Search results for "tracks"

showing 10 items of 21 documents

New Hettangian tracks from the Causses Basin (Lozère, southern France) complement the poor fossil record of earliest Jurassic crocodylomorphs in Euro…

2017

International audience; A new vertebrate ichnological assemblage is described from the Hettangian Dolomitic Formation of the Causses Basin, at Le Serre (Lozère, southern France). We report tracks that complement the poor fossil record of lowermost Jurassic crocodylomorphs in Europe. Tetradactyl pes and pentadactyl manus imprints form a unique trackway. Traces are ascribed to Batrachopus isp. and they represent the third occurrence of this ichnogenus in European Hettangian geological formations. This is the first report of Batrachopus in Hettangian deposits of the Causses Basin. The tracks share some similarities with Batrachopus deweyi previously described from the Sinemurian of the Causses…

0106 biological sciencesHettangian010506 paleontologyFossil Recordsouthern FranceCrocodylomorph tracksStructural basin[ SDU.STU.ST ] Sciences of the Universe [physics]/Earth Sciences/Stratigraphy010603 evolutionary biology01 natural sciencesComplement (complexity)PaleontologyLower Jurassicdinosaur tracks[SDU.STU.ST]Sciences of the Universe [physics]/Earth Sciences/StratigraphyAssemblage (archaeology)14. Life underwaterGeneral Agricultural and Biological Sciences[SDU.STU.PG]Sciences of the Universe [physics]/Earth Sciences/PaleontologyCausses BasinGeology0105 earth and related environmental sciences[ SDU.STU.PG ] Sciences of the Universe [physics]/Earth Sciences/Paleontology
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Archaeology and ichnology at Gombore II-2, Melka Kunture, Ethiopia: everyday life of a mixed age hominin group 700,000 years ago

2018

AbstractWe report the occurrence at 0.7 million years (Ma) of an ichnological assemblage at Gombore II-2, which is one of several archaeological sites at Melka Kunture in the upper Awash Valley of Ethiopia, 2000 m asl. Adults and children potentially as young as 12 months old left tracks in a silty substrate on the shore of a body of water where ungulates, as well as other mammals and birds, congregated. Furthermore, the same layers contain a rich archaeological and palaeontological record, confirming that knapping was taking place in situ and that stone tools were used for butchering hippo carcasses at the site. The site gives direct information on hominin landscape use at 0.7 Ma and may p…

0301 basic medicineOld Left010506 paleontologySciencegrowthtanzanialengthEnvironment01 natural sciencesArticlemultidisciplinary; growth; foot; children; site; footprints; tanzania; height; length; tracks; kenya; ethiopia03 medical and health sciencesIchnologychildrenGroup (stratigraphy)siteAssemblage (archaeology)AnimalsHumansEveryday lifeHistory Ancient0105 earth and related environmental sciencesShoregeography.geographical_feature_categoryKnappingFossilsQRPaleontologyHominidae15. Life on landfootprintstracksArchaeology030104 developmental biologyGeographykenyaArchaeologyfootMedicineethiopiamultidisciplinaryheight
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Search for correlations between the arrival directions of IceCube neutrino events and ultrahigh-energy cosmic rays detected by the Pierre Auger Obser…

2016

This paper presents the results of different searches for correlations between very high-energy neutrino candidates detected by IceCube and the highest-energy cosmic rays measured by the Pierre Auger Observatory and the Telescope Array. We first consider samples of cascade neutrino events and of high-energy neutrino-induced muon tracks, which provided evidence for a neutrino flux of astrophysical origin, and study their cross-correlation with the ultrahigh-energy cosmic ray (UHECR) samples as a function of angular separation. We also study their possible directional correlations using a likelihood method stacking the neutrino arrival directions and adopting different assumptions on the size…

