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showing 10 items of 3080 documents

Interpretation of the Ni K-edge EXAFS in nanocrystalline nickel oxide using molecular dynamics simulations

2011

Abstract Analysis of atomic structure at the nanoscale is a challenging task, complicated by relaxation phenomena and thermal disorder. In this work, the x-ray absorption spectroscopy at the Ni K-edge was used to address this problem in nanocrystalline NiO (nano-NiO) at 300 K. The analysis of the first two coordination shells using conventional two-shell single-scattering approximation allowed us to determine the expansion of the average lattice but contraction of the Ni―O bonds in the first coordination shell in nano-NiO in comparison with the bulk nickel oxide. The EXAFS signal generated within the first six coordination shells (up to ~ 6.5 A) was successfully interpreted using classical …

Absorption spectroscopyExtended X-ray absorption fine structureChemistryNickel oxideAb initioAnalytical chemistry02 engineering and technology021001 nanoscience & nanotechnologyCondensed Matter Physics01 natural sciencesNanocrystalline materialElectronic Optical and Magnetic MaterialsCondensed Matter::Materials ScienceMolecular dynamicsK-edgeChemical physicsSurface-extended X-ray absorption fine structure0103 physical sciencesMaterials ChemistryCeramics and Compositesddc:660010306 general physics0210 nano-technology
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External pressure and composition effects on the atomic and electronic structure of SnWO4

2015

The atomic and electronic structure of tin tungstates, α-SnWO4, α-Sn1.03W0.99O4 and β-SnWO4 ,w as studied by the W L3-edge X-ray absorption spectroscopy and first-principles linear combination of atomic orbital (LCAO) calculations based on the hybrid exchange-correlation density functional (DFT)/ Hartree–Fock (HF) scheme. It was found that the crystal structure of both α-phases is built up of strongly distorted WO6 octahedra, whereas that of β-SnWO4 is composed of nearly regular WO4 tetrahedra. In addition, there are distorted SnO6 octahedra in both α- and β-phases. The metal–oxygen octahedra distortion is explained by the second-order Jahn–Teller effect. The influence of pressure on the st…

Absorption spectroscopyExtended X-ray absorption fine structureRenewable Energy Sustainability and the EnvironmentBand gapChemistryElectronic structureCrystal structureMolecular physicsSurfaces Coatings and FilmsElectronic Optical and Magnetic MaterialsCrystallographyAtomic orbitalOctahedronLinear combination of atomic orbitalsddc:530
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Present status and first results of the final focus beam line at the KEK Accelerator Test Facility

2011

ATF2 is a final-focus test beam line which aims to focus the low emittance beam from the ATF damping ring to a vertical size of about 37 nm and to demonstrate nanometer level beam stability. Several advanced beam diagnostics and feedback tools are used. In December 2008, construction and installation were completed and beam commissioning started, supported by an international team of Asian, European, and U.S. scientists. The present status and first results are described.

Accelerator Physics (physics.acc-ph)Nuclear and High Energy PhysicsLow emittancePhysics and Astronomy (miscellaneous)Nuclear engineering[PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph]FOS: Physical sciencesbeam transport01 natural sciencesBeam characteristicslaw.inventionNuclear physicslaw0103 physical sciencesddc:530lcsh:Nuclear and particle physics. Atomic energy. RadioactivityBeam handling010306 general physicsAccelerator Test FacilityPhysicsFocus (computing)Research Groups and Centres\Physics\Low Temperature Physics010308 nuclear & particles physicsFaculty of Science\PhysicsBeam commissioningFísicaParticle acceleratorSurfaces and Interfaces29.27.Eg 29.27.Fh 29.20.dbAccelerators and Storage RingsStorage rings and collidersCOLLIDERSTechnology for normal conducting higher energy linear accelerators [9]BeamlineTest beamlcsh:QC770-798Physics - Accelerator PhysicsBeam (structure)
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Polarization-Dependent Disappearance of a Resonance Signal -- Indication for Optical Pumping in a Storage Ring?

2021

We report on laser spectroscopic measurements on Li$^+$ ions in the experimental storage ring ESR at the GSI Helmholtz Centre for Heavy Ion Research. Driving the $2s\,^3\!{S}_1\;(F=\frac{3}{2}) \,\leftrightarrow\,2p\,^3\!P_2\;(F=\frac{5}{2}) \leftrightarrow 2s\,^3\!{S}_1\;(F=\frac{5}{2})$ $\Lambda$-transition in $^7$Li$^+$ with two superimposed laser beams it was found that the use of circularly polarized light leads to a disappearance of the resonance structure in the fluorescence signal. This can be explained by optical pumping into a dark state of polarized ions. We present a detailed theoretical analysis of this process that supports the interpretation of optical pumping and demonstrate…

