Search results for " particles"

showing 10 items of 6711 documents

Response of AGATA segmented HPGe detectors to gamma rays up to 15.1MeV

2013

WOS: 000314826000009

AGATA; Gamma-ray spectroscopy; Gamma-ray tracking; HPGe detectors; Pulse-shape and gamma-ray tracking algorithms; Semiconductor detector performance and simulationsNuclear and High Energy PhysicsPulse-shape and gamma-ray tracking algorithmsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSemiconductor detector performance and simulationsTracking (particle physics)01 natural sciencesNuclear physicsGamma-ray tracking0103 physical sciencesGamma spectroscopyddc:530Gamma-ray spectroscopyNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentInstrumentationNuclear ExperimentDetectors de radiacióPhysicsSpectrometer010308 nuclear & particles physicsDetectorHPGe detectorsGamma ray81V35Semiconductor detectorAGATAFísica nuclearHpge detectorAGATA
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Microbiology and atmospheric processes: research challenges concerning the impact of airborne micro-organisms on the atmosphere and climate

2011

 Cet article a fait l'objet d'une discussion dans "Morris, C. E., Sands, D. C., Bardin, M., Jaenicke, R., Vogel, B., Leyronas, C., Ariya, P. A., and Psenner, R.: Microbiology and atmospheric processes: an upcoming era of research on bio-meteorology, Biogeosciences Discuss., 5, 191-212, doi:10.5194/bgd-5-191-2008, 2008."; International audience; For the past 200 years, the field of aerobiology has explored the abundance, diversity, survival and transport of micro-organisms in the atmosphere. Micro-organisms have been explored as passive and severely stressed riders of atmospheric transport systems. Recently, an interest in the active roles of these micro-organisms has emerged along with prop…

AIRBORNE DISSEMINATION010504 meteorology & atmospheric sciencesMeteorologyAEROBIOLOGY;BIOLOGICAL AEROSOLS;BIO-METEOROLOGY;TRANSPORT;AIRBORNE DISSEMINATION;BIOLOGICAL PROPERTIES;ATMOSPHERIC PROCESSES;BIOSPHERE;CLIMATE CHANGEEarth scienceBiomeCLIMATE CHANGEBiological particleslcsh:Lifemodélisation spatialeBIOSPHERE010501 environmental sciencesBiologyAtmosphere (architecture and spatial design)01 natural sciencesBIO-METEOROLOGYATMOSPHERIC PROCESSESBIOLOGICAL AEROSOLSlcsh:QH540-549.5AEROBIOLOGYddc:550microbiologieEcology Evolution Behavior and Systematics0105 earth and related environmental sciencesEarth-Surface Processeschangement climatiquemicroorganismeBIOLOGICAL PROPERTIESclimatlcsh:QE1-996.5microorganisme aerienRadiative forcingTRANSPORT[SDV.BBM.BC]Life Sciences [q-bio]/Biochemistry Molecular Biology/Biomolecules [q-bio.BM]lcsh:GeologyEarth sciencesatmosphèrelcsh:QH501-53113. Climate actionAtmospheric chemistrylcsh:EcologyMetabolic activityBiogeosciences
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Updated measurement of the τ lepton lifetime

1997

A new measurement of the mean lifetime of the tau lepton is presented. Three different analysis methods are applied to a sample of 90000 tau pairs, collected in 1993 and 1994 with the ALEPH detector at LEP. The average of this measurement and those previously published by ALEPH is tau_tau = 290.1 +- 1.5 +- 1.1 fs.

ALEPH Experiment; LEP; Tau lifetimeNuclear and High Energy PhysicsParticle physicsAleph[PHYS.HEXP] Physics [physics]/High Energy Physics - Experiment [hep-ex]Electron–positron annihilationFOS: Physical sciences01 natural sciencesTau lifetimeHigh Energy Physics - ExperimentNuclear physicsALEPH ExperimentHigh Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsALEPH experimentAnalysis methodPhysics010308 nuclear & particles physicsPhysicsDetectorSettore FIS/01 - Fisica SperimentaleLEPSample (graphics)Particle Physics - ExperimentLepton
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Heavy flavour decay muon production at forward rapidity in proton--proton collisions at sqrt(s) = 7 TeV

2012

The production of muons from heavy flavour decays is measured at forward rapidity in proton-proton collisions at $\sqrt{s} = 7$ TeV collected with the ALICE experiment at the LHC. The analysis is carried out on a data sample corresponding to an integrated luminosity $L_{\rm int} = 16.5$ nb$^{-1}$. The transverse momentum and rapidity differential production cross sections of muons from heavy flavour decays are measured in the rapidity range 2.5 < y < 4, over the transverse momentum range 2 < $p_{\rm T}$ < 12 GeV/$c$. The results are compared to predictions based on perturbative QCD calculations.

