Search results for "ExAC"

showing 10 items of 1440 documents

Rational solutions to the mKdV equation associated to particular polynomials

2021

International audience; Rational solutions to the modified Korteweg-de Vries (mKdV) equation are given in terms of a quotient of determinants involving certain particular polynomials. This gives a very efficient method to construct solutions. We construct very easily explicit expressions of these rational solutions for the first orders n = 1 until 10.

[PHYS]Physics [physics][SPI.ACOU]Engineering Sciences [physics]/Acoustics [physics.class-ph]Pure mathematicsApplied MathematicsRational solutionsMathematics::Analysis of PDEsGeneral Physics and Astronomy[SPI.MECA]Engineering Sciences [physics]/Mechanics [physics.med-ph]01 natural sciences010305 fluids & plasmasComputational MathematicsNonlinear Sciences::Exactly Solvable and Integrable SystemsModeling and Simulation0103 physical sciences010306 general physicsConstruct (philosophy)mKdV equationNonlinear Sciences::Pattern Formation and SolitonsQuotientMathematicsWave Motion
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Correlation of the highest-energy cosmic rays with the positions of nearby active galactic nuclei

2008

Data collected by the Pierre Auger Observatory provide evidence for anisotropy in the arrival directions of the cosmic rays with the ighest-energies, which are correlated with the positions of relatively nearby active galactic nuclei (AGN) [Pierre Auger Collaboration, Science 318 (2007) 938]. The correlation has maximum significance for cosmic rays with energy greater than ~6 x 1019 eV and AGN at a distance less than ~75 Mpc. We have confirmed the anisotropy at a confidence level of more than 99% through a test with parameters specified a priori, using an independent data set. The observed correlation is compatible with the hypothesis that cosmic rays with the highest-energies originate fro…

[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]AstronomyOsservatorio Pierre AugerAstrophysicsGALAXY CLUSTER SURVEYAstrophysicsauger01 natural sciencesHigh energy cosmic rayRaggi cosmiciAstrophysical jetGMFObservatoryUltra-high-energy cosmic ray010303 astronomy & astrophysicsPhysicsBL-LACERTAEGreisen–Zatsepin–Kuz’min effect[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]ORIGINUHECRAstrophysics (astro-ph)Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryGZKRadiación cósmicaAnisotropíaCATALOGobservatoryddc:540EGMFCUTOFFComputingMethodologies_DOCUMENTANDTEXTPROCESSINGRELATIVISTIC JETSActive galactic nucleusAstrophysics::High Energy Astrophysical PhenomenaCosmic background radiationFOS: Physical sciencesCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsACCELERATION[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciencesextra-galacticPARTICLESAGNAstrophysics::Galaxy AstrophysicsCiencias ExactasPierre Auger ObservatoryANISOTROPYhigh energy cosmic raysSciami atmosferici010308 nuclear & particles physicsFísicaAstronomyAstronomy and AstrophysicsCENTAURUSGalaxyExperimental High Energy Physics
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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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Modalités fonctionnelles et évolutives des parasitoses développées par les crabes Pinnotheridae aux dépens des échinides fouisseurs

2010

Ce travail s’est intéressé aux liens existant entre la stratégie d’exploitation développée par un crustacé ectoparasite et son comportement reproductif. Le crabe Pinnotheridae Dissodactylusprimitivus exploite deux espèces Spatangidae vivant dans la Mer des Caraïbes, Meomaventricosa et Plagiobrissus grandis. Des approches comportementales, démographiques etgénétiques ont été adoptées afin de mettre en lumière le fonctionnement et la biologie de cettesymbiose. Par son comportement alimentaire, le crabe occasionne des lésions tégumentairessur ses hôtes. Celles-ci affectent la fitness de M. ventricosa, au travers de son développementgonadique. Dissodactylus primitivus exploite ses deux espèces …

[SDV.BA] Life Sciences [q-bio]/Animal biologyBrachyuraÉchinidesEctoparasiteLife cycleEchinids[ SDV.BA ] Life Sciences [q-bio]/Animal biologyBrachyoureéchinidesCycle vitalmating systemMating systemSea-urchins[ SDV.SA ] Life Sciences [q-bio]/Agricultural sciencesOursinsMobility[SDV.SA] Life Sciences [q-bio]/Agricultural scienceslife cycle cycle vitalComportement reproductifCrabs -- ParasitesectoparasitemobilityMobilitécomportement reproductifechinidsCrabes -- ReproductionCrabs -- ReproductionBiologieCrabes -- ParasitesmobilitéSciences exactes et naturelles
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Modéliser la réponse des espèces marines antarctiques aux changements environnementaux. Méthodes, applications et limites.

