Search results for "ARTICLES"

showing 10 items of 9626 documents

STUDIES OF VARIABILITY IN PROTO-PLANETARY NEBULAE. II. LIGHT AND VELOCITY CURVE ANALYSES OF IRAS 22272+5435 AND 22223+4327

2013

We have carried out a detailed observational study of the light, color, and velocity variations of two bright, carbon-rich proto-planetary nebulae, IRAS 22223+4327 and 22272+5435. The light curves are based upon our observations from 1994 to 2011, together with published data by Arkhipova and collaborators. They each display four significant periods, with primary periods for IRAS 22223+4327 and 22272+5435 being 90 and 132 days, respectively. For each of them, the ratio of secondary to primary period is 0.95, a value much different from that found in Cepheids, but which may be characteristic of post-asymptotic giant branch (AGB) stars. Fewer significant periods are found in the smaller radia…

oscillations [stars]Cepheid variableFOS: Physical sciencesAstrophysics01 natural sciences0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicsgeneral [planetary nebulae]010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsGalaxy rotation curvePhysicsNebula010308 nuclear & particles physicsAstronomy and AstrophysicsLight curveAGB and post-AGB [stars]Planetary nebulaRadial velocityStarsAmplitudeAstrophysics - Solar and Stellar Astrophysicsvariables: general [stars]Space and Planetary Scienceindividual (IRAS 22223+4327 IRAS 22272+5435) [stars]Astrophysics::Earth and Planetary AstrophysicsThe Astrophysical Journal
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Pulsating B and Be stars in the Small Magellanic Cloud

2008

Context: Stellar pulsations in main-sequence B-type stars are driven by the kappa-mechanism due to the Fe-group opacity bump. The current models do not predict the presence of instability strips in the B spectral domain at very low metallicities. As the metallicity of the SMC is lower than Z=0.005, it constitutes a very suitable object to test these predictions. Aims: The main objective is to investigate the existence of B-type pulsators at low metallicities, searching for short-term periodic variability in absorption-line B and Be stars in the SMC. The analysis has been performed in a sample of 313 B and Be stars with fundamental astrophysical parameters accurately determined from high-res…

oscillations [stars]statistics [Stars]Be starHertzsprung–Russell diagramMetallicityFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesStars : emission-line Be; stars : oscillations; Stars : early-type; Stars : statistics; Galaxies : Magellanic Cloudssymbols.namesakeMagellanic Clouds [Galaxies]early-type [Stars]0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::GalaxiasAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsAstrophysics (astro-ph)Astronomy and AstrophysicsLight curveGalaxy:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Galaxias [UNESCO]Stars13. Climate actionSpace and Planetary Scienceemission-line Be [Stars]symbolsSmall Magellanic CloudAstrophysics::Earth and Planetary AstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::EstrellasInstability strip:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Estrellas [UNESCO]
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First measurement of quarkonium polarization in nuclear collisions at the LHC

2021

The polarization of inclusive J/$\psi$ and $\Upsilon(1{\rm S})$ produced in Pb-Pb collisions at $\sqrt{s_{\rm{NN}}}=5.02$ TeV at the LHC is measured with the ALICE detector. The study is carried out by reconstructing the quarkonium through its decay to muon pairs in the rapidity region $2.5<y<4$ and measuring the polar and azimuthal angular distributions of the muons. The polarization parameters $\lambda_{\theta}$, $\lambda_{\phi}$ and $\lambda_{\theta\phi}$ are measured in the helicity and Collins-Soper reference frames, in the transverse momentum interval $2<p_{\rm T}<10$ GeV/$c$ and $p_{\rm T}<15$ GeV/$c$ for the J/$\psi$ and $\Upsilon(1{\rm S})$, respectively. The polarization parameter…

p(p)over-bar collisions ; j/psi production ; pp collisions ; suppression ; rapidity ; matterheavy ion: scatteringPhysics::Instrumentation and DetectorsVDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Kjerne- og elementærpartikkelfysikk: 431P(P)OVER-BAR COLLISIONSQuarkoniumPb-Pb collisionshiukkasfysiikkanucl-ex01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)ALICE[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]J/psi(3100): polarizationNuclear Experiment (nucl-ex)Nuclear ExperimentNuclear ExperimentQuarkonium polarization ALICE nuclear collisionsquarkonium: polarizationPhysicsLarge Hadron ColliderPhysicsP(P)OVER-BAR COLLISIONS; J/PSI PRODUCTION; PP COLLISIONS; SUPPRESSION; RAPIDITY; MATTERPolarization (waves)QuarkoniumHelicitylcsh:QC1-9993. Good healthCERN LHC Collpolarisaatio (aaltoliike)polarization [Upsilon(9460)]LHCParticle Physics - ExperimentquarkoniumReference frameNuclear and High Energy Physicsmuon: angular distributionFOS: Physical sciencespolarization [J/psi(3100)]transverse momentum[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]114 Physical sciencesNuclear physicsscattering [heavy ion]0103 physical sciencesmuon: pairpolarization [quarkonium]Nuclear Physics - Experimentddc:530RapidityJ/PSI PRODUCTION5020 GeV-cms/nucleon010306 general physicsSUPPRESSIONALICE experiment heavy-ion collisions quarkoniapolarizationMuonPP COLLISIONShep-ex010308 nuclear & particles physicsangular distribution [muon]High Energy Physics::PhenomenologyALICE experimentheavy-ion collisionsquarkoniapolarization quarkonium Pb-Pb collisionsUpsilon(9460): polarizationLHC-Bpair [muon]rapidityQuarkonium; LHC; Pb-Pb collisionsQuark–gluon plasmaHigh Energy Physics::ExperimentMATTERlcsh:Physicsexperimental results
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Algebraic singularities have maximal reductive automorphism groups

