Search results for "Length"

showing 10 items of 2188 documents

The Pd3(dppm)3(CO)n clusters (n = 1-,2-); rare cases of anionic palladium species.

2010

Two novel anionic palladium clusters, Pd(3)(dppm)(3)(CO)(n-) (Pd(3)(n); n = 1-,2-) were electrochemically generated from the dicationic cluster Pd(3)(2+) in 0.2 M THF/Bu(4)NPF(6)via two first consecutive reversible 1-electron reductions (Pd(3)(2+) + 1 e(-) ⇌ Pd(3)(+), -0.210, and Pd(3)(+) + 1 e(-) ⇌ Pd(3)(0), -0.470 V vs. SCE) followed by two others at -2.350 (Pd(3)(0) + 1 e(-) ⇌ Pd(3)(1-), reversible) and at -2.690 V vs. SCE (Pd(3)(1-) + 1 e(-) ⇌ Pd(3)(2-), irreversible). The chemical stability and instability, respectively, of the Pd(3)(dppm)(3)(CO)(n-) clusters (Pd(3)(n); n = 1-,2-) at the time scale of the electrochemical experiments were addressed by DFT computations. Indeed, geometry …

Inorganic ChemistryBond lengthStereochemistryOxidation stateChemistryCluster (physics)Substrate (chemistry)chemistry.chemical_elementChemical stabilityElectrochemistryMedicinal chemistryRelative stabilityPalladiumDalton transactions (Cambridge, England : 2003)
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Molecular Multi‐Wavelength Optical Anion Sensors

2010

Polychromatic fingerprinting of simple anions (halides, oxo anions) is achieved by employing neutral and charged multicolor fluorescent probes based on ferrocene-spaced dansyl and naphthyl groups (1/1 + ; 2/2 + ). The conformation of the neutral double dye sensor 2 has been elucidated by NMR spectroscopic techniques (in solution), by X-ray crystallography (solid state) and by DFT calculations (gas phase). The double-dye receptors 2/2 + exhibit specific emission responses in the presence of anions X- when excited at the absorption maxima of the dyes (fingerprint).

Inorganic ChemistryChemistryExcited stateAnalytical chemistrySolid-statePhysical chemistryHalideMulti wavelengthAbsorption (chemistry)FluorescenceFluorescence spectroscopyIonEuropean Journal of Inorganic Chemistry
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Electron Transfer and Conformational Interconversions in 1, n ‐Diphenylpolyenes

1988

1,4-Diphenylbutadiene (1), 1,6-diphenylhexatriene (2), and 1,8-diphenylocatatetraene (3) are reduced with alkali metals and the resulting paramagnetic monoanions and diamagnetic dianions characterized by ESR and (1H-, 13C-)NMR spectroscopy, respectively. The stereodynamic behavior of the ions is studied as a function of chain length, charge, and counterion. The reduction of 1, 2, and 3 serves as a model experiment for the doping of extended linear polyenes (polyacetylenes). Elektronenubertragungen und Konformationsanderungen in 1,n-Diphenylpolyenen 1,4-Diphenylbutadien (1), 1,6-Diphenylhexatrien (2) und 1,8-Diphenyloctatetraen (3) werden mit Alkalimetallen reduziert, und die resultierenden …

Inorganic Chemistrychemistry.chemical_classificationParamagnetismChain lengthElectron transferCrystallographychemistryStereochemistryNuclear magnetic resonance spectroscopyCounterionAlkali metalIonChemische Berichte
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2020

The growth of cloud-based services is mainly supported by the core networking infrastructures of large-scale data centers, while the scalability of these services is influenced by the performance and dependability characteristics of data centers. Hence, the data center network must be agile and reconfigurable in order to respond quickly to the ever-changing application demands and service requirements. The network must also be able to interconnect the big number of nodes, and provide an efficient and fault-tolerant routing service to upper-layer applications. In response to these challenges, the research community began exploring novel interconnect topologies, namely: Flecube, DCell, Ficonn…

