Search results for "Relativistic quantum chemistry"

showing 10 items of 77 documents

Nuclear anapole moment interaction in BaF from relativistic coupled-cluster theory

2018

We present high accuracy relativistic coupled cluster calculations of the P-odd interaction coefficient $W_A$ describing the nuclear anapole moment effect on the molecular electronic structure. The molecule under study, BaF, is considered a promising candidate for the measurement of the nuclear anapole moment, and the preparation for the experiment is now underway [Altunas et al., Phys. Rev. Lett. 120, 142501 (2018)]. Influence of various computational parameters (size of the basis set, treatment of relativistic effects, and treatment of electron correlation) on the calculated $W_A$ coefficient is investigated and a recommended value of 147.7 Hz with an estimated uncertainty of 1.5% is prop…

ATOMIC PARITY NONCONSERVATIONDIATOMIC-MOLECULESP-ODDVIOLATIONAtomic Physics (physics.atom-ph)Nuclear TheoryDENSITY FUNCTIONALSFOS: Physical sciences01 natural sciences010305 fluids & plasmasPhysics - Atomic PhysicsENHANCEMENTMolecular electronic structure0103 physical sciencesIMPLEMENTATIONNuclear Experiment010306 general physicsBasis setPhysicsElectronic correlationELECTRIC-FIELD GRADIENTSDiatomic moleculeWEAK-INTERACTIONSCoupled clusterMoment (physics)Atomic physicsRelativistic quantum chemistryAPPROXIMATIONPhysical Review A
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TASCAを用いたCn, Nh, Fl化学実験のためのHg, Tl, PbのSiO2及びAu表面に対するオンライン化学吸着研究

2018

Online gas-solid adsorption studies with single atom quantities of Hg, Tl, and Pb on SiO$_{2}$ and Au surfaces were carried out using short-lived radioisotopes with half-lives in the range of 4-49 s. This is a model study to measure adsorption enthalpies of superheavy elements Cn, Nh, and Fl. The short-lived isotopes were produced and separated by the gas-filled recoil separator TASCA at GSI. The products were stopped in He gas, and flushed into gas chromatography columns made of Si detectors whose surfaces were covered by SiO$_{2}$ or Au. The short-lived Tl and Pb were successfully measured by the Si detectors with the SiO$_{2}$ surface at room temperature. On the other hand, the Hg did no…

Analytical chemistrychemistry.chemical_elementElectronic structure010402 general chemistry01 natural sciencesadsorption studiethermochromatographyHomologs of superheavy elementRELATIVISTIC PERIODIC DFTMetalGSIAdsorptionCHEMISTRY0103 physical sciencesisothermal chromatographyPhysical and Theoretical ChemistrySUPERHEAVY ELEMENTS010306 general physicsCoperniciumChemistryQUARTZ SURFACE0104 chemical sciencesgas phase chromatography of single atomHEAVIEST ELEMENTSFleroviumELECTRONIC-STRUCTUREvisual_artYield (chemistry)METALvisual_art.visual_art_mediumGas chromatographyRelativistic quantum chemistryphysical preseparationSYSTEMRadiochimica acta
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Study of the reflection spectrum of the accreting neutron star GX 3+1 using XMM-Newton and INTEGRAL

2015

Broad emission features of abundant chemical elements, such as Iron, are commonly seen in the X-ray spectra of accreting compact objects and their studies can provide useful information about the geometry of the accretion processes. In this work, we focus our attention on GX 3+1, a bright, persistent accreting low mass X-ray binary, classified as an atoll source. Its spectrum is well described by an accretion disc plus a stable comptonizing, optically thick corona which dominates the X-ray emission in the 0.3-20 keV energy band. In addition, four broad emission lines are found and we associate them with reflection of hard photons from the inner regions of the accretion disc where doppler an…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSpectral lineSettore FIS/05 - Astronomia E AstrofisicaIonizationAstrophysics::Solar and Stellar AstrophysicsEmission spectrumAccretion accretion discAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Accretion (meteorology)AstronomyAstronomy and AstrophysicsX-rays: binarieStars: neutronNeutron starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceReflection (physics)X-rays: individual (GX 3+1)Low MassRelativistic quantum chemistryAstrophysics - High Energy Astrophysical Phenomena
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The hyperfine structure in the rotational spectra of bromofluoromethane: Lamb-dip technique and quantum-chemical calculations