Accelerator Physics (physics.acc-ph)Nuclear and High Energy PhysicsPhysics and Astronomy (miscellaneous)Atomic Physics (physics.atom-ph)FOS: Physical sciences53001 natural sciencesIonlaw.inventionPhysics - Atomic PhysicsOptical pumpinglaw0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivityddc:530010306 general physicsCircular polarizationPhysics010308 nuclear & particles physicsSurfaces and InterfacesLaserPolarization (waves)FluorescenceDark statelcsh:QC770-798Physics - Accelerator PhysicsAtomic physicsStorage ring
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Direct Measurement of Focusing Fields in Active Plasma Lenses

2018

Physical review accelerators and beams 21(12), 122801 (2018). doi:10.1103/PhysRevAccelBeams.21.122801

Accelerator Physics (physics.acc-ph)Nuclear and High Energy PhysicsPhysics and Astronomy (miscellaneous)Field (physics)FOS: Physical sciences01 natural sciences530law.inventionOpticslaw0103 physical sciencesddc:530Thermal emittancelcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsphysics.acc-phPhysics010308 nuclear & particles physicsbusiness.industrySurfaces and InterfacesPlasmaNuclear & Particles PhysicsLens (optics)Physics::Space PhysicsPhysical SciencesCathode raylcsh:QC770-798Physics::Accelerator PhysicsPhysics - Accelerator PhysicsBeam emittancebusinessCharged particle beamBeam (structure)
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International workshop on next generation gamma-ray source

2022

Journal of physics / G 49(1), 010502 (2022). doi:10.1088/1361-6471/ac2827

Accelerator Physics (physics.acc-ph)Nuclear and High Energy Physics[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]Nuclear Theorynucleon: structurepi: photoproduction[PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph]conference summarynuclear astrophysicsFOS: Physical scienceslow-energy QCD[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]530bremsstrahlung01 natural scienceselectron: acceleratorNuclear Theory (nucl-th)parity: violationnuclear physicsquantum chromodynamics0103 physical sciencesAgency (sociology)ddc:530gamma-rayApplied researchNuclear Experiment (nucl-ex)010306 general physicsphoton: beamNuclear Experimentactivity reportenergy: lowPhysicsastrophysics010308 nuclear & particles physicsInformation sharinglaserhadronic parity violationgamma raynuclear structureSystems engineeringPhysics - Accelerator PhysicsCompton scatteringJournal of Physics G: Nuclear and Particle Physics
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Broadband Multi-wavelength Properties of M87 during the 2017 Event Horizon Telescope Campaign

2021

Full list of authors: EHT MWL Science Working Group; Algaba, J. C.; Anczarski, J.; Asada, K.; Baloković, M.; Chandra, S.; Cui, Y. -Z.; Falcone, A. D.; Giroletti, M.; Goddi, C.; Hada, K.; Haggard, D.; Jorstad, S.; Kaur, A.; Kawashima, T.; Keating, G.; Kim, J. -Y.; Kino, M.; Komossa, S.; Kravchenko, E. V.; Krichbaum, T. P.; Lee, S. -S.; Lu, R. -S.; Lucchini, M.; Markoff, S.; Neilsen, J.; Nowak, M. A.; Park, J.; Principe, G.; Ramakrishnan, V.; Reynolds, M. T.; Sasada, M.; Savchenko, S. S.; Williamson, K. E.; Event Horizon Telescope Collaboration; Akiyama, Kazunori; Alberdi, Antxon; Alef, Walter; Anantua, Richard; Azulay, Rebecca; Baczko, Anne-Kathrin; Ball, David; Barrett, John; Bintley, Dan; …

Accretion010504 meteorology & atmospheric sciencesAstronomyFluxAstrophysics7. Clean energy01 natural sciencesActive galactic nuclei; Radio cores; Low-luminosity active galactic nuclei; High energy astrophysics; Astrophysical black holes; Accretion; Astrophysics - High Energy Astrophysical Phenomena; Astrophysics - Cosmology and Nongalactic Astrophysics; Astrophysics - Astrophysics of Galaxies010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HERadio coreAccretion (meteorology)PhysicsAstrophysical black holes520 Astronomie und zugeordnete WissenschaftenActive galactic nuclei ; Radio cores ; Low-luminosity ; active galactic nuclei ; High energy astrophysics ; Astrophysical black holes ; AccretionAstrophysical black holeLow-luminosity active galactic nucleiastro-ph.COAstrophysics - High Energy Astrophysical PhenomenaAccretion; Active galactic nuclei; Astrophysical black holes; High energy astrophysics; Low-luminosity active galactic nuclei; Radio coresHigh energy astrophysicsRadio coresAstrophysics - Cosmology and Nongalactic AstrophysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusHigh-energy astronomyastro-ph.GAAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesF500Astrophysics::Cosmology and Extragalactic AstrophysicsHigh energy astrophysic0103 physical sciencesVery-long-baseline interferometryddc:530Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesEvent Horizon TelescopeSupermassive black holeActive galactic nucleiAstronomy and Astrophysics530 PhysikAstrophysics - Astrophysics of GalaxiesGalaxySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)ddc:520Active galactic nuclei; Radio cores; Low-luminosity active galactic nuclei; High energy astrophysics; Astrophysical black holes; AccretionHESS - Abteilung Hinton[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Audit and Earnings Management in Spanish SMEs

