Search results for " Pierre"

showing 10 items of 83 documents

Observation of the suppression of the flux of cosmic rays above 4x10^19eV

2008

The energy spectrum of cosmic rays above 2.5 × 10¹⁸ eV, derived from 20,000 events recorded at the Pierre Auger Observatory, is described. The spectral index γ of the particle flux, J ∝ E-γ, at energies between 4 × 10¹⁸ eV and 4 × 10¹⁹ eV is 2.69 ± 0.02(stat) ± 0.06(syst), steepening to 4.2 ± 0.4(stat) ± 0.06(syst) at higher energies. The hypothesis of a single power law is rejected with a significance greater than 6 standard deviations. The data are consistent with the prediction by Greisen and by Zatsepin and Kuz'min.

[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Astrophysics::High Energy Astrophysical Phenomenaenergy spectrumFOS: Physical sciencesGeneral Physics and AstronomyFluxOsservatorio Pierre Augerspectral indexCosmic rayparticle fluxAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsEXTENSIVE AIR-SHOWERSAstrophysicsUPPER LIMIT01 natural sciencesPower lawAugerNuclear physicsENERGY[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Raggi cosmicicosmic rays0103 physical sciencesddc:550Particle flux010303 astronomy & astrophysicsCiencias ExactasPhysicsPierre Auger ObservatorySpectral indexSPECTRUM[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsAstrophysics (astro-ph)Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsFísicaEnergia ultra altaARRAYHigh Energy Physics::ExperimentSciami atmosferici estesiEnergy (signal processing)
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Upper limit on the diffuse flux of ultrahigh energy tau neutrinos from the Pierre Auger Observatory

2008

The surface detector array of the Pierre Auger Observatory is sensitive to Earth-skimming tau neutrinos that interact in Earth’s crust. Tau leptons from ντ charged-current interactions can emerge and decay in the atmosphere to produce a nearly horizontal shower with a significant electromagnetic component. The data collected between 1 January 2004 and 31 August 2007 are used to place an upper limit on the diffuse flux of ντ at EeV energies. Assuming an E−2ν differential energy spectrum the limit set at 90% C.L. is E2νdNντdEν<1.3×10−7  GeV cm−2 s−1 sr−1 in the energy range 2×1017 eV<E<2×1019  eV.

[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]FLUORESCENCE DETECTORAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyOsservatorio Pierre AugerCosmic ray7. Clean energy01 natural sciencesNuclear physics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]PACS: 95.55.Vj 95.85.Ry 98.70.SaPionRaggi cosmicimuonSEARCH0103 physical sciencesNeutrinoEARTHPartículas ElementalesElectromagnetismo010306 general physicsCosmic raysCharged currentCiencias ExactasPierre Auger ObservatoryPhysicsAIR-SHOWERSRange (particle radiation)Muon[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicspionand other elementary particlesFísicaDETETOREScosmic ray detectorsEnergia ultra altaRadiación cósmicaCOSMIC-RAYSand other elementary particle detectors13. Climate actionHigh Energy Physics::ExperimentNeutrinoSciami atmosferici estesiLepton
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Large-scale distribution of arrival directions of cosmic rays detected above 1018 eV at the Pierre Auger Observatory

2012

A thorough search for large-scale anisotropies in the distribution of arrival directions of cosmic rays detected above 1018 eV at the Pierre Auger Observatory is presented. This search is performed as a function of both declination and right ascension in several energy ranges above 1018 eV, and reported in terms of dipolar and quadrupolar coefficients. Within the systematic uncertainties, no significant deviation from isotropy is revealed. Assuming that any cosmic-ray anisotropy is dominated by dipole and quadrupole moments in this energy range, upper limits on their amplitudes are derived. These upper limits allow us to test the origin of cosmic rays above 1018 eV from stationary Galactic …

[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Radiación CósmicaAstronomyMilky WayAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysicsEXTENSIVE AIR-SHOWERSSURFACE DETECTOR01 natural sciencesGALACTIC MAGNETIC-FIELDSAuger[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]cosmic raysObservatory0103 physical sciencesastroparticle physics; cosmic raysAnisotropy010303 astronomy & astrophysicsGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)Ciencias ExactasHigh Energy Astrophysical Phenomena (astro-ph.HE)Astroparticle physicsPhysicsPierre Auger ObservatoryANISOTROPY010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyFísicaAstronomy and AstrophysicsENERGY-SPECTRUMUltra-High Energy Cosmic Rays Pierre Auger Observatory Large Scale AnisotropiesSpace and Planetary Scienceastroparticle physicsExperimental High Energy PhysicsROTATIONARRAYFísica nuclearAstroparticle physicsRight ascensionAstrophysics - High Energy Astrophysical Phenomena
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Des signes lapidaires autour de l’An Mil sur les murs de l’église de Saint-Germain-des-Prés (Paris). Nouvelles données

