Nuclear Overhauser effect/Advanced: Difference between revisions
Jump to navigation
Jump to search
imported>Sekhar Talluri No edit summary |
imported>Sekhar Talluri No edit summary |
||
Line 3: | Line 3: | ||
The Noe enhancement is quantitatively defined as | The Noe enhancement is quantitatively defined as | ||
: <math> \eta = \frac{S_z - S_{z,equil}}{S_{z,equil}} Eq. 1 </math> | : <math> \eta = \frac{S_z - S_{z,equil}}{S_{z,equil}} \qquad Eq. 1 </math> | ||
For a pair of nonidentical spins I and S, : | For a pair of nonidentical spins I and S, : | ||
: <math> \frac{d<I_z>}{dt} = -\rho_I (<I_z> - <I_{z,equil}>) - \sigma (<S_z> - <S_{z,equil}>) Eq. 2</math> | : <math> \frac{d<I_z>}{dt} = -\rho_I (<I_z> - <I_{z,equil}>) - \sigma (<S_z> - <S_{z,equil}>) \qquad Eq. 2</math> | ||
: <math> \frac{d<S_z>}{dt} = -\rho_S (<S_z> - <S_{z,equil}>) - \sigma (<I_z> - <I_{z,equil}>) Eq. 3 </math> | : <math> \frac{d<S_z>}{dt} = -\rho_S (<S_z> - <S_{z,equil}>) - \sigma (<I_z> - <I_{z,equil}>) \qquad Eq. 3 </math> | ||
: <math> \sigma </math> is called the cross relaxation rate and is responsible for the Nuclear overhauser effect. | : <math> \sigma </math> is called the cross relaxation rate and is responsible for the Nuclear overhauser effect. | ||
: <math> \rho_I = \frac{\gamma_I^2\gamma_S^2\hbar^2}{10 r^6 } ( J(w_I-w_S) + 3J(w_I) + 6 J(w_I + w_S) ) Eq. 4 </math> | : <math> \rho_I = \frac{\gamma_I^2\gamma_S^2\hbar^2}{10 r^6 } ( J(w_I-w_S) + 3J(w_I) + 6 J(w_I + w_S) ) \qquad Eq. 4 </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) )) 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> | ||
: <math> \frac{1}{T_2} = \frac{\gamma^2\gamma_S^2\hbar^2}{20 r^6 } ( 4J(0) + J(w_I - w_S) + 3J(w_I) + 6 J(w_I + w_S) + 6 J(w_S) ) Eq. 6 </math> | : <math> \frac{1}{T_2} = \frac{\gamma^2\gamma_S^2\hbar^2}{20 r^6 } ( 4J(0) + J(w_I - w_S) + 3J(w_I) + 6 J(w_I + w_S) + 6 J(w_S) ) \qquad Eq. 6 </math> | ||
In the steady state <math> \frac{d<S_z>}{dt} = 0 </math>, when the resonance frequency of spin I is irradiated , <I_z> = 0, 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: | ||
: <math> (<S_z> - <S_{z,equil}>)= \frac{\sigma}{\rho_S} (<I_{z,equil}>) (from Eq. 3) </math> | : <math> (<S_z> - <S_{z,equil}>)= \frac{\sigma}{\rho_S} (<I_{z,equil}>) (from Eq. 3) </math> | ||
Therefore, | Therefore, | ||
: <math>\eta = \frac{<S_z> - <S_{z,equil}>}{<S_{z,equil}>} = \frac{\sigma}{\rho_S} \frac{\gamma_I}{\gamma_S} Eq. 7 </math> | : <math>\eta = \frac{<S_z> - <S_{z,equil}>}{<S_{z,equil}>} = \frac{\sigma}{\rho_S} \frac{\gamma_I}{\gamma_S} \qquad Eq. 7 </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. | ||
<br/> | <br/> | ||
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 01:59, 12 October 2008
{Def|Nuclear Overhauser effect}
The Noe enhancement is quantitatively defined as
For a pair of nonidentical spins I and S, :
- 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:
Therefore,
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.