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Computational prediction of the absolute configuration of stereogenic carbon center

Author
SANTELLI, Maurice1
[1] Laboratoire de synthèse organique, UMR 6180 et université Paul-Cézanne (Aix-Marseille-3), « Chimtechnoingies : catalyse et biocatalyse », avenue Escadrille-Normandie-Niemen, 13397 Marseille, France
Source

Comptes rendus. Chimie. 2005, Vol 8, Num 5, pp 923-930, 8 p ; ref : 13 ref

ISSN
1631-0748
Scientific domain
Chemistry
Publisher
Elsevier, Paris
Publication country
France
Document type
Article
Language
English
Author keyword
Atome de carbone stéréogénique Configurations absolues ; Signe du pouvoir rotatoire
Keyword (fr)
Activité optique Carbone composé Composé chiral Configuration absolue Etude théorique Rotation polarisation optique Théorie Hartree Fock avec contrainte 3315B 3355A
Keyword (en)
Optical activity Carbon compounds Chiral compound Absolute configuration Theoretical study Optical rotation Restricted Hartree Fock theory
Keyword (es)
Compuesto quiral Configuración absoluta Teoría Hartree Fock restringida
Classification
Pascal
001 Exact sciences and technology / 001B Physics / 001B30 Atomic and molecular physics / 001B30C Molecular properties and interactions with photons / 001B30C15 Properties of molecules and molecular ions / 001B30C15B General molecular conformation and symmetry; stereochemistry

Pascal
001 Exact sciences and technology / 001B Physics / 001B30 Atomic and molecular physics / 001B30C Molecular properties and interactions with photons / 001B30C55 Optical activity and dichroism; magnetooptical and electrooptical spectra / 001B30C55A Optical activity, optical rotation; circular dichroism

Discipline
Atomic and molecular physics
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
16736731

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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