Search results for "010308 nuclear & particles physics"

showing 10 items of 6362 documents

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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Quantum and classical dynamics of heavy quarks in a quark-gluon plasma

2018

We derive equations for the time evolution of the reduced density matrix of a collection of heavy quarks and antiquarks immersed in a quark gluon plasma. These equations, in their original form, rely on two approximations: the weak coupling between the heavy quarks and the plasma, the fast response of the plasma to the perturbation caused by the heavy quarks. An additional semi-classical approximation is performed. This allows us to recover results previously obtained for the abelian plasma using the influence functional formalism. In the case of QCD, specific features of the color dynamics make the implementation of the semi-classical approximation more involved. We explore two approximate…

heavy quarksheavy ion: scatteringNuclear Theoryapproximation: semiclassicalHigh Energy Physics::LatticeMonte Carlo methoddensity matrix: reducedhiukkasfysiikkaquantum chromodynamics: plasma01 natural sciencesBoltzmann equationLangevin equationHigh Energy Physics - Phenomenology (hep-ph)quarkonium: heavyquantum electrodynamicsQuarkonium suppression[ PHYS.NUCL ] Physics [physics]/Nuclear Theory [nucl-th]quark gluon: plasmaMathematical physics[PHYS]Physics [physics]Quantum chromodynamicsPhysicsquarkonium: suppressionBoltzmann equationquark gluon plasmaLangevin equationHigh Energy Physics - Phenomenologyheavy quark: couplingQuarkNuclear and High Energy Physicsquark-gluon plasma[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]FOS: Physical sciencesNuclear Theory (nucl-th)quantum chromodynamics0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivityheavy quarkstochastic010306 general physicsplasma: weak couplingta114010308 nuclear & particles physicsHigh Energy Physics::Phenomenologykvarkki-gluoniplasmaTime evolutionPlasmaHeavy Ion Phenomenologyfree energyrecombinationabelian[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Quark–gluon plasmalcsh:QC770-798[ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::ExperimentJournal of High Energy Physics
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Review of Particle Physics

2020

The Review summarizes much of particle physics and cosmology. Using data from previous editions, plus 2,143 new measurements from 709 papers, we list, evaluate, and average measured properties of gauge bosons and the recently discovered Higgs boson, leptons, quarks, mesons, and baryons. We summarize searches for hypothetical particles such as supersymmetric particles, heavy bosons, axions, dark photons, etc. Particle properties and search limits are listed in Summary Tables. We give numerous tables, figures, formulae, and reviews of topics such as Higgs Boson Physics, Supersymmetry, Grand Unified Theories, Neutrino Mixing, Dark Energy, Dark Matter, Cosmology, Particle Detectors, Colliders, …

