Search results for "high-energy"

showing 10 items of 161 documents

Search for a diffuse flux of astrophysical muon neutrinos with the IceCube 59-string configuration

2013

A search for high-energy neutrinos was performed using data collected by the IceCube Neutrino Observatory from May 2009 to May 2010, when the array was running in its 59-string configuration. The data sample was optimized to contain muon neutrino induced events with a background contamination of atmospheric muons of less than 1%. These data, which are dominated by atmospheric neutrinos, are analyzed with a global likelihood fit to search for possible contributions of prompt atmospheric and astrophysical neutrinos, neither of which have yet been identified. Such signals are expected to follow a harder energy spectrum than conventional atmospheric neutrinos. In addition, the zenith angle dist…

SELECTIONHIGH-ENERGY NEUTRINOSNuclear and High Energy PhysicsTELESCOPEAstrophysics::High Energy Astrophysical PhenomenaFluxFOS: Physical sciencesCosmic rayAstrophysics7. Clean energyIceCube Neutrino ObservatoryRATIOObservatoryDETECTORSddc:530Muon neutrinoZenithPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)MuonICEPERFORMANCEPhysics and AstronomyHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical Phenomena
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JIMWLK evolution of the odderon

2016

We study the effects of a parity-odd "odderon" correlation in JIMWLK renormalization group evolution at high energy. Firstly we show that in the eikonal picture where the scattering is described by Wilson lines, one obtains a strict mathematical upper limit for the magnitude of the odderon amplitude compared to the parity even pomeron one. This limit increases with N_c, approaching infinity in the infinite N_c limit. We use a systematic extension of the Gaussian approximation including both 2- and 3-point correlations which enables us to close the system of equations even at finite N_c. In the large-N_c limit we recover an evolution equation derived earlier. By solving this equation numeric…

SMALL-X EVOLUTIONWilson loopNuclear TheoryLARGE NUCLEIWilson linesFOS: Physical sciencesField (mathematics)114 Physical sciences01 natural sciencesHIGH-ENERGY SCATTERINGColor-glass condensateRENORMALIZATION-GROUPNuclear Theory (nucl-th)GLUON DISTRIBUTION-FUNCTIONSPomeronHigh Energy Physics - Phenomenology (hep-ph)Quantum mechanicsquantum chromodynamics0103 physical sciencesEQUATION010306 general physicsPhysicsta114evolution equations010308 nuclear & particles physicsScatteringEikonal equationHERA-DATAHigh Energy Physics::PhenomenologyCOLOR GLASS CONDENSATEodderonRenormalization groupHigh Energy Physics - PhenomenologyAmplitudeJIMWLKPA-COLLISIONSBK EVOLUTION
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Application of High Energy Shock Waves to Single Cells

1989

Extracorporeal shock wave lithotripsy has been in clinical use since 1980 with several hundred thousand patients treated to date. Striking complications, like perirenal hematomas, are rare with a range of approximately 0.5%–1.5%. High dose applications in pigs and dogs have shown devastating effects on renal parenchyma with intrarenal hemorrhage and later fibrosis (Muschter et al. 1987). However, very little is known about shock wave effects on single cells like cellular blood components. Chaussy and coworkers (Chaussy 1982; Eisenberger et al. 1977) could show an increase of free hemoglobin after exposing canine erythrocytes to shock waves. Russo and associates (1986) found a profound influ…

Shock wavePathologymedicine.medical_specialtyDiagnostic ultrasoundbusiness.industryRenal parenchymamedicine.medical_treatmentHigh-Energy Shock WavesTumor cellsmedicine.diseaseExtracorporeal shock wave lithotripsyFibrosisFree hemoglobinMedicinebusiness
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Isolated self-assembled InAs/InP(001) quantum wires obtained by controlling the growth front evolution

2007

6 páginas, 5 figuras. In this work we explore the first stages of quantum wire (QWR) formation studying the evolution of the growth front for InAs coverages below the critical thickness, θc, determined by reflection high energy electron diffraction (RHEED). Our results obtained by in situ measurement of the accumulated stress evolution during InAs growth on InP(001) show that the relaxation process starts at a certain InAs coverage θRθR this ensemble of isolated nanostructures progressively evolves towards QWRs that cover the whole surface for θ = θc. These results allow for a better understanding of the self-assembling process of QWRs and enable the study of the individual properties of In…

Single quantum wiresWork (thermodynamics)Materials scienceNanostructureReflection high-energy electron diffractionCondensed matter physicsMechanical EngineeringQuantum wireBioengineeringGeneral ChemistryCondensed Matter::Mesoscopic Systems and Quantum Hall EffectCondensed Matter::Materials ScienceCrystallographyReflection (mathematics)Electron diffractionMechanics of MaterialsGeneral Materials ScienceElectrical and Electronic EngineeringMolecular beam epitaxyQuantumMolecular beam epitaxyNanotechnology
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First results on ProtoDUNE-SP liquid argon time projection chamber performance from a beam test at the CERN Neutrino Platform