1989

LetX = On/ibe an analytic singularity where ṫ is an ideal of theC-algebraOnof germs of analytic functions on (Cn, 0). Letdenote the maximal ideal ofXandA= AutXits group of automorphisms. An abstract subgroupequipped with the structure of an algebraic group is calledalgebraic subgroupofAif the natural representations ofGon all “higher cotangent spaces”are rational. Letπbe the representation ofAon the first cotangent spaceandA1=π(A).

p-groupPure mathematics32B30010308 nuclear & particles physicsGeneral Mathematics010102 general mathematicsOuter automorphism groupCotangent spaceReductive groupAutomorphism01 natural sciences14B12Inner automorphismAlgebraic group0103 physical sciencesComputingMethodologies_DOCUMENTANDTEXTPROCESSINGMaximal ideal13J1520G200101 mathematics32M05MathematicsNagoya Mathematical Journal
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Performance of the ALICE experiment at the CERN LHC

2014

ALICE is the heavy-ion experiment at the CERN Large Hadron Collider. The experiment continuously took data during the first physics campaign of the machine from fall 2009 until early 2013, using proton and lead-ion beams. In this paper we describe the running environment and the data handling procedures, and discuss the performance of the ALICE detectors and analysis methods for various physics observables.

p-p and Pb-Pb and p-Pb collisions at the LHCPhysics::Instrumentation and Detectors01 natural sciences07.05.-tParticle identificationHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)ALICEData acquisition29.40.-nAtomic and Molecular Physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear Experiment (nucl-ex)Nuclear ExperimentNuclear ExperimentAnalysis methodPhysicsLarge Hadron ColliderLHC; ALICE; heavy-ion collisions; particle detectors.Physicsparticle detectorsAtomic and Molecular Physics and Optics3. Good healthPRIRODNE ZNANOSTI. Fizika.LHCParticle Physics - Experimentheavy-ion collisionNuclear and High Energy PhysicsParticle physicsGroup method of data handlingFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Nuclear physicsLHC; ALICE; heavy-ion collisions; particle detectors29.85.-c0103 physical sciences010306 general physicsALICE; Heavy-ion collisions; LHC; Particle detectors; Atomic and Molecular Physics and Optics; Astronomy and Astrophysics; Nuclear and High Energy Physics010308 nuclear & particles physics25.75.-qALICE experimentAstronomy and Astrophysicsheavy-ion collisionsNATURAL SCIENCES. Physics.Physics::Accelerator Physics25.75.-q; 29.40.-n; 29.85.-c; 07.05.-t; LHC ALICE heavy-ion collisions particle detectorsHigh Energy Physics::ExperimentHeavy ionALICE; Heavy-ion collisions; LHC; Particle detectorsand OpticsALICE (propellant)Detector performanceInternational Journal of Modern Physics A
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Measurement of the average shape of longitudinal profiles of cosmic-ray air showers at the Pierre Auger Observatory

2019

The profile of the longitudinal development of showers produced by ultra-high energy cosmic rays carries information related to the interaction properties of the primary particles with atmospheric nuclei. In this work, we present the first measurement of the average shower profile in traversed atmospheric depth at the Pierre Auger Observatory. The shapes of profiles are well reproduced by the Gaisser-Hillas parametrization within the range studied, for E>10 17.8 eV .A detailed analysis of the systematic uncertainties is performed using ten years of data and a full detector simulation. The average shape is quantified using two variables related to the width and asymmetry of the profile, and …

