exchangeUpgradeupgradeNeutrinoOrder of magnitudeexperimental results
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Rosenbluth Separation of the π^{0} Electroproduction Cross Section.

2016

We present deeply virtual $\pi^0$ electroproduction cross-section measurements at $x_B$=0.36 and three different $Q^2$--values ranging from 1.5 to 2 GeV$^2$, obtained from experiment E07-007 that ran in the Hall A at Jefferson Lab. The Rosenbluth technique was used to separate the longitudinal and transverse responses. Results demonstrate that the cross section is dominated by its transverse component, and thus is far from the asymptotic limit predicted by perturbative Quantum Chromodynamics. An indication of a non-zero longitudinal contribution is provided by the interference term $\sigma_{LT}$ also measured. Results are compared with several models based on the leading twist approach of G…

Particle physicslongitudinalinterferenceGeneral Physics and Astronomyparton: distribution functionPartonhard exclusive electroproduction; mesons[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesHigh Energy Physics - ExperimentNuclear physicspi: distribution amplitudegeneralized parton distribution: transversityPiondeep inelastic scattering0103 physical scienceshard exclusive electroproduction[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]quantum chromodynamics: perturbation theory010306 general physicsNuclear ExperimentNuclear ExperimentmesonsQuantum chromodynamicsPhysics010308 nuclear & particles physicsscattering amplitudemomentum transferSigmanucleon: generalized parton distributionScattering amplitudetransverseDistribution (mathematics)Amplitudepi0: electroproductiontwistHigh Energy Physics::ExperimentNucleonchannel cross section: measuredJefferson Labexperimental resultsPhysical review letters
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A glimpse of gluons through deeply virtual compton scattering on the proton

2017

The internal structure of nucleons (protons and neutrons) remains one of the greatest outstanding problems in modern nuclear physics. By scattering high-energy electrons off a proton we are able to resolve its fundamental constituents and probe their momenta and positions. Here we investigate the dynamics of quarks and gluons inside nucleons using deeply virtual Compton scattering (DVCS)—a highly virtual photon scatters off the proton, which subsequently radiates a photon. DVCS interferes with the Bethe-Heitler (BH) process, where the photon is emitted by the electron rather than the proton. We report herein the full determination of the BH-DVCS interference by exploiting the distinct energ…

Genetics and Molecular Biology (all)PhotonProtonHigh Energy Physics::LatticeNuclear TheoryGeneral Physics and AstronomyVirtual particleparton: distribution functionBiochemistry01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]p: structure functionNuclear Experiment (nucl-ex)[ PHYS.NEXP ] Physics [physics]/Nuclear Experiment [nucl-ex]lcsh:ScienceNuclear ExperimentNuclear ExperimentPhysicsenergy: highMultidisciplinarystrong interactionChemistry (all)QCompton scattering: form factorphoton: energy spectrumHigh Energy Physics - Phenomenologyconfinementelectron p --> electron p photonchannel cross section: measuredQuarkelectron p: deep inelastic scatteringParticle physicselectron: polarized beamScienceStrong interactionFOS: Physical sciencesBethe-Heitler[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]ArticleGeneral Biochemistry Genetics and Molecular Biologyenergy dependencequarkPhysics and Astronomy (all)[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]photon: emissiondeeply virtual Compton scattering0103 physical sciencesstructure010306 general physicsquantum mechanics: interference010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyCompton scatteringGeneral ChemistrygluonsensitivityGluon[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Quark–gluon plasmalcsh:Q[ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::ExperimentholographyChemistry (all); Biochemistry Genetics and Molecular Biology (all); Physics and Astronomy (all)photon: virtualexperimental results
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Using anatomic and metabolic imaging in stereotactic radio neuro-surgery treatments

