/usr/lib/python3/dist-packages/periodictable/nsf.py is in python3-periodictable 1.5.0-3.
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# This program is public domain
# Author: Paul Kienzle
r"""
Neutron scattering factors for the elements and isotopes.
For details of neutron scattering factor values, see :class:`Neutron`.
The property is set to *None* if there is no neutron scattering information
for the element. Individual isotopes may have their own scattering
information.
Example
=======
Print a table of coherent scattering length densities for isotopes
of a particular element:
.. doctest::
>>> import periodictable
>>> for iso in periodictable.Ni:
... if iso.neutron.has_sld():
... print("%s %7.4f"%(iso,iso.neutron.sld()[0]))
58-Ni 13.1526
60-Ni 2.5575
61-Ni 6.9417
62-Ni -7.9464
64-Ni -0.3379
Details
=======
There are a number of functions available in periodictable.nsf
:func:`neutron_energy`
Return neutron energy given wavelength.
:func:`neutron_wavelength`
Return wavelength given neutron energy.
:func:`neutron_wavelength_from_velocity`
Return wavelength given neutron velocity.
:func:`neutron_scattering`
Computes scattering length density, cross sections and
penetration depth for a compound.
:func:`neutron_sld`
Computes scattering length density for a compound.
:func:`neutron_composite_sld`
Returns a scattering length density for a compound whose composition
is variable.
:func:`energy_dependent_table`
Lists isotopes with energy dependence.
:func:`sld_table`
Lists scattering length densitys for all elements in natural abundance.
:func:`absorption_comparison_table`
Compares the imaginary bound coherent scattering length to the
absorption cross section.
:func:`coherent_comparison_table`
Compares the bound coherent scattering length to the
coherent scattering cross section.
:func:`total_comparison_table`
Compares the total scattering cross section to the sum of the
coherent and incoherent scattering cross sections.
For private tables use :func:`init` to set the data.
The neutron scattering information table is reproduced from the Atomic
Institute for Austrian Universities\ [#Rauch2003]_ (retrieve March 2008):
http://www.ati.ac.at/~neutropt/scattering/table.html
The above site has references to the published values for every entry in
the table. We have included these in the documentation directory
associated with the periodictable package.
.. Note:
Enteries in the table have been measured independently, so the values
measured for the scattering length of an element or isotope may be
inconsistent with the values measured for the corresponding cross section.
.. [#Rauch2003] Rauch, H. and Waschkowski, W. (2003)
Neutron Scattering Lengths in ILL
Neutron Data Booklet (second edition), A.-J. Dianoux, G. Lander, Eds.
Old City Publishing, Philidelphia, PA. pp 1.1-1 to 1.1-17.
.. [#Rauch2000] Rauch, H. and Waschkowski, W. (2000)
Neutron scattering lengths. Schopper, H. (ed.).
SpringerMaterials - The Landolt-Börnstein Database (http://www.springermaterials.com).
doi: 10.1007/10499706_6
.. [#Koester1991] Koester, L., Rauch, H., Seymann. E. (1991)
Atomic Data Nuclear Data Tables 49, 65
.. [#Lynn1990] Lynn, J.E. and Seeger, P.A. (1990)
Resonance effects in neutron scattering lengths of rare-earth nuclides.
Atomic Data and Nuclear Data Tables 44, 191-207.
.. [#Sears1999] Sears, V. F. (1999)
4.4.4 Scattering lengths for neutrons.
In Wilson & Prince eds. Intl. Tables for Crystallography C
Kluwer Academic Publishers. pp 383.
.. [#Sears1992] Sears, V.F. (1992)
Neutron scattering lengths and cross sections.
Neutron News 3, No. 3, 26-37.
.. [#May1982] May, R.P., Ibel, K. and Haas, J. (1982)
The forward scattering of cold neutrons by mixtures of light and heavy water.
J. Appl. Cryst. 15, 15-19.
.. [#Smith2006] Smith, G.S. and Majkrzak, C.M. (2006)
2.9 Neutron reflectometry.
In E. Prince ed. Intl. Tables for Crystallography C
Wiley InterScience. pp 126-146.
doi: 10.1107/97809553602060000584
.. [#Glinka2011] Glinka, C.J. (2011)
Incoherent Neutron Scattering from Multi-element Materials.
