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magic spinning

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Phil's note dated 3.31.08, apparently in his folder related to Levitt's NMR book. It places two spins in a rotating cylinder, writes their separation vector, and tries two arguments. Method 1, averaging cos² of the angle to B0, fails to give the hoped result. Method 2 averages the vector itself to the cylinder axis, so the (3cos²θ-1) dipole-dipole term vanishes at the magic angle, removing line broadening.

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Magic Angle Spinning PhL 3.31.08 Consider two arbitrarily located spins in our cylinder which is rotating with axis at the magic angle. But make the cylinder axis be and so B0 is then pointing off axis by the magic angle. Imagine two spins in our rotating sample located arbitrarily in the sample. We can express the position of each spin in cylindrical coordinates as follows: r1 = z1 + 1C1 ' + 1S1' r2 = z2 + 2C2 ' + 2S2' where due to our spin we have ' = Ct + St = -St + Ct Therefore, the vector e which connects the two spins is given by: e ~ r1- r2 = (z1-z2) + (1C1 2C2) ' + ( 1S1 2S2) ' = (z1-z2) + (1C1 2C2) (Ct + St) + ( 1S1 2S2) (-St + Ct) I think we have that e2 = (z1-z2)2 + [ 12 + 22 - 2 12 cos(1 - 2) ] Now let's put Bo in the x-z plane arbitrarily so we have B0 = B0 (sinm + cosm )/ Method #1 (no good) What is the angle between this B field and our e direction? cos = e (sinm + cosm ) / |e| Then, |e| cos = (z1-z2) cosm + {(1C1 2C2) Ct ( 1S1 2S2) St } sinm |e|2cos2 = (z1-z2)2 cos2 m + "the rest" If we time average, the cross term cosm sinm will average to zero, and the cross term of the second term will also average to zero, but there is a piece which does average away this, so we get |e|2<cos2> = (z1-z2)2 cos2 m + (1/2)[ 12 + 22 - 2 12 cos(1 - 2) ] sin2 m Now I am lost. I was hoping to find that <cos2> = cos2 m, but this does not seem possible. Method #2 (gives the desired result) If we do a time average, we get < Ct> = < St> = 0 so our result is <e> ~ (z1-z2) So the average value of the e-vector (for an arbitrary pair of spins) is strictly along the axis of the cylinder. For d-d coupling we know that H'(t) ~ (1/2)(3 cos2(t) - 1) We now have to make a tricky argument: if the angle (t) of our dipole pair axis against the B0 field direction varies rapidly relative to the d-d relaxation time frame, then we can replace (t) by <>. We are not averaging the secular Hamiltonian, we are averaging the parameter that goes into it, as was done in the case of libration. Assuming this is justified, we get H'(t)MAS ~ (1/2)(3 cos2<> - 1) If we set the cylinder at magic relative to B, then we have H'(t)MAS ~ 0 for any pair of spins which have a dipole-dipole coupling. Comment: To the extent that this coupling causes line broadening due to dipole-dipole relaxation [ the main source of relaxation in spin-1/2 systems says Malcolm] doing this spinning action removes this relaxation mechanism from the effective Hamiltonian, so the line broadening goes away and you can see fine peaks again!