0000000000946396

AUTHOR

D. Kang

showing 37 related works from this author

Experimental investigation of transverse spin asymmetries in muon-p SIDIS processes: Sivers asymmetries

2012

The COMPASS Collaboration at CERN has measured the transverse spin azimuthal asymmetry of charged hadrons produced in semi-inclusive deep inelastic scattering using a 160 GeV positive muon beam and a transversely polarised NH_3 target. The Sivers asymmetry of the proton has been extracted in the Bjorken x range 0.003 0.03. The asymmetry is different from zero and positive also in the low x region, where sea-quarks dominate. The kinematic dependence of the asymmetry has also been investigated and results are given for various intervals of hadron and virtual photon fractional energy. In contrast to the case of the Collins asymmetry, the results on the Sivers asymmetry suggest a strong depende…

QuarkNuclear and High Energy PhysicsParticle physicsmedia_common.quotation_subjectHadronFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesAsymmetryCOMPASSSIDISspin asymmetriesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Compass0103 physical sciences010306 general physicsNuclear Experimentmedia_commonPhysics[PHYS]Physics [physics]Sivers asymmetriesLarge Hadron Colliderta114010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyDeep inelastic scatteringCOMPASS; SIDIS; spin asymmetries; Sivers asymmetriesTransverse planeDistribution functionHigh Energy Physics::ExperimentCOMPASS SIDIS TMD Sivers asymmetryParticle Physics - Experiment
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A Search for IceCube Events in the Direction of ANITA Neutrino Candidates

2020

During the first three flights of the Antarctic Impulsive Transient Antenna (ANITA) experiment, the collaboration detected several neutrino candidates. Two of these candidate events were consistent with an ultra-high-energy up-going air shower and compatible with a tau neutrino interpretation. A third neutrino candidate event was detected in a search for Askaryan radiation in the Antarctic ice, although it is also consistent with the background expectation. The inferred emergence angle of the first two events is in tension with IceCube and ANITA limits on isotropic cosmogenic neutrino fluxes. Here, we test the hypothesis that these events are astrophysical in origin, possibly caused by a po…

010504 meteorology & atmospheric sciencesPoint sourceAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesStandard ModelHigh Energy Physics - Phenomenology (hep-ph)Tau neutrino0103 physical sciencesTRACK RECONSTRUCTIONSource spectrum010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEIsotropyAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysicshep-phHigh Energy Physics - PhenomenologyAir showerPhysics and Astronomy13. Climate actionSpace and Planetary ScienceNeutrinoAstrophysics - High Energy Astrophysical PhenomenaEvent (particle physics)
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Follow-up of Astrophysical Transients in Real Time with the IceCube Neutrino Observatory

2020

In multi-messenger astronomy, rapid investigation of interesting transients is imperative. As an observatory with a 4$\pi$ steradian field of view and $\sim$99\% uptime, the IceCube Neutrino Observatory is a unique facility to follow up transients, and to provide valuable insight for other observatories and inform their observing decisions. Since 2016, IceCube has been using low-latency data to rapidly respond to interesting astrophysical events reported by the multi-messenger observational community. Here, we describe the pipeline used to perform these follow up analyses and provide a summary of the 58 analyses performed as of July 2020. We find no significant signal in the first 58 analys…

High Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEPhysics010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsNeutrino astronomy; High energy astrophysicsFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics01 natural sciencesIceCube Neutrino ObservatoryNeutrino astronomySpace and Planetary ScienceObservatory0103 physical sciencesNeutrinoNeutrino astronomyAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)High energy astrophysics010303 astronomy & astrophysicsastro-ph.IM0105 earth and related environmental sciencesThe Astrophysical Journal
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Time-integrated Neutrino Source Searches with 10 years of IceCube Data

2020

Physical review letters 124(5), 051103 (1-9) (2020). doi:10.1103/PhysRevLett.124.051103

background [atmosphere]Astrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectGeneral Physics and AstronomyFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics53001 natural sciencesIceCubeparticle source [neutrino]TRACK RECONSTRUCTION0103 physical sciencesddc:530atmosphere [muon]010306 general physicsAstrophysics::Galaxy Astrophysicsmedia_commonastro-ph.HEPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)MuonAstrophysics::Instrumentation and Methods for AstrophysicsNorthern HemisphereAstronomyGalaxymessengerPhysics and AstronomySkycorrelationtime dependenceupgradegalaxyNeutrinoAstrophysics - High Energy Astrophysical Phenomenastatistical
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Large-scale genotyping identifies 41 new loci associated with breast cancer risk