2016

PET/MR imagingmedicine.medical_specialtyNeuro-radiosurgerybusiness.industryMetabolic imagingBiophysicsGeneral Physics and AstronomyGeneral MedicineRandom Walker algorithmFuzzy C-Means clustering030218 nuclear medicine & medical imagingBrain tumor03 medical and health sciences0302 clinical medicineRandom walker algorithm030220 oncology & carcinogenesismedicineRadiology Nuclear Medicine and imagingNeurosurgeryRadiologyPet mr imagingbusinessNuclear medicine
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New Measurements of the Transverse Beam Asymmetry for Elastic Electron Scattering from Selected Nuclei

2012

We have measured the beam-normal single-spin asymmetry $A_n$ in the elastic scattering of 1-3 GeV transversely polarized electrons from $^1$H and for the first time from $^4$He, $^{12}$C, and $^{208}$Pb. For $^1$H, $^4$He and $^{12}$C, the measurements are in agreement with calculations that relate $A_n$ to the imaginary part of the two-photon exchange amplitude including inelastic intermediate states. Surprisingly, the $^{208}$Pb result is significantly smaller than the corresponding prediction using the same formalism. These results suggest that a systematic set of new $A_n$ measurements might emerge as a new and sensitive probe of the structure of heavy nuclei.

Elastic scatteringPhysics010308 nuclear & particles physicsScatteringmedia_common.quotation_subjectFOS: Physical sciencesGeneral Physics and AstronomyElastic electronchemistry.chemical_elementElectron[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesAsymmetryAmplitudechemistryExcited state0103 physical sciencesNuclear Experiment (nucl-ex)Atomic physics010306 general physicsNuclear ExperimentNuclear ExperimentHeliummedia_common
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Alignment of the ALICE Inner Tracking System with cosmic-ray tracks

2010

ALICE (A Large Ion Collider Experiment) is the LHC (Large Hadron Collider) experiment devoted to investigating the strongly interacting matter created in nucleus-nucleus collisions at the LHC energies. The ALICE ITS, Inner Tracking System, consists of six cylindrical layers of silicon detectors with three different technologies; in the outward direction: two layers of pixel detectors, two layers each of drift, and strip detectors. The number of parameters to be determined in the spatial alignment of the 2198 sensor modules of the ITS is about 13,000. The target alignment precision is well below 10 micron in some cases (pixels). The sources of alignment information include survey measurement…

Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsperspectiveHigh Energy PhisicsDetector alignment and calibration methods (lasers sources particle-beams); Particle tracking detectors (Solid-state detectors); Instrumentation; Mathematical Physics01 natural sciences7. Clean energylaw.inventionHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)lawParticle tracking detectors[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Tracking detectors; High Energy Phisics; Heavy Ion PhysicsDetectors and Experimental TechniquesDetector alignment and calibration methodsNuclear ExperimentInstrumentationphysics.ins-detMathematical PhysicsdetectorsPhysicsLarge Hadron ColliderSolenoidal vector fieldPhysicsDetectorInstrumentation and Detectors (physics.ins-det)particle-beams)collisionsParticle tracking detectors (Solid-state detectors) ; Detector alignment and calibration methods (lasers ; sources ; particle-beams)collaboration; collisions; detector alignment and calibration methods (lasers; sources; particle-beams); detectors; particle tracking detectors (solid-state detectors); performance; perspective; quark-gluon plasmaColliding beam accelerators collisions Pb-Pb collisionsParticle tracking detectors (Solid-state detectors); Detector alignment and calibration methods (lasers sources particle-beams); QUARK-GLUON PLASMAperformancesourcesquark-gluon plasmaDetector alignment and calibration methodFOS: Physical sciencesCosmic ray114 Physical sciencesNuclear physicsTracking detectorsOpticsparticle tracking detectors (solid-state detectors)0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsColliderPixel010308 nuclear & particles physicsbusiness.industryhep-exHeavy Ion Physicsdetector alignment and calibration methods (laserscollaborationQuark–gluon plasmaDetector alignment and calibration methods; Particle tracking detectorsALICE (propellant)business
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The ANTARES telescope neutrino alert system

2012

The ANTARES telescope has the capability to detect neutrinos produced in astrophysical transient sources. Potential sources include gamma-ray bursts, core collapse supernovae, and flaring active galactic nuclei. To enhance the sensitivity of ANTARES to such sources, a new detection method based on coincident observations of neutrinos and optical signals has been developed. A fast online muon track reconstruction is used to trigger a network of small automatic optical telescopes. Such alerts are generated for special events, such as two or more neutrinos, coincident in time and direction, or single neutrinos of very high energy.