J. Appl. Cryst. 44, 618-624.
doi: 10.1107/S0021889811008223
"""
from __future__ import print_function
import numpy
from numpy import sqrt, pi, asarray, inf
from .core import Element, Isotope, default_table
from .constants import (avogadro_number, plancks_constant, electron_volt,
neutron_mass, atomic_mass_constant)
from .util import require_keywords
__all__ = ['init', 'Neutron',
'neutron_energy', 'neutron_wavelength',
'neutron_wavelength_from_velocity',
'neutron_scattering', 'neutron_sld', 'neutron_composite_sld',
'sld_plot',
'absorption_comparison_table', 'coherent_comparison_table',
'incoherent_comparison_table', 'total_comparison_table',
'energy_dependent_table', 'sld_table',
'neutron_sld_from_atoms',
#'scattering_potential',
]
ABSORPTION_WAVELENGTH = 1.798
# Velocity (m/s) <=> wavelength (A)
# lambda = h / p = h (eV) (J/eV) / ( m_n (kg) v (m/s) ) (10^10 A/m)
#
# Since plancks constant is in eV
# lambda = (1e10 * h*electron_volt/(neutron_mass/N_A)) / velocity
# Energy (eV) <=> wavelength (A)
# h^2/(2 m_n kg lambda A) (10^20 A/m) (1000 meV/eV) / (electron_volt J/eV)
# Since plancks constant is in eV
# (h J)^2/electron_volt = ((h eV)(electron_volt J/eV))^2/electron_volt
# = (h eV)^2 * electron_volt
ENERGY_FACTOR = (plancks_constant**2*electron_volt
/ (2 * neutron_mass * atomic_mass_constant)) * 1e23
VELOCITY_FACTOR = (plancks_constant*electron_volt
/ (neutron_mass * atomic_mass_constant)) * 1e10
def neutron_wavelength(energy):
r"""
Convert neutron energy to wavelength.
:Parameters:
*energy* : float or vector | meV
:Returns:
*wavelength* : float or vector | |Ang|
Energy is converted to wavelength using
.. math::
E = 1/2 m_n v^2 = h^2 / (2 m_n \lambda^2)
\Rightarrow \lambda = \sqrt{h^2 / (2 m_n E)}
where
$h$ = planck's constant in |Js|
$m_n$ = neutron mass in kg
"""
return sqrt(ENERGY_FACTOR / asarray(energy))
def neutron_wavelength_from_velocity(velocity):
r"""
Convert neutron velocity to wavelength.
:Parameters:
*velocity* : float or vector | m/s
:Returns:
*wavelength* : float or vector | |Ang|
Velocity is converted to wavelength using
.. math::
\lambda = h/p = h/(m_n v)
where
$h$ = planck's constant in |Js|
$m_n$ = neutron mass in kg
"""
return VELOCITY_FACTOR / velocity
def neutron_energy(wavelength):
r"""
Convert neutron wavelength to energy.
:Parameters:
*wavelength* : float or vector | |Ang|
:Returns:
*energy* : float or vector | meV
Wavelength is converted to energy using
.. math::
E = 1/2 m_n v^2 = h^2 / (2 m_n \lambda^2)
where:
$h$ = planck's constant in |Js|
$m_n$ = neutron mass in kg
"""
return ENERGY_FACTOR / asarray(wavelength)**2
def _CHECK_scattering_potential(sld):
r"""
Convert neutron scattering length density to energy potential.
:Parameters:
*sld* : float or vector | |1e-6/Ang^2|
Scattering length density.
:Returns:
*energy* : float or vector | $10^{-6}$ eV
Scattering potential.
Computes:[#Smith2006]_
.. math::
V = 2 \pi \hbar^2 N_b / m_n
where:
$\hbar = h / (2 \pi)$
$h$ = planck's constant in |Js|
$N_b = \sum{ n_i b_i } / V$
$m_n$ = neutron mass in kg
"""
return (ENERGY_FACTOR/pi) * asarray(sld)
class Neutron(object):
r"""
Neutron scattering factors are attached to each element in the periodic
table for which values are available. If no information is available,
then the neutron field of the element will be *None*. Even when neutron
information is available, it may not be complete, so individual fields
may be *None*.
