0000000001315018

AUTHOR

A. Ferrero

showing 63 related works from this author

HΛ3 and H‾Λ¯3 production in Pb–Pb collisions at sNN=2.76 TeV

2019

Abstract The production of the hypertriton nuclei H Λ 3 and H ‾ Λ ¯ 3 has been measured for the first time in Pb–Pb collisions at s NN = 2.76  TeV with the ALICE experiment at LHC. The p T -integrated H Λ 3 yield in one unity of rapidity, d N / d y × B . R . ( H Λ 3 → He 3 , π − ) = ( 3.86 ± 0.77 ( stat. ) ± 0.68 ( syst. ) ) × 10 − 5 in the 0–10% most central collisions, is consistent with the predictions from a statistical thermal model using the same temperature as for the light hadrons. The coalescence parameter B 3 shows a dependence on the transverse momentum, similar to the B 2 of deuterons and the B 3 of 3He nuclei. The ratio of yields S 3 = H Λ 3 / ( He 3 × Λ / p ) was measured to b…

PhysicsNuclear and High Energy PhysicsLarge Hadron Collider010308 nuclear & particles physicsNuclear TheoryHadron7. Clean energy01 natural sciencesExponential functionBaryonNuclear physicsHigh energy nuclear physicsDeuterium0103 physical sciencesMass spectrumHigh Energy Physics::ExperimentRapidityImpact parameterNuclear Experiment010306 general physicsGlauberHypertritonPhysics Letters B
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Search for muoproduction of X(3872) at COMPASS and indication of a new state X˜(3872)

2018

Abstract We have searched for exclusive production of exotic charmonia in the reaction μ + N → μ + ( J / ψ π + π − ) π ± N ′ using COMPASS data collected with incoming muons of 160 GeV/c and 200 GeV/c momentum. In the J / ψ π + π − mass distribution we observe a signal with a statistical significance of 4.1 σ. Its mass and width are consistent with those of the X ( 3872 ) . The shape of the π + π − mass distribution from the observed decay into J / ψ π + π − shows disagreement with previous observations for X ( 3872 ) . The observed signal may be interpreted as a possible evidence of a new charmonium state. It could be associated with a neutral partner of X ( 3872 ) with C = − 1 predicted b…

PhysicsNuclear and High Energy PhysicsMuonMass distribution010308 nuclear & particles physicsBranching fractionHadronState (functional analysis)01 natural sciencesMomentum0103 physical sciencesTetraquarkAtomic physics010306 general physicsX(3872)Physics Letters B
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Measurement of the energy spectrum of cosmic rays above 10^18 eV using the Pierre Auger Observatory

2010

We report a measurement of the flux of cosmic rays with unprecedented precision and Statistics using the Pierre Auger Observatory Based on fluorescence observations in coincidence with at least one Surface detector we derive a spectrum for energies above 10(18) eV We also update the previously published energy spectrum obtained with the surface detector array The two spectra are combined addressing the systematic uncertainties and, in particular. the influence of the energy resolution on the spectral shape The spectrum can be described by a broken power law E-gamma with index gamma = 3 3 below the ankle which is measured at log(10)(E-ankle/eV) = 18 6 Above the ankle the spectrum is describe…

Nuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Radiación CósmicaAstronomyAstrophysics::High Energy Astrophysical Phenomenaenergy spectrumFluxFOS: Physical sciencesCosmic rayAstrophysicsElectronSURFACE DETECTORUPPER LIMITENERGIAPHOTON FRACTION01 natural sciencesSpectral lineAugerNuclear physicscosmic raysObservatorySHOWERS0103 physical sciencesHigh-Energy Cosmic Ray010306 general physicsCosmic raysCiencias ExactasPhysicsPierre Auger ObservatoryHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Spectral densityFísicaPierre Auger ObservatoryCosmic rayELECTRONS3. Good healthPierre Auger Observatory; Cosmic rays; Energy spectrumSIMULATIONExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFluorescenciaARRAYFísica nuclearEnergy spectrumAstrophysics - High Energy Astrophysical PhenomenaSYSTEM
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Search for exclusive photoproduction ofZc±(3900) at COMPASS

2015

A search for the exclusive production of the Z(c)(+/-)(3900) hadron by virtual photons has been performed in the channel Z(c)(+/-)(3900). J/Psi pi(+/-). The data cover the range from 7GeV to 19GeV in the centre-of- mass energy of the photon-nucleon system. The full set of the COMPASS data set collected with a muon beam between 2002 and 2011 has been used. An upper limit for the ratio BR(Z(c)(+/-)(3900)-> J/Psi pi(+/-)) x sigma(gamma N) -> Z(c)(+/-)(3900) N/sigma gamma N -> J/Psi N 3.7 x10(-3) has been established at the confidence level of90%. (C) 2015 The Authors. Published by Elsevier B.V.

PhysicsNuclear and High Energy PhysicsParticle physicsMuonCompassHadronAnalytical chemistrySigmaHigh Energy Physics::ExperimentProduction (computer science)TetraquarkZc(3900)Range (computer programming)Physics Letters B
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Read-out electronics for fast photon detection with COMPASS RICH-1

2008

A new read-out electronics system has been developed for the fast photon detection of the central region of the COMPASS RICH-1. The project is based on multi-anode photomultipliers read out by the high-sensitivity MAD4 preamplifier-discriminator and the dead-time free F1 TDC chip characterised by high time resolution. The system has been designed taking into account the high photon flux in the central region of the detector and the high rate requirement of the COMPASS experiment. The system is described in detail together with the measured performances. The new electronics system has been installed and used for the 2006 data taking; it entirely fulfils the expected performances.

PhysicsNuclear and High Energy PhysicsPhotomultiplierbusiness.industryDetectorChipParticle identificationOpticsCompassCOMPASS experimentElectronicsbusinessInstrumentationPhoton detection
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Spin alignment and violation of the OZI rule in exclusive ω and ϕ production in pp collisions

2014

Exclusive production of the isoscalar vector mesons $\omega$ and $\phi$ is measured with a 190 GeV$/c$ proton beam impinging on a liquid hydrogen target. Cross section ratios are determined in three intervals of the Feynman variable $x_{F}$ of the fast proton. A significant violation of the OZI rule is found, confirming earlier findings. Its kinematic dependence on $x_{F}$ and on the invariant mass $M_{p\mathrm{V}}$ of the system formed by fast proton $p_\mathrm{fast}$ and vector meson $V$ is discussed in terms of diffractive production of $p_\mathrm{fast}V$ resonances in competition with central production. The measurement of the spin density matrix element $\rho_{00}$ of the vector mesons…

Particle physicsNuclear and High Energy PhysicsOZI rule testPOLARIZATIONProtonMesonPROTON-PROTON COLLISIONS; LOW-ENERGY PHOTOPRODUCTION; ZWEIG-IIZUKA RULE; MESON PRODUCTION; EXPERIMENTAL TESTS; SELECTION RULE; POLARIZATION; NUCLEON; PIONIsoscalarPROTON-PROTON COLLISIONSMESON PRODUCTIONNuclear TheoryEXPERIMENTAL TESTS530OZI ruleHigh Energy Physics - ExperimentNuclear physicstestPIONInvariant masslcsh:Nuclear and particle physics. Atomic energy. RadioactivityLOW-ENERGY PHOTOPRODUCTIONVector mesonNuclear ExperimentNUCLEONNuclear ExperimentSpin-½PhysicsHigh Energy Physics::PhenomenologySELECTION RULEBaryonOZI ruleZWEIG-IIZUKA RULElcsh:QC770-798High Energy Physics::ExperimentParticle Physics - Experiment
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Measurements of the T2K neutrino beam properties using the INGRID on-axis near detector

2012

Precise measurement of neutrino beam direction and intensity was achieved based on a new concept with modularized neutrino detectors. INGRID (Interactive Neutrino GRID) is an on-axis near detector for the T2K long baseline neutrino oscillation experiment. INGRID consists of 16 identical modules arranged in horizontal and vertical arrays around the beam center. The module has a sandwich structure of iron target plates and scintillator trackers. INGRID directly monitors the muon neutrino beam profile center and intensity using the number of observed neutrino events in each module. The neutrino beam direction is measured with accuracy better than 0.4 mrad from the measured profile center. The …

Nuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsNeutrino oscillationPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical Phenomenaon-axis near detectorFOS: Physical sciencesddc:500.201 natural sciences7. Clean energyNeutrino oscillation; on-axis near detectorneutrino oscillation; neutrino detector; wavelength shifting fiber; t2k; extruded scintillator; neutrino beamNeutrino detectorNuclear physicsNeutrino beamneutrino beam0103 physical sciencesExtruded scintillatorMuon neutrinoneutrino oscillation[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationInstrumentationT2KPhysicst2k010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyNeutrino oscillation; T2K; Neutrino beam; Neutrino detector; Extruded scintillator; Wavelength shifting fiberT2K experimentextruded scintillatorFísicaInstrumentation and Detectors (physics.ins-det)Neutrino detectorneutrino detectorWavelength shiftingfiberMeasurements of neutrino speedPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNeutrinoBeam (structure)Leptonwavelength shifting fiber
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Onset of nuclear vaporization inAu197+197Au collisions

1993

Multifragmentation has been measured for [sup 197]Au+[sup 197]Au collisions at [ital E]/[ital A]=100, 250, and 400 MeV. The mean fragment multiplicity increases monotonically with the charged particle multiplicity at [ital E]/[ital A]=100 MeV, but decreases for central collisions with incident energy, consistent with the onset of nuclear vaporization. Molecular dynamics calculations follow some trends but underpredict the observed fragment multiplicities. Including the statistical decay of excited residues improves the agreement for peripheral collisions but worsens it for central collisions.

PhysicsNuclear physicsNuclear reactionComputer Science::Information RetrievalExcited stateVaporizationGeneral Physics and AstronomyIncident energyMultiplicity (mathematics)Nuclear ExperimentCharged particlePhysical Review Letters
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The fast photon detection system of COMPASS RICH-1

2007

Abstract A fast photon detection system has been built for the upgrade of COMPASS RICH-1, the large size gaseous RICH detector in use at the COMPASS Experiment at the CERN SPS since 2001. The photon detectors of the central region have been replaced by a new system based on multi-anode photomultipliers coupled to individual fused silica lens telescopes and a fast readout electronics system, while in the outer region the existing MWPCs with CsI photocathodes have been equipped with a new readout system, based on the APV chip. RICH-1 has been successfully operated in its upgraded version during the 2006 run. We report on the upgrade design and construction, and on the preliminary characteriza…

PhotomultiplierNuclear and High Energy PhysicsPhotonMulti-anode photomultiplier tubesPhysics::Instrumentation and DetectorsUV lensesCOMPASS; Multi-anode photomultiplier tubes; Photon detection; RICH; UV lenses; Nuclear and High Energy Physics; InstrumentationCOMPASSlaw.inventionFAST-RICH; DEUTERON; READOUT; DESIGNOpticsDESIGNlawMulti-anode photomultiplier tubeCompassCOMPASS experimentRICHInstrumentationNuclear and High Energy PhysicPhysicsLarge Hadron Colliderbusiness.industryDetectorREADOUTDEUTERONLens (optics)UpgradePhoton detectionFAST-RICHUV lenseHigh Energy Physics::Experimentbusiness
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Pattern recognition and PID for COMPASS RICH-1

2008

A package for pattern recognition and PID by COMPASS RICH-1 has been developed and used for the analysis of COMPASS data collected in the years 2002 to 2004, and 2006-2007 with the upgraded RICH-1 photon detectors. It has allowed the full characterization of the detector in the starting version and in the upgraded one, as well as the PID for physics results. We report about the package structure and algorithms, and the detector characterization and PID results.

