Search results for "electromagnetic"

showing 10 items of 1595 documents

Scattering and absorption imaging of a highly fractured fluid-filled seismogenetic volume in a region of slow deformation

2020

Regions of slow strain often produce swarm-like sequences, characterized by the lack of a clear mainshock-aftershock pattern. The comprehension of their underlying physical mechanisms is challenging and still debated. We used seismic recordings from the last Pollino swarm (2010–2014) and nearby to separate and map seismic scattering (from P peak-delays) and absorption (from late-time coda-wave attenuation) at different frequencies in the Pollino range and surroundings. High-scattering and high-absorption anomalies are markers of a fluid-filled fracture volume extending from SE to NW (1.5–6 ​Hz) across the range. With increasing frequency, these anomalies approximately cover the area where t…

geographygeography.geographical_feature_category010504 meteorology & atmospheric sciencesDeformation (mechanics)ScatteringAttenuationlcsh:QE1-996.5Swarm behaviourActive faultFault (geology)010502 geochemistry & geophysics01 natural scienceslcsh:GeologyFracture (geology)General Earth and Planetary SciencesAbsorption (electromagnetic radiation)SeismologyGeology0105 earth and related environmental sciences
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Forward light-by-light scattering and electromagnetic correction to hadronic vacuum polarization

2023

Lattice QCD calculations of the hadronic vacuum polarization (HVP) have reached a precision where the electromagnetic (e.m.) correction can no longer be neglected. This correction is both computationally challenging and hard to validate, as it leads to ultraviolet (UV) divergences and to sizeable infrared (IR) effects associated with the massless photon. While we precisely determine the UV divergence using the operator-product expansion, we propose to introduce a separation scale $\Lambda\sim400\;$MeV into the internal photon propagator, whereby the calculation splits into a short-distance part, regulated in the UV by the lattice and in the IR by the scale $\Lambda$, and a UV-finite long-di…

hadronic contributionsNuclear and High Energy Physicsfusionmassless530 PhysicsFOS: Physical sciences[PHYS.HLAT] Physics [physics]/High Energy Physics - Lattice [hep-lat]operator product expansionhadronicHigh Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)vacuum polarizationultravioletquantum electrodynamicstree approximationphoton photonlattice[PHYS.HLAT]Physics [physics]/High Energy Physics - Lattice [hep-lat]effectscatteringphotonscattering amplitudeHigh Energy Physics - Lattice (hep-lat)lattice field theory530 Physikradiative correctionssum rule[PHYS.HPHE] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics - Phenomenologyelectromagneticfinite size[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]infrareddispersionlight-by-light scatteringpropagatorcorrectionJournal of High-Energy Physics
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Innovative and Applied Research in Biology: Proceedings, Vol. 3/2021

2021

The collection contains SCIENTIFIC articles on the topics of the LU 79 conference reports. The main focus is on innovative and applied research in biology and interdisciplinary fields.

iPBSBiofragmentationDrosophila melanogaster reproductive successProtecting organisms from UV-B radiation and extremely low-frequency electromagnetic fieldsBiotextile protection propertiesCloudberryGenetic diversitySoil burial testBacterial cellulose:NATURAL SCIENCES::Biology [Research Subject Categories]RetrotransposonsIsocitrate dehydrogenase as a candidate locusImmature gametic cellsAcetic acid bacteriaEcosystem servicesThe Daugava RiverTrifolium repensCypripedium calceolusScanning electron microscopy
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The study of time-resolved absorption and luminescence in PbWO4 crystals

2000

Abstract The transient absorption and luminescence under pulsed electron beam excitation were studied for undoped and La3+ doped PbWO4 crystals. The absorption band at ∼1.0 eV is suggested to be due to self-trapped electrons and the absorption band at 3.5 eV may be due to self-trapped holes. The formation of luminescence centers via electron–hole recombination is affected by La3+ in doped crystals. The large fraction of electrons and holes undergoes thermostimulated recombination within geminate pairs and the spatial separation of geminate pairs components is important in recombination process. The intrinsic (blue) luminescence arises in this recombination. The mechanism of La3+ influence o…

inorganic chemicalsNuclear and High Energy PhysicsAbsorption bandChemistryUltrafast laser spectroscopyDopingElectronAtomic physicsAbsorption (electromagnetic radiation)LuminescenceInstrumentationRecombinationExcitationNuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
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Testing effects of Lorentz invariance violation in the propagation of astroparticles with the Pierre Auger Observatory

