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2.. _models-intro:
3
4************
5Introduction
6************
7
8This software provides form factors for various particle shapes and computes
9resolution, polydispersity and angular dispersion. After giving a mathematical
10definition of each model, we show the list of parameters available to the user.
11Validation plots for each model are also presented.
12
13To easily compare to the scattering intensity measured in experiments, we
14normalize the form factors by the volume of the particle
15
16.. math::
17
18    P(\vec q) = \frac{P_o(\vec q)}{V} = \frac{1}{V} F(\vec q) F^*(\vec q)
19
20with
21
22.. math::
23
24    F(\vec q) = \int\int\int dV\rho(\vec r) e^{-i\vec q \cdot \vec r}
25
26where $P_0(\vec q)$ is the un-normalized form factor, $\rho(\vec r)$ is
27the scattering length density at a given point in space and the integration
28is done over the volume $V$ of the scatterer.
29
30For systems without inter-particle interference, the form factors we provide
31can be related to the scattering intensity by the particle volume fraction
32
33.. math::
34
35    I(\vec q) = \Phi P(\vec q)
36
37Our so-called 1D scattering intensity functions provide $P(Q)$ for the case
38where the scatterer is randomly oriented. In that case, the scattering
39intensity only depends on the length of $Q$ . The intensity measured on
40the plane of the SAS detector will have an azimuthal symmetry around $Q=0$.
41
42Our so-called 2D scattering intensity functions provide $P(Q,\phi)$ for an
43oriented system as a function of a $q$ vector in the plane of the detector.
44We define the angle $\phi$ as the angle between the $q$ vector and the
45horizontal ($x$) axis of the plane of the detector.
46
47For information about polarised and magnetic scattering, see :ref:`magnetism`.
48
49The models are used within the SasView package.  Instructions on how to
50use SasView itself are available separately.
51
52Many of our models use the form factor calculations as implemented in the
53C-library provided by the NIST Center for Neutron Research and thus some
54content and figures in this document are originated from or shared with
55the NIST SANS Igor-based analysis package.
56
57*Document History*
58
59| 2017-05-07 Paul Kienzle
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