Difference between revisions of "Talk:Neutron scattering lengths"

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(Origin of the scattering lengths)
(Origin of the scattering lengths)
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==Origin of the scattering lengths==
 
==Origin of the scattering lengths==
 
The following description is adapted from [http://www.ncnr.nist.gov/programs/sans/pdf/polymer_tut.pdf Boualem Hammouda's (NCNR) SANS tutorial].
 
The following description is adapted from [http://www.ncnr.nist.gov/programs/sans/pdf/polymer_tut.pdf Boualem Hammouda's (NCNR) SANS tutorial].
 +
 +
Consider first the energies of neutrons used in scattering experiments. A thermal neutron
 +
, the energy for even a thermal neutron (1.8 Å wavelength) is
  
 
Consider a neutron of energy <math>E_i</math> interacting with a nucleus, which exhibits an attractive square well of depth <math>-V_0</math> and width <math>2R</math>; where <math>V_0 \gg E_i</math>. The [http://en.wikipedia.org/wiki/Schr%C3%B6dinger_equation Schrödinger equation] is:
 
Consider a neutron of energy <math>E_i</math> interacting with a nucleus, which exhibits an attractive square well of depth <math>-V_0</math> and width <math>2R</math>; where <math>V_0 \gg E_i</math>. The [http://en.wikipedia.org/wiki/Schr%C3%B6dinger_equation Schrödinger equation] is:
 
:<math>
 
:<math>
\left[ - \frac{h^2}{8 \pi^2 m}\nabla^2  + V(r) \right] \psi = E \psi
+
\left[ - \frac{h^2}{8 \pi^2 m}\nabla^2  + V(r) \right] \psi(r) = E \psi(r)
 
</math>
 
</math>
  
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\psi_{s,\mathrm{in}} = A \frac{\sin(qr)}{qr}
 
\psi_{s,\mathrm{in}} = A \frac{\sin(qr)}{qr}
 
</math>
 
</math>
where <math>q=\sqrt{2m(E_i+V_0} 2 \pi/h</math>.
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where <math>q=\sqrt{2m(E_i+V_0)} 2 \pi/h</math>. The two solutions are subject to a continuity boundary condition at <math>|r|=R</math>:
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:<math>\begin{alignat}{2}
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\psi_{s,\mathrm{out}} (r=R) & = \psi_{s,\mathrm{in}} (r=R) \\
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\frac{\mathrm{d}}{\mathrm{d}r} \psi_{s,\mathrm{out}} (r=R) & = \frac{\mathrm{d}}{\mathrm{d}r}  \psi_{s,\mathrm{in}} (r=R)
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\end{alignat}
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</math>
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Note that the mass of a neutron is ~10<sup>−27</sup> kg
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Note that <math>kR = \sqrt{2 m E_i} R 2\pi/h \ll 1</math> for , and

Revision as of 00:34, 6 June 2014

Origin of the scattering lengths

The following description is adapted from Boualem Hammouda's (NCNR) SANS tutorial.

Consider first the energies of neutrons used in scattering experiments. A thermal neutron , the energy for even a thermal neutron (1.8 Å wavelength) is

Consider a neutron of energy interacting with a nucleus, which exhibits an attractive square well of depth and width ; where . The Schrödinger equation is:

Outside of the square-well (), , and so the equation is solved as simply:

where . Inside the square-well (), the potential is , and the solution becomes:

where . The two solutions are subject to a continuity boundary condition at :

Note that the mass of a neutron is ~10−27 kg

Note that for , and