2013

Journal article Breast cancer is the most common cancer among women. Common variants at 27 loci have been identified as associated with susceptibility to breast cancer, and these account for ~9% of the familial risk of the disease. We report here a meta-analysis of 9 genome-wide association studies, including 10,052 breast cancer cases and 12,575 controls of European ancestry, from which we selected 29,807 SNPs for further genotyping. These SNPs were genotyped in 45,290 cases and 41,880 controls of European ancestry from 41 studies in the Breast Cancer Association Consortium (BCAC). The SNPs were genotyped as part of a collaborative genotyping experiment involving four consortia (Collaborat…

signaling pathwayGenotypingGenotypeSingle-nucleotide polymorphismGenome-wide association studyBreast NeoplasmsconsortiumBiologyBreast Neoplasms; Case-Control Studies; Cooperative Behavior; Female; Gene-Environment Interaction; Genetic Loci; Genome-Wide Association Study; Genotype; Humans; Meta-Analysis as Topic; Polymorphism Single Nucleotide; Risk Factors; Genetic Predisposition to Disease; GeneticsPolymorphism Single NucleotideArticle03 medical and health sciences0302 clinical medicineBreast cancerSDG 3 - Good Health and Well-beingMeta-Analysis as TopicRisk FactorsGenotypecommon variantsexpressionGeneticsmedicineHumansGenetic Predisposition to DiseasePolymorphismCooperative BehaviorgeneGenotypinghormone-related protein030304 developmental biologyGenetic associationGenetics0303 health sciencesBreast cancer susceptibilityCancerSingle Nucleotidemedicine.diseaseconfer susceptibilitysusceptibility loci3. Good health14q24.1 rad51l1TOX3Genetic Loci030220 oncology & carcinogenesisCase-Control Studiesgenome-wide associationFemaleGene-Environment InteractionGenome-Wide Association Study
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IceCube-Gen2: The Window to the Extreme Universe

2020

The observation of electromagnetic radiation from radio to $\gamma$-ray wavelengths has provided a wealth of information about the universe. However, at PeV (10$^{15}$ eV) energies and above, most of the universe is impenetrable to photons. New messengers, namely cosmic neutrinos, are needed to explore the most extreme environments of the universe where black holes, neutron stars, and stellar explosions transform gravitational energy into non-thermal cosmic rays. The discovery of cosmic neutrinos with IceCube has opened this new window on the universe. In this white paper, we present an overview of a next-generation instrument, IceCube-Gen2, which will sharpen our understanding of the proce…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HENuclear and High Energy PhysicsActive galactic nucleus010308 nuclear & particles physicsHigh-energy astronomyGravitational wavemedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyFOS: Physical sciencesCosmic ray01 natural sciencesUniverseNeutron star0103 physical sciencesNeutrinoNeutrino astronomyAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsmedia_common
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EV-Scale Sterile Neutrino Search Using Eight Years of Atmospheric Muon Neutrino Data from the IceCube Neutrino Observatory

2020

Physical review letters 125(14), 141801 (1-11) (2020). doi:10.1103/PhysRevLett.125.141801

Sterile neutrinoPhysics::Instrumentation and DetectorsGeneral Physics and Astronomysterile [neutrino]01 natural sciencesCosmologyIceCubeHigh Energy Physics - ExperimentSubatomär fysikHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Astronomi astrofysik och kosmologiSubatomic PhysicsTOOLAstronomy Astrophysics and Cosmologyatmosphere [muon]Muon neutrinoPhysicsPhysicsoscillation [neutrino]Astrophysics::Instrumentation and Methods for Astrophysicshep-phneutrino: sterilemass difference [neutrino]ddc:muon: atmosphereobservatoryHigh Energy Physics - PhenomenologyPhysique des particules élémentairessignatureParticle physicsdata analysis methodScale (ratio)Astrophysics::High Energy Astrophysical Phenomenaneutrino: mass differenceFOS: Physical sciences530IceCube Neutrino Observatorystatistical analysis0103 physical sciencesOSCILLATIONSddc:530010306 general physicshep-exICEHigh Energy Physics::Phenomenologyneutrino: mixing angleCONVERSIONPhysics and AstronomyCOSMOLOGYHigh Energy Physics::Experimentneutrino: oscillationBAYESIAN-INFERENCEmixing angle [neutrino]experimental results
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Transverse spin effects in hadron-pair production from semi-inclusive deep inelastic scattering

2012

First measurements of azimuthal asymmetries in hadron-pair production in deep-inelastic scattering of muons on transversely polarised ^6LiD (deuteron) and NH_3 (proton) targets are presented. The data were taken in the years 2002-2004 and 2007 with the COMPASS spectrometer using a muon beam of 160 GeV/c at the CERN SPS. The asymmetries provide access to the transversity distribution functions, without involving the Collins effect as in single hadron production. The sizeable asymmetries measured on the NH_ target indicate non-vanishing u-quark transversity and two-hadron interference fragmentation functions. The small asymmetries measured on the ^6LiD target can be interpreted as indication …

Nuclear and High Energy PhysicsParticle physicsCOMPASS; SIDIS; two hadron azimuthal asymmetries; transversityHadronNuclear TheoryFOS: Physical sciencesCOMPASSSIDIS01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciences010306 general physicsNuclear ExperimenttransversityPhysicsLarge Hadron ColliderMuonSpectrometerta114010308 nuclear & particles physicsScatteringtwo hadron azimuthal asymmetrietwo hadron azimuthal asymmetriesHigh Energy Physics::PhenomenologyDeep inelastic scatteringPair productionDistribution functionHigh Energy Physics::ExperimentParticle Physics - ExperimentPhysics Letters B
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IceCube search for neutrinos coincident with compact binary mergers from LIGO-Virgo's first gravitational-wave transient catalog