PhysicsNuclear and High Energy PhysicsPhotomultiplierPhysics - Instrumentation and Detectorsbusiness.industryPhoton detectorDetectorPID controllerFOS: Physical sciencesPattern recognitionInstrumentation and Detectors (physics.ins-det)Photon yieldParticle identificationHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)CompassPattern recognition (psychology)Artificial intelligenceDetectors and Experimental TechniquesbusinessInstrumentation
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Design and status of COMPASS FAST-RICH

2006

In the context of the upgrade of COMPASS RICH-1, we are developing a fast photodetection system for RICH counters, based on UV extended Multi-Anode PhotoMultiplier Tubes (MAPMT) and a custom, low dead-time electronic readout system. Photons are concentrated on the MAPMT photocathode by an optical system that preserves the position information. The ratio between the collection and the photosensitive surfaces is ∼7.5 in our design, larger than in previous applications. A new front-end electronics, based on a modified version of the MAD4 discriminator chip, is being realized to digitize the MAPMT signals. We report about the design of the photodetection system and of the associated electronic …

PhysicsNuclear and High Energy PhysicsPhotomultiplierbusiness.industryContext (language use)PhotodetectionChipPhotocathodeOpticsUpgradeCompassElectronicsbusinessInstrumentation
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Fragment Flow and the Multifragmentation Phase Space

1995

Fragment distributions have been measured for Au+Au collisions at [ital E]/[ital A]=100 and 1000 MeV. A high detection efficiency for fragments was obtained by combining the ALADIN spectrometer and the MSU-Miniball/WU-Miniwall array. At both energies the maximum multiplicity of intermediate mass fragments (IMF) normalized to the size of the decaying system is about one IMF per 30 nucleons but the element distributions show significant differences. Within a coalescence picture the suppression of heavy fragments in central collisions at [ital E]/[ital A]=100 MeV may be related to a reduction of the density in momentum space which is caused by the collective expansion.

Nuclear reactionCoalescence (physics)PhysicsSpectrometer[PHYS.NEXP] Physics [physics]/Nuclear Experiment [nucl-ex]Computer Science::Information RetrievalGeneral Physics and AstronomyPosition and momentum space[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Space (mathematics)Nuclear physicsPhase spaceMultiplicity (chemistry)Atomic physicsNuclear ExperimentNucleonPhysical Review Letters
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The Lateral Trigger Probability function for the Ultra-High Energy Cosmic Ray Showers detected by the Pierre Auger Observatory

2011

In this paper we introduce the concept of Lateral Trigger Probability (LTP) function, i.e., the probability for an Extensive Air Shower (EAS) to trigger an individual detector of a ground based array as a function of distance to the shower axis, taking into account energy, mass and direction of the primary cosmic ray. We apply this concept to the surface array of the Pierre Auger Observatory consisting of a 1.5 km spaced grid of about 1600 water Cherenkov stations. Using Monte Carlo simulations of ultra-high energy showers the LTP functions are derived for energies in the range between 1017 and 1019 eV and zenith angles up to 65. A parametrization combining a step function with an exponenti…

[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]AstronomyAstrophysics::High Energy Astrophysical PhenomenaExtensive air showerUltra-high Energy Cosmic RayMonte Carlo methodFOS: Physical sciencesCosmic rayEXTENSIVE AIR-SHOWERSTrigger performance01 natural sciences7. Clean energyUltra-high Energy Cosmic Rays; Pierre Auger Observatory; Extensive air showers; Trigger performance; Surface detector; Hybrid detectorHigh Energy Physics - ExperimentAugerNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesUltra-high-energy cosmic ray010303 astronomy & astrophysicsCiencias ExactasZenithCherenkov radiationUltra-High Energy Cosmic RaysPhysicsPierre Auger ObservatoryHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsPhysicsHybrid detector[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Surface detectorAstrophysics::Instrumentation and Methods for AstrophysicsFísicaAstronomy and AstrophysicsPierre Auger ObservatoryUltra-high Energy Cosmic Rays[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Air showerExperimental High Energy PhysicsSIMULATIONComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearExtensive Air ShowersAstrophysics - High Energy Astrophysical PhenomenaRAIOS CÓSMICOS
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Particle identification with COMPASS RICH-1

2011

International audience; RICH-1 is a large size RICH detector in operation at the COMPASS experiment since 2001 and recently upgraded implementing a new photon detection system with increased performance.A dedicated software package has been developed to perform RICH-1 data reduction, pattern recognition and particle identification as well as a number of accessory tasks for detector studies.The software package, the algorithms implemented and the detector characterisation and performance are reported in detail.

Nuclear and High Energy PhysicsPhysics::Instrumentation and Detectors[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesCOMPASSParticle identificationParticle identificationCompass0103 physical sciencesCOMPASS experimentComputer vision010306 general physicsInstrumentationRICHPhysics010308 nuclear & particles physicsbusiness.industryDetectorSoftware packageParticle identification; COMPASS; Likelihood algorithmsPattern recognition (psychology)High Energy Physics::ExperimentArtificial intelligenceLikelihood algorithmsbusinessPhoton detectionData reduction
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First measurement of the |t|-dependence of coherent J/ψ photonuclear production

2021

The first measurement of the dependence on $|t|$, the square of the momentum transferred between the incoming and outgoing target nucleus, of coherent J/ψ photoproduction is presented. The data were measured with the ALICE detector in ultra-peripheral Pb-Pb collisions at a centre-of-mass energy per nucleon pair $\sqrt{s_{\rm NN}} = 5.02$ TeV with the J/$\psi$ produced in the central rapidity region $|y| < 0.8$, which corresponds to the small Bjorken-$x$ range $(0.3 − 1.4) \times 10 ^{−3}$. The measured $|t|$-dependence is not described by computations based only on the Pb nuclear form factor, while the photonuclear cross section is better reproduced by models including shadowing according t…

heavy ion: scatteringnucleon: pairVDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Kjerne- og elementærpartikkelfysikk: 431nucl-ex01 natural sciencesSquare (algebra)ALICEJ/psi(3100): photoproduction[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentQuantum chromodynamicsPhysicsPhysicsForm factor (quantum field theory)ultra-peripheral collisionsdependence [impact parameter]J/psi ALICE Pb-Pb collisionsBalitsky-Kovchegov equationQuarkoniumddc:3. Good healthPHOTOPRODUCTIONshadowingNucleonParticle Physics - ExperimentPB-PB COLLISIONSNuclear and High Energy PhysicsQC1-999nucleus: form factor[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]MomentumNuclear physicsPHYSICSCross section (physics)heavy-ion collisions ultra-peripheral collisions quarkoniaphotoproduction [J/psi(3100)]scattering [heavy ion]0103 physical sciencesNuclear Physics - Experimentddc:530Rapidity5020 GeV-cms/nucleonHeavy Ion experiments010306 general physicsimpact parameter: dependencehep-ex010308 nuclear & particles physicsnucleus: targetpair [nucleon]photonuclear productionheavy-ion collisionsquarkoniaform factor [nucleus]PB-PB COLLISIONS; PHOTOPRODUCTION; PHYSICStarget [nucleus]J/PsicoherenceJ/psi(3100): photoproduction ; impact parameter: dependence ; nucleus: form factor ; nucleus: target ; nucleon: pair ; heavy ion: scattering ; coherence ; Balitsky-Kovchegov equation ; shadowing ; rapidity ; ALICE ; experimental results ; 5020 GeV-cms/nucleonrapidityphotonuclear production J/Psi Pb-Pb collisionsHigh Energy Physics::Experimentexperimental results
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The fast readout system for the MAPMTs of COMPASS RICH-1

2007

A fast readout system for the upgrade of the COMPASS RICH detector has been developed and successfully used for data taking in 2006 and 2007. The new readout system for the multi-anode PMTs in the central part of the photon detector of the RICH is based on the high-sensitivity MAD4 preamplifier-discriminator and the dead-time free F1-TDC chip characterized by high-resolution. The readout electronics has been designed taking into account the high photon flux in the central part of the detector and the requirement to run at high trigger rates of up to 100 kHz with negligible dead-time. The system is designed as a very compact setup and is mounted directly behind the multi-anode photomultiplie…

PhysicsNuclear and High Energy PhysicsPhotomultiplierPhysics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorsbusiness.industryDetectorPhoton fluxFOS: Physical sciencesReadout electronicsInstrumentation and Detectors (physics.ins-det)ChipParticle identificationUpgradeOpticsCompassDetectors and Experimental TechniquesbusinessInstrumentationNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Limit on the diffuse flux of ultrahigh energy tau neutrinos with the surface detector of the Pierre Auger Observatory

2009

Data collected at the Pierre Auger Observatory are used to establish an upper limit on the diffuse flux of tau neutrinos in the cosmic radiation. Earth-skimming ντ may interact in the Earth's crust and produce a τ lepton by means of charged-current interactions. The τ lepton may emerge from the Earth and decay in the atmosphere to produce a nearly horizontal shower with a typical signature, a persistent electromagnetic component even at very large atmospheric depths. The search procedure to select events induced by τ decays against the background of normal showers induced by cosmic rays is described. The method used to compute the exposure for a detector continuously growing with time is de…

ACTIVE GALACTIC NUCLEIASTROPHYSICS[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Nuclear and High Energy PhysicsActive galactic nucleusPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayPROPAGATIONAstrophysics7. Clean energy01 natural sciencesLeptonSpectral lineSettore FIS/04 - Fisica Nucleare e SubnucleareAugerSEARCHTau neutrino0103 physical sciencesTau neutrinoOSCILLATIONS010306 general physicsCiencias ExactasHigh Energy Astrophysical Phenomena (astro-ph.HE)AIR-SHOWERSPierre Auger ObservatoryPhysicsSPECTRUM010308 nuclear & particles physicsPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsFísicaultrahigh energy cosmic rays ; tau neutrinos ; Pierre Auger ObservatoryDiffuse fluxPierre Auger ObservatoryPERFORMANCECOSMIC-RAYScosmic radiation13. Climate actionTELESCOPESHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaLeptonPhysical Review D
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The helminth community of the skink Chalcides sexlineatus from Gran Canaria (Canary Islands).