2021

Among tools that are used to fill knowledge gaps on natural systems, ecological modelling has been widely applied during the last two decades. Ecological models are simple representations of a complex reality. They allow to highlight environmental drivers of species ecological niche and better understand species responses to environmental changes. However, applying models to Southern Ocean benthic organisms raises several methodological challenges. Species presence datasets are often aggregated in time and space nearby research stations or along main sailing routes. Data are often limited in number to correctly describe species occupied space and physiology. Finally, environmental datasets …

[SDV.EE]Life Sciences [q-bio]/Ecology environmentphysiological modelModélisation écologiqueEspèces marines benthiquesmodel performancePhysiological modelsspecies distribution modellingModèles de distribution d’espècesOcéan Australdispersal model[SDV.EE] Life Sciences [q-bio]/Ecology environmentModèles de dispersion lagrangiensSpecies distribution modelsecological modellingLagrangian dispersal modelsSouthern OceanModèles physiologiquesEcological modellingMarine benthic speciesSciences exactes et naturelles
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The mKdV equation and multi-parameters rational solutions

2021

Abstract N -order solutions to the modified Korteweg–de Vries (mKdV) equation are given in terms of a quotient of two wronskians of order N depending on 2 N real parameters. When one of these parameters goes to 0, we succeed to get for each positive integer N , rational solutions as a quotient of polynomials in x and t depending on 2 N real parameters. We construct explicit expressions of these rational solutions for orders N = 1 until N = 6 .

[SPI.ACOU]Engineering Sciences [physics]/Acoustics [physics.class-ph][PHYS]Physics [physics]Pure mathematicsApplied MathematicsRational solutionsGeneral Physics and Astronomy[SPI.MECA]Engineering Sciences [physics]/Mechanics [physics.med-ph]01 natural sciences010305 fluids & plasmasComputational MathematicsNonlinear Sciences::Exactly Solvable and Integrable SystemsIntegerWronskiansModeling and Simulation0103 physical sciencesOrder (group theory)mKdV equation010301 acousticsQuotientMathematicsWave Motion
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Searches for anisotropies in the arrival directions of the highest energy cosmic rays detected by the Pierre Auger Observatory

2015

We analyze the distribution of arrival directions of ultra-high energy cosmic rays recorded at the Pierre Auger Observatory in 10 years of operation. The data set, about three times larger than that used in earlier studies, includes arrival directions with zenith angles up to $80^\circ$, thus covering from $-90^\circ$ to $+45^\circ$ in declination. After updating the fraction of events correlating with the active galactic nuclei (AGNs) in the V��ron-Cetty and V��ron catalog, we subject the arrival directions of the data with energies in excess of 40 EeV to different tests for anisotropy. We search for localized excess fluxes and for self-clustering of event directions at angular scales up t…

acceleration of particles; astroparticle physicsNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Upper LimitAstronomyCiencias FísicasAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFieldCosmic rayAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsOtras Ciencias Físicas01 natural sciencesSettore FIS/04 - Fisica Nucleare e SubnucleareSettore FIS/05 - Astronomia e AstrofisicaObservatorySpectrum0103 physical sciencesacceleration of particles astroparticle physicsSurface Detector010303 astronomy & astrophysicsacceleration of particleAstrophysics::Galaxy Astrophysicsacceleration of particlesPhysicsPierre Auger ObservatoryHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleArrayAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]astroparticle physicAstronomy and AstrophysicsASTROFÍSICANucleiSpace and Planetary Scienceastroparticle physicsExperimental High Energy Physicsacceleration of particles; astroparticle physics; Nuclear and High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearCatalogSkyAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTAS
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Direct C-H metalation with chromium(ii) and iron(ii): transition- metal host/benzenediide guest magnetic inverse-crown complexes

2009

Check M(etal)ate: The chessboard and the figures represent a special reaction in which different low-polarity metals can metalate arenes directly when they are brought into the right position. In a combination of queen (sodium) and knight (chromium or iron), it is possible for the knight (usually the weaker piece) to make a direct deadly hit on the king (benzene) in this game of elemental chess. Fil: Alborés, Pablo. Johannes Gutenberg Universitat Mainz; Alemania. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Fil: Carrella, Luca M.. Johannes Gutenberg Universitat Mainz; Alemania Fil: Clegg, William. University of Newcastle; Reino Unido Fil: García Álvarez, Pablo. Univ…

alkali metalsMetalationchemistry.chemical_elementMineralogyALKALI METALSmetalationCatalysisQueen (playing card)Chromiumchemistry.chemical_compoundironTransition metalCHROMIUMinverse crown compoundsBenzeneIRONOtras Ciencias QuímicasCiencias QuímicasGeneral ChemistryAlkali metalCommunicationsCrystallographychemistrychromiumINVERSE CROWN COMPOUNDSCIENCIAS NATURALES Y EXACTAS
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