Search results for "ODS"

showing 10 items of 5812 documents

Mechanism of aluminium incorporation into C–S–H from ab initio calculations

2014

Blended cements have great potential to reduce the CO2 footprint due to cement production. C(alcium)–S(ilicate)–H(ydrate) in these novel materials is known to incorporate a considerable amount of Al. We have for the first time applied large-scale first principles calculations to address the mechanism of Al incorporation into low C/S ratio C–S–H. In agreement with state-of-the-art NMR information, our calculations show that Al substitutes Si in bridging tetrahedra only, and that substitutions in pairing tetrahedra are strongly disfavoured in a wide range of conditions. In broad terms, the energy penalty for having an Al atom in a pairing position is of about 20 kcal mol−1. Al in bridging tet…

Work (thermodynamics)Range (particle radiation)Materials scienceRenewable Energy Sustainability and the Environmentchemistry.chemical_elementThermodynamicsContext (language use)02 engineering and technologyGeneral Chemistry010402 general chemistry021001 nanoscience & nanotechnology01 natural sciences0104 chemical sciencesCrystallographychemistryAluminiumAb initio quantum chemistry methodsPairingAtomTetrahedronGeneral Materials Science[PHYS.PHYS.PHYS-CHEM-PH]Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]0210 nano-technologyComputingMilieux_MISCELLANEOUS
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Ferromagnetic kinetic exchange interaction in magnetic insulators

2020

The superexchange theory predicts dominant antiferromagnetic kinetic interaction when the orbitals accommodating magnetic electrons are covalently bonded through diamagnetic bridging atoms/groups. Here we show that explicit consideration of magnetic and (leading) bridging orbitals, together with the electron transfer between the former, reveals a strong ferromagnetic kinetic exchange contribution. First principle calculations show that it is comparable in strength with antiferromagnetic superexchange in a number of magnetic materials with diamagnetic metal bridges. In particular, it is responsible for a very large ferromagnetic coupling ($-10$ meV) between the iron ions in a Fe$^{3+}$-Co$^{…

Work (thermodynamics)magneettiset ominaisuudetMaterials scienceelectronic-structurePhysics MultidisciplinaryFOS: Physical sciencesmagnetic couplingelektronitmagneettikentätKinetic energyteoriatORBITAL PHYSICSCondensed Matter - Strongly Correlated ElectronsCondensed Matter::Materials ScienceANTIFERROMAGNETISMHUBBARD-MODELPhysics - Chemical PhysicsSUPEREXCHANGE INTERACTIONSdensity functional theoryChemical Physics (physics.chem-ph)Condensed Matter - Materials SciencecomplexesScience & TechnologyStrongly Correlated Electrons (cond-mat.str-el)Condensed matter physicsCRYSTALmagnetic insulatorsPhysicsSUPERCONDUCTIVITYExchange interactionMaterials Science (cond-mat.mtrl-sci)transitionORDERhubbard-modelsuperexchange interactionsWannier function methodsELECTRONIC-STRUCTUREFerromagnetismPhysical SciencesCondensed Matter::Strongly Correlated ElectronsCOMPLEXESTRANSITION
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Tracking Changes in Frontal Lobe Hemodynamic Response in Individual Adults With Developmental Language Disorder Following HD tDCS Enhanced Phonologic…

2020

Background: Current research suggests a neurobiological marker of developmental language disorder (DLD) in adolescents and young adults may be an atypical neural profile coupled with behavioral performance that overlaps with that of normal controls. Although many imaging techniques are not suitable for the study of speech and language processing in DLD populations, fNIRS may be a viable option. In this study we asked if fNIRS can be used to identify atypical cortical activation patterns in individual adults with DLD and track potential changes in cortical activation patterns following a phonological working memory training protocol enhanced with anodal HD tDCS stimulation to the presuppleme…

Working memory trainingmedicine.medical_specialtyBrain activity and meditationdevelopmental language disorderAudiology050105 experimental psychologylcsh:RC321-57103 medical and health sciencesBehavioral Neurosciencespoken word processing0302 clinical medicinememory updating and inhibitionMethodsmedicinefunctional near-infrared spectroscopyhigh definition transcranial direct current stimulation0501 psychology and cognitive sciencesYoung adultn-backPrefrontal cortexlcsh:Neurosciences. Biological psychiatry. NeuropsychiatryBiological Psychiatryn-backprefrontal cortexWorking memorybusiness.industry05 social sciencesPsychiatry and Mental healthNeuropsychology and Physiological PsychologyNeurologyFrontal lobeFunctional near-infrared spectroscopybusiness030217 neurology & neurosurgeryNeuroscienceFrontiers in Human Neuroscience
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The Athena X-ray Integral Field Unit: a consolidated design for the system requirement review of the preliminary definition phase