2020

Using the IceCube Neutrino Observatory, we search for high-energy neutrino emission coincident with compact binary mergers observed by the LIGO and Virgo gravitational-wave (GW) detectors during their first and second observing runs. We present results from two searches targeting emission coincident with the sky localization of each GW event within a 1000 s time window centered around the reported merger time. One search uses a model-independent unbinned maximum-likelihood analysis, which uses neutrino data from IceCube to search for pointlike neutrino sources consistent with the sky localization of GW events. The other uses the Low-Latency Algorithm for Multi-messenger Astrophysics, which …

010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsBayesian7. Clean energy01 natural sciencesNeutrino astronomy; High energy astrophysics; Gravitational waveslocalizationIceCubeIceCube Neutrino ObservatoryGravitational wavesparticle source [neutrino]0103 physical sciencesLIGO010303 astronomy & astrophysics0105 earth and related environmental sciencesastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsGravitational wavegravitational radiationAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsLIGOobservatorymessengerMassless particleVIRGONeutrino detector13. Climate actionSpace and Planetary ScienceNeutrino astronomycompact [binary]Physique des particules élémentairesddc:520High Energy Physics::ExperimentNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical PhenomenaHigh energy astrophysicsLepton
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A search for time-dependent astrophysical neutrino emission with IceCube data from 2012 to 2017

2020

Abstract High-energy neutrinos are unique messengers of the high-energy universe, tracing the processes of cosmic ray acceleration. This paper presents analyses focusing on time-dependent neutrino point-source searches. A scan of the whole sky, making no prior assumption about source candidates, is performed, looking for a space and time clustering of high-energy neutrinos in data collected by the IceCube Neutrino Observatory between 2012 and 2017. No statistically significant evidence for a time-dependent neutrino signal is found with this search during this period, as all results are consistent with the background expectation. Within this study period, the blazar 3C 279, showed strong var…

010504 meteorology & atmospheric sciencesHigh-energy astronomyAstrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectmodel [emission]FOS: Physical sciencesCosmic rayAstrophysics01 natural scienceslaw.inventionIceCube Neutrino ObservatoryIceCubeblazarlawemission [gamma ray]0103 physical sciencesCosmic ray sources; High-energy astrophysics; Particle astrophysicsenergy: high [neutrino]Blazar010303 astronomy & astrophysics0105 earth and related environmental sciencesmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEAstroparticle physicsPhysicsbackgroundAstronomy and AstrophysicsCosmic ray sourcesUniverseHigh-energy astrophysicsmessengerobservatorySpace and Planetary Scienceddc:520time dependenceacceleration [cosmic radiation]NeutrinoAstrophysics - High Energy Astrophysical PhenomenaParticle astrophysicsFlare
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LeptonInjector and LeptonWeighter: A neutrino event generator and weighter for neutrino observatories

2021

We present a high-energy neutrino event generator, called LeptonInjector, alongside an event weighter, called LeptonWeighter. Both are designed for large-volume Cherenkov neutrino telescopes such as IceCube. The neutrino event generator allows for quick and flexible simulation of neutrino events within and around the detector volume, and implements the leading Standard Model neutrino interaction processes relevant for neutrino observatories: neutrino-nucleon deep-inelastic scattering and neutrino-electron annihilation. In this paper, we discuss the event generation algorithm, the weighting algorithm, and the main functions of the publicly available code, with examples.

Particle physicsPhysics::Instrumentation and DetectorsComputer scienceAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Physics and AstronomyCHERENKOV LIGHT YIELDWeighting01 natural sciencesHigh Energy Physics - Experiment010305 fluids & plasmasStandard ModelHigh Energy Physics - Experiment (hep-ex)Neutrino interactionHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsCherenkov radiationEvent generatorEvent generator; Neutrino generator; Neutrino interaction; Neutrino simulation; WeightingGenerator (computer programming)hep-exEvent (computing)ICEHigh Energy Physics::PhenomenologyDetectorhep-phComputational Physics (physics.comp-ph)Quantitative Biology::GenomicsHigh Energy Physics - Phenomenologyphysics.comp-phHardware and ArchitectureHigh Energy Physics::ExperimentNeutrino simulationNeutrino generatorEvent generatorNeutrinoPhysics - Computational PhysicsLeptonComputer Physics Communications
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Feasibility study for the measurement of πN transition distribution amplitudes at P¯ANDA in p¯p→J/ψπ0

2017

The exclusive charmonium production process in (P) over barp annihilation with an associated pi 0 meson (p) over barp -> J/psi pi(0) is studied in the framework of QCD collinear factorization. The feasibility of measuring this reaction through the J/psi -> e(+) e(-) decay channel with the AntiProton ANnihilation at DArmstadt ((P) over bar ANDA) experiment is investigated. Simulations on signal reconstruction efficiency as well as the background rejection from various sources including the (P) over barp -> pi(+)pi(-)pi(0) and (p) over barp -> J/psi pi(0)pi(0) reactions are performed with PANDAROOT, the simulation and analysis software framework of the (P) over bar ANDA experiment. It is show…