2012

AbstractA survey of the gastrointestinal helminth communities of a population of Chalcides sexlineatus Steindachner, a small skink endemic to Gran Canaria island (Canary Archipelago, Spain), was conducted to determine the prevalence, abundance and species diversity of intestinal parasites in these reptiles. Only three parasite species were found, one cestode, Oochoristica agamae Baylis, 1919 and two nematodes, Parapharyngodon micipsae (Seurat, 1917) and Pharyngodonidae gen. sp. Helminth infracommunities of C. sexlineatus showed low values of abundance and species richness and diversity, being more similar to the helminth community of Tarentola boettgeri boettgeri (Steindachner) rather than …

SkinkMaleeducation.field_of_studybiologyEcologyPopulationBiodiversitySpecies diversityGeneral MedicineBiodiversitybiology.organism_classificationGastrointestinal TractAbundance (ecology)SpainHelminthsTarentola boettgeriHelminthsAnimalsAnimal Science and ZoologyParasitologyFemaleSpecies richnesseducationChordataJournal of helminthology
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Search for signatures of magnetically-induced alignment in the arrival directions measured by the Pierre Auger Observatory

2011

We present the results of an analysis of data recorded at the Pierre Auger Observatory in which we search for groups of directionally-aligned events (or ‘multiplets’) which exhibit a correlation between arrival direc- tion and the inverse of the energy. These signatures are expected from sets of events coming from the same source after having been deflected by intervening coherent magnetic fields. The observation of several events from the same source would open the possibility to accurately reconstruct the position of the source and also measure the integral of the component of the magnetic field orthogonal to the trajectory of the cos- mic rays. We describe the largest multiplets found an…

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Field (physics)Astronomyultra-high energy cosmic rays; Pierre Auger Observatory; arrival directionsFOS: Physical sciencesCosmic rayAstrophysics01 natural sciencesCosmic RayAugerPosition (vector)0103 physical sciencesFIELDPierre auger observatory010303 astronomy & astrophysicsUltra-high energy cosmic rayDETECTORCiencias ExactasHigh Energy Astrophysical Phenomena (astro-ph.HE)Pierre Auger ObservatoryPhysicsArrival directions010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhysicsIsotropyFísicaAstronomy and AstrophysicsASTROFÍSICAUltra-high energy cosmic raysMagnetic fieldExperimental High Energy PhysicsData analysisComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]RAIOS CÓSMICOSArrival directionUltra-High Energy Cosmic Ray
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Measurement of the Proton-Air Cross Section ats=57  TeVwith the Pierre Auger Observatory

2012

We report a measurement of the proton-air cross section for particle production at the center-of-mass energy per nucleon of 57 TeV. This is derived from the distribution of the depths of shower maxima observed with the Pierre Auger Observatory: systematic uncertainties are studied in detail. Analyzing the tail of the distribution of the shower maxima, a proton-air cross section of [505 +/- 22(stat)(-36)(+28)(syst)] mb is found.

Pierre Auger ObservatoryPhysicsProton010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaHadronAstrophysics::Instrumentation and Methods for AstrophysicsGeneral Physics and Astronomy01 natural scienceslaw.inventionAugerNuclear physicsCross section (physics)law0103 physical sciencesHigh Energy Physics::ExperimentFermilabNuclear Experiment010306 general physicsNucleonColliderPhysical Review Letters
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Real-time data processing in the ALICE High Level Trigger at the LHC

2019

At the Large Hadron Collider at CERN in Geneva, Switzerland, atomic nuclei are collided at ultra-relativistic energies. Many final-state particles are produced in each collision and their properties are measured by the ALICE detector. The detector signals induced by the produced particles are digitized leading to data rates that are in excess of 48 GB/$s$. The ALICE High Level Trigger (HLT) system pioneered the use of FPGA- and GPU-based algorithms to reconstruct charged-particle trajectories and reduce the data size in real time. The results of the reconstruction of the collision events, available online, are used for high level data quality and detector-performance monitoring and real-tim…

calibration ; ALICE ; trigger ; monitoring ; quality ; data management ; programming ; FPGA ; multiprocessor: graphics ; performancePhysics - Instrumentation and DetectorsHigh level triggerPhysics::Instrumentation and DetectorsLevel datatutkimuslaitteetFPGA; GPUDetector calibrationGPUFOS: Physical sciencesGeneral Physics and AstronomyhiukkasfysiikkaPhysics and Astronomy(all)01 natural sciencesprogramming010305 fluids & plasmasCombinatoricsALICE0103 physical sciencesmultiprocessor: graphics[INFO]Computer Science [cs][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Detectors and Experimental Techniques010306 general physicsNuclear Experimentphysics.ins-detFPGAcomputer.programming_languagePhysicsLarge Hadron ColliderFPGA; GPU; TRACKsignaalinkäsittelyInstrumentation and Detectors (physics.ins-det)triggercalibrationmonitoringdatailmaisimetqualityHardware and ArchitectureTRACKHigh Energy Physics::Experimentdata managementAlice (programming language)computerperformance
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First Measurement of Transverse-Spin-Dependent Azimuthal Asymmetries in the Drell-Yan Process

2017

The first measurement of transverse-spin-dependent azimuthal asymmetries in the pion-induced Drell-Yan (DY) process is reported. We use the CERN SPS 190 GeV/$c$, $\pi^{-}$ beam and a transversely polarized ammonia target. Three azimuthal asymmetries giving access to different transverse-momentum-dependent (TMD) parton distribution functions (PDFs) are extracted using dimuon events with invariant mass between 4.3 GeV/$c^2$ and 8.5 GeV/$c^2$. The observed sign of the Sivers asymmetry is found to be consistent with the fundamental prediction of Quantum Chromodynamics (QCD) that the Sivers TMD PDFs extracted from DY have a sign opposite to the one extracted from semi-inclusive deep-inelastic sc…

Drell-Yan process550ComputerSystemsOrganization_COMPUTERSYSTEMIMPLEMENTATIONNuclear TheoryGeneral Physics and Astronomyparton: distribution functiontransverse momentum dependence01 natural sciencesCOMPASSHigh Energy Physics - ExperimentSivers functionHigh Energy Physics - Experiment (hep-ex)semi-inclusive reaction [deep inelastic scattering]High Energy Physics - Phenomenology (hep-ph)ddc:550[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimenttransversityPhysicsQuantum chromodynamics(muon+ muon-) [mass spectrum]Large Hadron Colliderdeep inelastic scattering: semi-inclusive reactionpolarized target: transverse190 GeV/ctransverse [polarized target]nucleonDrell–Yan processhep-phdimuon: mass spectrumAzimuthHigh Energy Physics - PhenomenologyTransverse planeasymmetry [angular distribution]pi- nucleus: scatteringmass spectrum [dimuon]distribution function [parton]Nucleonspin: asymmetryParticle Physics - ExperimentParticle physicsangular distribution: asymmetryscattering [pi- nucleus]ComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONFOS: Physical sciencesComputerApplications_COMPUTERSINOTHERSYSTEMSAccelerator Physics and InstrumentationGeneralLiterature_MISCELLANEOUSNuclear physicsPhysics and Astronomy (all)[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciencesquantum chromodynamicsuniversality010306 general physicsParticle Physics - Phenomenology010308 nuclear & particles physicshep-exHigh Energy Physics::PhenomenologyAcceleratorfysik och instrumenteringCERN SPSmass spectrum: (muon+ muon-)ComputingMethodologies_PATTERNRECOGNITION[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Physics::Accelerator Physics[ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::Experimentasymmetry [spin]experimental results
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Search for a common baryon source in high-multiplicity pp collisions at the LHC

2020

Physics letters / B B811, 135849 (2020). doi:10.1016/j.physletb.2020.135849

:Kjerne- og elementærpartikkelfysikk: 431 [VDP]HadronHadron - hadron reactionHEAVY-ION COLLISIONSHigh multiplicityhiukkasfysiikkanucl-exdecay [resonance]01 natural sciencesHigh Energy Physics - ExperimentExperimentHigh Energy Physics - Experiment (hep-ex)hadron–hadron interactions LHC ALICEBarions; strong interaction; LHCALICEstrong resonance decayIonic Collisionsscattering [p p][PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear Experiment (nucl-ex)Nuclear ExperimentNuclear ExperimentBarionsPION INTERFEROMETRYhadron-hadron scatteringPhysicsLarge Hadron ColliderMesonsHadron - hadron reactionsmass: transversestrong interactionPhysicsbaryon correlations ; invariant radius ; strong hadron–hadron interactions ; strong resonance decayVDP::Kjerne- og elementærpartikkelfysikk: 431RadiusAU+AUInvariant (physics)lcsh:QC1-999quark gluon plasmaPRIRODNE ZNANOSTI. Fizika.HEAVY-ION COLLISIONS; PION INTERFEROMETRY; SIGMA(0) PRODUCTION; AU+AU; COLLISIONS; FEMTOSCOPY; SYSTEMS; PB:Nuclear and elementary particle physics: 431 [VDP]CERN LHC CollVDP::Nuclear and elementary particle physics: 431Transverse massLHCPBParticle Physics - Experimentbaryon correlationsCOLLISIONSNuclear and High Energy Physicsp p: scatteringHigh Energy Physics; ExperimentcollectiveFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]530114 Physical sciencesNuclear physicsHadron - hadron reactions; LHCbaryon baryon: correlationSYSTEMSresonance: decay0103 physical sciencesfemtoscopyddc:530Nuclear Physics - ExperimentHigh Energy Physics010306 general physicshadron hadron: interactioninteraction [hadron hadron]010308 nuclear & particles physicshep-exhadron-hadron scattering ALICE experiment femtoscopySIGMA(0) PRODUCTIONHigh Energy Physics::PhenomenologyALICE experimentcorrelation [baryon baryon]Kaonsstrong hadron–hadron interactionsNATURAL SCIENCES. Physics.invariant radiusBaryonKaons; Ionic Collisions; Mesonstransverse [mass]Antiproton13000 GeV-cms/nucleonHigh Energy Physics::Experimentlcsh:Physicsexperimental results
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Particle identification with the fast COMPASS RICH-1 detector

2009

International audience; A new photon detection system for the COMPASS RICH-1 detector has been designed and installed. In the central region, the project is based on multi-anode photo-multiplier technology accompanied by charge sensitive, high resolution and dead-time free time digitization. In the outer area, only the readout electronics for the existing photon detectors has been replaced. Details on the detector upgrade and its performance are presented.

Nuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsPhoton detectorMulti-anode photo-multiplierComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONHigh resolution[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesCOMPASSParticle identificationTDCParticle identificationOpticsCompass0103 physical sciences010306 general physicsInstrumentationRICHPhysics010308 nuclear & particles physicsbusiness.industryDetectorCharge (physics)Front-end electronicsUpgradeCOMPASS; RICH; Multi-anode photo-multiplier; Particle identification; Front-end electronics; TDCHigh Energy Physics::ExperimentbusinessPhoton detectionFront-end electronic
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The Fluorescence Detector of the Pierre Auger Observatory

2010

The Pierre Auger Observatory is a hybrid detector for ultra-high energy cosmic rays. It combines a surface array to measure secondary particles at ground level together with a fluorescence detector to measure the development of air showers in the atmosphere above the array. The fluorescence detector comprises 24 large telescopes specialized for measuring the nitrogen fluorescence caused by charged particles of cosmic ray air showers. In this paper we describe the components of the fluorescence detector including its optical system, the design of the camera, the electronics, and the systems for relative and absolute calibration. We also discuss the operation and the monitoring of the detecto…

Physics::Instrumentation and DetectorsAstronomyAUGERPIERRE7. Clean energy01 natural sciencesAugerFluorescence detectorData acquisitionDEPENDENCEATMOSPHERIC MULTIPLE-SCATTERINGInstrumentationPhysicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsCOSMIC-RAYSUltra High Energy Cosmic RayCharged particleLIGHTSIMULATIONComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsAUGERNuclear and High Energy Physics[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaMeasure (physics)FOS: Physical sciencesCosmic rayEXTENSIVE AIR-SHOWERSENERGIAFluorescence spectroscopyOptics0103 physical sciencesCosmic rays; Fluorescence detectorRECONSTRUCTION010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Cosmic raysPierre Auger ObservatoryPIERRE010308 nuclear & particles physicsbusiness.industryFísicaULTRA-HIGH ENERGY[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Experimental High Energy PhysicsPierre Auger observatoryCAPABILITIESHigh Energy Physics::Experimentbusiness
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The spin-dependent structure function of the proton g1p and a test of the Bjorken sum rule

2010

Abstract The inclusive double-spin asymmetry, A 1 p , has been measured at COMPASS in deep-inelastic polarised muon scattering off a large polarised NH3 target. The data, collected in the year 2007, cover the range Q 2 > 1 ( GeV / c ) 2 , 0.004 x 0.7 and improve the statistical precision of g 1 p ( x ) by a factor of two in the region x 0.02 . The new proton asymmetries are combined with those previously published for the deuteron to extract the non-singlet spin-dependent structure function g 1 NS ( x , Q 2 ) . The isovector quark density, Δ q 3 ( x , Q 2 ) , is evaluated from a NLO QCD fit of g 1 NS . The first moment of Δ q 3 is in good agreement with the value predicted by the Bjorken su…

Quantum chromodynamicsPhysicsCoupling constantNuclear and High Energy PhysicsParticle physicsMuonIsovectorProton010308 nuclear & particles physicsDeep inelastic scattering01 natural sciencesNuclear physics0103 physical sciencesSum rule in quantum mechanics010306 general physicsSpin-½Physics Letters B
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Dielectron production in proton-proton and proton-lead collisions at √sNN=5.02TeV

2020

The first measurements of dielectron production at midrapidity (|ηe| &lt; 0.8) in proton–proton and proton–lead collisions at √sNN = 5.02 TeV at the LHC are presented. The dielectron cross section is measured with the ALICE detector as a function of the invariant mass mee and the pair transverse momentum pT, ee in the ranges mee &lt; 3.5 GeV/c2 and pT, ee &lt; 8 GeV/c, in both collision systems. In proton–proton collisions, the charm and beauty cross sections are determined at midrapidity from a fit to the data with two different event generators. This complements the existing dielectron measurements performed at √s = 7 and 13 TeV. The slope of the √s dependence of the three measurements is…

Nuclear and High Energy Physics:Kjerne- og elementærpartikkelfysikk: 431 [VDP]ProtonHadronNuclear Theorydielectrondielectron production01 natural sciences7. Clean energyNuclear physicshadron-ion interactionshadron-hadron collisions; dielectron production;Ionic Collisionsdielectron cross sectiondielectron nuclear modification factor0103 physical sciencesInvariant massDielectronCharm (quantum number)Dielectron; hadron-hadron interactions; hadron-ion interactionsPhysics::Atomic PhysicsIonic Collisions; Relativistic Heavy-ion Collisions; Quark-Gluon Plasma010306 general physicsNuclear ExperimentQuantum chromodynamicsPhysicsLarge Hadron Collider010308 nuclear & particles physicsPhysicsVDP::Kjerne- og elementærpartikkelfysikk: 431hadron-hadron interactionNuclear matterhadron-hadron collisionsNATURAL SCIENCES. Physics.ALICE LHC proton-lead collisions proton-proton collisionsPRIRODNE ZNANOSTI. Fizika.:Nuclear and elementary particle physics: 431 [VDP]VDP::Nuclear and elementary particle physics: 431dielectron ; LHC ; dielectron cross section ; dielectron nuclear modification factorQuark–gluon plasmaQuark-Gluon PlasmaHigh Energy Physics::ExperimentLHChadron-hadron interactionsRelativistic Heavy-ion Collisions
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The experience of building and operating COMPASS RICH-1

2010

COMPASS RICH-1 is a large size gaseous Imaging Cherenkov Detector providing hadron identification in the range from 3 to 55 GeV/c, in the wide acceptance spectrometer of the COMPASS Experiment at CERN SPS. It uses a 3 m long C(4)F(10) radiator, a 21 m(2) large VUV mirror surface and two kinds of photon detectors: MAPMTs and MWPCs with CsI photocathodes, covering a total of 5.5 m(2). It is in operation since 2002 and its performance has increased in time thanks to progressive optimization and mostly to a major upgrade which was implemented in 2006. The main characteristics of COMPASS RICH-1 components are described and some specific aspects related to the radiator gas system, the mirror alig…

Nuclear and High Energy PhysicsCherenkov detectorPhysics::Instrumentation and Detectors[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]COMPASS01 natural sciencesParticle identificationParticle identificationlaw.inventionNuclear physicsCOMPASS; CsI; MAPMT; Photon detection; PID; RICH; Instrumentation; Nuclear and High Energy PhysicsOpticslawCompass0103 physical sciencesCOMPASS experimentCsI photoconverter010306 general physicsRICHInstrumentationEvent reconstructionPhysicsLarge Hadron ColliderSpectrometer010308 nuclear & particles physicsbusiness.industryPIDUpgradePhoton detectionMAPMTCsIParticle identification; COMPASS; RICH; MAPMT; CsI photoconverterHigh Energy Physics::Experimentbusiness
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Flavour Separation of Helicity Distributions from Deep Inelastic Muon-Deuteron Scattering

2009

We present a LO evaluation of helicity densities of valence, \Delta u_v+\Delta d_v, non-strange sea, \Delta\bar{u}+\Delta\bar{d}, and strange quarks, \Delta s (assumed to be equal to \Delta\bar{s}). They have been obtained from the inclusive asymmetry A_{3,d} and the semi-inclusive asymmetries A^{\pi+}_{1,d}, A^{\pi-}_{1,d}, A^{K+}_{1,d}, A^{K-}_{1,d} measured in polarised deep inelastic muon-deuteron scattering. The full deuteron statistics of COMPASS (years 2002-2004 and 2006) has been used. The data cover the range Q^2 > 1 (GeV/c)^2 and 0.004<x<0.3. Both non-strange densities are found to be in a good agreement with previous measurements. The distribution of \Delta s(x) is compatible wit…

Strange quarkPOLARIZED TARGETNuclear TheoryVALENCE QUARK DISTRIBUTION; PARTON DISTRIBUTIONS; POLARIZED TARGET; NUCLEON; PROTON; DISPolarised DIS and SIDISPROTON01 natural sciencesCOMPASSParton distribution functionHigh Energy Physics - ExperimentCOMPASS; double-spin asymmetry; helicity density; parton distribution function; flavour sep- aration analysis; polarised DIS and SIDIS reactions; charged kaon asymmetrypolarised DIS and SIDIS reactionHigh Energy Physics - Experiment (hep-ex)Helicity densityVALENCE QUARK DISTRIBUTIONNUCLEONNuclear Experimentmedia_commonQuantum chromodynamicsPhysicsFlavour separation analysisHelicityCharged kaon asymmetryNucleondouble-spin asymmetryParticle Physics - Experimentcharged kaon asymmetryParticle physicsNuclear and High Energy Physicsreactionsflavour sep- aration analysismedia_common.quotation_subjectFOS: Physical sciencesparton distribution functionAsymmetryNuclear physics0103 physical sciencesflavour sep- aration analysiPolarised DIS and SIDIS reactions010306 general physicsfunctionDISMuonValence (chemistry)010308 nuclear & particles physicsScatteringParton distributionPARTON DISTRIBUTIONSHigh Energy Physics::Experimenthelicity densityDouble-spin asymmetry
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The COMPASS RICH-1 fast photon detection system

2008

Abstract A fast photon detection system has been built as a part of the upgrade of the COMPASS RICH-1 detector: it is based on 576 multi-anode photomultiplier tubes (MAPMTs) coupled to individual fused silica lens telescopes and fast readout electronics. This system has replaced the MWPCs with CsI photo-cathodes in the central region ( 1.3 m 2 , 25% of the total area) of the COMPASS RICH-1 photon detectors and has successfully been operated during the data taking in 2006 and 2007. We report about the fast photon detection system design, construction and commissioning, in particular about the design optimization and the validation tests of the lens telescopes. Preliminary values for the incr…

PhysicsNuclear and High Energy PhysicsPhotomultiplierPhysics::Instrumentation and Detectorsbusiness.industryPhoton detectorDetectorlaw.inventionLens (optics)OpticsUpgradelawCompassSystems designOptoelectronicsHigh Energy Physics::ExperimentbusinessInstrumentationPhoton detectionNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Indication of electron neutrino appearance from an accelerator-produced off-axis muon neutrino beam

2011

The T2K experiment observes indications of $\nu_\mu\rightarrow \nu_e$ appearance in data accumulated with $1.43\times10^{20}$ protons on target. Six events pass all selection criteria at the far detector. In a three-flavor neutrino oscillation scenario with $|\Delta m_{23}^2|=2.4\times10^{-3}$ eV$^2$, $\sin^2 2\theta_{23}=1$ and $\sin^2 2\theta_{13}=0$, the expected number of such events is 1.5$\pm$0.3(syst.). Under this hypothesis, the probability to observe six or more candidate events is 7$\times10^{-3}$, equivalent to 2.5$\sigma$ significance. At 90% C.L., the data are consistent with 0.03(0.04)$<\sin^2 2\theta_{13}<$ 0.28(0.34) for $\delta_{\rm CP}=0$ and a normal (inverted) hierarchy.