InterconnectionComputer Networks and CommunicationsNetwork packetbusiness.industryComputer scienceQuality of service020206 networking & telecommunicationsCloud computing02 engineering and technologyTopologyNetwork topologyAverage path lengthBottleneckComputer Science ApplicationsScalabilityNode (computer science)0202 electrical engineering electronic engineering information engineeringDependabilityData centerElectrical and Electronic EngineeringbusinessSoftwareIEEE/ACM Transactions on Networking
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Strongly decelerated expansion of SN 1979C

2002

We observed SN1979C in M100 on 4 June 1999, about twenty years after explosion, with a very sensitive four-antenna VLBI array at the wavelength of 18cm. The distance to M100 and the expansion velocities are such that the supernova cannot be fully resolved by our Earth-wide array. Model-dependent sizes for the source have been determined and compared with previous results. We conclude that the supernova shock was initially in free expansion for 6 +/- 2 yrs and then experienced a very strong deceleration. The onset of deceleration took place a few years before the abrupt trend change in the integrated radio flux density curves. We estimate the shocked swept-up mass to be about 1.6 solar masse…

InterferometricSupernova remnantsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsSN1979CUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsBinary starVery-long-baseline interferometryFree expansionAstrophysics::Solar and Stellar AstrophysicsISMAstrophysics::Galaxy AstrophysicsEnvelope (waves)PhysicsAstrophysics (astro-ph)Astronomy and AstrophysicsGalaxiesStars:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]GalaxyRadio continuumSupernovaStarsWavelengthSupernovaeInterferometric ; Supernovae ; SN1979C ; ISM ; Supernova remnants ; Radio continuum ; Stars ; M100 ; GalaxiesSpace and Planetary ScienceM100Astrophysics::Earth and Planetary AstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]Astronomy & Astrophysics
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Supporting parents of children with chronic conditions: A randomized controlled trial of web-based and self-help ACT interventions

2021

Objective Many parents of children with chronic conditions and developmental disabilities experience high rates of burnout and psychological distress. The aim of the current study was to examine the effects of two differently delivered interventions based on acceptance and commitment therapy (ACT) on symptoms of burnout, depression, quality of life, psychological flexibility, and mindfulness skills. Method A total of 110 parents of children aged 0.8 to 17 years with chronic conditions and developmental disabilities participated in a randomized controlled trial lasting 13 weeks with two intervention groups: (1) an iACT intervention, including three psychologist-led video conferencing session…

InternetPsykologiVideo conferencinghyväksymis- ja omistautumisterapiaAcceptance and commitment therapyInformation technologyT58.5-58.64113 Computer and information sciencesSelf-helpuupumusFull length ArticleBF1-990itseapu (psykologia)Parents of children with chronic conditionsvanhemmatvideoneuvottelutPsychologyBurnoutkrooniset tauditlapset (perheenjäsenet)
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Minimal star-varieties of polynomial growth and bounded colength

2018

Abstract Let V be a variety of associative algebras with involution ⁎ over a field F of characteristic zero. Giambruno and Mishchenko proved in [6] that the ⁎-codimension sequence of V is polynomially bounded if and only if V does not contain the commutative algebra D = F ⊕ F , endowed with the exchange involution, and M , a suitable 4-dimensional subalgebra of the algebra of 4 × 4 upper triangular matrices , endowed with the reflection involution. As a consequence the algebras D and M generate the only varieties of almost polynomial growth. In [20] the authors completely classify all subvarieties and all minimal subvarieties of the varieties var ⁎ ( D ) and var ⁎ ( M ) . In this paper we e…

Involution (mathematics)Algebra and Number Theory010102 general mathematicsSubalgebraTriangular matrix010103 numerical & computational mathematics01 natural sciencesCombinatoricsSettore MAT/02 - Algebra*-colength *-codimension *-cocharacterBounded function0101 mathematicsCommutative algebraAssociative propertyMathematicsJournal of Pure and Applied Algebra
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Characterization of micromixing in a Continuous Oscillatory Baffled Reactor

2018

International audience; Micromixing is the limiting step in the progress of fast reactions and fast crystallization processes. Micromixing performance of a Nitech© glass COBR has been characterized using the competing parallel iodide-iodate test reactions. Macromixing length was also qualitatively determined by visualization of a tracer. The results show that an increase in the amplitude to baffle space ratio and a decrease of oscillation frequency improves mixing performance.

