This file is indexed.

/usr/lib/python3/dist-packages/periodictable/cromermann.py is in python3-periodictable 1.5.0-3.

This file is owned by root:root, with mode 0o644.

The actual contents of the file can be viewed below.

  1
  2
  3
  4
  5
  6
  7
  8
  9
 10
 11
 12
 13
 14
 15
 16
 17
 18
 19
 20
 21
 22
 23
 24
 25
 26
 27
 28
 29
 30
 31
 32
 33
 34
 35
 36
 37
 38
 39
 40
 41
 42
 43
 44
 45
 46
 47
 48
 49
 50
 51
 52
 53
 54
 55
 56
 57
 58
 59
 60
 61
 62
 63
 64
 65
 66
 67
 68
 69
 70
 71
 72
 73
 74
 75
 76
 77
 78
 79
 80
 81
 82
 83
 84
 85
 86
 87
 88
 89
 90
 91
 92
 93
 94
 95
 96
 97
 98
 99
100
101
102
103
104
105
106
107
108
109
110
111
112
113
114
115
116
117
118
119
120
121
122
123
124
125
126
127
128
129
130
131
132
133
134
135
136
137
138
139
140
141
142
143
144
145
146
147
148
149
150
151
152
153
154
155
156
157
158
159
160
161
162
163
164
165
166
167
168
169
170
171
172
173
174
175
176
177
178
179
180
181
182
183
184
185
186
187
188
189
190
191
192
193
194
195
196
197
198
199
200
201
202
203
204
##############################################################################
# Copyright (c) 2009 Trustees of the Columbia University
# in the City of New York.  All rights reserved.
#
# DANSE Diffraction group, Simon J. L. Billinge
#
# File coded by:    Pavol Juhas
#
# Redistribution and use in source and binary forms, with or without
# modification, are permitted provided that the following conditions
# are met:
#
#  * Redistributions of source code must retain the above copyright
#    notice, this list of conditions and the following disclaimer.
#
#  * Redistributions in binary form must reproduce the above copyright
#    notice, this list of conditions and the following disclaimer in the
#    documentation and/or other materials provided with the distribution.
#
#  * Neither the name of Columbia University nor the names of its
#    contributors may be used to endorse or promote products derived from
#    this software without specific prior written permission.
#
# THIS SOFTWARE IS PROVIDED BY THE COPYRIGHT HOLDERS AND CONTRIBUTORS
# "AS IS" AND ANY EXPRESS OR IMPLIED WARRANTIES, INCLUDING, BUT NOT
# LIMITED TO, THE IMPLIED WARRANTIES OF MERCHANTABILITY AND FITNESS FOR
# A PARTICULAR PURPOSE ARE DISCLAIMED.  IN NO EVENT SHALL THE COPYRIGHT
# OWNER OR CONTRIBUTORS BE LIABLE FOR ANY DIRECT, INDIRECT, INCIDENTAL,
# SPECIAL, EXEMPLARY, OR CONSEQUENTIAL DAMAGES (INCLUDING, BUT NOT LIMITED
# TO, PROCUREMENT OF SUBSTITUTE GOODS OR SERVICES; LOSS OF USE, DATA, OR
# PROFITS; OR BUSINESS INTERRUPTION) HOWEVER CAUSED AND ON ANY THEORY OF
# LIABILITY, WHETHER IN CONTRACT, STRICT LIABILITY, OR TORT (INCLUDING
# NEGLIGENCE OR OTHERWISE) ARISING IN ANY WAY OUT OF THE USE OF THIS
# SOFTWARE, EVEN IF ADVISED OF THE POSSIBILITY OF SUCH DAMAGE.
##############################################################################


"""
Cromer-Mann formula for calculating x-ray scattering factors.
"""

# module version
__id__ = "$Id: cromermann.py 1051 2010-01-30 01:01:43Z juhas $"

import os
import logging
import numpy
from periodictable import core


def getCMformula(symbol):
    """
    Obtain Cromer-Mann formula and coefficients for a specified element.

    *symbol* : string
        symbol of an element

    Return instance of CromerMannFormula.
    """
    if not _cmformulas:
        _update_cmformulas()
    return _cmformulas[symbol]


def fxrayatq(symbol, Q, charge=None):
    """
    Return x-ray scattering factors of an element at a given Q.

