Difference between revisions of "Talk:Neutron scattering lengths"
KevinYager (talk | contribs) (→Origin of the scattering lengths) |
KevinYager (talk | contribs) (→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>. | + | 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>: |
+ | :<math>\begin{alignat}{2} | ||
+ | \psi_{s,\mathrm{out}} (r=R) & = \psi_{s,\mathrm{in}} (r=R) \\ | ||
+ | \frac{\mathrm{d}}{\mathrm{d}r} \psi_{s,\mathrm{out}} (r=R) & = \frac{\mathrm{d}}{\mathrm{d}r} \psi_{s,\mathrm{in}} (r=R) | ||
+ | \end{alignat} | ||
+ | </math> | ||
+ | Note that the mass of a neutron is ~10<sup>−27</sup> kg | ||
+ | |||
+ | 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