Search results for "Hydrogen compounds"

showing 5 items of 5 documents

Intrinsic generation of OH groups in dry silicon dioxide upon thermal treatments

2008

We show the existence of an intrinsic generation mechanism of OH groups in synthetic dry silica upon thermal treatments. Samples are treated for ~160 h at 390 °C in He at 2.7 or 180 bar, and the growth of the OH IR absorption band at 3670 cm−1 is observed. An OH concentration of ~10^18 cm^−3 is estimated. Possible contributions of reactions with molecules absorbed from the atmosphere are excluded. Reactions with H2O already contained in the samples are rejected by IR measurements. The observed OH generation is attributed to the reaction of network sites with H2 already present in the material. Possible reaction paths are examined

Hydrogen compoundsIr absorptionPhysics and Astronomy (miscellaneous)Silicon dioxideInorganic chemistryInfrared spectroscopysistemi amorfi difetti di puntoAtmospherechemistry.chemical_compoundchemistryThermalMoleculeOrganic chemistryBar (unit)
researchProduct

Assessment for the mean value total dressing method: Comparison with coupled cluster including triples methods for BF, NO+, CN+, C2, BeO, NH3, CH2, H…

1997

Limited previous experience with the mean value total dressing (MVTD) method had shown that MVTD energies for closed shell systems are generally better than CCSD(T) ones compared to FCI. The method, previously published as total dressing 2′(td-2′), is based on the single reference intermediate Hamiltonian theory. It is not a CC method but deals in a great part with the same physical effects that CC methods that incorporate amplitudes of triples such as CCSDT or its CCSDT-1n approaches. A number of test calculations comparing to diverse CC methods, as well as FCI and experiment when available, have been performed. The tests concern equilibrium energies in NH3 and CH2, equilibrium energies an…

Carbon compoundsGeneral Physics and AstronomyBoron compounds ; Nitrogen compounds ; Water ; Ammonia ; Ozone ; Organic compounds ; Carbon compounds ; Beryllium compounds ; Hydrogen compounds ; Silicon compounds ; Lithium ; Lithium compounds ; Carbon ; Neon compounds ; Coupled cluster calculations ; Dissociation ; Dissociation energies ; Positive ionsLithiumDissociation (chemistry)Nitrogen compoundsIonDissociation energiesOzoneCoupled cluster calculationsAmmoniaBeryllium compoundsOrganic compoundsMoleculeSilicon compoundsPhysical and Theoretical Chemistry:FÍSICA::Química física [UNESCO]Open shellChemistryNeon compoundsMean valueWaterLithium compoundsHydrogen compoundsDiatomic moleculeCarbonUNESCO::FÍSICA::Química físicaCoupled clusterAmplitudeBoron compoundsPositive ionsAtomic physicsDissociation
researchProduct

Anharmonic force fields from analytic CCSD(T) second derivatives: HOF and F2O

1999

The recent implementation of analytic second derivatives for CCSD(T) (coupled cluster theory with single and double excitations augmented by a perturbational treatment of connected triple excitations) has been combined with a numerical finite difference procedure to calculate cubic and semidiagonal quartic force fields. Computational details of this approach are outlined. Applications are reported for HOF and F2O. The CCSD(T) results are in excellent agreement with experiment and represent a substantial improvement over the results obtained from MP2 (Mo/ller–Plesset second-order perturbation theory).

Coupled clusterHydrogen compoundsChemistryQuartic functionQuantum mechanicsAnharmonicityPhysics::Atomic and Molecular ClustersFinite difference methodFinite differenceGeneral Physics and AstronomyPhysical and Theoretical ChemistryPerturbation theorySecond derivativeThe Journal of Chemical Physics
researchProduct

HAWC J2227+610 and its association with G106.3+2.7, a new potential Galactic PeVatron

2020

We present the detection of VHE gamma-ray emission above 100 TeV from HAWC J2227+610 with the HAWC observatory. Combining our observations with previously published results by VERITAS, we interpret the gamma-ray emission from HAWC J2227+610 as emission from protons with a lower limit in their cutoff energy of 800 TeV. The most likely source of the protons is the associated supernova remnant G106.3+2.7, making it a good candidate for a Galactic PeVatron. However, a purely leptonic origin of the observed emission cannot be excluded at this time.

HAWC - Abteilung HintonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Hydrogen compounds010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesLower limitGalaxySpace and Planetary ScienceObservatory0103 physical sciencesSupernova remnantAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciences
researchProduct

Researches concerning the construction of ultrasonic gas filters

2018

Coalescence (physics)DiffractionHydrogen compoundsMaterials scienceScatteringEconomies of agglomerationlawAttenuationUltrasonic sensorFiltrationComputational physicslaw.inventionIOP Conference Series: Materials Science and Engineering
researchProduct