Particle physicsFOS: Physical sciencesGeneral Physics and Astronomyddc:500.2CHOOZ01 natural sciencesParticle identificationHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)neutrino14.60.Pq 13.15.+g 25.30.Pt 95.55.Vj0103 physical sciencesneutrino oscillationMuon neutrino[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)ComputingMilieux_MISCELLANEOUSPhysicsNOνATribimaximal mixinghep-ex010308 nuclear & particles physicsT2K experimentFísicaT2K Collaborationparticle identificationElectron neutrinoexperimental resultsPhysical Review Letters
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The Polarised Valence Quark Distribution from semi-inclusive DIS

2007

The semi-inclusive difference asymmetry A^{h^{+}-h^{-}} for hadrons of opposite charge has been measured by the COMPASS experiment at CERN. The data were collected in the years 2002-2004 using a 160 GeV polarised muon beam scattered off a large polarised ^6LiD target and cover the range 0.006 &lt; x &lt; 0.7 and 1 &lt; Q^2 &lt; 100 (GeV/c)^2. In leading order QCD (LO) the asymmetry A_d^{h^{+}-h^{-}} measures the valence quark polarisation and provides an evaluation of the first moment of Delta u_v + Delta d_v which is found to be equal to 0.40 +- 0.07 (stat.) +- 0.05 (syst.) over the measured range of x at Q^2 = 10 (GeV/c)^2. When combined with the first moment of g_1^d previously measured …

QuarkNuclear and High Energy PhysicsParticle physicsmagnetic spectrometer: COMPASSStructure functionsmedia_common.quotation_subjectHadronpolarization: longitudinalFOS: Physical sciencespolarized targetcross section: ratioDeep inelastic scattering; Structure functionsmuon deuteron: deep inelastic scattering01 natural sciencesAsymmetryx-dependenceHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)charged particle: multiple productionnegative particle: electroproductionExperiment-HEP13.88.+e0103 physical sciencesstructure function: moment010306 general physicsNuclear Experimentmedia_commonPhysicsQuantum chromodynamicsMuonValence (chemistry)010308 nuclear & particles physicsHigh Energy Physics::Phenomenologycross section: differenceCERN SPSDeep inelastic scatteringpositive particle: electroproductionDeuteriumquark: valenceHigh Energy Physics::Experimentmuon: polarized beamquark: polarization140-180 GeVspin: asymmetry13.60.HbDeep inelastic scatteringParticle Physics - Experimentexperimental results
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A study of the effect of molecular and aerosol conditions in the atmosphere on air fluorescence measurements at the Pierre Auger Observatory

2010

The air fluorescence detector of the Pierre Auger Observatory is designed to perforin calorimetric measurements of extensive air showers created by Cosmic rays of above 10(18) eV. To correct these measurements for the effects introduced by atmospheric fluctuations, the Observatory contains a group Of monitoring instruments to record atmospheric conditions across the detector site, ail area exceeding 3000 km(2). The atmospheric data are used extensively in the reconstruction of air showers, and are particularly important for the correct determination of shower energies and the depths of shower maxima. This paper contains a summary of the molecular and aerosol conditions measured at the Pierr…

Angstrom exponentAstronomyAstrophysics01 natural sciencesAugerCROSS-SECTIONSCOSMIC-RAY SHOWERSObservatoryDEPENDENCEHigh-Energy Cosmic Ray010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Lidar[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]ANGSTROM EXPONENTPierre Auger ObservatoryBi-static lidarELECTRONSComputingMethodologies_DOCUMENTANDTEXTPROCESSINGMULTIPLE-SCATTERINGLight emissionFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaLIGHT-EMISSIONAstrophysics - Cosmology and Nongalactic Astrophysics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Cosmology and Nongalactic Astrophysics (astro-ph.CO)Extensive air showerFOS: Physical sciencesCosmic raySURFACE DETECTORAir fluorescence method0103 physical sciencesExtensive air showersRECONSTRUCTIONAerosolInstrumentation and Methods for Astrophysics (astro-ph.IM)Cosmic raysPierre Auger ObservatoryAerosolsCalorimeter (particle physics)Atmospheric effect010308 nuclear & particles physicsAtmosphereFísicaAstronomy and AstrophysicsCosmic rays; Extensive air showers; Air fluorescence method; Atmosphere; Aerosols; Lidar; Bi-static lidarCosmic rayNITROGENAir showerFluorescence Telescopes13. Climate actionExperimental High Energy PhysicsAEROSSOL
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Collins and Sivers asymmetries for pions and kaons in muon-deuteron DIS

2008

The measurements of the Collins and Sivers asymmetries of identified hadrons produced in deep-inelastic scattering of 160 GeV/c muons on a transversely polarised 6LiD target at COMPASS are presented. The results for charged pions and charged and neutral kaons correspond to all data available, which were collected from 2002 to 2004. For all final state particles both the Collins and Sivers asymmetries turn out to be small, compatible with zero within the statistical errors, in line with the previously published results for not identified charged hadrons, and with the expected cancellation between the u- and d-quark contributions.

QuarkNuclear and High Energy PhysicsParticle physicsSivers asymmetryHadronNuclear TheoryFOS: Physical sciences01 natural sciencesCOMPASSHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)PionIdentifiedCompass0103 physical sciencesTransverse spin effects; Deuteron; Collins asymmetry; Sivers asymmetry; COMPASSDeuteronTransverse spin effect010306 general physicsNuclear ExperimentPhysicsMuon010308 nuclear & particles physicsScatteringHigh Energy Physics::PhenomenologyTransverse single-spin asymmetryTransverse spin effectsCollins asymmetryhadronsDeuteriumTransversityHigh Energy Physics::Experiment
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Search for First Harmonic Modulation in the Right Ascension Distribution of Cosmic Rays Detected at the Pierre Auger Observatory

2011

We present the results of searches for dipolar-type anisotropies in different energy ranges above 2.5 × 1017 eV with the surface detector array of the Pierre Auger Observatory, reporting on both the phase and the amplitude measurements of the first harmonic modulation in the right-ascension distribution. Upper limits on the amplitudes are obtained, which provide the most stringent bounds at present, being below 2% at 99% C.L. for EeV energies. We also compare our results to those of previous experiments as well as with some theoretical expectations.

Large scale anisotripies[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Auger ExperimentAstronomyAstrophysics::High Energy Astrophysical PhenomenaPhase (waves)FOS: Physical sciencesCosmic rayAstrophysicsanisotropySURFACE DETECTOR01 natural sciencesCosmic RayAugerLarge scale anisotropiesObservatoryLarge scale anisotropie0103 physical sciences010303 astronomy & astrophysicsUltra-high energy cosmic rayCiencias ExactasHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger ObservatoryFÍSICA DE PARTÍCULASUltra High Energy Cosmic Rays.010308 nuclear & particles physicsORIGINPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsFísicaAstronomy and AstrophysicsPierre Auger ObservatoryUltra-high energy cosmic raysENERGY-SPECTRUMRadiación cósmicaAnisotropíaAmplitudeHarmonicsUltra-high energy cosmic rays; Large scale anisotropies; Pierre Auger ObservatoryExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGARRAYFísica nuclearRight ascensionAstrophysics - High Energy Astrophysical Phenomena
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First Muon-Neutrino Disappearance Study with an Off-Axis Beam

2012

We report a measurement of muon-neutrino disappearance in the T2K experiment. The 295-km muon-neutrino beam from Tokai to Kamioka is the first implementation of the off-axis technique in a long-baseline neutrino oscillation experiment. With data corresponding to 1.43 × 10(20) protons on target, we observe 31 fully-contained single μ-like ring events in Super-Kamiokande, compared with an expectation of 104 ± 14(syst) events without neutrino oscillations. The best-fit point for two-flavor νμ → ντ oscillations is sin 2(2θ(23)) = 0.98 and |Δm(2)(32)| = 2.65 × 10(−3) eV2. The boundary of the 90% confidence region includes the points (sin2 (2θ(23)), |Δm(2)(32)|) = (1.0, 3.1 × 10(−3) eV2), (0.84, …

Nuclear and High Energy Physics530 PhysicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:500.27. Clean energy01 natural sciencesNeutrino scatteringHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Muon neutrino010306 general physicsNeutrino oscillationQCPhysics010308 nuclear & particles physicshep-exHigh Energy Physics::PhenomenologyT2K experimentFísicaPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentBeam (structure)
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The characterisation of the multianode photomultiplier tubes for the RICH-1 upgrade project at COMPASS

2008

Abstract A major upgrade of the Cherenkov photon detection system of COMPASS RICH-1 has been performed and it has been in operation since the 2006 physics run. The inner part of the photon detector has been replaced by a different technology in order to measure Cherenkov photons at high photoelectron rates, up to several times 10 6 per second and per channel. Cherenkov photons from 200 to 750 nm are detected by 576 multianode photomultiplier tubes (MAPMTs) with 16 channels each, coupled to individual fused silica lens telescopes and fast, high sensitivity and high time resolution electronics read-out. To guarantee an optimal performance of the complete system, parameters like dark current, …

PhysicsNuclear and High Energy PhysicsPhotomultiplierPhotonPhysics::Instrumentation and Detectorsbusiness.industryDetectorOpticsUpgradeCompassQuantum efficiencybusinessInstrumentationCherenkov radiationDark current
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Advanced functionality for radio analysis in the Offline software framework of the Pierre Auger Observatory

2011

The advent of the Auger Engineering Radio Array (AERA) necessitates the development of a powerful framework for the analysis of radio measurements of cosmic ray air showers. As AERA performs ‘‘radio- hybrid’’ measurements of air shower radio emission in coincidence with the surface particle detectors and fluorescence telescopes of the Pierre Auger Observatory, the radio analysis functionality had to be incorporated in the existing hybrid analysis solutions for fluorescence and surface detector data. This goal has been achieved in a natural way by extending the existing Auger Offline software framework with radio functionality. In this article, we lay out the design, highlights and features …

Source codeAstronomycomputer.software_genre01 natural sciencesObservatoryAuger experimentRadio detectionSOFTWARES (ANÁLISE)Instrumentationcosmic rays; radio detection; analysis software; detector simulationmedia_commonPhysicsPhysicsDetectoranalysis softwareAstrophysics::Instrumentation and Methods for AstrophysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsComputer hardwareNuclear and High Energy Physics[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]media_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAnalysis softwareDetector simulationCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsCosmic Rayradio detectionNuclear physicscosmic raysRAY AIR-SHOWERS0103 physical sciencesDETECTORSInstrumentation (computer programming)010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Cosmic raysCiencias ExactasNuclear and High Energy PhysicPierre Auger Observatory010308 nuclear & particles physicsbusiness.industrydetector simulationFísicaCosmic ray[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Software frameworkAir showerExperimental High Energy PhysicsEMISSIONbusinesscomputerMONTE-CARLO SIMULATIONS
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Changes in surgicaL behaviOrs dUring the CoviD-19 pandemic. The SICE CLOUD19 Study

2021

Abstract Background The spread of the SARS-CoV2 virus, which causes COVID-19 disease, profoundly impacted the surgical community. Recommendations have been published to manage patients needing surgery during the COVID-19 pandemic. This survey, under the aegis of the Italian Society of Endoscopic Surgery, aims to analyze how Italian surgeons have changed their practice during the pandemic. Methods The authors designed an online survey that was circulated for completion to the Italian departments of general surgery registered in the Italian Ministry of Health database in December 2020. Questions were divided into three sections: hospital organization, screening policies, and safety profile of…