Optical telescopesPhysics::Instrumentation and DetectorsAstrophysics7. Clean energy01 natural sciencesGamma ray burstsFOLLOW-UP OBSERVATIONSlaw.inventionlawFlaring activeVery high energiesHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsGAMMA-RAY BURSTS[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsSupernovaNeutrino detectorNeutrino astronomyFísica nuclearNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaFLUX[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesOptical telescopeTelescopeMuon tracksCoincidentSEARCHDetection methods0103 physical sciencesCore collapse supernovae010306 general physicsOptical follow-upInstrumentation and Methods for Astrophysics (astro-ph.IM)Neutronsantares; neutrino astronomy; optical follow-up; transient sourcesANTARES010308 nuclear & particles physicsGamma raysAstronomyAstronomy and AstrophysicsAlert systemsStarsTransient sources[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Optical signalsPotential sources13. Climate actionFISICA APLICADAHigh Energy Physics::ExperimentNeutrino astronomyGamma-ray burst
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Midrapidity Antiproton-to-Proton Ratio inppCollisons ats=0.9and 7 TeV Measured by the ALICE Experiment

2010

The ratio of the yields of antiprotons to protons in pp collisions has been measured by the ALICE experiment at root s = 0.9 and 7 TeV during the initial running periods of the Large Hadron Collider. The measurement covers the transverse momentum interval 0.45 < p(t) < 1.05 GeV/c and rapidity vertical bar y vertical bar < 0.5. The ratio is measured to be R-vertical bar y vertical bar<0.5 = 0.957 +/- 0.006(stat) +/- 0.0014(syst) at 0.9 Tev and R-vertical bar y vertical bar<0.5 = 0.991 +/- 0.005 +/- 0.014(syst) at 7 TeV and it is independent of both rapidity and transverse momentum. The results are consistent with the conventional model of baryon-number transport and set stringent limits on a…

PhysicsParticle physicsLarge Hadron ColliderProton010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyHadronGeneral Physics and Astronomy01 natural sciences7. Clean energyParticle identificationBaryonNuclear physicsAntiproton0103 physical sciencesHigh Energy Physics::ExperimentRapidityNuclear Experiment010306 general physicsBar (unit)Physical Review Letters
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Search for B+→K+νν¯ Decays Using an Inclusive Tagging Method at Belle II

2021

A search for the flavor-changing neutral-current decay B^{+}→K^{+}νν[over ¯] is performed at the Belle II experiment at the SuperKEKB asymmetric energy electron-positron collider. The data sample corresponds to an integrated luminosity of 63 fb^{-1} collected at the ϒ(4S) resonance and a sample of 9 fb^{-1} collected at an energy 60 MeV below the resonance. Because the measurable decay signature involves only a single charged kaon, a novel measurement approach is used that exploits not only the properties of the B^{+}→K^{+}νν[over ¯] decay, but also the inclusive properties of the other B meson in the ϒ(4S)→BB[over ¯] event, to suppress the background from other B meson decays and light-qua…

PhysicsParticle physicsLuminosity (scattering theory)010308 nuclear & particles physicsBranching fractionElectron–positron annihilationGeneral Physics and AstronomyResonance01 natural scienceslaw.inventionPair productionlaw0103 physical sciencesHigh Energy Physics::ExperimentB meson010306 general physicsColliderEnergy (signal processing)Physical Review Letters
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Recent results on Heavy-Ion induced reactions of interest for 0νββ decay

