source: sasmodels/sasmodels/models/hardsphere.py @ 3bcd03d

core_shell_microgelscostrafo411magnetic_modelrelease_v0.94release_v0.95ticket-1257-vesicle-productticket_1156ticket_1265_superballticket_822_more_unit_tests
Last change on this file since 3bcd03d was 3bcd03d, checked in by krzywon, 8 years ago

Revert hardsphere model and changed Product model to accept radius_effective instead of effect_radius

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[301e096]1# Note: model title and parameter table are inserted automatically
[529b8b4]2r"""Calculate the interparticle structure factor for monodisperse
3spherical particles interacting through hard sphere (excluded volume)
4interactions.
[d529d93]5May be a reasonable approximation for other shapes of particles that
6freely rotate, and for moderately polydisperse systems. Though strictly
7the maths needs to be modified (no \Beta(Q) correction yet in sasview).
[301e096]8
[3bcd03d]9radius_effective is the effective hard sphere radius.
[d529d93]10volfraction is the volume fraction occupied by the spheres.
11
12In sasview the effective radius may be calculated from the parameters
13used in the form factor $P(q)$ that this $S(q)$ is combined with.
14
15For numerical stability the computation uses a Taylor series expansion
16at very small $qR$, there may be a very minor glitch at the transition point
17in some circumstances.
18
19The S(Q) uses the Percus-Yevick closure where the interparticle
[529b8b4]20potential is
[301e096]21
[eb69cce]22.. math::
[529b8b4]23
24    U(r) = \begin{cases}
25    \infty & r < 2R \\
26    0 & r \geq 2R
27    \end{cases}
[301e096]28
[eb69cce]29where $r$ is the distance from the center of the sphere of a radius $R$.
[301e096]30
31For a 2D plot, the wave transfer is defined as
32
33.. math::
34
[529b8b4]35    q = \sqrt{q_x^2 + q_y^2}
[301e096]36
37
[eb69cce]38References
39----------
[301e096]40
41J K Percus, J Yevick, *J. Phys. Rev.*, 110, (1958) 1
42"""
43
[3c56da87]44from numpy import inf
[301e096]45
[034e19a]46name = "hardsphere"
47title = "Hard sphere structure factor, with Percus-Yevick closure"
[301e096]48description = """\
[3e428ec]49    [Hard sphere structure factor, with Percus-Yevick closure]
[301e096]50        Interparticle S(Q) for random, non-interacting spheres.
[3e428ec]51    May be a reasonable approximation for other shapes of
52    particles that freely rotate, and for moderately polydisperse
53        systems. Though strictly the maths needs to be modified -
54    which sasview does not do yet.
[3bcd03d]55    radius_effective is the hard sphere radius
[3e428ec]56    volfraction is the volume fraction occupied by the spheres.
[301e096]57"""
[a5d0d00]58category = "structure-factor"
[8e45182]59structure_factor = True
[301e096]60
[3e428ec]61#             ["name", "units", default, [lower, upper], "type","description"],
[3bcd03d]62parameters = [["radius_effective", "Ang", 50.0, [0, inf], "volume",
[3e428ec]63               "effective radius of hard sphere"],
64              ["volfraction", "", 0.2, [0, 0.74], "",
65               "volume fraction of hard spheres"],
66             ]
[301e096]67
68# No volume normalization despite having a volume parameter
69# This should perhaps be volume normalized?
70form_volume = """
71    return 1.0;
72    """
73
74Iq = """
[f0fb9fe]75      double D,A,B,G,X,X2,X4,S,C,FF,HARDSPH;
76
[3bcd03d]77      if(fabs(radius_effective) < 1.E-12) {
[f0fb9fe]78               HARDSPH=1.0;
79               return(HARDSPH);
80      }
[97e6d3c]81      // removing use of pow(xxx,2) and rearranging the calcs of A, B & G cut ~40% off execution time ( 0.5 to 0.3 msec)
82      X = 1.0/( 1.0 -volfraction);
83      D= X*X;
84      A= (1.+2.*volfraction)*D;
85      A *=A;
[3bcd03d]86      X=fabs(q*radius_effective*2.0);
[f0fb9fe]87
88      if(X < 5.E-06) {
89                 HARDSPH=1./A;
90                 return(HARDSPH);
91      }
[97e6d3c]92      X2 =X*X;
93      B = (1.0 +0.5*volfraction)*D;
94      B *= B;
95      B *= -6.*volfraction;