high energyleptonmixing [neutrino]High Energy Physics::LatticeCosmic microwave backgrounddiffractionTechnicolorAstrophysicsOmega01 natural sciencesPhysics Particles & Fieldshiggs-boson productionBig Bang nucleosynthesiscosmological model: parameter spacetaudark energyMonte CarlofieldspentaquarkinstrumentationSettore FIS/01gauge bosonAnomalous magnetic dipole momentdeep-inelastic scatteringnew physicsPhysicsDOUBLE-BETA-DECAYElectroweak interactiondensity [dark matter]HEAVY FLAVOURQuarkoniumreview; particle; physicsSUPERSYMMETRIC STANDARD MODELsquare-root-sPhysics Nucleargrand unified theoryboson: heavystatisticsPhysical SciencesHiggs bosonaxion: massflavor: violationNeutrinoELECTROWEAK SYMMETRY-BREAKINGnumerical calculations: Monte Carlophysicson-lineS013EPHQuarkheavy [boson]particle[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]Physics Multidisciplinaryanomalous magnetic-momentelectroweak radiative-correctionsdark matter: densityHiggs particlemesonneutrino masses neutrino mixing; neutrino oscillations114 Physical sciencesCHIRAL PERTURBATION-THEORYneutrino mixingStandard Modelquark0202 Atomic Molecular Nuclear Particle And Plasma PhysicsNucleosynthesisquantum chromodynamicsCP: violationDark matterddc:530particle physicsStrong Interactions010306 general physicssparticleS013DFgrand unified theoriesPRODUCTIONGauge bosonScience & Technologyneutrino oscillationsneutrino masses010308 nuclear & particles physicsC50 Other topics in experimental particle physicsParticle Data GroupAstronomy and AstrophysicsDeep inelastic scatteringto-leading-order* Automatic Keywords *heavy bosonaxiontables (particle physics)Tetraquarkproton-proton collisionsSupersymmetryhadronneutrino: mixing[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]cosmologyVolume (compression)HIGGS-BOSONUB-VERTICAL-BARcosmological modeldark energy densityexperimental methodsddc:539.72021Physics beyond the Standard Modelstandard modelgroup theoryGeneral Physics and Astronomytables particle physicshigh energy physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Quantum chromodynamicsPhysicsenergy: highE Rev 2016[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Settore FIS/01 - Fisica SperimentalephotonSupersymmetryNuclear & Particles Physicsparameter space [cosmological model]dark energy: densityhigh [energy]M013WXfermion-pair productionNuclear and High Energy PhysicsParticle physicsHiggs bosonreviewAstrophysics::Cosmology and Extragalactic AstrophysicsAstronomy & Astrophysics530dark matterstatistical analysisDouble beta decay0103 physical sciencesconservation lawcold dark-matterTAU LEPTONSAstrophysics::Galaxy AstrophysicstablesDEEP-INELASTIC-SCATTERINGelectroweak interactionHigh Energy Physics::Phenomenology750 GeV diphoton excessPRODUCTION CROSS-SECTIONbaryondensity [dark energy]Physics and AstronomygravitationCKM matrix[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::ExperimentsupersymmetryMinimal Supersymmetric Standard Model
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Measurement of the top quark pair production cross-section with ATLAS in the single lepton channel

2012

A measurement of the production cross-section for top quark pairs (t[bar over t]) in pp collisions at √s = 7 TeV is presented using data recorded with the ATLAS detector at the Large Hadron Collider. Events are selected in the single lepton topology by requiring an electron or muon, large missing transverse momentum and at least three jets. With a data sample of 35 pb[superscript −1], two different multivariate methods, one of which uses b-quark jet identification while the other does not, use kinematic variables to obtain cross-section measurements of σ[subscript t bar over t] = 187 ± 11 (stat.) [+18 over −17] (syst.) ± 6 (lumi.) pb and σ[subscript t bar over t] = 173 ± 17 (stat.) [+18 ove…

high-energy collider experimentcross-sectionTop quarkPhysics::Instrumentation and DetectorsAtlas detectortop physicsHadronHigh-energy collider experimentElectron01 natural sciences7. Clean energySettore FIS/04 - Fisica Nucleare e SubnucleareHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentQCDetectors de radiacióPhysicsQuantum chromodynamicsAtlas (topology)Settore FIS/01 - Fisica SperimentaleATLASTop physicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGLHCParticle Physics - ExperimentNuclear and High Energy PhysicsParticle physicsCross-sectionHigh-energy collider experiment; Cross-section; Top physicsCiências Naturais::Ciências Físicascross-section; high-energy collider experiment; top physics:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesTOP QUARK530Partícules (Física nuclear)Nuclear physics0103 physical sciencesddc:530High Energy Physics010306 general physicsScience & TechnologyPP COLLISIONS010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaPair productionHADRON-HADRON COLLISIONStop physics; high-energy collider experiment; cross-sectionCol·lisions (Física nuclear)Experimental High Energy PhysicsTEVHigh Energy Physics::ExperimentLepton
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SEU characterization of commercial and custom-designed SRAMs based on 90 nm technology and below

2020

International audience; The R2E project at CERN has tested a few commercial SRAMs and a custom-designed SRAM, whose data are complementary to various scientific publications. The experimental data include low- and high-energy protons, heavy ions, thermal, intermediate- and high-energy neutrons, high-energy electrons and high-energy pions.