    *symbol* : string
         symbol of an element or ion, e.g., "Ca", "Ca2+"
    *Q* : float or [float] | |1/Ang|
         Q value
    *charge* : int
         ion charge, overrides any valence suffixes such as "-", "+", "3+".

    Return float or numpy array.
    """
    stol = numpy.array(Q) / (4 * numpy.pi)
    rv = fxrayatstol(symbol, stol, charge)
    return rv


def fxrayatstol(symbol, stol, charge=None):
    """
    Calculate x-ray scattering factors at specified sin(theta)/lambda

    *symbol* : string
        symbol of an element or ion, e.g., "Ca", "Ca2+"
    *stol* : float or [float] | |1/Ang|
        sin(theta)/lambda
    *charge* : int
        ion charge, overrides any valence suffixes such as "-", "+", "3+".

    Return float or numpy.array.
    """
    # resolve lookup symbol smbl, by default symbol
    smbl = symbol
    # build standard element or ion symbol
    if charge is not None:
        smbl = symbol.rstrip('012345678+-')
        if charge:
            smbl += ("%+i" % charge)[::-1]
    # convert Na+ or Cl- to Na1+, Cl1-
    elif symbol[-1:] in '+-' and not symbol[-2:-1].isdigit():
        smbl = (symbol[:-1] + "1" + symbol[-1:])
    # smbl is resolved here
    cmf = getCMformula(smbl)
    rv = cmf.atstol(stol)
    return rv


class CromerMannFormula(object):
    """
    Cromer-Mann formula for x-ray scattering factors.
    Coefficient storage and evaluation.

    Class data:

    *stollimit* : float | |1/Ang|
        maximum sin(theta)/lambda for which the formula works

    Attributes:

    *symbol* : string
        symbol of an element
    *a* : [float]
        a-coefficients
    *b* : [float]
        b-coefficients
    *c* : float
        c-coefficient
    """

    # obtained from tables/f0_WaasKirf.dat and the associated reference
    # D. Waasmaier, A. Kirfel, Acta Cryst. (1995). A51, 416-413
    # http://dx.doi.org/10.1107/S0108767394013292
    stollimit = 6

    def __init__(self, symbol, a, b, c):
        """
        Create a new instance of CromerMannFormula for specified element.

        No return value
        """
        self.symbol = symbol
        self.a = numpy.asarray(a, dtype=float)
        self.b = numpy.asarray(b, dtype=float)
        self.c = float(c)
        return


    def atstol(self, stol):
        """
        Calculate x-ray scattering factors at specified sin(theta)/lambda

        *stol* : float or [float] | |1/Ang|
            sin(theta)/lambda

        Return float or numpy.array.
        """
        stolflat = numpy.array(stol).flatten()
        n = len(stolflat)
        stol2row = numpy.reshape(stolflat ** 2, (1, n))
        bcol = self.b.reshape((len(self.a), 1))
        bstol2 = numpy.dot(bcol, stol2row)
        adiag = numpy.diag(self.a)
        rvrows = numpy.dot(adiag, numpy.exp(-bstol2))
        rvflat = rvrows.sum(axis=0) + self.c
        rvflat[stolflat > self.stollimit] = numpy.nan
        # when stol is scalar, addition of zero converts the rv array to float
        rv = rvflat.reshape(numpy.shape(stol)) + 0.0
        return rv

# class CromerMannFormula


def _update_cmformulas():
    """
    Update the static dictionary of CromerMannFormula instances.
    """
    data_path = core.get_data_path('xsf')
    filename = os.path.join(data_path, 'f0_WaasKirf.dat')
    fp = open(filename)
    lineiter = iter(fp)
    for line in lineiter:
        w = line.split()
        if w[0] == "#S":
            smbl = w[2]
            continue
        if w[0] == "#L":
            assert smbl is not None
            line1 = next(lineiter)
            w1 = line1.split()
            assert len(w1) == 11
            a = list(map(float, w1[0:5]))
            b = list(map(float, w1[6:11]))
            c = float(w1[5])
            cmf = CromerMannFormula(smbl, a, b, c)
            _cmformulas[cmf.symbol] = cmf
            smbl = None
    return
_cmformulas = {}

# End of file