2019

An updated overview of recent results on Heavy-Ion induced reactions of interest for neutrinoless double beta decay is reported in the framework of the NUMEN project. The NUMEN idea is to study heavy-ion induced Double Charge Exchange (DCE) reactions with the aim to get information on the nuclear matrix elements for neutrinoless double beta (0νββ) decay. Moreover, to infer the neutrino average masses from the possible measurement of the half- life of 0νββ decay, the knowledge of the nuclear matrix elements is a crucial aspect. Uma visão geral atualizada dos resultados recentes sobre reações induzidas por íons pesados ​​de interesse para o decaimento beta duplo sem neutrinos é relatada na es…

Historymeasurement methodsnuclear matrix elements[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]heavy-ion induced Double Charge Exchange; nuclear matrix elements; neutrinoless double beta decay01 natural sciencesneutrinoless double beta decayEducationNuclear physicsoxygen: nuclidedouble-beta decay: (0neutrino)Double beta decay0103 physical sciencesBeta (velocity)neutrino: mass010306 general physicsNuclear ExperimentPhysicsnucleus: semileptonic decayMeasurement methodoperator: transition010308 nuclear & particles physicsHigh Energy Physics::Phenomenologyparticle: Majoranacharge exchangemagnetic spectrometerBeta decayheavy ionComputer Science Applicationsneon: nuclideheavy-ion induced Double Charge ExchangeHeavy ionHigh Energy Physics::ExperimentNeutrinoCharge exchange
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Measurement of atmospheric neutrino oscillations with the ANTARES neutrino telescope

2012

The data taken with the ANTARES neutrino telescope from 2007 to 2010, a total live time of 863 days, are used to measure the oscillation parameters of atmospheric neutrinos. Muon tracks are reconstructed with energies as low as 20 GeV. Neutrino oscillations will cause a suppression of vertical upgoing muon neutrinos of such energies crossing the Earth. The parameters determining the oscillation of atmospheric neutrinos are extracted by fitting the event rate as a function of the ratio of the estimated neutrino energy and reconstructed flight path through the Earth. Measurement contours of the oscillation parameters in a two-flavour approximation are derived. Assuming maximal mixing, a mass …

Nuclear and High Energy PhysicsParticle physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:500.2Neutrino telescope01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Experiment0103 physical sciencesNeutrinsHigh Energy PhysicsNeutrinos010306 general physicsNeutrino oscillationPhysicsMuonANTARES:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsNeutrino oscillations[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]High Energy Physics::PhenomenologySolar neutrino problemNeutrino astrophysicsCosmic neutrino backgroundNeutrino detectorFISICA APLICADAMeasurements of neutrino speedFísica nuclearHigh Energy Physics::ExperimentNeutrino[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Physics Letters B
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Measuring nuclear reaction cross sections to extract information on neutrinoless double beta decay

2017

Neutrinoless double beta decay (0v\b{eta}\b{eta}) is considered the best potential resource to access the absolute neutrino mass scale. Moreover, if observed, it will signal that neutrinos are their own anti-particles (Majorana particles). Presently, this physics case is one of the most important research "beyond Standard Model" and might guide the way towards a Grand Unified Theory of fundamental interactions. Since the 0v\b{eta}\b{eta} decay process involves nuclei, its analysis necessarily implies nuclear structure issues. In the NURE project, supported by a Starting Grant of the European Research Council (ERC), nuclear reactions of double charge-exchange (DCE) are used as a tool to extr…

double-beta decay: neutrinolessNuclear reactionHistoryParticle physicsdouble beta decayFOS: Physical sciencesnucleus: structure function[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]nuclear reaction7. Clean energy01 natural sciencesQUADRUPOLE MAGNETSEducationStandard Modelnucleus: productionPhysics and Astronomy (all)mass: scaleydinreaktiotFIELD MEASUREMENTdouble-beta decay: (0neutrino)Double beta decay0103 physical sciencesGrand Unified Theorystructureneutrino: massNuclear Experiment (nucl-ex)Nuclear Experiment010306 general physicsDETECTORNuclear ExperimentPhysicsoperator: transition010308 nuclear & particles physicsparticle: MajoranaOrder (ring theory)semileptonic decaycharge exchangeantiparticleComputer Science ApplicationsMAGNEX SPECTROMETER* Automatic Keywords *MAJORANAgrand unified theoryMAGNEX SPECTROMETER QUADRUPOLE MAGNETS FIELD MEASUREMENT DETECTOR.upgradeHigh Energy Physics::ExperimentProduction (computer science)NeutrinoJournal of Physics: Conference Series
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Deeply virtual compton scattering off the neutron.

