Nuclear Overhauser effect/Advanced: Difference between revisions
imported>Sekhar Talluri No edit summary |
imported>Sekhar Talluri No edit summary |
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: <math> \sigma = \frac{\gamma_I^2\gamma_S^2\hbar^2}{10 r^6 } ( -J(w_I-w_S) + 6 J(w_I + w_S) )) \qquad Eq. 5 </math> | : <math> \sigma = \frac{\gamma_I^2\gamma_S^2\hbar^2}{10 r^6 } ( -J(w_I-w_S) + 6 J(w_I + w_S) )) \qquad Eq. 5 </math> | ||
In the steady state <math> \frac{d<S_z>}{dt} = 0 </math>, when the resonance frequency of spin I is irradiated , <math> <I_z> = 0</math>, therefore: | In the steady state <math> \frac{d<S_z>}{dt} = 0 </math>, when the resonance frequency of spin I is irradiated , <math> <I_z> = 0</math>, therefore: | ||
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Assuming that the expectation values of magnetization are proportional to the magnetogyric ratios: | Assuming that the expectation values of magnetization are proportional to the magnetogyric ratios: | ||
: <math>\eta = \frac{<S_z> - <S_{z,equil}>}{<S_{z,equil}>} = \frac{\sigma}{\rho_S} \frac{\gamma_I}{\gamma_S} \qquad Eq. | : <math>\eta = \frac{<S_z> - <S_{z,equil}>}{<S_{z,equil}>} = \frac{\sigma}{\rho_S} \frac{\gamma_I}{\gamma_S} \qquad Eq. 6 </math> | ||
This indicates that considerable enhancement in the intensity of the S signal can be obtained by irradiation at the frequency of the I spin, provided that <math> \frac{\gamma_I}{\gamma_S} > 1 </math>, because <math> \frac{\sigma}{\rho_S} \rightarrow 1/2 </math> when <math> w\tau_c << 1 </math>. | This indicates that considerable enhancement in the intensity of the S signal can be obtained by irradiation at the frequency of the I spin, provided that <math> \frac{\gamma_I}{\gamma_S} > 1 </math>, because <math> \frac{\sigma}{\rho_S} \rightarrow 1/2 </math> when <math> w\tau_c << 1 </math>. | ||
However, when <math> w\tau_c >> 1 </math>, <math> \frac{\sigma}{\rho_S} \rightarrow -1 </math> and negative Noe enhancements are obtained. | However, when <math> w\tau_c >> 1 </math>, <math> \frac{\sigma}{\rho_S} \rightarrow -1 </math> and negative Noe enhancements are obtained. | ||
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The sign of <math> \eta </math> changes from positive to negative when <math> w\tau_c </math> is close to one and under such conditions the Noe effect may not be observable. This happens for rigid molecules with relative molecular mass about 500 at room temperature e.g. many hexapeptides. | The sign of <math> \eta </math> changes from positive to negative when <math> w\tau_c </math> is close to one and under such conditions the Noe effect may not be observable. This happens for rigid molecules with relative molecular mass about 500 at room temperature e.g. many hexapeptides. |
Revision as of 02:14, 12 October 2008
Nuclear Overhauser effect: Noe(Definition) : Change in intensity of a signal when irradiation is carried out at the resonance frequency of a spatially proximal nucleus.
The following discussion is relevant for studies in solution/liquid where the molecules are undergoing rapid isotropic rotational motion.
The Noe enhancement is quantitatively defined as
For a pair of nonidentical spins I and S with dipolar interactions, the time dependence of the the expectation values of the magnetization is:
- is called the cross relaxation rate and is responsible for the Nuclear overhauser effect.
In the steady state , when the resonance frequency of spin I is irradiated , , therefore:
Assuming that the expectation values of magnetization are proportional to the magnetogyric ratios:
This indicates that considerable enhancement in the intensity of the S signal can be obtained by irradiation at the frequency of the I spin, provided that , because when .
However, when , and negative Noe enhancements are obtained.
The sign of changes from positive to negative when is close to one and under such conditions the Noe effect may not be observable. This happens for rigid molecules with relative molecular mass about 500 at room temperature e.g. many hexapeptides.