2021

The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargüe. We are very grateful to the following agencies and organizations for financial support: Argentina — Comisión Nacional de Energía Atómica; Agencia Nacional de Promoción Científica y Tecnológica (ANPCyT); Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET); Gobierno de la Provincia de Mendoza; Municipalidad de Malargüe; NDM Holdings and Valle Las Leñas; in gratitude for their continuing cooperation over land access; Australia — the Australian Research Council; Be…

interaction [cosmic radiation]mass spectrum [cosmic radiation]dispersion relationAstronomyAstrophysics::High Energy Astrophysical Phenomenaenergy spectrumcosmic ray experimentFOS: Physical sciencesultra high energy cosmic rayscosmic radiation: interactioninvariance: Lorentz01 natural sciences530UHEultra high energy cosmic rayenergy: thresholdFundamental physics gravitational waves LISA Tests of general relativityCosmic ray experiments0103 physical sciencespropagationddc:530physics of the early universeHigh Energy PhysicsLorentz [invariance]010303 astronomy & astrophysicsphoton: fluxflux [photon]Lorentz [violation]High Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEenergy: high010308 nuclear & particles physicscosmic radiation: mass spectrumcosmic ray experiments; ultra high energy cosmic rays; physics of the early universeSettore FIS/01 - Fisica SperimentaleAstronomy and AstrophysicsASTROFÍSICAUltra-high energy cosmic raysthreshold [energy]violation: LorentzAugerobservatoryelectromagnetickinematicsExperimental High Energy Physicshigh [energy]cosmic ray experimentsAstrophysics - High Energy Astrophysical PhenomenaPhysics of the early universe
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Measurement of the Fluctuations in the Number of Muons in Extensive Air Showers with the Pierre Auger Observatory

2021

The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargue. We are very grateful to the following agencies and organizations for financial support: Argentina-Comision Nacional de Energia Atomica, Agencia Nacional de Promocion Cientifica y Tecnologica (ANPCyT), Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET), Gobierno de la Provincia de Mendoza, Municipalidad de Malargue, NDM Holdings and Valle Las Lenas; in gratitude for their continuing cooperation over land access; Australia-the Australian Research Council; Brazil…

interaction: modelPhysics::Instrumentation and DetectorsAstronomyHadronGeneral Physics and AstronomyUltra-high energy cosmic rays muons properties hadronic models01 natural sciencescosmic ray; particle interaction; astroparticle detectorsAugerHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)ironsurface [detector]Observatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]cosmic rayPhysics4. EducationPhysicsSettore FIS/01 - Fisica Sperimentalemeasured [fluctuation]model [interaction]Astrophysics::Instrumentation and Methods for Astrophysicsmodel: hadronicfluctuation: measured3. Good healthAugerobservatoryparticle interactionSciences exactes et naturellesatmosphere [showers]model [particle]airCherenkov counter: waterAstrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]FOS: Physical sciencesCosmic raydetector: fluorescenceNuclear physicsastroparticle detectorscosmic raysmuon0103 physical sciencescalorimeterddc:53014. Life underwatercosmic radiation: UHEHigh Energy Physicsdistribution functionelectromagnetic component010306 general physicsAstrophysiquePierre Auger Observatoryfluorescence [detector]Muonshowers: atmospherehep-exdetector: surfacewater [Cherenkov counter]particle: modelSmall deviationsFísicaASTROFÍSICAAir showerExperimental High Energy PhysicsElementary Particles and Fieldshadronic [model]High Energy Physics::Experiment
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Spins and magnetic moments of 58;60;62;64Mn ground states and isomers

