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Sample records for fh-cn fh-nc h2o-cn

  1. A high level Ab initio study of the anionic hydrogen-bonded complexes FH-CN-, FH-NC-, H2O-CN- and H2O-NC-

    NASA Technical Reports Server (NTRS)

    Lee, Timothy J.

    1989-01-01

    HF, H2O, CN- and their hydrogen-bonded complexes were studied using state-of-the-art ab initio quantum mechanical methods. A large Gaussian one particle basis set consisting of triple zeta plus double polarization plus diffuse s and p functions (TZ2P + diffuse) was used. The theoretical methods employed include self consistent field, second order Moller-Plesset perturbation theory, singles and doubles configuration interaction theory and the singles and doubles coupled cluster approach. The FH-CN- and FH-NC- and H2O-CN-, H2O-NC- pairs of complexes are found to be essentially isoenergetic. The first pair of complexes are predicted to be bound by approx. 24 kcal/mole and the latter pair bound by approximately 15 kcal/mole. The ab initio binding energies are in good agreement with the experimental values. The two being shorter than the analogous C-N hydrogen bond. The infrared (IR) spectra of the two pairs of complexes are also very similar, though a severe perturbation of the potential energy surface by proton exchange means that the accurate prediction of the band center of the most intense IR mode requires a high level of electronic structure theory as well as a complete treatment of anharmonic effects. The bonding of anionic hydrogen-bonded complexes is discussed and contrasted with that of neutral hydrogen-bonded complexes.

  2. A high-level ab initio study of the anionic hydrogen-bonded complexes FH-CN(-), FH-NC(-), H2O-CN(-), and H2O-NC(-)

    NASA Technical Reports Server (NTRS)

    Lee, Timothy J.

    1989-01-01

    HF, H2O, CN- and their hydrogen-bonded complexes were studied using state-of-the-art ab initio quantum mechanical methods. A large Gaussian one particle basis set consisting of triple zeta plus double polarization plus diffuse s and p functions (TZ2P + diffuse) was used. The theoretical methods employed include self consistent field, second order Moller-Plesset perturbation theory, singles and doubles configuration interaction theory and the singles and doubles coupled cluster approach. The FH-CN- and FH-NC- and H2O-CN-, H2O-NC- pairs of complexes are found to be essentially isoenergetic. The first pair of complexes are predicted to be bound by approx. 24 kcal/mole and the latter pair bound by approximately 15 kcal/mole. The ab initio binding energies are in good agreement with the experimental values. The two being shorter than the analogous C-N hydrogen bond. The infrared (IR) spectra of the two pairs of complexes are also very similar, though a severe perturbation of the potential energy surface by proton exchange means that the accurate prediction of the band center of the most intense IR mode requires a high level of electronic structure theory as well as a complete treatment of anharmonic effects. The bonding of anionic hydrogen-bonded complexes is discussed and contrasted with that of neutral hydrogen-bonded complexes.

  3. A high-level ab initio study of the anionic hydrogen-bonded complexes FH-CN(-), FH-NC(-), H2O-CN(-), and H2O-NC(-)

    NASA Technical Reports Server (NTRS)

    Lee, Timothy J.

    1989-01-01

    HF, H2O, CN- and their hydrogen-bonded complexes were studied using state-of-the-art ab initio quantum mechanical methods. A large Gaussian one particle basis set consisting of triple zeta plus double polarization plus diffuse s and p functions (TZ2P + diffuse) was used. The theoretical methods employed include self consistent field, second order Moller-Plesset perturbation theory, singles and doubles configuration interaction theory and the singles and doubles coupled cluster approach. The FH-CN- and FH-NC- and H2O-CN-, H2O-NC- pairs of complexes are found to be essentially isoenergetic. The first pair of complexes are predicted to be bound by approx. 24 kcal/mole and the latter pair bound by approximately 15 kcal/mole. The ab initio binding energies are in good agreement with the experimental values. The two being shorter than the analogous C-N hydrogen bond. The infrared (IR) spectra of the two pairs of complexes are also very similar, though a severe perturbation of the potential energy surface by proton exchange means that the accurate prediction of the band center of the most intense IR mode requires a high level of electronic structure theory as well as a complete treatment of anharmonic effects. The bonding of anionic hydrogen-bonded complexes is discussed and contrasted with that of neutral hydrogen-bonded complexes.

  4. Mechanism for the formation of substituted manganese(V) cyanidonitrido complexes: crystallographic and kinetic study of the substitution reactions of trans-[MnN(H2O)(CN)4]2- with monodentate pyridine and bidentate pyridine-carboxylate ligands.

    PubMed

    van der Westhuizen, Hendrik J; Meijboom, Reinout; Schutte, Marietjie; Roodt, Andreas