2020

The ProtoDUNE-SP detector was constructed and operated on the CERN Neutrino Platform. We thank the CERN management for providing the infrastructure for this experiment and gratefully acknowledge the support of the CERN EP, BE, TE, EN, IT and IPT Departments for NP04/ProtoDUNE-SP. This documentwas prepared by theDUNEcollaboration using the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359. This work was supported by CNPq, FAPERJ, FAPEG and FAPESP, Brazil; CFI, IPP and NSERC, Canada; CERN; MSMT, Czech Republi…

TechnologyHIGH-ENERGYPhysics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorsfar detectorbeam transportNoble liquid detectors (scintillation ionization double-phase)Cms Experıment01 natural sciences7. Clean energy09 EngineeringParticle identificationHigh Energy Physics - Experiment030218 nuclear medicine & medical imagingHigh Energy Physics - Experiment (hep-ex)0302 clinical medicineNoble liquid detectors (scintillationDetectors and Experimental TechniquesInstrumentationInstruments & Instrumentationphysics.ins-dettime resolutionMathematical PhysicsPhysics02 Physical SciencesTime projection chamberLarge Hadron ColliderDetectorInstrumentation and Detectors (physics.ins-det)double-phase)Nuclear & Particles PhysicsLIGHTNeutrinoParticle Physics - ExperimentperformanceNoble liquid detectors(scintillation ionization double-phase)noiseCERN LabLarge detector systems for particle and astroparticle physics Noble liquid detectors (scintillation ionization double-phase) Time projection Chambers (TPC)530 Physicsenergy lossTime projection chambersFOS: Physical sciencesParticle detectorNuclear physics03 medical and health sciencesneutrino: deep underground detector0103 physical sciencesionizationDeep Underground Neutrino ExperimentHigh Energy Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]signal processingactivity reportScience & Technology010308 nuclear & particles physicshep-exLarge detector systems for particle and astroparticle physicsTime projection Chambers (TPC)530 Physiksensitivitycalibrationtime projection chamber: liquid argonExperimental High Energy PhysicsLarge detector systems for particle and astroparticle physicsingle-phase)Large detector systems for particle and astroparticle physics; Noble liquid detectors (scintillation ionization double-phase); Time projection Chambers (TPC)High Energy Physics::Experimentphoton: detectorparticle identificationcharged particle: irradiationBeam (structure)
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The response behaviour of LiF:Mg,Cu,P thermoluminescence dosimeters to high-energy electron beams used in radiotherapy

1995

To ensure the effectiveness of radiation-therapy treatments, both in-phantom and in-patient reliable dose measurements are required. Thermoluminescence dosimeters are used commonly for both applications. Among the various available materials, the relatively new LiF:Mg,Cu,P phosphor is a suitable candidate for quality control of in vivo dosimetry in electron-beam therapy. The response behaviour of LiF:Mg,Cu,P chips to 6-21 MeV electron beams used in radiotherapy was studied. Batch homogeneity, dose linearity, sensitivity change after use, dose and dose-rate response, energy dependence and fading characteristics were investigated. The contribution from each factor to the overall uncertainty i…

Time FactorsDosimeterMaterials scienceRadiological and Ultrasound Technologybusiness.industryRadiochemistryDose profilePhosphorElectronModels TheoreticalThermoluminescenceRadiotherapy High-EnergyThermoluminescent DosimetryCathode rayHumansDosimetryThermoluminescent DosimetryRadiology Nuclear Medicine and imagingNuclear medicinebusinessPhysics in Medicine and Biology
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Trigger and aperture of the surface detector array of the Pierre Auger Observatory

2010

The surface detector array of the Pierre Auger Observatory consists of 1600 water-Cherenkov detectors, for the study of extensive airshowers (EAS) generated by ultra-high-energy cosmic rays. We describe the trigger hierarchy, from the identification of candidates howers at the level of a single detector, amongst a large background (mainly random single cosmic ray muons), up to the selection of real events and the rejection of random coincidences. Such trigger makes the surface detector array fully efficient for the detection of EAS with energy above 3 x 1018 eV, for all zenith angles between 03 and 603, independently of the position of the impact point and of the mass of the primary particl…

Ultra high energy cosmic rays; Auger Observatory; Extensive air showers; Trigger; ExposurePhysics::Instrumentation and DetectorsAstronomyHigh-Energy Cosmi Ray7. Clean energy01 natural sciencesAugerAcceptance and Trigger Efficiency010303 astronomy & astrophysicsInstrumentationComputingMilieux_MISCELLANEOUSPhysicsRange (particle radiation)PhysicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryHigh energyFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsNuclear and High Energy Physics[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]AIR SHOWERSApertureInstrumentationAstrophysics::High Energy Astrophysical PhenomenaExtensive air showerFOS: Physical sciencesCosmic rayENERGIACosmic RayUltra high energy cosmic rayExposureOpticsultra high energy cosmic rays Auger Observatory extensive airshowers trigger exposure0103 physical sciencesPARTICLESExtensive air showersSurface DetectorInstrumentation and Methods for Astrophysics (astro-ph.IM)ZenithCiencias ExactasNuclear and High Energy PhysicPierre Auger Observatory010308 nuclear & particles physicsbusiness.industryFísicaUltra high energy cosmic raysUltra-high energy cosmic rays[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]TriggerAuger ObservatoryExperimental High Energy PhysicsHigh Energy Physics::Experimentbusiness
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Search for transient sources with the ANTARES and KM3NeT neutrino telescopes in the multi-messenger astronomy era