2018

International audience

[SHS.ARCHEO] Humanities and Social Sciences/Archaeology and Prehistory[SHS.ARCHEO]Humanities and Social Sciences/Archaeology and PrehistoryTaille de pierreMarques lapidaires[SHS] Humanities and Social SciencesComputingMilieux_MISCELLANEOUSSaint-Germain-des-Prés[SHS]Humanities and Social Sciences
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L’abbaye Saint-Germain : matériaux et techniques du bâti – Les matériaux de construction

2000

International audience

[SHS.ARCHEO] Humanities and Social Sciences/Archaeology and Prehistory[SHS.ARCHEO]Humanities and Social Sciences/Archaeology and Prehistory[ SHS.ARCHEO ] Humanities and Social Sciences/Archaeology and PrehistoryTaille de pierreArchéomatériauxComputingMilieux_MISCELLANEOUS
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Massangis, Vau Chevrau et La Côme Gérarde (Yonne) : centrale photovoltaïque, zone 3 nord et zone 5 : rapport de diagnostic

2012

L’opération n’a révélé que peu de vestiges en raison de l’érosion générale subie par les niveaux en sommet de plateau. Toutefois, quelques ensembles archéologiques méritent d’être notés.Si la protohistoire ancienne n’est que peu représentée (un enclos circulaire très arasé), la période de La Tène Finale et l’époque gallo-romaine sont, quant à elles, un peu mieux connues. On note en effet la présence d’une voie antique est-ouest repérée sur environ 130 m, sans doute en grande partie érodée de part et d’autre de ce tronçon.En bordure nord et sud, deux pôles funéraires, totalement inédits, sont installés dès La Tène Finale et fonctionnent visiblement jusqu’à l’époque flavienne. Ils sont marqué…

[SHS.ARCHEO] Humanities and Social Sciences/Archaeology and Prehistorynécropole à incinérationsiloenclos circulairefour à chauxProtohistoirehabitat ruralvoie romaineLa Tène IIIcoffre en pierrebalsamaireparuremonnaie romaineurnecéramique gallo-romaineEmpire romain[SHS] Humanities and Social Sciences
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La mémoire de Pierre Semard chez les cheminots CGT

2007

[SHS.DROIT]Humanities and Social Sciences/LawCGT[SHS.DROIT] Humanities and Social Sciences/Lawmémoire de Pierre Semardcheminots[ SHS.DROIT ] Humanities and Social Sciences/Law
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L'Estoil(l)e Pierre de

2007

[SHS.DROIT]Humanities and Social Sciences/Law[SHS.DROIT] Humanities and Social Sciences/LawL'Estoil(l)e Pierre de[ SHS.DROIT ] Humanities and Social Sciences/Law
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Qu'est-ce que le structuralisme génétique ?

2021

International audience

[SHS.SOCIO]Humanities and Social Sciences/Sociologysociologie[SHS.SOCIO] Humanities and Social Sciences/Sociology[SHS] Humanities and Social Sciencesstructuralisme génétiqueBourdieu PierreComputingMilieux_MISCELLANEOUS[SHS]Humanities and Social Sciences
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BORDERS AND BORDER CROSSING BETWEEN ART WORLDS. Successful attempts and epic failures to enter new domains in recent British art

2016

The paper attempts to answer, whether it is possible for successful artists in one specific sector to access the domain of another artistic field at their free will. In doing so, this contribution analyses the possible existence of borders and gatekeepers between different art worlds. The aim is not just finding or defining boundaries between art fields, but rather understanding, if boundaries can be pierced through, as well as the conditions that might hinder acceptance. Moving from an art theoretical and philosophical perspective, the present paper will discuss the thesis of Pierre Bourdieu, Howard Becker, Berys Gaut and Joseph Margolis on boundary conditions in the arts. Subsequently the…

border crossing art worldsSettore M-FIL/04 - EsteticaSettore L-ART/03 - Storia dell'Arte ContemporaneaBorder crossing Art worlds Art field Gatekeepers Pierre Bourdieu Howard Becker Damien Hirst Steve McQueen Douglas Gordonart worldsborder crossing
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