ALICE experiment; P-P collisions; Heavy flavour muon decayProtonAlicePhysics::Instrumentation and DetectorsHeavy flavour muon decayheavy flavour01 natural sciencesPp CollisionsSingle MuonsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)ALICEHeavy Flavour Production[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentAlice ExperimentALICE experiment; Heavy flavour production; LHC; Pp collisions; Single muons; Nuclear and High Energy PhysicsP-P collisionsQuantum chromodynamicsPhysicsLarge Hadron ColliderLuminosity (scattering theory)PhysicsProduction Cross-SectionPerturbative QCDP-P collisionP(P)Over-Bar CollisionsLHC ALICE experiment pp collisions Single muons Heavy flavour productionLHCLhcpp collisionsParticle Physics - ExperimentHeavy flavour productionParticle physicsNuclear and High Energy PhysicsLHC; ALICE; heavy flavourFOS: Physical sciencesalice experiment; pp collisions; heavy flavour production; single muons; lhcNuclear physicsmuon0103 physical sciencesALICE; heavy flavour; muonRapidity010306 general physicsHadron-CollisionsMuonta114Bottom-Quark Production010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyALICE; LHC; CERN; strange particle; pp; 7 TeV; Heavy flavour production; Single muonsALICE experimentSingle muonsJ/Psi ProductionHigh Energy Physics::ExperimentLepton
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Measurement of the AtmosphericνeSpectrum with IceCube

2015

We present a measurement of the atmospheric $\nu_e$ spectrum at energies between 0.1 TeV and 100 TeV using data from the first year of the complete IceCube detector. Atmospheric $\nu_e$ originate mainly from the decays of kaons produced in cosmic-ray air showers. This analysis selects 1078 fully contained events in 332 days of livetime, then identifies those consistent with particle showers. A likelihood analysis with improved event selection extends our previous measurement of the conventional $\nu_e$ fluxes to higher energies. The data constrain the conventional $\nu_e$ flux to be $1.3^{+0.4}_{-0.3}$ times a baseline prediction from a Honda's calculation, including the knee of the cosmic-…

AMANDANuclear and High Energy PhysicsParticle physicsAstrophysics::High Energy Astrophysical PhenomenaHadronCASCADES01 natural sciences7. Clean energyPower lawIceCubeNuclear physicsFlux (metallurgy)DESIGNLikelihood analysisDIGITIZATION0103 physical sciencesNEUTRINO FLUX010306 general physicsDETECTORPhysics010308 nuclear & particles physicsICEHigh Energy Physics::PhenomenologySpectrum (functional analysis)DetectorPERFORMANCEENERGY-SPECTRUMEvent selectionPhysics and AstronomyHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaphysicsSYSTEMPhysical Review D
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Search for neutrino emission from gamma-ray flaring blazars with the ANTARES telescope

2012

The ANTARES telescope observes a full hemisphere of the sky all the time with a duty cycle close to 100%. This makes it well suited for an extensive observation of neutrinos produced in astrophysical transient sources. In the surrounding medium of blazars, i.e. active galactic nuclei with their jets pointing almost directly towards the observer, neutrinos may be produced together with gamma-rays by hadronic interactions, so a strong correlation between neutrinos and gamma-rays emissions is expected. The time variability information of the studied source can be obtained by the gamma-ray light curves measured by the LAT instrument on-board the Fermi satellite. If the expected neutrino flux ob…

ASTROPHYSICSAstrofísicaAstrophysicsNeutrino Astronomy01 natural sciences7. Clean energyLARGE-AREA TELESCOPElaw.inventionlawWATERInstrumentation010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Time-dependent searchCATALOGLIGHTNeutrino astronomyFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical PhenomenaACTIVE GALACTIC NUCLEINuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Active galactic nucleus[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Point sourceAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsfermi lat transient sources; neutrino astronomy; time-dependent search; antares; blazarsTelescopeMUONS0103 physical sciencesANTARES; Neutrino Astronomy; Fermi LAT transient sourcesBlazarANTARES010308 nuclear & particles physicsAstronomyAstronomy and AstrophysicsFermi LAT transient sourcesLight curveNeutrino astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]MODEL13. Climate actionFISICA APLICADA:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]Neutrino astronomy[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]BlazarsFermi Gamma-ray Space Telescope
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Revised rates for the stellar triple-alpha process from measurement of C-12 nuclear resonances

2005

4 pages, 3 figures.-- PMID: 15650733 [PubMed].