2020

En el presente manuscrito se expone el trabajo realizado en el seno de la Collaboración ANTARES-KM3NeT sobre la astronomía multi-mensanjero con neutrinos, que se ha enfocado en dos ejes: la detección de neutrinos de supernova a bajas energías (MeV) con los telecopios KM3NeT y la búsqueda de neutrinos de alta energía (TeV-PeV) en ANTARES en coincidencia con fuentes transitorias detectadas en ondas gravitationales o rayos gamma de muy alta energía O(TeV). El primer análisis, explora la capacidad de los telescopios de neutrinos KM3NeT para detectar la señal de una explosión de supernova (CCSN), así como el potencial de explotar dicha detección para aprender sobre la física que hay detrás, en p…

UniversastroparticlesAstroparticulesTransitoire[PHYS.PHYS]Physics [physics]/Physics [physics]astrophysicsUNESCO::FÍSICAneutrinosmulti-messengerUNESCO::ASTRONOMÍA Y ASTROFÍSICATransientsgravitational waves:FÍSICA [UNESCO]supernovaHaute energieMulti-messagershigh-energyAstrophysique:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Structure of longitudinal chromomagnetic fields in high energy collisions

2014

We compute expectation values of spatial Wilson loops in the forward light cone of high-energy collisions. We consider ensembles of gauge field configurations generated from a classical Gaussian effective action as well as solutions of high-energy renormalization group evolution with fixed and running coupling. The initial fields correspond to a color field condensate exhibiting domain-like structure over distance scales of order the saturation scale. At later times universal scaling emerges at large distances for all ensembles, with a nontrivial critical exponent. Finally, we compare the results for the Wilson loop to the two-point correlator of magnetic fields.

We compute expectation values of spatial Wilson loops in the forward light cone of high-energy collisions. We consider ensembles of gauge field configurations generated from a classical Gaussian effective action as well as solutions of high-energy renormalization group evolution with fixed and running coupling. The initial like structure over distance scales of oder the saturation scale. At later times universal scaling emerges at large distances for all ensembles with a nontrivial critical exponent. Finally we compare the resulats for the Wilson loop to the two-point correlator of magnetic fields. (C) 2014 The Authors. Published by Elsevier BV This is an open access article under the CC BY licenseNuclear and High Energy PhysicsWilson loopLARGE NUCLEINuclear TheoryField (physics)FOS: Physical sciences114 Physical sciences01 natural sciencesColor-glass condensateRENORMALIZATION-GROUPNuclear Theory (nucl-th)GLUON DISTRIBUTION-FUNCTIONSHigh Energy Physics - Phenomenology (hep-ph)Light cone0103 physical sciencesSCATTERINGGauge theory010306 general physicsSMALL-XEffective actionPhysicsCORRELATORSta114010308 nuclear & particles physicsCOLOR GLASS CONDENSATERenormalization groupEVOLUTIONJIMWLK EQUATIONHigh Energy Physics - PhenomenologySATURATIONQuantum electrodynamicsCritical exponentPhysics Letters B
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XIPE: the x-ray imaging polarimetry explorer

2016

XIPE, the X-ray Imaging Polarimetry Explorer, is a mission dedicated to X-ray Astronomy. At the time of writing XIPE is in a competitive phase A as fourth medium size mission of ESA (M4). It promises to reopen the polarimetry window in high energy Astrophysics after more than 4 decades thanks to a detector that efficiently exploits the photoelectric effect and to X-ray optics with large effective area. XIPE uniqueness is time-spectrally-spatially- resolved X-ray polarimetry as a breakthrough in high energy astrophysics and fundamental physics. Indeed the payload consists of three Gas Pixel Detectors at the focus of three X-ray optics with a total effective area larger than one XMM mirror bu…

X-ray AstronomyHigh-energy astronomyPolarimetryX-ray opticsX-ray telescopeCondensed Matter Physic01 natural sciencesObservatory0103 physical sciencesPolarimetryElectronicOptical and Magnetic MaterialsSpectral resolutionElectrical and Electronic Engineering010303 astronomy & astrophysicsGas Pixel DetectorPhysicsX-ray astronomyta115X-ray optics010308 nuclear & particles physicsElectronic Optical and Magnetic MaterialApplied MathematicsVegaAstronomyComputer Science Applications1707 Computer Vision and Pattern RecognitionGas Pixel Detector; Polarimetry; X-ray Astronomy; X-ray opticsCondensed Matter PhysicsComputer Science ApplicationsApplied MathematicGas Pixel Detector; Polarimetry; X-ray Astronomy; X-ray optics; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringGas Pixel Detector; Polarimetry; X-ray Astronomy; X-ray optics; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications; Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringComputer Vision and Pattern RecognitionX-ray optic
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