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].
 
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===Neutron energy===
Consider first the energies of neutrons used in scattering experiments. A thermal neutron
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Consider first the energies of neutrons used in scattering experiments (recall the neutron mass is 1.67×10<sup>−27</sup> kg). A thermal neutron (~100°C) would have energy of:
, the energy for even a thermal neutron (1.8 Å wavelength) is
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:<math>
 
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\mathrm{KE} = \frac{1}{2} m v^2 = \frac{3}{2} kT = 7 \times 10^{-21} \, \mathrm{J} = 48 \,\mathrm{meV}
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</math>
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The velocity of such neutrons is ~3000 m/s, and the momentum is <math>p=mv=5\times10^{-24} \, \mathrm{kgm/s}</math>. Finally, the deBroglie wavelength would be:
 +
:<math>
 +
\lambda = \frac{h}{p} = 1.3 \, \AA
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</math>
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A cold neutron (~18 K) would have energy of 4×10<sup>−22</sup> J = 2 meV, velocity of ~660 m/s, and wavelength of 6 Å.
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===Potential well===
 
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>

Revision as of 01:57, 6 June 2014

Origin of the scattering lengths

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

Neutron energy

Consider first the energies of neutrons used in scattering experiments (recall the neutron mass is 1.67×10−27 kg). A thermal neutron (~100°C) would have energy of:

The velocity of such neutrons is ~3000 m/s, and the momentum is . Finally, the deBroglie wavelength would be:

A cold neutron (~18 K) would have energy of 4×10−22 J = 2 meV, velocity of ~660 m/s, and wavelength of 6 Å.

Potential well

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