p: showersphoton: Cherenkovinteraction: modelAstronomyHadronpiastro-ph.HE; astro-ph.HE01 natural sciencesnitrogenironParametrization (atmospheric modeling)Monte Carlomedia_commonPhysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Range (particle radiation)photomultiplierSettore FIS/01 - Fisica SperimentaleDetectorAstrophysics::Instrumentation and Methods for AstrophysicsDETETOREScosmic rays detectors; ultra high energy cosmic rays; Astronomy and AstrophysicsAugerobservatorycosmic rays detectorscosmic rays detectors; ultra high energy cosmic raysgeometricalAstrophysics - High Energy Astrophysical PhenomenaasymmetrylongitudinalCherenkov counter: waterairmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayheliumultra high energy cosmic raysnucleus: atmosphereAsymmetry0103 physical sciencesHigh Energy Physicscosmic radiation: UHEcosmic rays detectorFLUORESCENCEAstrophysiquePierre Auger Observatoryelectron positronshowers: atmosphere010308 nuclear & particles physicsbackgrounddetector: surfaceshowers: spatial distributionparametrizationAstronomy and AstrophysicsAstronomieComputational physics13. Climate actiongamma rayExperimental High Energy Physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)Journal of Cosmology and Astroparticle Physics
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Feedback and Communication in Active Hydrogel Spheres with pH Fronts: Facile Approaches to Grow Soft Hydrogel Structures

2021

Abstract Compartmentalized reaction networks regulating signal processing, communication and pattern formation are central to living systems. Towards achieving life‐like materials, we compartmentalized urea‐urease and more complex urea‐urease/ester‐esterase pH‐feedback reaction networks into hydrogel spheres and investigate how fuel‐driven pH fronts can be sent out from these spheres and regulated by internal reaction networks. Membrane characteristics are installed by covering urease spheres with responsive hydrogel shells. We then encapsulate the two networks (urea‐urease and ester‐esterase) separately into different hydrogel spheres to devise communication, pattern formation and attracti…

pH feedback system540 Chemistry and allied sciencesSystems ChemistrySupramolecular chemistry3D printingPattern formationlife-like systemsNanotechnology010402 general chemistry01 natural sciencessupramolecular chemistryCatalysisResearch Articleshydrogels010405 organic chemistrybusiness.industrychemical reaction networksGeneral MedicineGeneral ChemistrySoft materials0104 chemical sciencesLiving systems540 ChemieSelf-healing hydrogelsSPHERESAlginate hydrogelbusinessResearch ArticleAngewandte Chemie International Edition
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Det finska prästerskapets roll i allmogens klagomål till kungs under Vasatiden (cirka 1550-1610-talet)

2018

papisto1500-lukupoliittinen kulttuuriArticlesArtikkelit
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The PANDA Endcap Disc DIRC

2018

Journal of Instrumentation 13(02), C02002 - C02002 (2018). doi:10.1088/1748-0221/13/02/C02002

particle identification [K]Physics::Instrumentation and Detectors61001 natural sciencesDIRCK: particle identificationOpticsPionDetection of internally reflected Cherenkov light0103 physical sciencesparticle identification [pi]ddc:610010306 general physicsNuclear ExperimentInstrumentationMathematical PhysicsCherenkov radiationPhysicsCherenkov counter: designRange (particle radiation)010308 nuclear & particles physicsbusiness.industryPANDADetectorSolid angleDESYLight guideTest beamdesign [Cherenkov counter]Radiator (engine cooling)Facility for Antiproton and Ion ResearchHigh Energy Physics::ExperimentPhotonicsbusinesspi: particle identificationperformance
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Open-source QCD analysis of nuclear parton distribution functions at NLO and NNLO

2019

We present new sets of nuclear parton distribution functions (nPDFs) at next-to-leading order (NLO) and next-to-next-to-leading order (NNLO). Our analyses are based on deeply inelastic scattering data with charged-lepton and neutrino beams on nuclear targets. In addition, a set of proton baseline PDFs is fitted within the same framework with the same theoretical assumptions. The results of this global QCD analysis are compared to existing nPDF sets and to the fitted cross sections. Also, the uncertainties resulting from the limited constraining power of the included experimental data are presented. The published work is based on an open-source tool, xFitter, which has been modified to be ap…

particle interactionsParticle physicsHEAVY FLAVOR PRODUCTIONProtonPREDICTIONSFOS: Physical sciencesPartonhiukkasfysiikkaInelastic scatteringPROTON114 Physical sciences01 natural sciencesUNCERTAINTIESnucleus-neutrino interactionsCROSS-SECTIONSSet (abstract data type)High Energy Physics - Phenomenology (hep-ph)DEPENDENCEquantum chromodynamics0103 physical sciencesnonperturbative effects in field theory010306 general physicsNuclear Experimentquantum field theoryperturbation theoryDEEP-INELASTIC-SCATTERINGQuantum chromodynamicsPhysics010308 nuclear & particles physics3-LOOP SPLITTING FUNCTIONSnucleon distributionSTRUCTURE-FUNCTION RATIOSDeep inelastic scatteringEVOLUTIONHigh Energy Physics - PhenomenologyDistribution functionQCD in nuclear reactionsnuclear matterHigh Energy Physics::ExperimentNeutrinoydinfysiikka
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