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2D NMR: Overview of Homonuclear Correlation Techniques01:16

2D NMR: Overview of Homonuclear Correlation Techniques

Homonuclear correlation spectroscopy (COSY) is a powerful technique used in Nuclear Magnetic Resonance (NMR) spectroscopy to study the correlations between nuclei of the same type within a molecule. It provides information about scalar couplings between adjacent nuclei, which helps determine connectivity and structural information. There are several COSY variants, each with its unique strengths and experimental parameters.
COSY90 is the standard two-dimensional (2D) COSY experiment that...
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2D NMR: Homonuclear Correlation Spectroscopy (COSY)

Homonuclear correlation spectroscopy, or COSY, is a 2-dimensional NMR technique that provides information about coupled protons. Typically, the geminal and vicinal coupling are observed. For example, consider the COSY spectrum of ethyl acetate, where its 1D proton NMR spectrum is plotted along the vertical and horizontal axes with their corresponding chemical shift scale. Three spots on the diagonal corresponding to the three peaks in the 1D proton spectrum are called diagonal peaks. The COSY...
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Hydrogen Bonds Control the World!
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A hydrogen bond is formed when a weakly positive hydrogen atom already bonded to one electronegative atom (for example, the oxygen in the water molecule) is attracted to another electronegative atom from another polar molecule, such as water (H2O), hydrogen fluoride (HF), or ammonia (NH3). The huge electronegativity difference between the H atom (2.1) and the atom to which it is bonded (4.0 for an F atom, 3.5 for an O atom, or 3.0 for an N atom), combined with the very small size of an H atom...
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The molecular orbital theory describes the distribution of electrons in molecules in a manner similar to the distribution of electrons in atomic orbitals. The region of space in which a valence electron in a molecule is likely to be found is called a molecular orbital. Mathematically, the linear combination of atomic orbitals (LCAO) generates molecular orbitals. Combinations of in-phase atomic orbital wave functions result in regions with a high probability of electron density, while...

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Evaluating the COSMO-RS method for modeling hydrogen bonding in solution.

Sofja Tshepelevitsh1, Merit Oss, Astrid Pung

  • 1Institute of Chemistry, University of Tartu, Ravila 14a, 50411 Tartu, Estonia.

Chemphyschem : a European Journal of Chemical Physics and Physical Chemistry
|May 1, 2013
PubMed
Summary
This summary is machine-generated.

The Conductor-like Screening Model for Realistic Solvation (COSMO-RS) accurately predicts hydrogen bond formation for neutral molecules but struggles with anion interactions in solution. This study validates its performance across various solvent systems.

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Area of Science:

  • Computational chemistry
  • Physical chemistry
  • Solution chemistry

Background:

  • Hydrogen bonding (HB) is crucial in chemical and biological systems.
  • Accurate modeling of HB in solution is essential for predicting molecular interactions.
  • The Conductor-like Screening Model for Realistic Solvation (COSMO-RS) is a computational method for solvation studies.

Purpose of the Study:

  • To evaluate the accuracy of the COSMO-RS method in modeling hydrogen bond formation in various solution environments.
  • To compare COSMO-RS predictions with experimental data for different types of hydrogen bonding interactions.
  • To assess the performance of COSMO-RS in mixed solvent systems, a novel aspect of this research.

Main Methods:

  • Utilized the Conductor-like Screening Model for Realistic Solvation (COSMO-RS) computational method.
  • Employed both the supermolecule (SM) and contact probability (CP) approaches for HB analysis.
  • Compared calculated equilibrium constants, Gibbs' free energies, and enthalpies with literature experimental data.

Main Results:

  • COSMO-RS demonstrated good to very good correlation with experimental data for HB formation between neutral species.
  • Quantitative predictions were enabled for complexes involving neutral molecules.
  • Correlations were poor for systems where an anion acted as the hydrogen bond acceptor, with failures in qualitative predictions.

Conclusions:

  • COSMO-RS is a reliable tool for quantitatively predicting hydrogen bond formation involving neutral molecules in solution.
  • The method's accuracy is significantly limited when modeling hydrogen bonds with anions as acceptors.
  • Further development of computational methods is needed to accurately describe anion-involved hydrogen bonding interactions in solution.