Quantum chromodynamicsPhysicsParticle physicsLuminosity (scattering theory)AnnihilationMeson010308 nuclear & particles physics7. Clean energy01 natural sciencesParticle identificationNuclear physicsFactorizationAntiproton0103 physical sciencesHigh Energy Physics::Experiment010306 general physicsBar (unit)Physical Review D
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Leading order determination of the gluon polarisation from DIS events with high-pThadron pairs

2013

We present a determination of the gluon polarisation Delta g/g in the nucleon, based on the longitudinal double-spin asymmetry of DIS events with Q(2) > 1 (GeV/c)(2) including a pair of large transverse-momentum hadrons in the final state. The data were obtained by the COMPASS experiment at CERN using a 160 GeV/c polarised muon beam scattering off a polarised (LiD)-Li-6 target. The gluon polarisation is evaluated by a Neural Network approach for three intervals of the gluon momentum fraction x(g) covering the range 0.04 < x(g) < 0.27. The values obtained at leading order in QCD do not show any significant dependence on x(g). Their average is Delta g/g = 0.125 +/- 0.060 (stat.) +/- 0.063 (sy…

PhysicsQuantum chromodynamicsNuclear and High Energy PhysicsParticle physicsMuonProton010308 nuclear & particles physicsHadronDeep inelastic scattering01 natural sciencesGluonNuclear physics0103 physical sciencesCOMPASS experimentHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsNucleonPhysics Letters B
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Exclusive muoproduction on transversely polarised protons and deuterons

2012

The transverse target spin azimuthal asymmetry A(UT)(sin(phi-phi s)) in hard exclusive production of rho(0) mesons was measured at COMPASS by scattering 160 GeV/c muons off transversely polarised protons and deuterons. The measured asymmetry is sensitive to the nucleon helicity-flip generalised parton distributions E-q, which are related to the orbital angular momentum of quarks in the nucleon. The Q(2), x-B-j and p(T)(2) dependence of A(UT)(sin(phi-phi s)) is presented in a wide kinematic range: 1 (GeV/c)(2) < Q(2) < 10 (GeV/c)(2), 0.003 < xB(j) < 0.3 and 0.05 (GeV/c)(2) < p(T)(2) < 0.5 (GeV/c)(2) for protons or 0.10 (GeV/c)(2) < p(T)(2) < 0.5 (GeV/c)(2) for deuterons. Results for deuteron…

QuarkPhysicsNuclear and High Energy PhysicsParticle physicsAngular momentumMuonMeson010308 nuclear & particles physicsmedia_common.quotation_subjectNuclear TheoryParton01 natural sciencesAsymmetryNuclear physics0103 physical sciencesHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsNucleonmedia_commonSpin-½Nuclear Physics B
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Identification and characterization of novel associations in the CASP8/ALS2CR12 region on chromosome 2 with breast cancer risk.

2014

Previous studies have suggested that polymorphisms in CASP8 on chromosome 2 are associated with breast cancer risk. To clarify the role of CASP8 in breast cancer susceptibility, we carried out dense genotyping of this region in the Breast Cancer Association Consortium (BCAC). Single-nucleotide polymorphisms (SNPs) spanning a 1 Mb region around CASP8 were genotyped in 46 450 breast cancer cases and 42 600 controls of European origin from 41 studies participating in the BCAC as part of a custom genotyping array experiment (iCOGS). Missing genotypes and SNPs were imputed and, after quality exclusions, 501 typed and 1232 imputed SNPs were included in logistic regressionmodels adjusting for stud…

Genotyping TechniquesResearch Support U.S. Gov't P.H.S.CASP8 and FADD-Like Apoptosis Regulating ProteinGenome-wide association studyP.H.S.Medical and Health SciencesBreast and Ovarian Cancer Susceptibility (BOCS) StudyMedizinische FakultätGenetics(clinical)Non-U.S. Gov'tGenetics (clinical)GeneticsGenetics & HeredityvariantsCaspase 8Research Support Non-U.S. Gov'tAssociation Studies ArticlesGeneral MedicineBiological Sciencesddc:Chromosomes Human Pair 2kConFab InvestigatorsFemaleGENICA NetworkAustralian Ovarian Cancer Study GroupEuropean Continental Ancestry GroupNon-P.H.S.Single-nucleotide polymorphismBreast Neoplasms-BiologyResearch SupportPolymorphism Single NucleotideWhite PeopleN.I.H.Breast cancerResearch Support N.I.H. ExtramuralSDG 3 - Good Health and Well-beingmedicineGeneticsJournal ArticleHumansGenetic Predisposition to Diseaseddc:610geneGenotyping TechniquesGenotypingMolecular BiologyGenetic associationdiseaseExtramuralProteinsOdds ratiomedicine.diseasesusceptibility lociMinor allele frequencyCase-Control Studiesgenome-wide associationenhancersU.S. Gov'tcasp8Research Support U.S. Gov't Non-P.H.S.Genome-Wide Association Study
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Study of doubly strange systems using stored antiprotons