AstronomyAstrophysicsNeutrino experiments ultra high energy cosmic rays cosmic ray experiments neutrino astronomy.01 natural sciencesASTROPHYSICAL SOURCESultra high energy cosmic raylaw.inventionIceCubeAstronomi astrofysik och kosmologimagnetic [deflection]lawAstronomy Astrophysics and Cosmologycosmic ray experiments; neutrino astronomy; neutrino experiments; ultra high energy cosmic rays; Astronomy and Astrophysics010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAngular distanceAstrophysics::Instrumentation and Methods for AstrophysicsVHE [neutrino]GALACTIC MAGNETIC-FIELDcascadeAugerobservatorycosmic radiationCascadestackingcosmic ray experi- mentsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical Phenomenaphysics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::High Energy Astrophysical Phenomenacosmic ray experimentFOS: Physical sciencesCosmic rayultra high energy cosmic raysSURFACE DETECTORTelescopeneutrino astronomyneutrino experiments0103 physical sciencesddc:530Angular resolutionHigh Energy PhysicsPierre Auger ObservatorySPECTRUMMuon010308 nuclear & particles physicsAstronomy and Astrophysicsflux [neutrino]ASTROFÍSICAPhysics and Astronomyangular resolutioncorrelationExperimental High Energy Physicsneutrino experimenttracks [muon]cosmic ray experiments
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Nanorod orientation control by swift heavy ion irradiation

2022

Highly energetic ions have been previously used to modify the shape of metal nanoparticles embedded in an insulating matrix. In this work, we demonstrate that under suitable conditions, energetic ions can be used not only for shape modification but also for manipulation of nanorod orientation. This observation is made by imaging the same nanorod before and after swift heavy ion irradiation using a transmission electron microscope. Atomistic simulations reveal a complex mechanism of nanorod re-orientation by an incremental change in its shape from a rod to a spheroid and further back into a rod aligned with the beam. Highly energetic ions have been previously used to modify the shape of meta…

DYNAMICSTRACKSPhysics and Astronomy (miscellaneous)ELONGATIONSURFACEionisoiva säteilyPhysics::Medical PhysicsPhysics::Optics114 Physical sciencesNANOPARTICLESAUnanohiukkasetGOLDSILICAmuotohiukkassäteily
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Pathways fostering mobility to higher education for vulnerable immigrants in France, Switzerland and Canada

2016

In this article we wish to clarify not only if, but also how – through which institutional settings – higher education is accessed by students from vulnerable immigrant groups in France, Switzerland and Canada. We are interested in the possible educational mobility that immigrant youths can experience arising from country-specific educational policies designed to increase the enrolment in higher education, particularly the flow from upper-secondary vocational educational tracks to higher education ones. We analyse using panel data in each country the accessibility of different pathways to higher education while taking into account the characteristics of the students. In terms of educational…

Economic growth050402 sociologySecondary educationHigher educationmedia_common.quotation_subjectvocational tracks[SHS.EDU]Humanities and Social Sciences/EducationImmigrationpathwaysEducation0504 sociologySociologyDemocratization10. No inequalitymedia_common300 Social sciences sociology & anthropologybusiness.industry4. Education05 social scienceseducational mobilityinternational comparison[ SHS.EDU ] Humanities and Social Sciences/EducationEducational attainmentAccess050902 family studiesVocational education8. Economic growth370 Education0509 other social sciencesbusinessEducational systemsPanel data
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Flavor Ratio of Astrophysical Neutrinos above 35 TeV in IceCube

2015

A diffuse flux of astrophysical neutrinos above $100\,\mathrm{TeV}$ has been observed at the IceCube Neutrino Observatory. Here we extend this analysis to probe the astrophysical flux down to $35\,\mathrm{TeV}$ and analyze its flavor composition by classifying events as showers or tracks. Taking advantage of lower atmospheric backgrounds for shower-like events, we obtain a shower-biased sample containing 129 showers and 8 tracks collected in three years from 2010 to 2013. We demonstrate consistency with the $(f_e:f_{\mu}:f_\tau)_\oplus\approx(1:1:1)_\oplus$ flavor ratio at Earth commonly expected from the averaged oscillations of neutrinos produced by pion decay in distant astrophysical sou…