[f0fb9fe]96      G=0.5*volfraction*A;
97
98      if(X < 0.2) {
[97e6d3c]99      // RKH Feb 2016, use Taylor series expansion for small X, IT IS VERY PICKY ABOUT THE X CUT OFF VALUE, ought to be lower in double.
100      // else no obvious way to rearrange the equations to avoid needing a very high number of significant figures.
[f0fb9fe]101      // Series expansion found using Mathematica software. Numerical test in .xls showed terms to X^2 are sufficient
[97e6d3c]102      // for 5 or 6 significant figures, but I put the X^4 one in anyway
103            //FF = 8*A +6*B + 4*G - (0.8*A +2.0*B/3.0 +0.5*G)*X2 +(A/35. +B/40. +G/50.)*X4;
104            // refactoring the polynomial makes it very slightly faster (0.5 not 0.6 msec)
105            //FF = 8*A +6*B + 4*G + ( -0.8*A -2.0*B/3.0 -0.5*G +(A/35. +B/40. +G/50.)*X2)*X2;
106
107            FF = 8.0*A +6.0*B + 4.0*G + ( -0.8*A -B/1.5 -0.5*G +(A/35. +0.0125*B +0.02*G)*X2)*X2;
108
[f0fb9fe]109            // combining the terms makes things worse at smallest Q in single precision
110            //FF = (8-0.8*X2)*A +(3.0-X2/3.)*2*B + (4+0.5*X2)*G +(A/35. +B/40. +G/50.)*X4;
111            // note that G = -volfraction*A/2, combining this makes no further difference at smallest Q
[97e6d3c]112            //FF = (8 +2.*volfraction + ( volfraction/4. -0.8 +(volfraction/100. -1./35.)*X2 )*X2 )*A  + (3.0 -X2/3. +X4/40.)*2.*B;
[f0fb9fe]113            HARDSPH= 1./(1. + volfraction*FF );
114            return(HARDSPH);
115      }
[97e6d3c]116      X4=X2*X2;
[f0fb9fe]117      SINCOS(X,S,C);
118
[97e6d3c]119// RKH Feb 2016, use version FISH code as is better than original sasview one at small Q in single precision, and more than twice as fast in double.
120      //FF=A*(S-X*C)/X + B*(2.*X*S -(X2-2.)*C -2.)/X2 + G*( (4.*X2*X -24.*X)*S -(X4 -12.*X2 +24.)*C +24. )/X4;
121      // refactoring the polynomial here & above makes it slightly faster
122
123      FF=  (( G*( (4.*X2 -24.)*X*S -(X4 -12.*X2 +24.)*C +24. )/X2 + B*(2.*X*S -(X2-2.)*C -2.) )/X + A*(S-X*C))/X ;
[f0fb9fe]124      HARDSPH= 1./(1. + 24.*volfraction*FF/X2 );
125
[97e6d3c]126      // changing /X and /X2 to *MX1 and *MX2, no significantg difference?
127      //MX=1.0/X;
128      //MX2=MX*MX;
129      //FF=  (( G*( (4.*X2 -24.)*X*S -(X4 -12.*X2 +24.)*C +24. )*MX2 + B*(2.*X*S -(X2-2.)*C -2.) )*MX + A*(S-X*C)) ;
130      //HARDSPH= 1./(1. + 24.*volfraction*FF*MX2*MX );
131
132// grouping the terms, was about same as sasmodels for single precision issues
[f0fb9fe]133//     FF=A*(S/X-C) + B*(2.*S/X - C +2.0*(C-1.0)/X2) + G*( (4./X -24./X3)*S -(1.0 -12./X2 +24./X4)*C +24./X4 );
134//     HARDSPH= 1./(1. + 24.*volfraction*FF/X2 );
135// remove 1/X2 from final line, take more powers of X inside the brackets, stil bad
136//      FF=A*(S/X3-C/X2) + B*(2.*S/X3 - C/X2 +2.0*(C-1.0)/X4) + G*( (4./X -24./X3)*S -(1.0 -12./X2 +24./X4)*C +24./X4 )/X2;
137//      HARDSPH= 1./(1. + 24.*volfraction*FF );
138      return(HARDSPH);
[301e096]139   """
140
141Iqxy = """
142    // never called since no orientation or magnetic parameters.
[529b8b4]143    return Iq(sqrt(qx*qx+qy*qy), IQ_PARAMETERS);
[301e096]144    """
145
146# ER defaults to 0.0
147# VR defaults to 1.0
148
[3bcd03d]149demo = dict(radius_effective=200, volfraction=0.2, radius_effective_pd=0.1, radius_effective_pd_n=40)
[301e096]150oldname = 'HardsphereStructure'
[3bcd03d]151oldpars = dict(radius_effective="effect_radius",radius_effective_pd="effect_radius_pd",radius_effective_pd_n="effect_radius_pd_n")
[093f754]152# Q=0.001 is in the Taylor series, low Q part, so add Q=0.1, assuming double precision sasview is correct
[7f47777]153tests = [
[3bcd03d]154        [ {'scale': 1.0, 'background' : 0.0, 'radius_effective' : 50.0, 'volfraction' : 0.2,
155           'radius_effective_pd' : 0}, [0.001,0.1], [0.209128,0.930587]]
[7f47777]156        ]
[d529d93]157# ADDED by: RKH  ON: 16Mar2016  using equations from FISH as better than orig sasview, see notes above. Added Taylor expansions at small Q,
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