2016

Abstract Evidence about the relation between earnings management and voluntary audits is scarce, and there is no research about the effectiveness of mandatory audits to improve earnings quality. Using a sample of Spanish SMEs, where some companies are mandatorily audited and some are exempt from audit, we examine if audits, either mandatory or voluntary, help to improve accounting quality by constraining earnings management. We also examine differences between voluntary and mandatory audits, as well as the role of Big 4 and Middle-Tier auditors. After controlling for other characteristics that affect earnings management, we find that audited companies have lower absolute discretionary accru…

Accrualmedia_common.quotation_subjecteducationSMEsAccountingSample (statistics)Auditlcsh:BusinessConservatismEarnings qualityEarnings managementhealth services administration0502 economics and businessddc:650Earnings qualityQuality (business)health care economics and organizationsmedia_commonFinance050208 financebusiness.industry05 social sciencesAuditing050201 accountingGeneral MedicineEarnings managementSpainBusinesslcsh:HF5001-6182SSRN Electronic Journal
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Measurement of acoustic attenuation in South Pole ice

2010

Using the South Pole Acoustic Test Setup (SPATS) and a retrievable transmitter deployed in holes drilled for the IceCube experiment, we have measured the attenuation of acoustic signals by South Pole ice at depths between 190 m and 500 m. Three data sets, using different acoustic sources, have been analyzed and give consistent results. The method with the smallest systematic uncertainties yields an amplitude attenuation coefficient alpha = 3.20 \pm 0.57 km^(-1) between 10 and 30 kHz, considerably larger than previous theoretical estimates. Expressed as an attenuation length, the analyses give a consistent result for lambda = 1/alpha of ~1/300 m with 20% uncertainty. No significant depth or …

Acoustic attenuation; Acoustics; Ice; Neutrino astronomy; South Pole[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]010504 meteorology & atmospheric sciences[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]iceFOS: Physical sciencesAetiology screening and detection [ONCOL 5]Lambda01 natural sciencesneutrino astronomy[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]OpticsSpectrum0103 physical sciencesacousticsInstrumentation and Methods for Astrophysics (astro-ph.IM)0105 earth and related environmental sciencesPhysicsSouth Pole010308 nuclear & particles physicsbusiness.industryAttenuation[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]TransmitterAttenuation lengthAstronomy and AstrophysicsGeodesy004AmplitudeAttenuation coefficientddc:540NeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsbusinessAcoustic attenuationinfo:eu-repo/classification/ddc/004acoustic attenuation
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First Multi-wavelength Campaign on the Gamma-ray-loud Active Galaxy IC 310

2017

The extragalactic VHE gamma-ray sky is rich in blazars. These are jetted active galactic nuclei viewed at a small angle to the line-of-sight. Only a handful of objects viewed at a larger angle are known so far to emit above 100 GeV. Multi-wavelength studies of such objects up to the highest energies provide new insights into the particle and radiation processes of active galactic nuclei. We report the results from the first multi-wavelength campaign observing the TeV detected nucleus of the active galaxy IC 310, whose jet is observed at a moderate viewing angle of 10 deg - 20 deg. The multi-instrument campaign was conducted between 2012 Nov. and 2013 Jan., and involved observations with MAG…

Active galactic nucleusAstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesEnergy fluxAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGalaxies: active; Galaxies: individual: IC 310; Gamma rays: galaxies; Astronomy and Astrophysics; Space and Planetary Science01 natural scienceslaw.inventionlawGalaxies: individual: IC 3100103 physical sciencesindividual: IC 310 [galaxies]Blazar010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsgalaxie [Gamma rays]010308 nuclear & particles physicsGamma rayAstronomy and AstrophysicsGalaxies: activeAstronomy and AstrophysicAstrophysics - Astrophysics of GalaxiesSynchrotrongamma rays: galaxies ; galaxies: active ; individual (IC 310)Gamma rays: galaxiesSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)active [galaxies]galaxies [gamma rays]ComputingMethodologies_DOCUMENTANDTEXTPROCESSINGSpectral energy distributionddc:520Astrophysics - High Energy Astrophysical PhenomenaFermi Gamma-ray Space TelescopeFlare
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