Search results for "Universe"

showing 10 items of 2171 documents

A method for detection of muon induced electromagnetic showers with the ANTARES detector

2012

The primary aim of ANTARES is neutrino astronomy with upward going muons created in charged current muon neutrino interactions in the detector and its surroundings. Downward going muons are background for neutrino searches. These muons are the decay products of cosmic-ray collisions in the Earths atmosphere far above the detector. This paper presents a method to identify and count electromagnetic showers induced along atmospheric muon tracks with the ANTARES detector. The method is applied to both cosmic muon data and simulations and its applicability to the reconstruction of muon event energies is demonstrated. © 2012 Elsevier B.V. All rights reserved.

Physics::Instrumentation and DetectorsAtmospheric muonsDecay productsNeutrino telescopeElectromagnetic shower identification01 natural sciences7. Clean energyneutrino telescope electromagnetic shower identification high energy muons energy reconstruction; high energy muons; neutrino telescope; electromagnetic shower identification; energy reconstructionMuon neutrinoNEUTRINO TELESCOPE010303 astronomy & astrophysicsInstrumentationEnergy reconstructionPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]DetectorAstrophysics::Instrumentation and Methods for AstrophysicsDetectorsHigh energy muonNeutrino detectorMuon colliderNeutrino astronomyFísica nuclearNeutrinoNeutrino telescope; Energy reconstruction; High energy muonsAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaFLUXNuclear and High Energy PhysicsParticle physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Charged current[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayMuon neutrinoNuclear physicsElectromagnetism0103 physical sciencesHigh energy physicsneutrino telescope electromagnetic shower identification high energy muons energy reconstructionInstrumentation and Methods for Astrophysics (astro-ph.IM)MuonANTARES010308 nuclear & particles physicsCharged particles[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]FISICA APLICADATEVPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNeutrino astronomyNeutrino telescopesElectro-magnetic showersHigh energy muons
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Search for point-like sources of ultra-high energy neutrinos at the pierre auger observatory and improved limit on the diffuse flux of tau neutrinos

2012

The surface detector array of the Pierre Auger Observatory can detect neutrinos with energy Eν between 1017 eV and 1020 eV from point-like sources across the sky south of +55º and north of −65º declinations. A search has been performed for highly inclined extensive air showers produced by the interaction of neutrinos of all flavors in the atmosphere (downward-going neutrinos), and by the decay of tau leptons originating from tau neutrino interactions in Earth’s crust (Earth-skimming neutrinos). No candidate neutrinos have been found in data up to 2010 May 31. This corresponds to an equivalent exposure of ∼3.5 years of a full surface detector array for the Earth-skimming channel and ∼2 years…

Physics::Instrumentation and DetectorsSolar neutrinoAstronomyAstrophysics01 natural sciences7. Clean energyneutrinoTelescopiosTau neutrinoastroparticle physics; cosmic rays; neutrinos; telescopes010303 astronomy & astrophysicsGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)cosmic rayPhysics[PHYS]Physics [physics]High Energy Astrophysical Phenomena (astro-ph.HE)[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]neutrinosCOSMIC-RAYSCosmic neutrino backgroundastroparticle physicsMeasurements of neutrino speedFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Radiación CósmicaAstrophysics::High Energy Astrophysical PhenomenaTELESCÓPIOSFOS: Physical sciencesAstroparticle physiccosmic rays0103 physical sciencesDETECTORCiencias ExactasPierre Auger Observatory010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaAstronomy and AstrophysicstelescopesSolar neutrino problem13. Climate actionSpace and Planetary ScienceExperimental High Energy PhysicsHigh Energy Physics::ExperimentAstroparticle physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Lepton
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Search for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger Observatory

2011

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

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

2020

The concordance of the $\Lambda$CDM cosmological model in light of current observations has been the subject of an intense debate in recent months. The 2018 Planck Cosmic Microwave Background (CMB) temperature anisotropy power spectrum measurements appear at face value to favour a spatially closed Universe with curvature parameter $\Omega_K<0$. This preference disappears if Baryon Acoustic Oscillation (BAO) measurements are combined with Planck data to break the geometrical degeneracy, although the reliability of this combination has been questioned due to the strong tension present between the two datasets when assuming a curved Universe. Here, we approach this issue from yet another point…