Laparoscopic surgerySettore MED/18 - CHIRURGIA GENERALEmedicine.medical_treatmentlaparoscopyCOVID-19; Elective surgery; Emergency surgery; Laparoscopic surgery; SurveyOral HealthLaparoscopic surgerycross infection (MeSH)COVID-19; Elective surgery; Emergency surgery; Laparoscopic surgery; Survey.Surveys and QuestionnairesEpidemiologyPandemicInfection controlPractice Patterns Physicians'emergency surgeryLaparoscopySurveyhumansmedicine.diagnostic_testGeneral Commentarylaparoscopic surgeryinfection controlItalyEmergency surgeryphysicians'Original ArticleElective Surgical ProcedureHumanheating ventilation air conditioningmedicine.medical_specialtyCoronavirus disease 2019 (COVID-19)fallow periodelective surgical procedurespandemicsNOaerosol generating proceduresSurvey.COVID-19; elective surgery; emergency surgery; laparoscopic surgery; survey; COVID-19; elective surgical procedures; humans; infection control; Italy; laparoscopy; pandemics; practice patterns physicians'; SARS-CoV-2; surveys and questionnairesmedicinesurveyElective surgeryElective surgeryInfection ControlElective Surgical ProcedurePandemicbusiness.industrySARS-CoV-2General surgerySurvey; Laparoscopic surgery; COVID-19; Elective surgery; Emergency surgeryCOVID-19practice patternsSurgeryelective surgerysurveys and questionnairesLaparoscopySurgerybusiness
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Study of Σ(1385) and Ξ(1321) hyperon and antihyperon production in deep inelastic muon scattering

2013

Large samples of \Lambda, \Sigma(1385) and \Xi(1321) hyperons produced in deep-inelastic muon scattering off a ^6LiD target were collected with the COMPASS experimental setup at CERN. The relative yields of \Sigma(1385)^+, \Sigma(1385)^-, \bar{\Sigma}(1385)^-, \bar{\Sigma}(1385)^+, \Xi(1321)^-, and \bar{\Xi}(1321)^+ hyperons decaying into \Lambda(\bar{\Lambda})\pi were measured. The heavy hyperon to \Lambda and heavy antihyperon to \bar{\Lambda} yield ratios were found to be in the range 3.8% to 5.6% with a relative uncertainty of about 10%. They were used to tune the parameters relevant for strange particle production of the LEPTO Monte Carlo generator.

disParticle physicsStrange quarkdis; hyperon productionPhysics and Astronomy (miscellaneous)diLambda01 natural sciencesCOMPASSHigh Energy Physics - Experimenthyperon production0103 physical sciencesCHARGED CURRENT INTERACTIONSCHARGED CURRENT INTERACTIONS; (LAMBDA)OVER-BAR POLARIZATION; COMPASS010306 general physicsNuclear ExperimentEngineering (miscellaneous)Nuclear ExperimentPhysicsMuon010308 nuclear & particles physicsGenerator (category theory)High Energy Physics::PhenomenologyHyperon(LAMBDA)OVER-BAR POLARIZATIONSigmaProduction (computer science)High Energy Physics::ExperimentParticle Physics - ExperimentBar (unit)
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Transverse-momentum-dependent Multiplicities of Charged Hadrons in Muon-Deuteron Deep Inelastic Scattering

2017

A semi-inclusive measurement of charged hadron multiplicities in deep inelastic muon scattering off an isoscalar target was performed using data collected by the COMPASS Collaboration at CERN. The following kinematic domain is covered by the data: photon virtuality $Q^{2}&gt;1$ (GeV/$c$)$^2$, invariant mass of the hadronic system $W &gt; 5$ GeV/$c^2$, Bjorken scaling variable in the range $0.003 &lt; x &lt; 0.4$, fraction of the virtual photon energy carried by the hadron in the range $0.2 &lt; z &lt; 0.8$, square of the hadron transverse momentum with respect to the virtual photon direction in the range 0.02 (GeV/$c)^2 &lt; P_{\rm{hT}}^{2} &lt; 3$ (GeV/$c$)$^2$. The multiplicities are pres…

CERN LabComputerSystemsOrganization_COMPUTERSYSTEMIMPLEMENTATIONMULTIPLICITIESdimension: 3PT DEPENDENTComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONFOS: Physical sciencesComputerApplications_COMPUTERSINOTHERSYSTEMStarget: isoscalarmuon deuteron: deep inelastic scattering[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]nucl-extransverse momentum dependencehadron: transverse momentumSIDISCOMPASSGeneralLiterature_MISCELLANEOUSHigh Energy Physics - Experimentscaling: BjorkenSubatomär fysikcharged particle: multiplicityHigh Energy Physics - Experiment (hep-ex)[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]mass: hadronicSubatomic Physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear Physics - Experiment[ PHYS.NEXP ] Physics [physics]/Nuclear Experiment [nucl-ex]Nuclear Experiment (nucl-ex)quantum chromodynamics: perturbation theoryNuclear ExperimentNuclear ExperimentDIShep-exhadron: multiplicityeffect: nonperturbativeperturbation theory: higher-orderCERN SPSphoton: energysemi-inclusive reactionComputingMethodologies_PATTERNRECOGNITIONkinematicsDIS; SIDIS; MULTIPLICITIES; PT DEPENDENTHigh Energy Physics::ExperimentParticle Physics - Experimentexperimental resultsphoton: virtual
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Present status of the caloric curve of nuclei

1998

Abstract Spectator decay was studied for the system Au + Au at an energy of 1000 A·MeV and the decay of the interaction region at energies between 50 and 200 A·MeV. In both cases temperatures were derived from several double-ratios of neighboring isotopes and from the population of excited states in 5 Li and 4 He. Agreement was found among the different isotope temperatures and also among the two excited state temperatures. The comparison of isotope and excited state temperatures, however, reveals large differences, which cannot be explained by feeding corrections. At incident energies between 600 and 1000 A·MeV the energy spectra of fragments and also neutrons of the decaying projectile sp…

PhysicsNuclear and High Energy Physicseducation.field_of_studyIsotopeProjectileNuclear TheoryPopulationSpectral lineCaloric curveExcited stateIncident energyNeutronAtomic physicsNuclear ExperimenteducationNuclear Physics A
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The COMPASS experiment at CERN

2007

The COMPASS experiment makes use of the CERN SPS high-intensitymuon and hadron beams for the investigation of the nucleon spin structure and the spectroscopy of hadrons. One or more outgoing particles are detected in coincidence with the incoming muon or hadron. A large polarized target inside a superconducting solenoid is used for the measurements with the muon beam. Outgoing particles are detected by a two-stage, large angle and large momentum range spectrometer. The setup is built using several types of tracking detectors, according to the expected incident rate, required space resolution and the solid angle to be covered. Particle identification is achieved using a RICH counter and both…

Nuclear and High Energy Physicsstraw tube detectorPhysics::Instrumentation and DetectorsProject commissioningFOS: Physical sciencesfixed-target experimentRICH detectorhadron structureHigh Energy Physics - ExperimenttargetMWPCNuclear physicsHigh Energy Physics - Experiment (hep-ex)CompassHadron spectroscopyCOMPASS experimentscintillating fibre detectorNuclear Experimentsilicon microstrip detectorsInstrumentationSilicon microstrip detectorsPhysicsLarge Hadron ColliderStructure functionMicroMegas detectorfront-end electronicsDAQmicromegas detectordrift chamberPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentpolarisedGEM detectorcalorimetryParticle Physics - Experimentpolarised DISNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Observation of the suppression of the flux of cosmic rays above 4x10^19eV

2008

The energy spectrum of cosmic rays above 2.5 × 10¹⁸ eV, derived from 20,000 events recorded at the Pierre Auger Observatory, is described. The spectral index γ of the particle flux, J ∝ E-γ, at energies between 4 × 10¹⁸ eV and 4 × 10¹⁹ eV is 2.69 ± 0.02(stat) ± 0.06(syst), steepening to 4.2 ± 0.4(stat) ± 0.06(syst) at higher energies. The hypothesis of a single power law is rejected with a significance greater than 6 standard deviations. The data are consistent with the prediction by Greisen and by Zatsepin and Kuz'min.

[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Astrophysics::High Energy Astrophysical Phenomenaenergy spectrumFOS: Physical sciencesGeneral Physics and AstronomyFluxOsservatorio Pierre Augerspectral indexCosmic rayparticle fluxAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsEXTENSIVE AIR-SHOWERSAstrophysicsUPPER LIMIT01 natural sciencesPower lawAugerNuclear physicsENERGY[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Raggi cosmicicosmic rays0103 physical sciencesddc:550Particle flux010303 astronomy & astrophysicsCiencias ExactasPhysicsPierre Auger ObservatorySpectral indexSPECTRUM[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsAstrophysics (astro-ph)Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsFísicaEnergia ultra altaARRAYHigh Energy Physics::ExperimentSciami atmosferici estesiEnergy (signal processing)
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Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter

2010

Data collected by the Pierre Auger Observatory through 31 August 2007 showed evidence for anisotropy in the arrival directions of cosmic rays above the Greisen-Zatsepin-Kuz'min energy threshold, 6 x 10(19) eV. The anisotropy was measured by the fraction of arrival directions that are less than 3.1 degrees from the position of an active galactic nucleus within 75 Mpc (using the Veron-Cetty and Veron 12th catalog). An updated measurement of this fraction is reported here using the arrival directions of cosmic rays recorded above the same energy threshold through 31 December 2009. The number of arrival directions has increased from 27 to 69, allowing a more precise measurement. The correlating…

AstronomyAstrophysicsUltra High Energy Cosmic ray01 natural scienceslaw.inventionObservatorylawAnisotropy010303 astronomy & astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]UHECRAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryGZKAnisotropíaGALAXIESNEUTRINOSGreisen–Zatsepin–Kuz’minComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaACTIVE GALACTIC NUCLEIHIPASS CATALOG[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Active galactic nucleusRadiación Cósmicamedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsTelescope0103 physical sciencesCosmic raysCiencias ExactasAstrophysics::Galaxy AstrophysicsPierre Auger ObservatorySPECTRUM010308 nuclear & particles physicsAstronomyFísicaAstronomy and AstrophysicsCosmic rayGalaxyCorrelation with astrophysical sourcesCosmic rays; UHECR; Anisotropy; Pierre Auger Observatory; Extra-galactic; GZKSkyExperimental High Energy PhysicsAnisotropyExtra-galactic
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Gluon Polarisation in the Nucleon and Longitudinal Double Spin Asymmetries from Open Charm Muoproduction

2009

The gluon polarisation in the nucleon has been determined by detecting charm production via D0 meson decay to charged K and pi in polarised muon scattering off a longitudinally polarised deuteron target. The data were taken by the COMPASS Collaboration at CERN between 2002 and 2006 and corresponds to an integrated luminosity of 2.8 fb^-1. The dominant underlying process of charm production is the photon-gluon fusion to a cc-bar pair. A leading order QCD approach gives an average gluon polarisation of (Delta g/g)_x= -0.49 +- 0.27(stat) +- 0.11(syst) at a scale mu^2 ~ 13 (GeV/c)^2 and at an average gluon momentum fraction (x) ~ 0.11. The longitudinal cross-section asymmetry for D0 production …

Nuclear and High Energy PhysicsParticle physicsMesonHigh Energy Physics::LatticeNuclear TheoryFOS: Physical sciences01 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsMomentumHigh Energy Physics - Experiment (hep-ex)Spin0103 physical sciencesCharm (quantum number)010306 general physicsNuclear ExperimentSpin-½Quantum chromodynamicsPhysicsMuon010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyInelastic muon scatteringAsymmetryGluonInelastic muon scattering; Spin; Asymmetry; Gluon polarisationGluon polarisationHigh Energy Physics::ExperimentNucleonParticle Physics - Experiment
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Fast photon detection for COMPASS RICH-1

2007

A fast photon detection system has been built and assembled for the upgrade of COMPASS RICH-1. The system is based on multianode photomultipliers coupled to fused silica lenses to collect the light from a larger surface and to guide it to the photocathode, preserving the position information. The emphasis is on the fast response and high rate capability of the detectors and the associated electronics. The photon detection system is now ready and it will be employed in the 2006 COMPASS data taking. We report about the system design and construction.