    2010-10-18

    Dissolution of [(CH(3))N](2)Na[MnN(CN)(5)]·H(2)O in water results in the rapid dissociation of the trans-CN(-) ligand to form trans-[MnN(H(2)O)(CN)(4)](2-)(aq), which reacts with monodentate pyridine ligands such as 3-methyl and 4-methyl pyridine to form the corresponding mono-substituted complexes, of which the molecular structures obtained from X-ray crystallography, trans-[MnN(3-pic)(CN)(4)](2-) and trans-[MnN(4-pic)(CN)(4)](2-), are reported. [MnN(H(2)O)(CN)(4)](2-)(aq) also reacts with bidentate nucleophiles such as pyridine-2-carboxylate (pico) and quinoline-2-carboxylate (quino), yielding the corresponding [MnN(η(2)-pico)(CN)(3)](2-) and [MnN(η(2)-quino)(CN)(3)](2-) complexes as determined by X-ray crystallography. The formation kinetics of pyridine-2-carboxylate and three different pyridine-2,x-dicarboxylate ligands (x = 3, 4, 5) are reported, and two consecutive reaction steps are proposed, defined as the formation of the [MnN(η(1)-pico)(CN)(4)](3-) and [MnN(η(2)-pico)(CN)(3)](3-) complexes, respectively. Only the second steps could be spectrophotometrically observed and kinetically investigated. The first reaction is attributed to the rapid aqua substitution of [MnN(H(2)O)(CN)(4)](2-), thermodynamically unfavored and too fast to observe by conventional rapid third generation stopped-flow techniques. The second, slower reaction is attributed to cyanido substitution, with overall formation rate constants (25 °C; k(1)'; M(-1) s(-1)) and corresponding activation parameters (ΔH(k1')(double dagger), kJ mol(-1), ΔS(k1')(double dagger), J K(-1) mol(-1)) for the following entering bidentate nucleophiles: pyridine-2-carboxylate: (1.15 ± 0.04) × 10(-3), 102 ± 1, and 48 ± 3; pyridine-2,3-dicarboxylate: (1.1 ± 0.1) × 10(-3), 93 ± 2, and 20 ± 4; pyridine-2,4-dicarboxylate (8.5 ± 0.5) × 10(-4), 123 ± 5, and 115 ± 14; pyridine-2,5-dicarboxylate: (1.08 ± 0.04) × 10(-3), 106 ± 1, and 60 ± 2. A dissociative activation for the cyanido substitution

  5. The Coma of Comet 9P/Tempel 1

    NASA Astrophysics Data System (ADS)

    Farnham, T. L.; Lisse, C. M.; A'Hearn, M. F.; Groussin, O.; Meech, K. J.; Fink, U.; Schleicher, D. G.

    2004-11-01

    The coma of comet Tempel 1 is of interest to the DI mission for a number of reasons: as a phenomenon unto itself; as a proxy for the nucleus composition; as a component of the flux measured in the DI observations; and as an obstacle through which the spacecraft must traverse. It is important to understand the normal baseline state of the coma, for planning purposes as well as to determine exactly how it is changed by the impact. To this end, we have collected all available observations, old, new, published and unpublished, and performed an analysis to produce as complete a picture of the coma as possible. Our results indicate that Tempel 1 is not an unusual comet with respect to dust and gas. Narrowband photometry and spectral measurements show that the production rates of H2O, CN and dust (Afρ ) exhibit clear seasonal variations, with the peak production occurring about two months before perihelion. We expect the total outgassing rate at the time of the encounter to be about 2×1028 mol sec-1. The abundance ratio of carbon chain molecules is at the lower end of the range of ``typical'' in the A'Hearn et al. (1995) classification. Pre-perihelion images from 1994 show at least one jet in the coma, and changes in illumination of its source could be a major cause of the seasonal variations. The column density through the jet is only about twice that in the average coma, so the jet ejecta is not considered to be a significant additional threat to the spacecraft beyond the 0.1 g m-2 total dust fluence already expected from traversing the coma. Thermophysical models of the nucleus' surface indicate that approximately 8% of the comet's surface is active, which is consistent with the existence of isolated active areas. We will present these and other coma properties in more detail, and discuss how they impact the DI mission.

  6. Dinuclear iron(II)-cyanocarbonyl complexes linked by two/three bridging ethylthiolates: relevance to the active site of [Fe] hydrogenases.

    PubMed

    Liaw, Wen-Feng; Tsai, Wen-Ting; Gau, Hung-Bin; Lee, Chien-Ming; Chou, Shin-Yuan; Chen, Wen-Yuan; Lee, Gene-Hsiang

    2003-04-21

    Dinuclear iron(II)-cyanocarbonyl complex [PPN](2)[Fe(CN)(2)(CO)(2)(mu-SEt)](2) (1) was prepared by the reaction of [PPN][FeBr(CN)(2)(CO)(3)] and [Na][SEt] in THF at ambient temperature. Reaction of complex 1 with [PPN][SEt] produced the triply thiolate-bridged dinuclear Fe(II) complex [PPN][(CN)(CO)(2)Fe(mu-SEt)(3)Fe(CO)(2)(CN)] (2) with the torsion angle of two CN(-) groups (C(5)N(2) and C(3)N(1)) being 126.9 degrees. The extrusion of two sigma-donor CN(-) ligands from Fe(II)Fe(II) centers of complex 1 as a result of the reaction of complex 1 and [PPN][SEt] reflects the electron-rich character of the dinuclear iron(II) when ligated by the third bridging ethylthiolate. The Fe-S distances (2.338(2) and 2.320(3) A for complexes 1 and 2, respectively) do not change significantly, but the Fe(II)-Fe(II) distance contracts from 3.505 A in complex 1 to 3.073 A in complex 2. The considerably longer Fe(II)-Fe(II) distance of 3.073 A in complex 2, compared to the reported Fe-Fe distances of 2.6/2.62 A in DdHase and CpHase, was attributed to the presence of the third bridging ethylthiolate, instead of pi-accepting CO-bridged ligand as observed in [Fe] hydrogenases. Additionally, in a compound of unusual composition ([Na.(5)/(2)H(2)O][(CN)(CO)(2)Fe(mu-SEt)(3)Fe(CO)(2)(CN)])(n)((1)/(2)O(Et)(2))(n) (3), the Na(+) cations and H(2)O molecules combining with dinuclear [(CN)(CO)(2)Fe(mu-SEt)(3)Fe(CO)(2)(CN)](-) anions create a polymeric framework wherein two CN(-) ligands are coordinated via CN(-)-Na(+)/CN(-)-(Na(+))(2) linkages, respectively.