Planckcosmological modelCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectCosmological parametersSpatial curvatureDark matterCosmic microwave backgroundCosmic background radiationFOS: Physical sciencesanisotropycosmic background radiationAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)power spectrumCurvature01 natural sciencesGeneral Relativity and Quantum Cosmologydark matterCosmologyacousticsymbols.namesake0103 physical sciencesPlanck010303 astronomy & astrophysicsmedia_commonPhysics[PHYS.GRQC] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]010308 nuclear & particles physicstemperatureAstronomy and AstrophysicsoscillationtensionUniverseGalaxybaryonCosmological tensionsSpace and Planetary Sciencecurvature[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]symbolsgalaxy[PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic AstrophysicsPhysics of the Dark Universe
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Particle energization in colliding subcritical collisionless shocks investigated in the laboratory

2022

Context. Colliding collisionless shocks appear across a broad variety of astrophysical phenomena and are thought to be possible sources of particle acceleration in the Universe. Aims. The main goal of our experimental and computational work is to understand the effect of the interpenetration between two subcritical collisionless shocks on particle energization. Methods. To investigate the detailed dynamics of this phenomenon, we performed a dedicated laboratory experiment. We generated two counter-streaming subcritical collisionless magnetized shocks by irradiating two Teflon (C2F4) targets with 100 J, 1 ns laser beams on the LULI2000 laser facility. The interaction region between the plasm…

Plasma Physics (physics.plasm-ph)Settore FIS/05 - Astronomia E Astrofisica[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU]Sciences of the Universe [physics]Space and Planetary ScienceAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and Astrophysicsshock wavesinterplanetary mediumPhysics - Plasma Physicsacceleration of particles
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Macroecological properties of ammonites : spatial distribution, phylogeny, and faunal similarity

2016

The present work, which lies between macroecology and macroevolution, focuses on the spatio-temporal dynamics of early Pliensbachian ammonites of the western Tethys. Two main questions are addressed: how does inter-assemblage compositional similarity decrease with geographical distance? What is the relationship between species range size and phylogeny, species duration and latitudinal position?Ammonite dispersal dynamics are studied through a multi-scale Similarity Distance Decay analysis. We show that their long-distance dispersal is facilitated when the environment is more homogeneous and that it is not related to their morphology. This suggests that their long-distance dispersal occurred…

Pliensbachien inférieurPhylogénieTéthys de l’OuestDistribution spatialeDispersalDispersionAmmonitesProvincialismeGeological durationRapoport’s ruleDurée de vieEarly PliensbachianProvincialismSpatial distribution[SDU.STU.PG] Sciences of the Universe [physics]/Earth Sciences/PaleontologyMacroecologyMacroécologieRègle de RapoportPhylogenyWestern Tethys
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Le gisement pléistocène moyen récent de Romain-la-Roche (Doubs, France) : synthèse biostratigraphique et paléoécologique

2010

Accessible à l'adresse : http://www.ville-ge.ch/mhng/paleo/paleo-pdf/29-2/pal_29_2_07_20.pdf; International audience; L'aven de Romain-la-Roche est une cavité karstique ayant fonctionné comme un piège naturel dans lequel sont tombés de nombreux grands animaux, et où divers petits vertébrés ont été amenés en tant que proies d'oiseaux rapaces. Le gisement a été fouillé de 1980 à 1991 par Patrick Paupe et son équipe, qui y a recueilli 52 espèces de mammifères (plus de 10 000 restes déterminables), au moins 13 espèces d'oiseaux, deux de reptiles, une d'amphibien, deux espèces de poissons et des gastéropodes indéterminés. Les espèces de mammifères présentes sont pour 34,6 % des rongeurs (3975 re…

Pléistocène moyen récentNord-Est de la France[SDU.STU] Sciences of the Universe [physics]/Earth Sciencespaléoécologie[SDU.STU]Sciences of the Universe [physics]/Earth Sciences[ SDU.STU ] Sciences of the Universe [physics]/Earth Sciencesbiostratigraphiepaléontologie
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Analyse odontométrique comparée de populations du campagnol des neiges Chionomys nivalis (Martins, 1842) (Rodentia, Arvicolinae).

