hollow_rectangular_prism_thin_walls¶
Hollow rectangular parallelepiped with thin walls.
Parameter |
Description |
Units |
Default value |
---|---|---|---|
scale |
Scale factor or Volume fraction |
None |
1 |
background |
Source background |
cm-1 |
0.001 |
sld |
Parallelepiped scattering length density |
10-6Å-2 |
6.3 |
sld_solvent |
Solvent scattering length density |
10-6Å-2 |
1 |
length_a |
Shorter side of the parallelepiped |
Å |
35 |
b2a_ratio |
Ratio sides b/a |
Å |
1 |
c2a_ratio |
Ratio sides c/a |
Å |
1 |
The returned value is scaled to units of cm-1 sr-1, absolute scale.
Definition This model provides the form factor, \(P(q)\), for a hollow rectangular prism with infinitely thin walls. It computes only the 1D scattering, not the 2D. The 1D scattering intensity for this model is calculated according to the equations given by Nayuk and Huber[1].
Assuming a hollow parallelepiped with infinitely thin walls, edge lengths \(A \le B \le C\) and presenting an orientation with respect to the scattering vector given by \(\theta\) and \(\phi\), where \(\theta\) is the angle between the \(z\) axis and the longest axis of the parallelepiped \(C\), and \(\phi\) is the angle between the scattering vector (lying in the \(xy\) plane) and the \(y\) axis, the form factor is given by
where
and
The 1D scattering intensity is then calculated as
where \(V\) is the surface area of the rectangular prism, \(\rho_\text{p}\) is the scattering length density of the parallelepiped, \(\rho_\text{solvent}\) is the scattering length density of the solvent, and (if the data are in absolute units) scale is related to the total surface area.
The 2D scattering intensity is not computed by this model.
Validation
Validation of the code was conducted by qualitatively comparing the output of the 1D model to the curves shown in (Nayuk, 2012[1]).
Source
hollow_rectangular_prism_thin_walls.py
\(\ \star\ \) hollow_rectangular_prism_thin_walls.c
\(\ \star\ \) gauss76.c
References
See also Onsager [2].
Authorship and Verification
Author: Miguel Gonzales Date: February 26, 2016
Last Modified by: Paul Kienzle Date: October 15, 2016
Last Reviewed by: Paul Butler Date: September 07, 2018