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Neutron Scattering

Neutron Scattering - JuSER - Forschungszentrum Jülich

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k[Ä-1 ]z 0.695<br />

E<br />

meV<br />

,,[Ä] 9.0451 VE meV (3 .11)<br />

E[meV ~t<br />

81.8/2[Ä]<br />

To give an exaniple, neutrons of wavelength a,<br />

= 2.4 A have an energy of 14 .2 meV with a<br />

magnitude ofthe neutron wave vector ofk = 2.6 A_ 1 .<br />

To obtain solutions of the wave equation (3 .9) in matter, we reformulate the differential<br />

equation by explicitly separating the interaction terni :<br />

(A+k<br />

2m V . IP = : x<br />

2<br />

(3 .12)<br />

Here k denotes the wave vector for propagation in empty space . The advantage of this<br />

formulation is that the solution of the left hand side are already known. They are the plane<br />

waves in empty space . Equation (3 .12) is a linear partial differential equation, i . e. the<br />

superposition principle holds : the general solution can be obtained as a linear combination of<br />

a complete set of solution functions . The coefficients in the series are determined by the<br />

boundary conditions . To solve (3 .12) one can apply a method developed for inhomogeneous<br />

linear differential equations . For the moment, we assume that the right hand side is fixed<br />

(given as x) . We deine a "Greensfunetion" by:<br />

(A+k''~(r,r')=8(r-r')<br />

(3 .13)<br />

We can easily verify that a solution of (3 .l3) is given by :<br />

G( :,<br />

e iklr-r'I<br />

z^') = (3 .14)<br />

4mlr- r'I<br />

3-6

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