2023

The Athena X-ray Integral Unit (X-IFU) is the high resolution X-ray spectrometer, studied since 2015 for flying in the mid-30s on the Athena space X-ray Observatory, a versatile observatory designed to address the Hot and Energetic Universe science theme, selected in November 2013 by the Survey Science Committee. Based on a large format array of Transition Edge Sensors (TES), it aims to provide spatially resolved X-ray spectroscopy, with a spectral resolution of 2.5 eV (up to 7 keV) over an hexagonal field of view of 5 arc minutes (equivalent diameter). The X-IFU entered its System Requirement Review (SRR) in June 2022, at about the same time when ESA called for an overall X-IFU redesign (i…

X-IFU: The X-ray Integral Field UnitCosmology and Nongalactic Astrophysics (astro-ph.CO)The X-ray Integral Field Unit [X-IFU]Solar and stellar astrophysicsFOS: Physical sciences/dk/atira/pure/sustainabledevelopmentgoals/responsible_consumption_and_production[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Settore FIS/05 - Astronomia E AstrofisicaX-raysSDG 7 - Affordable and Clean EnergyInstrumentation and Methods for Astrophysics (astro-ph.IM)Solar and Stellar Astrophysics (astro-ph.SR)High Energy Astrophysical Phenomena (astro-ph.HE)/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyAstrophysics of GalaxiesAthena: the advanced telescope for high energy astrophysicsAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesAstrophysical phenomenaSpace instrumentationAstrophysics - Solar and Stellar AstrophysicsHigh energySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]the advanced telescope for high energy astrophysics [Athena]Athena: the advanced telescope for high energy astrophysics · X-IFU: The X-ray Integral Field Unit · Space instrumentation · X-rays · ObservatoryObservatoryAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaSDG 12 - Responsible Consumption and ProductionAstrophysics - Cosmology and Nongalactic Astrophysics
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Electronic structure of single-crystal rocksalt CdO studied by soft x-ray spectroscopies andab initiocalculations

2008

Soft x-ray emission spectroscopy (XES) and x-ray absorption spectroscopy (XAS) are employed to investigate the occupied and unoccupied electronic structures in rocksalt-phase single-crystal CdO. Resonant XES at the OK edge reveals a clear Cd 4d-O 2p hybridized peak and momentum-dependent coherent contributions to the resonant emission spectra. Good agreement is obtained between the above-threshold XES and XAS spectra, and the calculated O 2p local partial density of states (PDOS). Calculation of the O 2p PDOS was performed within the GW framework of many-body perturbation theory.

X-ray absorption spectroscopyMaterials scienceAbsorption spectroscopyAb initio quantum chemistry methodsAstrophysics::High Energy Astrophysical PhenomenaElectronic structureEmission spectrumPerturbation theoryAtomic physicsCondensed Matter PhysicsSingle crystalSpectral lineElectronic Optical and Magnetic MaterialsPhysical Review B
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Interplay between local structure, vibrational and electronic properties on CuO under pressure

2020

The electronic and local structural properties of CuO under pressure have been investigated by means of X-ray absorption spectroscopy (XAS) at Cu K edge and ab initio calculations, up to 17 GPa. The crystal structure of CuO consists of Cu motifs within CuO4 square planar units and two elongated apical Cu-O bonds. The CuO4 square planar units are stable in the studied pressure range, with Cu-O distances that are approximately constant up to 5 GPa, and then decrease slightly up to 17 GPa. In contrast, the elongated Cu-O apical distances decrease continuously with pressure in the studied range. An anomalous increase of the mean square relative displacement (EXAFS Debye-Waller, s2) of the elong…

X-ray absorption spectroscopyMaterials scienceAbsorption spectroscopyCondensed matter physicsExtended X-ray absorption fine structureBand gapGeneral Physics and Astronomy02 engineering and technologyCrystal structure021001 nanoscience & nanotechnology01 natural sciencesIonK-edgeAb initio quantum chemistry methods0103 physical sciencesPhysical and Theoretical Chemistry010306 general physics0210 nano-technology
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ATHENA X-IFU thermal filters development status toward the end of the instrument phase-A

2018

Copyright 2018 Society of Photo-Optical Instrumentation Engineers (SPIE). One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited. The X-ray Integral Field Unit (X-IFU) is one of the two instruments of the Athena astrophysics space mission approved by ESA in the Cosmic Vision 2015-2025 Science Programme. The X-IFU consists of a large array of transition edge sensor micro-calorimeters that will operate at 100 mK inside a sophisticated cryostat. A set of thin filters, highly transparent to X-rays, will be m…

X-ray detectorCryostatCosmic VisionPhotonComputer scienceShieldsCondensed Matter Physicmicrocalorimeter01 natural sciences7. Clean energySettore FIS/05 - Astronomia E AstrofisicaX-ray Integral Field Unit (X-IFU)0103 physical sciencesthermal thin-film filterElectrical and Electronic EngineeringAerospace engineering010306 general physics010303 astronomy & astrophysicsbusiness.industryElectronic Optical and Magnetic MaterialDetectorAstrophysics::Instrumentation and Methods for AstrophysicsShot noiseComputer Science Applications1707 Computer Vision and Pattern RecognitionTransition Edge SensorApplied MathematicATHENA X-ray observatoryRadio frequencyTransition edge sensorbusinessSpace Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray
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The LOFT mission concept: a status update