ASTROPHYSICSchemistry.chemical_elementAstrophysics7. Clean energy01 natural sciencesTriple-alpha processNuclear physicsNucleosynthesis0103 physical sciencesELEMENTSPARTICLESBETA-DECAY010303 astronomy & astrophysicsHeliumPhysicsNUCLEOSYNTHESISMultidisciplinary010308 nuclear & particles physicsB-12Carbon-12Cell BiologyAlpha particleStarsSupernovachemistry13. Climate actionExcited stateSTARS
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A parametric description of the 3D structure of the Galactic bar/bulge using the VVV survey

2017

We study the structure of the inner Milky Way using the latest data release of the Vista Variables in Via Lactea (VVV) survey. The VVV is a deep near-infrared, multi-colour photometric survey with a coverage of 300 square degrees towards the Bulge/Bar. We use Red Clump (RC) stars to produce a high-resolution dust map of the VVV's field of view. From de-reddened colour-magnitude diagrams we select Red Giant Branch stars to investigate their 3D density distribution within the central 4 kpc. We demonstrate that our best-fit parametric model of the Bulge density provides a good description of the VVV data, with a median percentage residual of 5$\%$ over the fitted region. The strongest of the o…

Absolute magnitudeInitial mass functionastro-ph.GAMilky WayFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGalaxy: bulgeBulge0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsRed clumpGalaxy: structureAstrophysics::Galaxy AstrophysicsComputingMilieux_MISCELLANEOUSLuminosity function (astronomy)Physics010308 nuclear & particles physicsGalactic CenterAstronomyAstronomy and AstrophysicsGalaxy: fundamental parametersAstrophysics - Astrophysics of GalaxiesGalaxy: centregalaxies: individual: Milky WayRed-giant branchSpace and Planetary ScienceGalaxy: formationAstrophysics of Galaxies (astro-ph.GA)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Detection of deuterated molecules, but not of lithium hydride, in the z = 0.89 absorber toward PKS 1830−211

2020

Deuterium and lithium are light elements of high cosmological and astrophysical importance. In this work we report the first detection of deuterated molecules and a search for lithium hydride, 7LiH, at redshift z=0.89 in the spiral galaxy intercepting the line of sight to the quasar PKS1830-211. We used ALMA to observe several submillimeter lines of ND, NH2D, and HDO, and their related isotopomers NH2, NH3, and H2^18O, in absorption against the southwest image of the quasar, allowing us to derive XD/XH abundance ratios. The absorption spectra mainly consist of two distinct narrow velocity components for which we find remarkable differences. One velocity component shows XD/XH abundances that…

Absorption spectroscopyquasarsFOS: Physical scienceschemistry.chemical_elementAstrophysics01 natural scienceschemistry.chemical_compound0103 physical sciencesISM -galaxiesgalaxiesindividual010303 astronomy & astrophysicsLine (formation)Physics[PHYS]Physics [physics]Spiral galaxy010308 nuclear & particles physicsmolecules -radio linesAstronomy and AstrophysicsQuasarAstrophysics - Astrophysics of GalaxiesRedshift3. Good healthPKS 1830−211 -galaxiesabundances -ISMDeuteriumchemistry13. Climate actionSpace and Planetary ScienceLithium hydride[SDU]Sciences of the Universe [physics]Astrophysics of Galaxies (astro-ph.GA)Lithium[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]absorption lines -quasars
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DENN, EIGENTLICH, ÜBERHAUPT - THREE “PRAGMATIC PARTICLES” IN GERMAN

2015

A peculiarity of the German language is the extensive use of “pragmatic particles” in spoken language. These particles are generally called Abtönungspartikel (“modulating particles”) and are used to modulate the speaker’s attitude. They have an elusive meaning which is quite difficult for non-native speakers to discern, and they are a challenge to translate into Italian due to the lack of equivalents. Three particularly interesting particles are “denn”, “eigentlich” and “überhaupt”, which are typical of the speech act of asking questions. After a general introduction to the vast field of conversational particles (showing how differently German grammars treat this topic), the present contrib…

Abtoenungspartikeln ModalpartikelnSettore L-LIN/14 - Lingua E Traduzione - Lingua TedescaGerman modal particlesparticelle modali particelle communicative
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