PhysicsNuclear and High Energy PhysicsPhotomultiplierbusiness.industryUV lensesEmphasis (telecommunications)DetectorCOMPASSPhotocathodeOpticsUpgradePhoton detectionCompassCOMPASS; RICH; Multianode photomultiplier tubes; UV lenses; Photon detectionMultianode photomultiplier tubesSystems designElectronicsbusinessInstrumentationRICH
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The exposure of the hybrid detector of the Pierre Auger Observatory

2010

The Pierre Auger Observatory is a detector for ultra-high energy cosmic rays. It consists of a surface array to measure secondary particles at ground level and a fluorescence detector to measure the development of air showers in the atmosphere above the array. The ‘‘hybrid” detection mode combines the information from the two subsystems. We describe the determination of the hybrid exposure for events observed by the fluorescence telescopes in coincidence with at least one water-Cherenkov detector of the surface array. A detailed knowledge of the time dependence of the detection operations is crucial for an accurate evaluation of the exposure. We discuss the relevance of monitoring data coll…

Physics::Instrumentation and DetectorsAstronomy01 natural sciencesCoincidenceAugerFluorescence detectorData acquisitionAuger experimentHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsFÍSICA DE PARTÍCULASSettore INF/01 - InformaticaCascada atmosférica extensaPhysicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger Observatoryultra high energy cosmic rays; Pierre Auger Observatory; extensive air showers; trigger; exposure; fluorescence detector; hybridENERGY-SPECTRUMRadiación cósmicaSIMULATIONComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFluorescenciaFísica nuclearAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaExtensive air showerMeasure (physics)FOS: Physical sciencesCosmic rayCosmic RayFluorescence spectroscopyUltra high energy cosmic rayExposureNuclear physicsOpticsSHOWERS0103 physical sciencesExtensive air showers010306 general physicsCiencias ExactasPierre Auger Observatory010308 nuclear & particles physicsbusiness.industryFísicaAstronomy and AstrophysicsUltra high energy cosmic raysHybrid[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]fluxTriggerExperimental High Energy PhysicsbusinessSYSTEMAstroparticle Physics
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Atmospheric effects on extensive air showers observed with the Surface Detector of the Pierre Auger Observatory

2009

Atmospheric parameters, such as pressure (P), temperature (T) and density (ρ ∝ P/T), affect the development of extensive air showers initiated by energetic cosmic rays. We have studied the impact of atmospheric variations on extensive air showers by means of the surface detector of the Pierre Auger Observatory. The rate of events shows a ∼ 10% seasonal modulation and ∼ 2% diurnal one. We find that the observed behaviour is explained by a model including the effects associated with the variations of P and ρ. The former affects the longitudinal development of air showers while the latter influences the Molière radius and hence the lateral distribution of the shower particles. The model is val…

[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]: 96.50.sdRadiación CósmicaIMPACTAstronomyExtensive air showerFOS: Physical sciencesCosmic rayAstrophysicsExtensive air showers; UHECR; Atmosphere; Weather01 natural sciencesCOSMIC-RAY CASCADESAugerAtmosphereENERGYObservatory0103 physical sciencesExtensive air showersRECONSTRUCTION96.50.sf010303 astronomy & astrophysicsMolière radiusWeatherInstrumentation and Methods for Astrophysics (astro-ph.IM)96.50.sbPierre Auger ObservatoryPhysics010308 nuclear & particles physicsAtmosphereUHECRDetectorFísicaAstronomy and AstrophysicsPresión AtmosféricaPROFILES[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Longitudinal developmentATMOSFERA (ESTUDO)13. Climate actionExperimental High Energy PhysicsSIMULATIONComputingMethodologies_DOCUMENTANDTEXTPROCESSINGClimaAstrophysics - Instrumentation and Methods for Astrophysics
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Collins and Sivers asymmetries in muonproduction of pions and kaons off transversely polarised protons

2015

Measurements of the Collins and Sivers asymmetries for charged pions and charged and neutral kaons produced in semi-inclusive deep-inelastic scattering of high energy muons off transversely polarised protons are presented. The results were obtained using all the available COMPASS proton data, which were taken in the years 2007 and 2010. The Collins asymmetries exhibit in the valence region a non-zero signal for pions and there are hints of non-zero signal also for kaons. The Sivers asymmetries are found to be positive for positive pions and kaons and compatible with zero otherwise.

High energyParticle physicsNuclear and High Energy PhysicsProtonNuclear TheoryFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]spin01 natural sciencesSIDIS530SINGLE SPIN ASYMMETRIESHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)TMD PDF and FFPionNuclear and High Energy Physics; TMD PDF and FF; SIDIS; spinRATIO0103 physical sciencesDISTRIBUTIONSSCATTERING[ PHYS.NEXP ] Physics [physics]/Nuclear Experiment [nucl-ex]010306 general physicsNuclear ExperimentNuclear and High Energy PhysicPhysicsMuon010308 nuclear & particles physicsScatteringlcsh:QC1-999ddc:High Energy Physics::ExperimentParticle Physics - Experimentlcsh:Physics
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Erratum to "Atmospheric effects on extensive air showers observed with the surface detector of the Pierre Auger observatory"[Astroparticle Physics 32…

2010

The Pierre Auger Collaboration... K.B. Barber... J.A. Bellido... R.W. Clay... B.R. Dawson... V.C. Holmes... J. Sorokin... P. Wahrlich... B.J. Whelan... M.G. Winnick... et al.

Astroparticle physicsPhysicsPierre Auger Observatory[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]010308 nuclear & particles physicsAstronomyDetectorAstronomyAstronomy and AstrophysicsAstrophysics01 natural sciencesAuger[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Experimental High Energy Physics0103 physical sciences010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSAstroparticle Physics
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Measurement of the Depth of Maximum of Extensive Air Showers above 10(18) eV

2010

We describe the measurement of the depth of maximum, Xmax, of the longitudinal development of air showers induced by cosmic rays. Almost four thousand events above 10¹⁸ eV observed by the fluorescence detector of the Pierre Auger Observatory in coincidence with at least one surface detector station are selected for the analysis. The average shower maximum was found to evolve with energy at a rate of (106⁺³⁵₋₂₁) g/cm²/decade below 1018.24 ± 0.05 eV and (24 ± 3) g/cm²/decade above this energy. The measured shower-to-shower fluctuations decrease from about 55 to 26 g/cm². The interpretation of these results in terms of the cosmic ray mass composition is briefly discussed.

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]FLUORESCENCE LIGHTGeneral Physics and AstronomyPierre Auger Observatory; depth of maximum; fluorescence detector; cosmic raysFOS: Physical sciencesCosmic rayChemical CompositionAstrophysicsMass compositionENERGIA01 natural sciencesCoincidenceAugerNuclear physicsPhysics and Astronomy (all)cosmic rays0103 physical sciencesRECONSTRUCTIONHigh-Energy Cosmic Ray010303 astronomy & astrophysicsDETECTORCiencias ExactasPierre Auger ObservatoryPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)MeasurementSPECTRUM010308 nuclear & particles physicsPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Pierre Auger ExperimentDetectorPrimary compositionFísicaPierre Auger ObservatoryCOSMIC-RAYSCosmic raylongitudinal developmentLongitudinal developmentRESOLUTIONFísica nuclearfluorescenceAstrophysics - High Energy Astrophysical PhenomenaenergyPhysical Review Letters
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Measurements of mixed harmonic cumulants in Pb–Pb collisions at sNN=5.02 TeV

2021

Correlations between moments of different flow coefficients are measured in Pb–Pb collisions at sNN=5.02 TeV recorded with the ALICE detector. These new measurements are based on multiparticle mixed harmonic cumulants calculated using charged particles in the pseudorapidity region |η|&lt;0.8 with the transverse momentum range 0.2&lt;pT&lt;5.0 GeV/c. The centrality dependence of correlations between two flow coefficients as well as the correlations between three flow coefficients, both in terms of their second moments, are shown. In addition, a collection of mixed harmonic cumulants involving higher moments of v2 and v3 is measured for the first time, where the characteristic signature of ne…

Quantum chromodynamicsPhysicsNuclear and High Energy PhysicsLarge Hadron Collider010308 nuclear & particles physics01 natural sciencesCharged particleNuclear physicsPseudorapidity0103 physical sciencesHarmonicRapidity010306 general physicsAnisotropyCumulantPhysics Letters B
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Measurement of azimuthal hadron asymmetries in semi-inclusive deep inelastic scattering off unpolarised nucleons

2014

Spin-averaged asymmetries in the azimuthal distributions of positive and negative hadrons produced in deep inelastic scattering were measured using the CERN SPS muon beam at $160$ GeV/c and a $^6$LiD target. The amplitudes of the three azimuthal modulations $\cos\phi_h$, $\cos2\phi_h$ and $\sin\phi_h$ were obtained binning the data separately in each of the relevant kinematic variables $x$, $z$ or $p_T^{\,h}$ and binning in a three-dimensional grid of these three variables. The amplitudes of the $\cos \phi_h$ and $\cos 2\phi_h$ modulations show strong kinematic dependencies both for positive and negative hadrons.