2016

Bound nuclear systems with two units of strangeness are still poorly known despite their importance for many strong interaction phenomena. Stored antiprotons beams in the GeV range represent an unparalleled factory for various hyperon-antihyperon pairs. Their outstanding large production probability in antiproton collisions will open the floodgates for a series of new studies of systems which contain two or even more units of strangeness at the PANDA experiment at FAIR. For the first time, high resolution gamma-spectroscopy of doubly strange Lambda Lambda-hypernuclei will be performed, thus complementing measurements of ground state decays of Lambda Lambda-hypernuclei at J-PARC or possible …

Particle physicsNuclear and High Energy PhysicsCOLLISIONSStrong interactionNuclear TheoryhyperatomsAntiprotons; Hyperatoms; Hypernuclei; Strangeness; Nuclear and High Energy PhysicsEXCHANGE CURRENTSAntiprotonsStrangeness01 natural sciencesPartícules (Física nuclear)NONuclear physicsSubatomär fysikHypemucleistrangenessDECUPLET BARYONSELECTRIC QUADRUPOLE-MOMENTSHyperatoms0103 physical sciencesSubatomic PhysicsHypernuclei010306 general physicsNuclear ExperimentPhysicshypernucleiNUCLEI010308 nuclear & particles physicsHyperonStrangenessTransport theoryDOUBLE-LAMBDA-HYPERNUCLEIMODELOMEGAAntiprotonPhysics::Accelerator PhysicsHeavy ionHigh Energy Physics::ExperimentantiprotonsINTERMEDIATE ENERGIESEMULSIONNuclear Physics A
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Spin asymmetry A1d and the spin-dependent structure function g1d of the deuteron at low values of x and Q2

2007

Abstract We present a precise measurement of the deuteron longitudinal spin asymmetry A 1 d and of the deuteron spin-dependent structure function g 1 d at Q 2 1 ( GeV / c ) 2 and 4 × 10 −5 x 2.5 × 10 −2 based on the data collected by the COMPASS experiment at CERN during the years 2002 and 2003. The statistical precision is tenfold better than that of the previous measurement in this region. The measured A 1 d and g 1 d are found to be consistent with zero in the whole range of x.

PhysicsNuclear and High Energy PhysicsRange (particle radiation)Large Hadron Collider010308 nuclear & particles physicsmedia_common.quotation_subjectStructure functionZero (complex analysis)01 natural sciencesAsymmetryNuclear physicsDeuterium0103 physical sciencesCOMPASS experiment010306 general physicsSpin-½media_commonPhysics Letters B
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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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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 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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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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Erratum to: Hadron transverse momentum distributions in muon deep inelastic scattering at 160 GeV/ $$c$$ c

2015

Author(s): Adolph, C; Alekseev, MG; Alexakhin, VY; Alexandrov, Y; Alexeev, GD; Amoroso, A; Andrieux, V; Austregesilo, A; Badelek, B; Balestra, F; Barth, J; Baum, G; Bedfer, Y; Berlin, A; Bernhard, J; Bertini, R; Bicker, K; Bieling, J; Birsa, R; Bisplinghoff, J; Boer, M; Bordalo, P; Bradamante, F; Braun, C; Bravar, A; Bressan, A; Buchele, M; Burtin, E; Capozza, L; Chiosso, M; Chung, SU; Cicuttin, A; Crespo, ML; Dalla Torre, S; Dasgupta, SS; Dasgupta, S; Denisov, OY; Donskov, SV; Doshita, N; Duic, V; Dunnweber, W; Dziewiecki, M; Efremov, A; Elia, C; Eversheim, PD; Eyrich, W; Faessler, M; Ferrero, A; Filin, A; Finger, M; Finger Jr, M; Fischer, H; Franco, C; du Fresne von Hohenesche, N; Friedri…

Nuclear physicsPhysicsMuonPhysics and Astronomy (miscellaneous)010308 nuclear & particles physics0103 physical sciencesHadronTransverse momentum010306 general physicsDeep inelastic scattering53001 natural sciencesEngineering (miscellaneous)The European Physical Journal C
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A Convolutional Neural Network based Cascade Reconstruction for the IceCube Neutrino Observatory

2021

Continued improvements on existing reconstruction methods are vital to the success of high-energy physics experiments, such as the IceCube Neutrino Observatory. In IceCube, further challenges arise as the detector is situated at the geographic South Pole where computational resources are limited. However, to perform real-time analyses and to issue alerts to telescopes around the world, powerful and fast reconstruction methods are desired. Deep neural networks can be extremely powerful, and their usage is computationally inexpensive once the networks are trained. These characteristics make a deep learning-based approach an excellent candidate for the application in IceCube. A reconstruction …