high-energy protonsCOTS[PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph]käyttömuistitNuclear TheoryElectronHardware_PERFORMANCEANDRELIABILITY01 natural sciences7. Clean energyIonelektroniikkakomponentitNuclear physicsCross section (physics)Pion0103 physical sciencesNeutronionisoimaton säteilyStatic random-access memory010306 general physicsheavy ionsNuclear Experimentlow-energy protonsPhysicsLarge Hadron Collidercross section010308 nuclear & particles physicsionisoiva säteilyelectronsneutronsmuistit (tietotekniikka)SRAMCharacterization (materials science)säteilyfysiikkapionsSEU
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Lignin and Cellulose Content of Fermented Rice Straw with Aspergillus niger (van Tieghem) and Trichoderma mutan AA1

2021

The rice straw has potential to be used as an alternative ruminant feed. However, it has limiting factors i.e low crude protein, high crude fiber, lignin, cellulose, and silica content. To overcome the limiting factors, immersion in a solution of alkaline (lime) or fermentation by using inoculum microbial cellulolytic and lignocellulolytic (Trichoderma mutan AA1 and Aspergillus niger.). The research method was experimental, with four treatments and repeated five times. Completely randomized design was used and if there are differences among treatments a further test with DMRT was carried out (level 1 % and 5 %). These treatments were T0: The rice straw without t fermentation; T1: Fermented …

increase feed quality020209 energy02 engineering and technologyengineering.material01 natural scienceschemistry.chemical_compoundRuminant0103 physical sciences0202 electrical engineering electronic engineering information engineeringLigninFood scienceCellulosefermentationCompletely randomized designlcsh:Environmental sciencesLimelcsh:GE1-350biology010308 nuclear & particles physicsChemistryAspergillus nigerfungusfood and beveragesbiology.organism_classificationTrichodermaengineeringFermentationwaste to feedinoculumE3S Web of Conferences
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Sub-milliarcsecond imaging of a bright flare and ejection event in the extragalactic jet 3C 111

2020

Context. Flares in radio-loud active galactic nuclei are thought to be associated with the injection of fresh plasma into the compact jet base. Such flares are usually strongest and appear earlier at shorter radio wavelengths. Hence, very long baseline interferometry (VLBI) at millimeter(mm)-wavelengths is the best-suited technique for studying the earliest structural changes of compact jets associated with emission flares. Aims. We study the morphological changes of the parsec-scale jet in the nearby (z = 0.049) γ-ray bright radio galaxy 3C 111 following a flare that developed into a major radio outburst in 2007. Methods. We analyse three successive observations of 3C 111 at 86 GHz with th…

individual: 3C 111 [Galaxies]active [Galaxies]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesLibrary scienceAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGalaxies: individual: 3C 1117. Clean energy01 natural sciencesTechniques: high angular resolutionObservatory0103 physical sciencesVery-long-baseline interferometryAstrophysics::Solar and Stellar Astrophysicsmedia_common.cataloged_instanceEuropean union010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsVery Long Baseline Arraymedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsEuropean researchAstronomy and AstrophysicsGalaxies: activeMonitoring programRadio astronomy observatory3. Good healthhigh angular resolution [Techniques]Galaxies: jetsSpace and Planetary Sciencejets [Galaxies]Christian ministryAstrophysics - High Energy Astrophysical PhenomenaAstronomy &amp; Astrophysics
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A measurement of the neutron to 199Hg magnetic moment ratio

2014

The neutron gyromagnetic ratio has been measured relative to that of the 199Hg atom with an uncertainty of 0.8 ppm. We employed an apparatus where ultracold neutrons and mercury atoms are stored in the same volume and report the result γn/γHg=3.8424574(30).

inorganic chemicalsNuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsNeutron magnetic momentAtomic Physics (physics.atom-ph)Astrophysics::High Energy Astrophysical PhenomenaGyromagnetic ratioFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesPhysics - Atomic PhysicsNuclear physicsMagnetic momentGyromagnetic ratio0103 physical sciencesAtomNeutron[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Physics::Atomic PhysicsNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentPhysicsCondensed Matter::Quantum Gases[PHYS.PHYS.PHYS-ATOM-PH]Physics [physics]/Physics [physics]/Atomic Physics [physics.atom-ph]Magnetic moment010308 nuclear & particles physicsProton magnetic momenttechnology industry and agricultureQC0793Instrumentation and Detectors (physics.ins-det)Ultracold neutrons; Mercury atoms; Magnetic moment; Gyromagnetic ratioQC0770lcsh:QC1-999Mercury atomsElectric dipole momentbiological sciencesUltracold neutronslipids (amino acids peptides and proteins)Astrophysics::Earth and Planetary AstrophysicsAtomic physicsUltracold neutronslcsh:PhysicsPhysics Letters B
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Measurement of Atmospheric Neutrino Oscillations at 6–56 GeV with IceCube DeepCore

