Electroweak quantum chemistry for nuclear-magnetic-resonance-shielding constants: Impact of electron correlation
One promising route towards the first experimental verification of parity violation (PV) in chiral molecular systems is the detection of line splittings between nuclear magnetic resonance (NMR) spectra of enantiomers. Those numerical methods which can be systematically refined and allow for an accur...
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Veröffentlicht in: | Physical review. A, Atomic, molecular, and optical physics Atomic, molecular, and optical physics, 2006-09, Vol.74 (3), Article 032105 |
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Sprache: | eng |
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Zusammenfassung: | One promising route towards the first experimental verification of parity violation (PV) in chiral molecular systems is the detection of line splittings between nuclear magnetic resonance (NMR) spectra of enantiomers. Those numerical methods which can be systematically refined and allow for an accurate and reliable prediction of molecular PV effects will play a crucial role for the preparation and interpretation of such experiments. In this work the ab initio calculation of isotropic parity-violating NMR-shielding constants ({sigma}{sup PV}) within coupled cluster and multiconfiguration linear response approaches to electroweak quantum chemistry is reported and the results are compared to data obtained at the uncoupled density functional theory level. The {sigma}{sup PV} of the heavy nuclei in hydrogen peroxide, disulfane and diselane (H{sub 2}X{sub 2} with X={sup 17}O, {sup 33}S, {sup 77}Se) computed at the coupled cluster singles and doubles level are found to typically deviate from their electron-uncorrelated counterparts by approximately 20%, while in 2-fluorooxirane, electron correlation alters {sigma}{sup PV} of individual nuclei by almost a factor of 2. It is therefore imperative in the accurate prediction of parity-nonconserving phenomena in NMR experiments that systematically improvable electron-correlating electroweak quantum chemical approaches, such as those presented in this study, are employed. |
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ISSN: | 1050-2947 1094-1622 |
DOI: | 10.1103/PhysRevA.74.032105 |