FOS: Computer and information sciencesComputer Science - Machine LearningAstrophysics::High Energy Astrophysical Phenomenacs.LGData analysisFOS: Physical sciencesFitting methods01 natural sciencesConvolutional neural networkCalibration; Cluster finding; Data analysis; Fitting methods; Neutrino detectors; Pattern recognitionHigh Energy Physics - ExperimentIceCube Neutrino ObservatoryMachine Learning (cs.LG)High Energy Physics - Experiment (hep-ex)Pattern recognition0103 physical sciencesNeutrino detectors010303 astronomy & astrophysicsInstrumentationMathematical Physics010308 nuclear & particles physicsbusiness.industryhep-exDeep learningCluster findingDetectorNeutrino detectorComputer engineeringOrders of magnitude (time)13. Climate actionCascadeCalibrationPattern recognition (psychology)Artificial intelligencebusiness
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Characteristics of the diffuse astrophysical electron and Tau neutrino flux with six years of IceCube high energy cascade data

2020

We report on the first measurement of the astrophysical neutrino flux using particle showers (cascades) in IceCube data from 2010-2015. Assuming standard oscillations, the astrophysical neutrinos in this dedicated cascade sample are dominated (∼90%) by electron and tau flavors. The flux, observed in the sensitive energy range from 16 TeV to 2.6 PeV, is consistent with a single power-law model as expected from Fermi-type acceleration of high energy particles at astrophysical sources. We find the flux spectral index to be γ=2.53±0.07 and a flux normalization for each neutrino flavor of φastro=1.66-0.27+0.25 at E0=100 TeV, in agreement with IceCube's complementary muon neutrino results and wit…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Physics and AstronomyElectronpower spectrumflux [electron]energy [particle]01 natural sciencesIceCubeNuclear physics5/3Tau neutrinomuon0103 physical scienceslow [energy]Muon neutrinoddc:530010303 astronomy & astrophysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSPECTRUMSpectral indexMuon010308 nuclear & particles physicsHigh Energy Physics::Phenomenologyflavor [neutrino]RAYSflux [neutrino]accelerationshowersoscillationPhysics and Astronomy13. Climate actionEnergy cascadePhysique des particules élémentairesastro-ph.COhigh [energy]cascade [energy]High Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaFermi Gamma-ray Space TelescopeAstrophysics - Cosmology and Nongalactic Astrophysics
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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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Combined sensitivity to the neutrino mass ordering with JUNO, the IceCube Upgrade, and PINGU

2020

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

Physics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorsantineutrino/e: energy spectrumJoint analysishiukkasfysiikka7. Clean energy01 natural sciencesString (physics)PINGUHigh Energy Physics - ExperimentSubatomär fysikHigh Energy Physics - Experiment (hep-ex)neutrino: atmosphereSubatomic Physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Particle Physics Experimentsneutrino: massphysics.ins-detPhysicsJUNOPhysicsneutriinotoscillation [neutrino]Instrumentation and Detectors (physics.ins-det)massa (fysiikka)atmosphere [neutrino]tensionneutrino: nuclear reactormass difference [neutrino]ddc:UpgradePhysique des particules élémentairesnuclear reactor [neutrino]proposed experimentNeutrinoperformanceParticle physicsAstrophysics::High Energy Astrophysical Phenomenaneutrino: mass differenceFOS: Physical sciencesddc:500.25300103 physical sciencesEnergy spectrumIceCube: upgradeOSCILLATIONSddc:530Sensitivity (control systems)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationenergy spectrum [antineutrino/e]hep-ex010308 nuclear & particles physicssensitivityPhysics and Astronomymass [neutrino]stringupgrade [IceCube]High Energy Physics::ExperimentReactor neutrinoneutrino: oscillationMATTER
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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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The Deuteron Spin-dependent Structure Function g1(d) and its First Moment

2007

We present a measurement of the deuteron spin-dependent structure function g1d based on the data collected by the COMPASS experiment at CERN during the years 2002-2004. The data provide an accurate evaluation for Gamma_1^d, the first moment of g1d(x), and for the matrix element of the singlet axial current, a0. The results of QCD fits in the next to leading order (NLO) on all g1 deep inelastic scattering data are also presented. They provide two solutions with the gluon spin distribution function Delta G positive or negative, which describe the data equally well. In both cases, at Q^2 = 3 (GeV/c)^2 the first moment of Delta G is found to be of the order of 0.2 - 0.3 in absolute value.

Nuclear and High Energy PhysicsParticle physicsg(1)FOS: Physical sciencesAbsolute valuespinspin structure function g101 natural sciencesCOMPASSHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)polarised deep inelastic scatteringdeep inelastic scatteringstructure function0103 physical sciencesCOMPASS experimentA(1)polarised deep inelastic scattering; COMPASS; spin structure function g1; QCD analysisSinglet state010306 general physicsSpin-½Quantum chromodynamicsPhysics010308 nuclear & particles physicsDeep inelastic scatteringGluonQCD analysisDistribution functionHigh Energy Physics::ExperimentParticle Physics - Experiment
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A new measurement of the Collins and Sivers asymmetries on a transversely polarised deuteron target

2007

New high precision measurements of the Collins and Sivers asymmetries of charged hadrons produced in deep-inelastic scattering of muons on a transversely polarised 6LiD target are presented. The data were taken in 2003 and 2004 with the COMPASS spectrometer using the muon beam of the CERN SPS at 160 GeV/c. Both the Collins and Sivers asymmetries turn out to be compatible with zero, within the present statistical errors, which are more than a factor of 2 smaller than those of the published COMPASS results from the 2002 data. The final results from the 2002, 2003 and 2004 runs are compared with naive expectations and with existing model calculations.

QuarkdeuteronNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsSivers asymmetryHadrontransversity and Sivers functionFOS: Physical sciencesCOMPASS01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)nucleon structure; transverse spin and transverse momentum; transversity and Sivers functions; deuteron; COMPASS experimentCompass0103 physical sciencesCOMPASS experimentCollins010306 general physicsNuclear ExperimentCOMPASS experimenttransversityPhysicsLarge Hadron ColliderMuonSpectrometer010308 nuclear & particles physicsScatteringtransversity and Sivers functionsnucleon structureHigh Energy Physics::Experimenttransverse spin and transverse momentumasymmetryParticle Physics - Experimenttransverse single-spin asymmetry
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Feasibility study for the measurement of pi N transition distribution amplitudes at (P)over-barANDA in (P)over-barp -> J/psi pi(0)

2017

The exclusive charmonium production process in pp¯ annihilation with an associated π0 meson pp¯ → J=ψπ0 is studied in the framework of QCD collinear factorization. The feasibility of measuring this reaction through the J=ψ → eþe− decay channel with the AntiProton ANnihilation at DArmstadt (PANDA ¯ ) experiment is investigated. Simulations on signal reconstruction efficiency as well as the background rejection from various sources including the pp¯ → πþπ−π0 and pp¯ → J=ψπ0π0 reactions are performed with PANDAROOT, the simulation and analysis software framework of the PANDA ¯ experiment. It is shown that the measurement can be done at PANDA ¯ with significant constraining power under the assu…

Partícules (Física nuclear)
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Constraints on neutrino emission from nearby galaxies using the 2MASS redshift survey and IceCube

2020

The distribution of galaxies within the local universe is characterized by anisotropic features. Observatories searching for the production sites of astrophysical neutrinos can take advantage of these features to establish directional correlations between a neutrino dataset and overdensities in the galaxy distribution in the sky. The results of two correlation searches between a seven-year time-integrated neutrino dataset from the IceCube Neutrino Observatory, and the 2MASS Redshift Survey (2MRS) catalog are presented here. The first analysis searches for neutrinos produced via interactions between diffuse intergalactic Ultra-High Energy Cosmic Rays (UHECRs) and the matter contained within …

Astrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]FOS: Physical sciencesanisotropyAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesIceCubeIceCube Neutrino Observatoryneutrino astronomyneutrino experiments0103 physical sciencessiteAstrophysics::Galaxy Astrophysicsastro-ph.HEPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)densityneutrino astronomy; neutrino detectors; neutrino experiments010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysicsflux [neutrino]redshiftRedshift surveyGalaxyRedshiftobservatoryNeutrino detectorPhysics and Astronomymultiplet13. Climate actioncorrelationPhysique des particules élémentairesIntergalactic travelHigh Energy Physics::ExperimentgalaxyNeutrinoNeutrino astronomyAstrophysics - High Energy Astrophysical Phenomenaneutrino detectors
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Computational Techniques for the Analysis of Small Signals in High-Statistics Neutrino Oscillation Experiments

2020

The current and upcoming generation of Very Large Volume Neutrino Telescopes – collecting unprecedented quantities of neutrino events – can be used to explore subtle effects in oscillation physics, such as (but not restricted to) the neutrino mass ordering. The sensitivity of an experiment to these effects can be estimated from Monte Carlo simulations. With the high number of events that will be collected, there is a trade-off between the computational expense of running such simulations and the inherent statistical uncertainty in the determined values. In such a scenario, it becomes impractical to produce and use adequately-sized sets of simulated events with traditional methods, such as M…

data analysis methodNuclear and High Energy PhysicsMonte Carlo methodFVLV nu TData analysis; Detector; KDE; MC; Monte Carlo; Neutrino; Neutrino mass ordering; Smoothing; Statistics; VLVνTData analysisKDEFOS: Physical sciences01 natural sciencesIceCubeHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)statistical analysisnumerical methods0103 physical sciencesStatisticsNeutrinoddc:530Sensitivity (control systems)MC010306 general physicsNeutrino oscillationInstrumentation and Methods for Astrophysics (astro-ph.IM)InstrumentationMonte CarloPhysicsVLVνT010308 nuclear & particles physicsOscillationStatisticsoscillation [neutrino]ObservableDetectorMonte Carlo [numerical calculations]WeightingNeutrino mass orderingPhysics and AstronomyPhysics - Data Analysis Statistics and ProbabilityPhysique des particules élémentairesNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsMATTERData Analysis Statistics and Probability (physics.data-an)SmoothingSmoothing
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IceCube Search for High-Energy Neutrino Emission from TeV Pulsar Wind Nebulae