Iodide-iodate test reactionsMicromixing[SPI]Engineering Sciences [physics][SPI] Engineering Sciences [physics][SPI.GPROC] Engineering Sciences [physics]/Chemical and Process Engineering[SPI.FLUID]Engineering Sciences [physics]/Reactive fluid environmentVillermaux- Dushman[SPI.GPROC]Engineering Sciences [physics]/Chemical and Process Engineering[SPI.FLUID] Engineering Sciences [physics]/Reactive fluid environmentOscillatory baffled reactorMixing length
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Classical ionic fluids in the mean spherical approximation

1980

The recently obtained analytical solution of the mean spherical approximation has been used to calculate thermodynamic and structural properties of aqueous solutions of asymmetric electrolytes. The same approximation has also been used to calculate structure functions of pure and mixed molten salts. The agreement between experimental or “quasi-experimental” structure functions and those obtained within the framework of the MSA is quite good especially when the ionic radii are obtained by fitting the long wavelength limit of the structure functions to the isothermal compressibility of the system, under the condition that the diameter ratio is the same as in the crystal.

Ionic radiusLong wavelength limitChemistryIonic bondingThermodynamicsElectrolyteRadial distribution functionInorganic ChemistryCrystalMaterials ChemistryCompressibilityPhysical chemistryPhysical and Theoretical ChemistryMolten saltInorganica Chimica Acta
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The THESEUS space mission concept: science case, design and expected performances

2018

THESEUS is a space mission concept aimed at exploiting Gamma-Ray Bursts for investigating the early Universe and at providing a substantial advancement of multi-messenger and time-domain astrophysics. These goals will be achieved through a unique combination of instruments allowing GRB and X-ray transient detection over a broad field of view (more than 1sr) with 0.5¿1 arcmin localization, an energy band extending from several MeV down to 0.3¿keV and high sensitivity to transient sources in the soft X-ray domain, as well as on-board prompt (few minutes) follow-up with a 0.7¿m class IR telescope with both imaging and spectroscopic capabilities. THESEUS will be perfectly suited for addressing …

IonizationAtmospheric Sciencecosmological modelCherenkov Telescope Array[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]AstronomyDark ageMASSIVE SINGLE STARSStar formation rates Gamma ray01 natural sciencesCosmology: observationlocalizationlaw.inventionAstrophysicEinstein Telescopeobservational cosmologylawObservational cosmologyRe-ionizationCosmology: observations; Dark ages; First stars; Gamma-ray: bursts; Re-ionizationLIGOobservations [Cosmology]Telescope010303 astronomy & astrophysicsHigh sensitivityHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMulti-wavelengthenergy: highsezelegamma-ray burstsCosmology: observationsCosmology: observations; Dark ages; First stars; Gamma-ray: bursts; Re-ionization; Aerospace Engineering; Space and Planetary ScienceAstrophysics::Instrumentation and Methods for Astrophysicsimagingstar: formationburst [Gamma-ray]observatoryGeophysicsDark agesX rays Cosmology: observationAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenasignatureStarTIDAL DISRUPTIONGamma-ray: burstAstrophysics::High Energy Astrophysical PhenomenaSIMILAR-TO 6Socio-culturaleFOS: Physical sciencesAerospace EngineeringGamma-ray: burstsobservation [Cosmology]galaxy: luminosityX-ray astronomy: instrumentation7 CANDIDATE GALAXIESAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burst114 Physical sciencesSettore FIS/03 - Fisica della MateriaTelescopeX-raybursts [Gamma-ray]FIS/05 - ASTRONOMIA E ASTROFISICASettore FIS/05 - Astronomia e AstrofisicaFirst star0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]KAGRAInstrumentation and Methods for Astrophysics (astro-ph.IM)Astrophysics::Galaxy AstrophysicsFirst starsLIGHT CURVESEinstein Telescope010308 nuclear & particles physicsGravitational wavegravitational radiationAstronomyAstronomy and Astrophysics115 Astronomy Space scienceCherenkov Telescope ArrayredshiftsensitivityRedshiftNEUTRON-STAR MERGERmessengerVIRGOelectromagneticLUMINOSITY FUNCTIONSpace and Planetary ScienceBLACK-HOLEGeneral Earth and Planetary SciencesGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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