2008

International audience; The hyperfine structure in the rotational spectra of six isotopic species of bromofluoromethane, namely CH2{79}BrF, CH2{81}BrF, CDH{79}BrF, CDH{81}BrF, CD2{79}BrF, and CD2{81}BrF, has been investigated using the Lamb-dip technique in the submillimeter-wave frequency range. Measurements as well as assignment procedures have been supported by high-level quantum-chemical calculations of the hyperfine parameters at the coupled-cluster level. For all species, the accuracy of the determined rotational and centrifugal distortion constants as well as the bromine quadrupole-coupling constants have been improved with respect to available literature data, whereas the full bromi…

Bromine010304 chemical physicsBromofluoromethaneBiophysicschemistry.chemical_element010402 general chemistryCondensed Matter Physics01 natural sciencesSpectral line0104 chemical scienceschemistry.chemical_compoundchemistryDistortion0103 physical sciencesPhysical SciencesIsotopologuePhysics::Atomic PhysicsTensorPhysical and Theoretical ChemistryAtomic physicsRelativistic quantum chemistryMolecular BiologyHyperfine structure
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Treatment of scalar-relativistic effects on nuclear magnetic shieldings using a spin-free exact-two-component approach.

2013

A cost-effective treatment of scalar-relativistic effects on nuclear magnetic shieldings based on the spin-free exact-two-component theory in its one-electron variant (SFX2C-1e) is presented. The SFX2C-1e scheme gains its computational efficiency, in comparison to the four-component approach, from a focus on spin-free contributions and from the elimination of the small component. For the calculation of nuclear magnetic shieldings, the separation of spin-free and spin-dependent terms in the parent four-component theory is carried out here for the matrix representation of the Dirac equation in terms of a restricted-magnetically balanced gauge-including atomic orbital basis. The resulting spin…

ChemistryMatrix representationGeneral Physics and Astronomychemistry.chemical_elementIonsymbols.namesakeXenonAtomic orbitalMolybdenum compoundsDirac equationQuantum mechanicssymbolsPhysical and Theoretical ChemistryAtomic physicsHamiltonian (quantum mechanics)Relativistic quantum chemistryThe Journal of chemical physics
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Karplus-Type Dependence of Vicinal119Sn-13C and119Sn-1H Spin-Spin Couplings in Organotin(IV) Derivatives: A DFT Study

2009

The empirical Karplus-type dependence of (3)J((119)Sn,(13)C) and (3)J((119)Sn,(1)H) couplings in organotin(IV) derivatives has been computationally validated by DFT methods both at the nonrelativistic and scalar ZORA relativistic level. A preliminary calibration of the computational protocols, by comparing experimental and calculated couplings for a Set Of Suitable rigid molecules, revealed their high predictive power: in particular, relativistic results for (3)J((119)Sn,(13)C) have a mean absolute error of just above 2 Hz, over a range of values up to about 70 Hz. The latter protocol has then been used to study in detail the influence of substituents and multiple paths connecting the coupl…

Coupling constantChemistryKarplus equationOrganic ChemistryCarbon-13Scalar (mathematics)Relativistic effectsNuclear magnetic resonance spectroscopyRelativistic effects DFT NMR spectroscopy tinMolecular physicsDensity functional calculations; NMR spectroscopy; Relativistic effects; TinDensity functional calculationsNMR spectroscopyNuclear magnetic resonanceTinMoleculePhysical and Theoretical ChemistryRelativistic quantum chemistryorganotinVicinalSpin-½European Journal of Organic Chemistry
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Relativistic DFT Calculation of (119)Sn Chemical Shifts and Coupling Constants in Tin Compounds.