2020

Pulsar wind nebulae (PWNe) are the main gamma-ray emitters in the Galactic plane. They are diffuse nebulae that emit nonthermal radiation. Pulsar winds, relativistic magnetized outflows from the central star, shocked in the ambient medium produce a multiwavelength emission from the radio through gamma-rays. Although the leptonic scenario is able to explain most PWNe emission, a hadronic contribution cannot be excluded. A possible hadronic contribution to the high-energy gamma-ray emission inevitably leads to the production of neutrinos. Using 9.5 yr of all-sky IceCube data, we report results from a stacking analysis to search for neutrino emission from 35 PWNe that are high-energy gamma-ray…

010504 meteorology & atmospheric sciencesHigh-energy astronomyAstrophysics::High Energy Astrophysical PhenomenaNeutrino astronomy; High energy astrophysicsFOS: Physical sciencesCosmic rayAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences7. Clean energyPulsar0103 physical sciences010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEAstronomy and AstrophysicsGalactic planeCOSMIC-RAYSCRAB-NEBULACrab NebulaPhysics and AstronomyNeutrino astronomy13. Climate actionSpace and Planetary ScienceGALACTIC SOURCESDISCOVERYPhysique des particules élémentairesHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyAstrophysics - High Energy Astrophysical PhenomenaHigh energy astrophysicsGAMMA-RAY EMISSIONLepton
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Measurement of the Spin Structure of the Deuteron in the DIS Region

2005

We present a new measurement of the longitudinal spin asymmetry A_1^d and the spin-dependent structure function g_1^d of the deuteron in the range 1 GeV^2 &lt; Q^2 &lt; 100 GeV^2 and 0.004&lt; x &lt;0.7. The data were obtained by the COMPASS experiment at CERN using a 160 GeV polarised muon beam and a large polarised 6-LiD target. The results are in agreement with those from previous experiments and improve considerably the statistical accuracy in the region 0.004 &lt; x &lt; 0.03.

Nuclear and High Energy PhysicsParticle physicsmedia_common.quotation_subjectFOS: Physical sciencesSpin structure01 natural sciencesAsymmetryCOMPASSHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)deep inelastic scatteringstructure function0103 physical sciencesCOMPASS experiment010306 general physicsNuclear Experimentmedia_commonSpin-½PhysicsLarge Hadron ColliderMuon010308 nuclear & particles physicsDeep inelastic scatteringstructure function; COMPASS; DEEP INELASTIC-SCATTERINGstructure functionsDEEP INELASTIC-SCATTERINGHigh Energy Physics::ExperimentParticle Physics - ExperimentBeam (structure)
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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 Collins and Sivers asymmetries on transversely polarised protons

2010

The Collins and Sivers asymmetries for charged hadrons produced in deeply inelastic scattering on transversely polarised protons have been extracted from the data collected in 2007 with the CERN SPS muon beam tuned at 160 GeV/c. At large values of the Bjorken x variable non-zero Collins asymmetries are observed both for positive and negative hadrons while the Sivers asymmetry for positive hadrons is slightly positive over almost all the measured x range. These results nicely support the present theoretical interpretation of these asymmetries, in terms of leading-twist quark distribution and fragmentation functions.

QuarkNuclear and High Energy PhysicsParticle physicsProtonmedia_common.quotation_subjectSivers asymmetryNuclear TheoryHadronFOS: Physical sciencesInelastic scattering01 natural sciencesAsymmetryCOMPASSHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesTransverse spin effectNuclear Experiment010306 general physicsmedia_commonPhysicsMuonLarge Hadron Collider010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyTransverse spin effectsCollins asymmetryPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentTransverse spin effects; Proton; Collins asymmetry; Sivers asymmetry; COMPASSProtonParticle Physics - Experiment
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Gluon polarization in the nucleon from quasi-real photoproduction of high-pT hadron pairs

2006

Abstract We present a determination of the gluon polarization Δ G / G in the nucleon, based on the helicity asymmetry of quasi-real photoproduction events, Q 2 1 ( GeV / c ) 2 , with a pair of large transverse-momentum hadrons in the final state. The data were obtained by the COMPASS experiment at CERN using a 160 GeV polarized muon beam scattered on a polarized 6 LiD target. The helicity asymmetry for the selected events is 〈 A ∥ / D 〉 = 0.002 ± 0.019 ( stat ) ± 0.003 ( syst ) . From this value, we obtain in a leading-order QCD analysis Δ G / G = 0.024 ± 0.089 ( stat ) ± 0.057 ( syst ) at x g = 0.095 and μ 2 ≃ 3 ( GeV / c ) 2 .

Quantum chromodynamicsPhysicsNuclear and High Energy PhysicsParticle physicsMuon010308 nuclear & particles physicsHadronDeep inelastic scattering01 natural sciencesHelicityGluonNuclear physics0103 physical sciencesCOMPASS experimentHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsNucleonPhysics Letters B
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