2016

The Large Observatory For x-ray Timing (LOFT) is a mission concept which was proposed to ESA as M3 and M4 candidate in the framework of the Cosmic Vision 2015-2025 program. Thanks to the unprecedented combination of effective area and spectral resolution of its main instrument and the uniquely large field of view of its wide field monitor, LOFT will be able to study the behaviour of matter in extreme conditions such as the strong gravitational field in the innermost regions close to black holes and neutron stars and the supra-nuclear densities in the interiors of neutron stars. The science payload is based on a Large Area Detector (LAD, >8m2 effective area, 2-30 keV, 240 eV spectral resolut…

X-ray timing[ SDU.ASTR.GA ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]Field of viewAstrophysics01 natural scienceslaw.inventionlawObservatorytiming010303 astronomy & astrophysicsQBPhysicsmicrochannel plates. PROPORTIONAL COUNTER ARRAYCALIBRATIONX-ray astronomyElectronic Optical and Magnetic MaterialApplied MathematicsAstrophysics::Instrumentation and Methods for AstrophysicsComputer Science Applications1707 Computer Vision and Pattern RecognitionX-ray detectorsCondensed Matter Physicscompact objectsX-ray spectroscopy[SDU.ASTR.GA]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]spectroscopyCosmic Vision[ INFO ] Computer Science [cs]Silicon detectorAstrophysics::High Energy Astrophysical PhenomenaCondensed Matter PhysicTelescopeX-rayX-ray astronomySilicon detectors; spectroscopy; timing; X-ray astronomy; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Applied Mathematics; Electrical and Electronic EngineeringSettore FIS/05 - Astronomia e Astrofisica0103 physical sciencesElectronic[INFO]Computer Science [cs]Optical and Magnetic MaterialsSpectral resolutionElectrical and Electronic EngineeringDETECTORta115X-ray astronomy Silicon detectors timing spectroscopy010308 nuclear & particles physicsX-ray imagingX-ray timing; X-ray spectroscopy; X-ray imaging; compact objects; X-ray detectors; microchannel plates. PROPORTIONAL COUNTER ARRAY; CALIBRATION; DETECTORApplied MathematicNeutron starQB460-466 AstrophysicsSilicon detectors; spectroscopy; timing; X-ray astronomy; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringSilicon detectors; spectroscopy; timing; X-ray astronomySilicon detectorsLarge Observatory For x-ray Timing (LOFT) Large Area Detector (LAD) Wide Field Monitor (WFM) Large Area Silicon Drift Detectors (SDD)Gamma-ray burst
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IBIS: The Imager on-board INTEGRAL

2003

The IBIS telescope is the high angular resolution gamma-ray imager on-board the INTEGRAL Observatory, successfully launched from Baikonur (Kazakhstan) the 17th of October 2002. This medium size ESA project, planned for a 2 year mission with possible extension to 5, is devoted to the observation of the gamma-ray sky in the energy range from 3 keV to 10 MeV (Winkler 2001). The IBIS imaging system is based on two independent solid state detector arrays optimised for low ( 15-1000 keV) and high ( 0.175-10.0 MeV) energies surrounded by an active VETO System. This high efficiency shield is essential to minimise the background induced by high energy particles in the highly excentric out of van All…

X-ray transientAstrophysics::High Energy Astrophysical PhenomenaINTEGRAL ; IBIS ; Gamma-ray imagingUNESCO::ASTRONOMÍA Y ASTROFÍSICAlaw.inventionTelescopesymbols.namesakeOpticslawObservatoryGamma-ray imagingAngular resolutionCoded aperturePhysicsIbisbiologyINTEGRALbusiness.industryAstrophysics::Instrumentation and Methods for AstrophysicsGamma rayAstronomy and Astrophysicsbiology.organism_classification:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Space and Planetary ScienceVan Allen radiation beltsymbolsIBISUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniabusiness:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]Astronomy & Astrophysics
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Science case study and scientific simulations for the enhanced X-ray Timing Polarimetry mission, eXTP

2022

The X-ray astronomy mission eXTP (enhanced X-ray Timing Polarimetry) is designed to study matter under extreme conditions of density, gravity and magnetism. Primary goals are the determination of the equation of state (EoS) of matter at supranuclear density, the physics in extremely strong magnetic fields, the study of accretion in strong-field gravity (SFG) regime. Primary targets include isolated and binary neutron stars, strong magneticfield systems like magnetars, and stellar-mass and supermassive black holes. In this paper we report about key observations and simulations with eXTP on the primary objectives involving accretion under SFG regimes and determination of NS-EoS.

X-raymethods and techniquesdense matterSettore FIS/05 - Astronomia E AstrofisicaaccretionNeutron starBlack HoleAstronomical instrumentation
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