2018

We present a measurement of the atmospheric neutrino oscillation parameters using three years of data from the IceCube Neutrino Observatory. The DeepCore infill array in the center of IceCube enables the detection and reconstruction of neutrinos produced by the interaction of cosmic rays in Earth's atmosphere at energies as low as ∼5 GeV. That energy threshold permits measurements of muon neutrino disappearance, over a range of baselines up to the diameter of the Earth, probing the same range of L/Eν as long-baseline experiments but with substantially higher-energy neutrinos. This analysis uses neutrinos from the full sky with reconstructed energies from 5.6 to 56 GeV. We measure Δm322=2.31…

interaction [cosmic radiation]Physics::Instrumentation and DetectorsSolar neutrinoGeneral Physics and Astronomy01 natural sciences7. Clean energyHigh Energy Physics - ExperimentIceCubeSubatomär fysikHigh Energy Physics - Experiment (hep-ex)ObservatorySubatomic PhysicsTOOLPhysicsoscillation [neutrino]Astrophysics::Instrumentation and Methods for Astrophysicsatmosphere [neutrino]threshold [energy]mass difference [neutrino]ddc:observatoryNeutrino detectorPhysique des particules élémentairesAstrophysics::Earth and Planetary AstrophysicsNeutrinoParticle physicscosmic radiation [neutrino]acceleratorAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:500.2Physics and Astronomy(all)IceCube Neutrino ObservatoryPhysics and Astronomy (all)0103 physical sciencesneutrino/muddc:530energy: high [neutrino]010306 general physicsNeutrino oscillationAstroparticle physics010308 nuclear & particles physicsICEHigh Energy Physics::PhenomenologyAstronomySolar neutrino problemPhysics and Astronomy13. Climate actionmass [neutrino]High Energy Physics::ExperimentSYSTEMmixing angle [neutrino]experimental resultsPhysical Review Letters
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Testing effects of Lorentz invariance violation in the propagation of astroparticles with the Pierre Auger Observatory

2021

The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargüe. We are very grateful to the following agencies and organizations for financial support: Argentina — Comisión Nacional de Energía Atómica; Agencia Nacional de Promoción Científica y Tecnológica (ANPCyT); Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET); Gobierno de la Provincia de Mendoza; Municipalidad de Malargüe; NDM Holdings and Valle Las Leñas; in gratitude for their continuing cooperation over land access; Australia — the Australian Research Council; Be…

interaction [cosmic radiation]mass spectrum [cosmic radiation]dispersion relationAstronomyAstrophysics::High Energy Astrophysical Phenomenaenergy spectrumcosmic ray experimentFOS: Physical sciencesultra high energy cosmic rayscosmic radiation: interactioninvariance: Lorentz01 natural sciences530UHEultra high energy cosmic rayenergy: thresholdFundamental physics gravitational waves LISA Tests of general relativityCosmic ray experiments0103 physical sciencespropagationddc:530physics of the early universeHigh Energy PhysicsLorentz [invariance]010303 astronomy & astrophysicsphoton: fluxflux [photon]Lorentz [violation]High Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEenergy: high010308 nuclear & particles physicscosmic radiation: mass spectrumcosmic ray experiments; ultra high energy cosmic rays; physics of the early universeSettore FIS/01 - Fisica SperimentaleAstronomy and AstrophysicsASTROFÍSICAUltra-high energy cosmic raysthreshold [energy]violation: LorentzAugerobservatoryelectromagnetickinematicsExperimental High Energy Physicshigh [energy]cosmic ray experimentsAstrophysics - High Energy Astrophysical PhenomenaPhysics of the early universe
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