An excerpt from
New Scientist:
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These bonds govern the way the molecules fold up, like DNA's double helix. They also change their bulk properties: without H bonding, it would take less energy to separate water molecules from each other so water would boil at a lower temperature. But an exact definition has proved elusive. Scientists argue about exactly which atoms must be involved for an interaction to be classified as an H bond, as well as the bond's spectroscopic signatures and the forces that hold it together.
A previous definition, from the 1997 version of the International Union of Pure and Applied Chemistry (IUPAC)'s Gold Book, lists nitrogen, oxygen or fluorine - some of the most electronegative atoms in the periodic table - as most likely to tug on hydrogen's electron cloud and lead to an H bond. Recent experiments have found this definition wanting. It's now clear that a hydrogen bonded to a carbon, which is slightly more electronegative than hydrogen, but much less than nitrogen, oxygen or fluorine, can still form an H bond in some circumstances.
So, under the new definition, the brainchild of an IUPAC committee, an atom bonded to hydrogen need only be more electronegative than the hydrogen itself to be a candidate for an H bond. Spectroscopic observations, or even computer simulations, could then show that the particular interaction meets the criteria to be an H bond, such as having the characteristic bond length, angle or energy density (Pure and Applied Chemistry,
DOI: 10.1351/pac-rec-10-01-02).
The new definition could improve computer models used to predict molecular structure, says Steven Scheiner of Utah State University in Logan who co-led the IUPAC group. Current versions don't allow for the possibility of hydrogen bonds forming between a hydrogen atom covalently bonded to a carbon and sitting near an oxygen, even though it is now clear this is possible.
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