Particle physicsNuclear and High Energy PhysicsTMD SIDIS PDFHadronFOS: Physical sciencesSIVERS ASYMMETRIESMUON PROTON-SCATTERINGCOLLINSSIDISPDF01 natural sciences530High Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)LEPTOPRODUCTIONDEPENDENCE0103 physical sciencesDISTRIBUTIONSlcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsNuclear ExperimentPhysicsLarge Hadron ColliderMuon010308 nuclear & particles physicsTMDELECTROPRODUCTIONDeep inelastic scatteringAzimuthAmplitudeMUON PROTON-SCATTERING; SIVERS ASYMMETRIES; SPIN ASYMMETRIES; DISTRIBUTIONS; ELECTROPRODUCTION; LEPTOPRODUCTION; DEPENDENCE; COLLINSlcsh:QC770-798High Energy Physics::ExperimentNucleonSPIN ASYMMETRIESParticle Physics - ExperimentBeam (structure)
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Measurement of the Charged-Pion Polarizability

2015

The COMPASS collaboration at CERN has investigated pion Compton scattering, $\pi^-\gamma\rightarrow \pi^-\gamma$, at centre-of-mass energy below 3.5 pion masses. The process is embedded in the reaction $\pi^-\mathrm{Ni}\rightarrow\pi^-\gamma\;\mathrm{Ni}$, which is initiated by 190\,GeV pions impinging on a nickel target. The exchange of quasi-real photons is selected by isolating the sharp Coulomb peak observed at smallest momentum transfers, $Q^2<0.0015$\,(GeV/$c$)$^2$. From a sample of 63\,000 events the pion electric polarisability is determined to be $\alpha_\pi\ =\ (\,2.0\ \pm\ 0.6_{\mbox{\scriptsize stat}}\ \pm\ 0.7_{\mbox{\scriptsize syst}}\,) \times 10^{-4}\,\mbox{fm}^3$ under the …

Particle physicsChiral perturbation theoryPhotonComputerSystemsOrganization_COMPUTERSYSTEMIMPLEMENTATIONStrong interactionComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONGeneral Physics and AstronomyFOS: Physical sciencesComputerApplications_COMPUTERSINOTHERSYSTEMSGeneralLiterature_MISCELLANEOUSHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)PionPolarizabilityNuclear Experiment (nucl-ex)Nuclear ExperimentNuclear ExperimentPhysicsChPTMuonCompton scatteringpolarisabilitypolarisability; ChPTComputingMethodologies_PATTERNRECOGNITIONHigh Energy Physics::ExperimentMagnetic dipoleParticle Physics - Experiment
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Search for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger Observatory

2011

Erratum: Phys. Rev. D 85, 029902(E) (2012) [http://dx.doi.org/10.1103/PhysRevD.85.029902]

Physics::Instrumentation and DetectorsSolar neutrinoAstrophysicsUPPER LIMITPHOTON FRACTION01 natural sciences7. Clean energyneutrinoObservatoryHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsORIGINPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]pionAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryCOSMIC-RAYScosmic ray detectorsand other elementary particle detectorsCosmic neutrino backgroundNEUTRINOSFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical PhenomenaFLUXFERMI-LATNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]TELESCOPEAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayEXTENSIVE AIR-SHOWERSSURFACE DETECTORCosmic RayPionmuon0103 physical sciencesNeutrino010306 general physicsCosmic raysPierre Auger ObservatoryMuon010308 nuclear & particles physicsFísicaand other elementary particlesUltra-high energy cosmic raysPERFORMANCECosmic rayneutrino flavor; air showers; surface detector; observatory; atmosphere; Auger; cosmic radiation; energy spectrum13. Climate actionHigh Energy Physics::Experiment
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Electromagnetic fission of $^{238}$U at 600 and 1000 MeV per nucleon

1995

Electromagnetic fission of238U projectiles at E/A =600 and 1000 MeV was studied with the ALADIN spectrometer at the heavy-ion synchrotron SIS. Seven different targets (Be, C, Al, Cu, In, Au and U) were used. By considering only those fission events where the two charges added up to 92, most of the nuclear interactions were excluded. The nuclear contributions to the measured fission cross sections were determined by extrapolating from beryllium to the heavier targets with the concept of factorization. The obtained cross sections for electromagnetic fission are well reproduced by extended Weizsacker-Williams calculations which include E1 and E2 excitations. The asymmetry of the fission fragme…

PhysicsNuclear and High Energy PhysicsCold fissionCluster decayFissionNuclear Theorychemistry.chemical_elementUraniumResonance (particle physics)Nuclear physicschemistryNuclear fusionAtomic physicsBerylliumNuclear ExperimentNucleonNuclear Physics
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Time projection chambers for the T2K near detectors

2011

The T2K experiment is designed to study neutrino oscillation properties by directing a high intensity neutrino beam produced at J-PARC in Tokai, Japan, towards the large Super-Kamiokande detector located 295 km away, in Kamioka, Japan. The experiment includes a sophisticated near detector complex, 280 m downstream of the neutrino production target in order to measure the properties of the neutrino beam and to better understand neutrino interactions at the energy scale below a few GeV. A key element of the near detectors is the ND280 tracker, consisting of two active scintillator–bar target systems surrounded by three large time projection chambers (TPCs) for charged particle tracking. The d…

Nuclear and High Energy PhysicsNeutrino oscillationPhysics::Instrumentation and Detectorsddc:500.2Tracking (particle physics)01 natural sciences7. Clean energyNuclear physics0103 physical sciences010306 general physicsNeutrino oscillationInstrumentationPhysicsTime projection chamber010308 nuclear & particles physicsDetectorT2K experimentDrift chamber Gas system Micromegas Neutrino oscillation Time projection chamberFísicaMicroMegas detectorTime projectionchamberGas systemCharged particleTime projection chamberDrift chamberHigh Energy Physics::ExperimentNeutrinoMicromegas
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The effect of the geomagnetic field on cosmic ray energy estimates and large scale anisotropy searches on data from the Pierre Auger Observatory

2011

We present a comprehensive study of the influence of the geomagnetic field on the energy estimation of extensive air showers with a zenith angle smaller than $60^\circ$, detected at the Pierre Auger Observatory. The geomagnetic field induces an azimuthal modulation of the estimated energy of cosmic rays up to the ~2% level at large zenith angles. We present a method to account for this modulation of the reconstructed energy. We analyse the effect of the modulation on large scale anisotropy searches in the arrival direction distributions of cosmic rays. At a given energy, the geomagnetic effect is shown to induce a pseudo-dipolar pattern at the percent level in the declination distribution t…

[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencescosmic ray experimentCosmic rayAstrophysicsultra high energy cosmic raysEXTENSIVE AIR-SHOWERS01 natural sciencesDeclinationultra high energy cosmic ray0103 physical sciencescosmic rays detectors; cosmic ray experiments; ultra high energy cosmic rayscosmic rays detectorAnisotropyInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsZenithParticle detectors.Pierre Auger ObservatoryPhysics010308 nuclear & particles physicsPhysicsOBSERVATÓRIOSAstrophysics::Instrumentation and Methods for AstrophysicsFísicaAstronomy and Astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]AzimuthMODELEarth's magnetic fieldPhysics::Space PhysicsLarge detector systems for particle and astroparticle physicARRAYFísica nuclearcosmic rays detectorscosmic ray experimentsAstrophysics - Instrumentation and Methods for AstrophysicsEnergy (signal processing)Cherenkov detectorJournal of Cosmology and Astroparticle Physics
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Trigger and aperture of the surface detector array of the Pierre Auger Observatory

2010

The surface detector array of the Pierre Auger Observatory consists of 1600 water-Cherenkov detectors, for the study of extensive airshowers (EAS) generated by ultra-high-energy cosmic rays. We describe the trigger hierarchy, from the identification of candidates howers at the level of a single detector, amongst a large background (mainly random single cosmic ray muons), up to the selection of real events and the rejection of random coincidences. Such trigger makes the surface detector array fully efficient for the detection of EAS with energy above 3 x 1018 eV, for all zenith angles between 03 and 603, independently of the position of the impact point and of the mass of the primary particl…

Ultra high energy cosmic rays; Auger Observatory; Extensive air showers; Trigger; ExposurePhysics::Instrumentation and DetectorsAstronomyHigh-Energy Cosmi Ray7. Clean energy01 natural sciencesAugerAcceptance and Trigger Efficiency010303 astronomy & astrophysicsInstrumentationComputingMilieux_MISCELLANEOUSPhysicsRange (particle radiation)PhysicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryHigh energyFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsNuclear and High Energy Physics[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]AIR SHOWERSApertureInstrumentationAstrophysics::High Energy Astrophysical PhenomenaExtensive air showerFOS: Physical sciencesCosmic rayENERGIACosmic RayUltra high energy cosmic rayExposureOpticsultra high energy cosmic rays Auger Observatory extensive airshowers trigger exposure0103 physical sciencesPARTICLESExtensive air showersSurface DetectorInstrumentation and Methods for Astrophysics (astro-ph.IM)ZenithCiencias ExactasNuclear and High Energy PhysicPierre Auger Observatory010308 nuclear & particles physicsbusiness.industryFísicaUltra high energy cosmic raysUltra-high energy cosmic rays[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]TriggerAuger ObservatoryExperimental High Energy PhysicsHigh Energy Physics::Experimentbusiness
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The T2K Experiment

2011

The T2K experiment is a long-baseline neutrino oscillation experiment. Its main goal is to measure the last unknown lepton sector mixing angle {\theta}_{13} by observing {\nu}_e appearance in a {\nu}_{\mu} beam. It also aims to make a precision measurement of the known oscillation parameters, {\Delta}m^{2}_{23} and sin^{2} 2{\theta}_{23}, via {\nu}_{\mu} disappearance studies. Other goals of the experiment include various neutrino cross section measurements and sterile neutrino searches. The experiment uses an intense proton beam generated by the J-PARC accelerator in Tokai, Japan, and is composed of a neutrino beamline, a near detector complex (ND280), and a far detector (Super-Kamiokande)…

Nuclear and High Energy PhysicsParticle physicsSterile neutrinoPhysics - Instrumentation and DetectorsNeutrino oscillationPhysics::Instrumentation and Detectorsddc:500.27. Clean energy01 natural sciencesHigh Energy Physics - ExperimentNuclear physics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Long baseline[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Neutrinos010306 general physicsNeutrino oscillationphysics.ins-detInstrumentationQCPhysicsT2Khep-ex010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyT2K experimentNeutrinos; Neutrino oscillation; Long baseline; T2K; J-PARC; Super-KamiokandeFísicaNeutrino detectorJ-PARCHigh Energy Physics::ExperimentJ-PARCSuper-KamiokandeNeutrinoSuper-KamiokandeLepton
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A highly integrated low-cost readout system for the COMPASS RICH-1 detector

2007

Particle identification at high multiplicities is a key feature of the COMPASS experiment at CERN's SPS. Hadrons up to 50 GeV/c are identified by a RICH detector with a large horizontal and vertical acceptance of plusmn250 mrad and plusmn180 mrad, respectively. The central region of the photon detector is equipped with multi-anode photomultiplier tubes, the remaining 75% of the total active area are covered by MWPCs with Csl photocathodes. In order to improve the performance of the detector at very high beam intensities, more than 62000 channels of a new analog readout system of the MWPCs, based on the APV25 chip, were developed and installed in 2006. The new system features good single pho…

PhysicsPhotomultiplierPhysics::Instrumentation and Detectorsbusiness.industryDetectorPhotodetectorDead timeParticle identificationNuclear physicsOpticsCompassNuclear electronicsCOMPASS experimentHigh Energy Physics::Experimentbusiness2007 IEEE Nuclear Science Symposium Conference Record
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"Table 1" of "Electromagnetic fission of U-238 at 600-MeV and 1000-MeV per nucleon"

1997

Electromagnetic fission.

Nuclear TheoryIntegrated Cross SectionU238 U --&gt; 2FRAGB XU238 C --&gt; 2FRAGB XU238 AU --&gt; 2FRAGB XCross SectionPhysics::Classical PhysicsSIGU238 AL --&gt; 2FRAGB XU238 IN --&gt; 2FRAGB XInclusiveU238 CU --&gt; 2FRAGB XPhysics::Atomic and Molecular ClustersNUCLEUS NUCLEUS --&gt; 2FRAGB XNuclear Experiment
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