In chemistry, NMR line broadening techniques (or NMR line broadening experiments) can be used to determine the rate constant and the Gibbs free energy of exchange reactions of two different chemical compounds. If the two species are in equilibrium and exchange to each other, peaks of both species get broadened in the spectrum. This observation of broadened peaks can be used to obtain kinetic and thermodynamic information of the exchange reaction.
Determining bond rotational energies A basic NMR line broadening experiment is to determine the rotational energy barrier of a certain chemical bond. If the bond rotates slowly enough compared to the NMR time scale (e.g., amide bond), two different species can be detected by the NMR spectrometer. Considering that the time scale of NMR spectroscopy is about a few seconds, this technique can be used to examine the kinetics and/or thermodynamics of chemical exchange reactions on the order of seconds. In general, the energy barrier to rotate a bond is low enough at room temperature, which means that the rotation is fast, making the two different species indistinguishable. At low temperatures, however, it is harder for a bond to overcome the energy barrier to rotate, resulting in two separate peaks in the spectrum. With these principles, NMR spectra of a molecule with a high rotational barrier should be obtained at several different temperatures (i.e., variable temperature NMR) to distinguish two different peaks at low temperature in slow exchange and to find the temperature at which the two peaks merge.
Especially at the coalescence temperature ( T c {\displaystyle T_{c}} ), where the two peaks coalesce, the rate constant of rotation at T c {\displaystyle T_{c}} and the energy barrier of the rotation can be easily calculated. As increasing the temperature, the exchange reaction get faster, and at a certain temperature, which is T c {\displaystyle T_{c}} , the appearance of the peaks changes from two separate peaks in slow exchange to a single peak in fast exchange. The rate constant k {\displaystyle k} at T c {\displaystyle T_{c}} can be calculated with the following equation: k = π ∣ ν A − ν B ∣ 2 {\textstyle \ k={\frac {\pi \mid \nu _{A}-\nu _{B}\mid }{\sqrt {2}}}} ,where ν A {\displaystyle \nu _{A}} and ν B {\displaystyle \nu _{B}} are the chemical shift of each species at lower temperatures where they are in slow exchange. By using the Eyring equation, the Gibbs free energy of rotation, Δ G ‡ {\displaystyle \Delta G^{\ddagger }} , can be determined: k = k B T h e − Δ G ‡ R T {\displaystyle k={\frac {k_{\text{B}}T}{h}}\mathrm {e} ^{-{\frac {\Delta G^{\ddagger }}{RT}}}} (Eyring equation) Δ G ‡ = R T c ln k B T c 2 π h ∣ ν A − ν B ∣ {\displaystyle \Delta G^{\ddagger }=RT_{c}\ln {\frac {k_{\text{B}}T_{c}{\sqrt {2}}}{\pi h\mid \nu _{A}-\nu _{B}\mid }}} where R {\displaystyle R} is gas constant, k B {\displaystyle k_{\text{B}}} is the Boltzmann constant, and h {\displaystyle h} is the Planck constant.
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