2007

14 pages; La morphométrie comparée de la première molaire inférieure (M1) de onze populations du campagnol des neiges Chionomys nivalis (Rodentia, Arvicolinae) (Martins, 1842) du Pléistocène supérieur et de l'Holocène de France, d'Allemagne et de Roumanie, montre une nette différenciation morphologique entre les populations de ces trois pays, exprimée par un gradient morphologique est-ouest. A l'échelle du pays, des divergences morphologiques, plus modérées, sont observées, en particulier chez les populations de France et des Carpates méridionales et occidentales.

Pléistocène supérieur et Holocène[ SDV.BID ] Life Sciences [q-bio]/BiodiversityMorphométrieEurope occidentaleArvicolinaeCampagnol Chionomys nivalisRodentia[SDV.BID]Life Sciences [q-bio]/Biodiversitycentrale et orientale.[SDU.STU.PG] Sciences of the Universe [physics]/Earth Sciences/Paleontology[SDU.STU.PG]Sciences of the Universe [physics]/Earth Sciences/Paleontologycentrale et orientale[SDV.BID] Life Sciences [q-bio]/Biodiversity[ SDU.STU.PG ] Sciences of the Universe [physics]/Earth Sciences/Paleontology
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INTEGRAL/SPI ground calibration

2003

Three calibration campaigns of the spectrometer SPI have been performed before launch in order to determine the instrument characteristics, such as the effective detection area, the spectral resolution and the angular resolution. Absolute determination of the effective area has been obtained from simulations and measurements. At 1 MeV, the effective area is 65 cm^2 for a point source on the optical axis, the spectral resolution ~2.3 keV. The angular resolution is better than 2.5 deg and the source separation capability about 1 deg. Some temperature dependant parameters will require permanent in-flight calibration.

Point source[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]FOS: Physical sciencesInstrumentation ; Detectors ; Spectrographs ; Space vehicles ; Gamma rays ; ObservationsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]OpticsSpectrographs0103 physical sciencesCalibrationSource separationAngular resolutionSpectral resolutionspace vehicles: instrumentsInstrumentation010303 astronomy & astrophysicsObservations:ASTRONOMÍA Y ASTROFÍSICA::Astronomía óptica [UNESCO]instrumentation: spectrographsPhysicsSpectrometer[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsbusiness.industryinstrumentation: detectorsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Astronomía ópticaGamma raysAntenna apertureAstrophysics (astro-ph)DetectorsSpace vehiclesAstronomy and AstrophysicsOptical axisSpace and Planetary Sciencebusiness:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]gamma rays: observations
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Origin of atmospheric lead in Johannesburg, South Africa

2006

International audience; The origin of lead in the atmosphere of Johannesburg, South Africa was investigated on the basis of elemental and lead isotopic analyses of coals, mine dumps, gasoline, and about 30 epiphytic lichen samples. Lead predominantly comes from automotive exhausts in urban and suburban areas, as leaded antiknock additives were still in use in South Africa at the time of the study. Although dust emissions from the numerous mine-tailing dumps were expected to contribute significantly to the heavy metal budget, the southern townships that are surrounded by the dumps (such as Soweto and other historically Black residential areas) do not appear to be more than partially influenc…

PollutionAtmospheric Science010504 meteorology & atmospheric sciencesmedia_common.quotation_subjectMine dumpAir pollutionMixing modelLichen010501 environmental sciencesUrban areamedicine.disease_cause01 natural sciencesLead (geology)Coal burningEnvironmental protectionmedicine[ SDU.ENVI ] Sciences of the Universe [physics]/Continental interfaces environmentAnthropogenic factor[SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces environment0105 earth and related environmental sciencesGeneral Environmental Sciencemedia_commonIsotope analysisgeographygeography.geographical_feature_categoryEnvironmental engineeringLead isotopeTailingsPollution13. Climate actionEnvironmental science
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