FLUXAMANDAParticle physicsPhysics::Instrumentation and DetectorsENERGIESAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Physics and AstronomyFluxCosmic rayAstrophysicsACCELERATION01 natural sciencesflavor : ratioHigh Energy Physics - ExperimentIceCube Neutrino ObservatoryIceCubeHigh Energy Physics - Experiment (hep-ex)PionObservatory0103 physical sciencesddc:550010306 general physicsNeutrino oscillationHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsSigmashowersCOSMIC-RAYSatmosphere : backgroundtracksneutrino : flavor : rationeutrino : oscillationfluxobservatoryPhysics and Astronomy13. Climate actionHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical Phenomenaneutrino : VHEpi : decay
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Searching for long-lived particles beyond the Standard Model at the Large Hadron Collider

2020

Particles beyond the Standard Model (SM) can generically have lifetimes that are long compared to SM particles at the weak scale. When produced at experiments such as the Large Hadron Collider (LHC) at CERN, these longlived particles (LLPs) can decay far from the interaction vertex of the primary proton–proton collision. Such LLP signatures are distinct from those of promptly decaying particles that are targeted by the majority of searches for new physics at the LHC, often requiring customized techniques to identify, for example, significantly displaced decay vertices, tracks with atypical properties, and short track segments. Given their non-standard nature, a comprehensive overview of LLP…

HIGH-ENERGYbeyond the Standard Modellarge hadron colliderPhysics::Instrumentation and DetectorsPROTON-PROTON COLLISIONSPhysics beyond the Standard Modelbeyond the standard model01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)high-luminosity lhcHigh Energy Physics - Phenomenology (hep-ph)MAGNETIC MONOPOLESlong-lived [particle]high-energy collider experimentsdecay: vertexscattering [p p][PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]long-lived particlesQCproposed [detector]Physicslifetimedark gauge forcesLarge Hadron ColliderCMSROOT-S=13 TEVroot-s=13 tevPhysicsnew physics: search forscale: electroweak interactionhep-phATLASelectroweak interaction [scale]vertex [decay]upgrade [detector]High Energy Physics - Experiment; High Energy Physics - Experiment; High Energy Physics - Phenomenologydetector: upgradeSettore FIS/02 - Fisica Teorica Modelli e Metodi Matematiciprimary [vertex]ddc:High Energy Physics - PhenomenologyCERN LHC CollLarge Hadron Colliderbaryon asymmetryvertex: primaryLHCcolliding beams [p p]exclusion limitspp collisionsParticle Physics - ExperimentsignatureNuclear and High Energy PhysicsParticle physicsp p: scatteringCERN LabPAIR PRODUCTIONcollider phenomenologyreviewFOS: Physical sciencesDARK GAUGE FORCES530search for [new physics]BARYON ASYMMETRY0103 physical sciencesddc:530010306 general physicsnumerical calculationsParticle Physics - PhenomenologyEXCLUSION LIMITSmagnetic monopolesPP COLLISIONS010308 nuclear & particles physicshep-exbackgroundbibliographyshowersMAJORANA NEUTRINOSCollisiontracksLHC-Bdetector: proposedhigh-luminosity LHCpair productionMATHUSLAPhysics and Astronomy[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]proton-proton collisionshigh-energymajorana neutrinosparticle: long-livedp p: colliding beamsPhysics BSMexperimental results
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Dislocation mobility study of heavy ion induced track damage in LiF crystals

2008

Track damage created in LiF crystals by swift U, Kr, Xe and Ni ions with a specific energy of 11.1 MeV/u was studied using dislocation mobility measurements, track etching, SEM, AFM and optical microscopy. The results demonstrate continuity of etching of U tracks while discontinuities of etching are observed in the case of Xe ions. The relationship between the track structure and dislocation mobility in irradiated crystals is discussed. The dislocation mobility technique can serve as a highly sensitive method for track core damage studies.