2007

The present experiment exploits the interference between the Deeply Virtual Compton Scattering (DVCS) and the Bethe-Heitler processes to extract the imaginary part of DVCS amplitudes on the neutron and on the deuteron from the helicity-dependent D$({\vec e},e'\gamma)X$ cross section measured at $Q^2$=1.9 GeV$^2$ and $x_B$=0.36. We extract a linear combination of generalized parton distributions (GPDs) particularly sensitive to $E_q$, the least constrained GPD. A model dependent constraint on the contribution of the up and down quarks to the nucleon spin is deduced.

QuarkPhysicsParticle physicsPhoton010308 nuclear & particles physicsScatteringHigh Energy Physics::PhenomenologyNuclear TheoryCompton scatteringFOS: Physical sciencesGeneral Physics and AstronomyVirtual particleParton[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesNuclear physicsIsospin0103 physical sciences25.30.-c 13.60.Fz 13.85.Hd 14.20.DhHigh Energy Physics::ExperimentNuclear Experiment (nucl-ex)010306 general physicsNucleonNuclear ExperimentNuclear ExperimentPhysical review letters
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First search for neutrinos in correlation with gamma-ray bursts with the ANTARES neutrino telescope

2013

A search for neutrino-induced muons in correlation with a selection of 40 gamma-ray bursts that occurred in 2007 has been performed with the ANTARES neutrino telescope. During that period, the detector consisted of 5 detection lines. The ANTARES neutrino telescope is sensitive to TeV-PeV neutrinos that are predicted from gamma-ray bursts. No events were found in correlation with the prompt photon emission of the gamma-ray bursts and upper limits have been placed on the flux and fluence of neutrinos for different models.

AstrofísicaFLUX[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]neutrino experiments; neutrino astronomy; gamma ray bursts theoryPOINT SOURCESPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaREDSHIFTFluxFOS: Physical sciencesAstrophysics01 natural sciencesICECUBEneutrino astronomyneutrino experiments0103 physical sciencesgamma ray bursts theory010303 astronomy & astrophysicsNeutrino experimentsATMOSPHERIC MUONSPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)MuonGamma ray bursts theory010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]High Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsAstronomygamma ray bursts theory; neutrino astronomy; neutrino experimentsAstronomy and Astrophysicsgamma ray burstsCATALOGRedshiftNeutrino detectorNeutrino astronomyFISICA APLICADAneutrino experimentHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical PhenomenaGamma-ray burstSYSTEM
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Performance of the First ANTARES Detector Line

2009

In this paper we report on the data recorded with the first Antares detector line. The line was deployed on the 14th of February 2006 and was connected to the readout two weeks later. Environmental data for one and a half years of running are shown. Measurements of atmospheric muons from data taken from selected runs during the first six months of operation are presented. Performance figures in terms of time residuals and angular resolution are given. Finally the angular distribution of atmospheric muons is presented and from this the depth profile of the muon intensity is derived.

MODULEPhysics::Instrumentation and DetectorsFOS: Physical sciencesAstrophysics01 natural sciencesNuclear physicsNEUTRINO TELESCOPESAngular distributionantares; deep-sea; first line; neutrino0103 physical sciencesNeutrino[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]WATERAngular resolutionNEUTRINO TELESCOPE010306 general physicsATMOSPHERIC MUONSAstroparticle physicsPhysicsMuonANTARES010308 nuclear & particles physicsAstrophysics (astro-ph)DetectorDeep-seaAstronomy and AstrophysicsTime resolutionGeodesyMUON FLUXFirst lineSINGLEFísica nuclearUNDERWATER DETECTORLine (text file)NeutrinoSYSTEM
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