2006

The nuclear shielding and spin-spin coupling constants of (119)Sn in stannane, tetramethylstannane, methyltin halides Me4-nSnXn (X = Cl, Br, I; n = 1-3), tin halides, and some stannyl cations have been investigated computationally by DFT methods and Slater all-electron basis sets, including relativistic effects by means of the zeroth order regular approximation (ZORA) method up to spin-orbit coupling. Calculated (119)Sn chemical shifts generally correlate well with experimental values, except when several heavy halogen atoms, especially iodine, are bound to tin. In such cases, calculated chemical shifts are almost constant at the scalar (spin-free) ZORA level; only at the spin-orbit level i…

Coupling constantchemistry.chemical_classificationNMR spectroscopy; computational chemistry; tin compounds; tin-119Chemical shifttin compoundsHalidechemistry.chemical_elementOrganotin(IV) NMR DFT coupling constantstin-119Stannanecomputational chemistryComputer Science Applicationschemistry.chemical_compoundNMR spectroscopychemistryComputational chemistryHalogenPhysics::Atomic and Molecular ClustersPhysics::Chemical PhysicsPhysical and Theoretical ChemistryTinRelativistic quantum chemistryAlkylJournal of chemical theory and computation
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Precision Measurement of the First Ionization Potential of Nobelium

2018

One of the most important atomic properties governing an element's chemical behavior is the energy required to remove its least-bound electron, referred to as the first ionization potential. For the heaviest elements, this fundamental quantity is strongly influenced by relativistic effects which lead to unique chemical properties. Laser spectroscopy on an atom-at-a-time scale was developed and applied to probe the optical spectrum of neutral nobelium near the ionization threshold. The first ionization potential of nobelium is determined here with a very high precision from the convergence of measured Rydberg series to be 6.626 21±0.000 05  eV. This work provides a stringent benchmark for st…

ENERGIESGeneral Physics and Astronomychemistry.chemical_elementElectron[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energysymbols.namesakeIonizationEQUAL-TO 1040103 physical sciencesLAWRENCIUMBUFFER GASPhysics::Atomic PhysicsSUPERHEAVY ELEMENTSLASER SPECTROSCOPY010306 general physicsSpectroscopyPhysicsNEUTRAL YTTERBIUM010308 nuclear & particles physicsHEAVIEST ELEMENTSchemistryRydberg formulasymbolsEXCITED-LEVELSNobeliumACTINIDESIonization energyAtomic physicsRelativistic quantum chemistryLawrencium
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55-Atom clusters of silver and gold: Symmetry breaking by relativistic effects

2006

Abstract Anionic 55-atom clusters of gold and silver are studied using density functional theory, scalar relativistic ab initio pseudopotentials and self-consistent generalized gradient corrections. An almost perfect icosahedron is found to be the clear ground state of Ag 55 - , and its electronic density of states agrees almost perfectly with recently measured high-resolution photoelectron spectra, up to the magnitude of the splitting of the highest free-electron shells by the Ih crystal field. A comparison between theory and a recent experiment allows one to assign icosahedral-based structures also for the Ag 57 - cluster. On the other hand, the Au 55 - cluster has several close-lying low…

General Computer ScienceChemistryIcosahedral symmetryAb initioElectron shellGeneral Physics and AstronomyGeneral ChemistryComputational MathematicsMechanics of MaterialsAb initio quantum chemistry methodsPhysics::Atomic and Molecular ClustersCluster (physics)General Materials ScienceDensity functional theoryAtomic physicsRelativistic quantum chemistryGround stateComputational Materials Science
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A very short uranium-uranium bond: The predicted metastable U22+

2005

Quantum chemical calculations, based on multiconfigurational wave functions and including relativistic effects, show that the U(2)2+ system has a large number of low-lying electronic states with S of 0 to 2 and Lambda ranging from zero to ten. These states share a very small bond length of about 2.30 A, compared to 2.43 A in neutral U2. The Coulomb explosion to 2 U+ lowers the energy by only 1.6 eV and is separated by a broad barrier.

General Physics and Astronomychemistry.chemical_element02 engineering and technology010402 general chemistry7. Clean energy01 natural sciencesMetastabilityTheoretical chemistryPhysical and Theoretical ChemistryWave function010405 organic chemistryBondCoulomb explosionActinideGeneral MedicineUranium021001 nanoscience & nanotechnology3. Good health0104 chemical sciencesBond lengthchemistryddc:540Physical chemistryAtomic physicsRelativistic quantum chemistry0210 nano-technology
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