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Pulsed-field gradient nuclear magnetic resonance as a tool for ...

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318<br />

PRICE<br />

probability of a spin starting from r 0 and moving<br />

to r in time is given by Žrecall Eq. 24. 1<br />

Ž . Ž . <br />

r P r ,r , . 73<br />

0 0 1<br />

The NMR signal is proportional to the vector<br />

sum of the transverse components of the magnetization,<br />

and so the signal from one spin is given<br />

by<br />

Ž . Ž . igŽr 1r 0. <br />

r P r ,r , e . 74<br />

0 0 1<br />

But in NMR, the signal results from the ensemble<br />

of spins, and thus we must integrate over all<br />

possible starting and finishing positions, and finally<br />

we arrive at our result Ž 55, 56.<br />

EŽ g,. HH Ž r . PŽ r ,r ,.<br />

0 0 1<br />

igŽr e 1r0. dr dr . 75 0 1<br />

Thus, the total signal is a superposition of signals<br />

Ž transverse magnetizations . , in which each ph<strong>as</strong>e<br />

term is weighted by the probability <strong>for</strong> a spin to<br />

begin at r 0 and move to r1 during .<br />

As an example, let us rederive Eq. 51 using<br />

the SGP approximation Ži.e., Eq. 75 . . From Eq.<br />

75 and 27 ,<br />

we have<br />

1 2<br />

Žr 1r 0.<br />

4 D<br />

HH 0 32<br />

EŽ g,. Ž r .<br />

e<br />

Ž 4D.<br />

igŽr 1r 0. <br />

e dr dr . 76<br />

1 0<br />

In the present c<strong>as</strong>e, we set g g Ž z we will drop<br />

the subscript z, however . , and R r1r 0.Us-<br />

ing spherical polar coordinates Ži.e.,<br />

R is the<br />

radius and and are the polar and azimuthal<br />

angles, respectively . , we note that dR <br />

R2 sin dR d d; also, since is the angle between<br />

R and g we have<br />

1 2 2 R 4 D 2<br />

32<br />

H H<br />

EŽ g,. <br />

Ž 4D.<br />

0<br />

d<br />

0<br />

e R<br />

igR cos H e sin d dR<br />

0<br />

77 As there is no dependence, it can be integrated<br />

out<br />

2 2 R 4 D 2<br />

e R<br />

32<br />

H<br />

Ž 4D.<br />

0<br />

igR cos H e sin d dR<br />

0<br />

78 then, by noting that d cos sin d, we get<br />

2 2<br />

1<br />

R 4 D 2 igR<br />

32H<br />

H<br />

Ž . 0 1<br />

4D<br />

e R e d dR.<br />

<br />

79<br />

The integral over is then per<strong>for</strong>med and evalu-<br />

<br />

ated using Eq. 11 , resulting in<br />

4 <br />

2 R 4 D Ž .<br />

32<br />

H<br />

g Ž 4D.<br />

0<br />

Re sin gR dR<br />

<br />

80<br />

We note from a table of standard integrals e.g.,<br />

Ž 53. Eq. 3.952 1. that<br />

2 2 a 2 2<br />

p x Ž . a 4p<br />

xe sin ax dx e . 81 4p<br />

'<br />

H 3<br />

0<br />

Ž . 12<br />

In our c<strong>as</strong>e, x R, p 4D , and a g,<br />

and thus we obtain the final result<br />

Ž . Ž 2 2 2 . <br />

E g, exp g D . 82<br />

This is the same <strong>as</strong> Eq. 51 ,<br />

but in the limit of<br />

0; thus the 3 term which accounts <strong>for</strong> the<br />

finite width of the <strong>gradient</strong> pulse is absent. When<br />

we consider restricted diffusion, the evaluation of<br />

Eq. 75 proceeds in exactly the same manner,<br />

except that we must substitute the relevant Ž r . 0<br />

and PŽ r , r , t . 0 1 . However, <strong>as</strong> the confining geometry<br />

becomes more complicated, so does the<br />

mathematical complexity.<br />

The Analogy between PFG Me<strong>as</strong>urements and Scattering.<br />

Returning back to the derivation of the<br />

SGP approximation, and in particular, Eq. 72 ,<br />

because we are using a constant Žcommonly<br />

termed ‘‘linear’’ . <strong>gradient</strong>, what is important is<br />

not the actual starting and finishing positions of<br />

the spin but the net displacement between the<br />

two points in the direction of the <strong>gradient</strong>. As<br />

be<strong>for</strong>e, we can write R r1r0 and, analogously<br />

to Eq. 73 ,<br />

the probability that a particle<br />

that starts at r 0 displacing a distance R during <br />

is given by Žrecall Eq. 24. Ž . Ž . <br />

r P r ,r R, . 83<br />

0 0 0

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