2015

The odd-odd 54;56;58;60;62;64Mn isotopes (Z = 25) were studied using bunched-beam collinear laser spectroscopy at ISOLDE, CERN. From the measured hyperfine spectra the spins and magnetic moments of Mn isotopes up to N = 39 were extracted. The previous tentative ground state spin assignments of 58;60;62;64Mn are now firmly determined to be I = 1 along with an I = 4 assignment for the isomeric states in 58;60;62Mn. The I = 1 magnetic moments show a decreasing trend with increasing neutron number while the I = 4 moments remain quite constant between N = 33 and N = 37. The results are compared to large-scale shell-model calculations using the GXPF1A and LNPS effective interactions. The excellen…

isotoopitSpin parity and isobaric spinFOS: Physical sciencesmangaaniElectromagnetic momentsShell modelmagnetic momentsNuclear Physics - ExperimentPräzisionsexperimente - Abteilung BlaumLaser spectroscopyNuclear Experiment (nucl-ex)Nuclear ExperimentNuclear Experimentspins
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Local Structure Studies of Ti for SrTi16O3 and SrTi18O3 by Advanced X-ray Absorption Spectroscopy Data Analysis

2015

Strontium titanate is a model quantum paraelectric in which in the region of dominating quantum statistics the ferroelectric instability is inhibited due to nearly complete compensation of the harmonic contribution into ferroelectric soft mode frequency by the zero-point motion contribution. The enhancement of atomic masses by the substitution of 18O for 16O decreases the zero-point atomic motion and low-T ferroelectricity in SrTi18O3 is realized. In this study we report on the local structure of Ti in SrTi16O3 and SrTi18O3 by Ti K-edge extended x-ray absorption fine structure measurements in temperature range 6 – 300 K.

isotopic effectX-ray absorption spectroscopylocal atomic structureMaterials scienceCondensed matter physicsX-ray absorption spectroscopySoft modesDielectricAtmospheric temperature rangeCondensed Matter PhysicsFerroelectricityAtomic massElectronic Optical and Magnetic Materialsphase transitionsquantum paraelectricchemistry.chemical_compoundCondensed Matter::Materials ScienceNuclear magnetic resonancechemistryStrontium titanateStrontium titanateAbsorption (electromagnetic radiation)
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All-Organic Waveguide Sensor for Volatile Solvent Sensing

2019

This work was supported by ERDF 1.1.1.1 Activity Project Nr. 1.1.1.1/16/A/046 “Application assessment of novel organic materials by prototyping of photonic devices”. We acknowledge Igors MIHAILOVS for valuable discussions.

lcsh:Applied optics. PhotonicsMaterials scienceMach-Zehnder interferencePhysics::Optics02 engineering and technologywaveguide01 natural sciencesWaveguide (optics)Electromagnetic interference010309 optics020210 optoelectronics & photonics0103 physical sciences0202 electrical engineering electronic engineering information engineering:NATURAL SCIENCES:Physics [Research Subject Categories]Absorption (electromagnetic radiation)business.industrylcsh:TA1501-1820Cladding (fiber optics)Atomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsCore (optical fiber)Solventorganic materialsOptical sensorOptoelectronicsPhotonicsbusinessSensitivity (electronics)Photonic Sensors
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Time of flight for photon in human skin

2016

The time of flight for photons in human skin was measured using picosecond diode laser. Two different wavelength lasers were used - 405 nm and 510 nm. A difference for time of flight in normal skin and in nevus was observed as well as a difference for different wavelength laser irradiation was observed. For 405 nm laser irradiation the difference was 41 ps while comparison of time of flights skin and nevi using 510 nm irradiation showed a result of 32 ps. Results allow to conclude that the time photon travels in skin might depend on the characteristics of the medium and wavelength of the irradiation. This can be related to known data for light penetration depth in human skin for different w…

lcsh:Applied optics. PhotonicsMaterials sciencelcsh:Medical technologyAcoustics and UltrasonicsBiomedical EngineeringHuman skinmedical physicslaw.inventionBiomaterialsOpticslawIrradiationAbsorption (electromagnetic radiation)integumentary systembusiness.industrybiophotonicslcsh:TA1501-1820absorbtionLaserAtomic and Molecular Physics and OpticsBiophotonicsTime of flightWavelengthlight impulselcsh:R855-855.5PicosecondOptoelectronicsbusinessJournal of Biomedical Photonics & Engineering
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