Nuclear and High Energy PhysicsMaterials science[PHYS.HEXP] Physics [physics]/High Energy Physics - Experiment [hep-ex]LiFmacromolecular substances02 engineering and technology01 natural sciencesIon tracksIonlaw.inventionPACS: 61.80.Jh; 65.72.FfCondensed Matter::Materials ScienceOptical microscopelawEtching (microfabrication)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Specific energyInstrumentation010302 applied physicsTrack etchingIon trackTrack (disk drive)fungitechnology industry and agricultureDislocation mobility021001 nanoscience & nanotechnology[PHYS.COND.CM-MS] Physics [physics]/Condensed Matter [cond-mat]/Materials Science [cond-mat.mtrl-sci]Core (optical fiber)[PHYS.COND.CM-MS]Physics [physics]/Condensed Matter [cond-mat]/Materials Science [cond-mat.mtrl-sci]Atomic physicsDislocation0210 nano-technologyNuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
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A fast algorithm for muon track reconstruction and its application to the ANTARES neutrino telescope.

2011

An algorithm is presented, that provides a fast and robust reconstruction of neutrino induced upward-going muons and a discrimination of these events from downward-going atmospheric muon background in data collected by the ANTARES neutrino telescope. The algorithm consists of a hit merging and hit selection procedure followed by fitting steps for a track hypothesis and a point-like light source. It is particularly well-suited for real time applications such as online monitoring and fast triggering of optical follow-up observations for multi-messenger studies. The performance of the algorithm is evaluated with Monte Carlo simulations and various distributions are compared with that obtained …

Optical telescopesAMANDASelection proceduresRobust reconstructionMonte Carlo methodAtmospheric muonsReal-time applicationNeutrino telescope01 natural sciencesHigh Energy Physics - ExperimentFast algorithmsHigh Energy Physics - Experiment (hep-ex)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsDetectorMonte Carlo SimulationMonte Carlo methodsComputer simulationLIGHTddc:540Física nuclearNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaAlgorithmAlgorithmsFLUXOnline monitoring[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeFOS: Physical sciencesTrack reconstructionOptical telescopeNuclear physicsMuon tracks0103 physical sciencesAngular resolutionLight sources010306 general physicsOptical follow-upDETECTORInstrumentation and Methods for Astrophysics (astro-ph.IM)MuonANTARESneutrino telescope; track reconstruction010308 nuclear & particles physicsCharged particlesTrack (disk drive)track reconstructionAstronomy and Astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics - Data Analysis Statistics and ProbabilityFISICA APLICADAATMOSPHERIC NEUTRINOSNeutrino telescopesSYSTEMData Analysis Statistics and Probability (physics.data-an)
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The ANTARES telescope neutrino alert system

2012

The ANTARES telescope has the capability to detect neutrinos produced in astrophysical transient sources. Potential sources include gamma-ray bursts, core collapse supernovae, and flaring active galactic nuclei. To enhance the sensitivity of ANTARES to such sources, a new detection method based on coincident observations of neutrinos and optical signals has been developed. A fast online muon track reconstruction is used to trigger a network of small automatic optical telescopes. Such alerts are generated for special events, such as two or more neutrinos, coincident in time and direction, or single neutrinos of very high energy.

Optical telescopesPhysics::Instrumentation and DetectorsAstrophysics7. Clean energy01 natural sciencesGamma ray burstsFOLLOW-UP OBSERVATIONSlaw.inventionlawFlaring activeVery high energiesHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsGAMMA-RAY BURSTS[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]Astrophysics::Instrumentation and Methods for AstrophysicsSupernovaNeutrino detectorNeutrino astronomyFísica nuclearNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaFLUX[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesOptical telescopeTelescopeMuon tracksCoincidentSEARCHDetection methods0103 physical sciencesCore collapse supernovae010306 general physicsOptical follow-upInstrumentation and Methods for Astrophysics (astro-ph.IM)Neutronsantares; neutrino astronomy; optical follow-up; transient sourcesANTARES010308 nuclear & particles physicsGamma raysAstronomyAstronomy and AstrophysicsAlert systemsStarsTransient sources[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Optical signalsPotential sources13. Climate actionFISICA APLICADAHigh Energy Physics::ExperimentNeutrino astronomyGamma-ray burst
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