The following fields are defined:
* b_c (fm)
Bounds coherent scattering length.
* total (barn)
Total scattering cross section $\sigma_s$. This does not include the
absorption cross section. To compute the total collision cross
section use $\sigma_t = \sigma_s + \sigma_a$
* absorption (barn)
Absorption cross section $\sigma_a$ at 1.798 |Ang|. Scale to your beam
by dividing by periodictable.nsf.ABSORPTION_WAVELENGTH and multiplying
by your wavelength.
Additional fields not used for calculation include:
* b_c_i (fm)
Imaginary bound coherent scattering length. This is
related to absorption cross section by $\sigma_a = 4 \pi b_i/k$ where
$k = 2 \pi/\lambda$ and an additional factor of 1000 for converting
between |Ang|\ |cdot|\ fm and barns. b_c_i is not available
for all isotopes for which absorption cross sections have been measured.
* bp, bm (fm)
Spin-dependent scattering for I+1/2 and I-1/2 (not always available).
Incoherent scattering arises from the spin-dependent scattering b+
and b-. The Neutron Data Booklet\ [#Rauch2003]_ gives formulas for
calculating coherent and incoherent scattering from b+ and b- alone.
* bp_i, bm_i (fm)
Imaginary portion of bp and bm.
* is_energy_dependent (boolean)
Do not use this data if scattering is energy dependent.
* coherent (barn)
Coherent scattering cross section. This is tabulated but not used.
In theory coherent scattering is related to bound coherent scattering
by $\sigma_s = 4 \pi b_c^2/100$. In practice, these values are
different, with the following table showing the largest relative
difference:
======== ======== ======== ======== ========
Sc 3% Ti 4% V 34% Mn 1% Cd 4%
Te 4% Xe 9% Sm 100% Eu 46% Gd 61%
Tb 1% Ho 11% W 4% Au 7% Hg 2%
======== ======== ======== ======== ========
* incoherent (barn)
Incoherent scattering cross section $\sigma_i$. This is tabulated but
not used. Instead, the incoherent cross section is computed from the
total cross section minus the coherent cross section even for single
atoms so that results from compounds are consistent with results from
single atoms.
For elements, the scattering cross-sections are based on the natural
abundance of the individual isotopes. Individual isotopes may have
the following additional fields
* abundance (%)
Isotope abundance used to compute the properties of the element in
natural abundance.
* nuclear_spin (string)
Spin on the nucleus: '0', '1/2', '3/2', etc.
Each field ``T`` above has a corresponding ``T_units`` attribute with
the name of the units. For scattering calculations, the scattering
length density is the value of interest. This is computed from the
*number_density* of the individual elements, as derived from the element
density and atomic mass.
.. Note:: 1 barn = 100 |fm^2|
"""
b_c = None
b_c_i = None
b_c_units = "fm"
bp = None
bp_i = None
bp_units = "fm"
bm = None
bm_i = None
bm_units = "fm"
coherent = None
coherent_units = "barn"
incoherent = None
incoherent_units = "barn"
total = None
total_units = "barn"
absorption = None
absorption_units = "barn"
abundance = 0.
abundance_units = "%"
is_energy_dependent = False
def __init__(self):
self._number_density = None
def __str__(self):
return ("b_c=%.3g coh=%.3g inc=%.3g abs=%.3g"
% (self.b_c, self.coherent, self.incoherent, self.absorption))
def has_sld(self):
"""Returns *True* if sld is defined for this element/isotope."""
return None not in [self.b_c, self._number_density]
@require_keywords
def sld(self, wavelength=ABSORPTION_WAVELENGTH):
"""
Returns scattering length density for the element at natural
abundance and density.
:Parameters:
*wavelength* : float | |Ang|
:Returns:
*sld* : (float, float, float) | |1e-6/Ang^2|
(*real*, -*imaginary*, *incoherent*) scattering length density.
.. Note:
Values may not be correct when the element or isotope has
*is_energy_dependent=True*
See :func:`neutron_scattering` for details.
"""
# Compute number and absorption density assuming isotope has
# same structure as the bulk element
if not self.has_sld():
return None, None, None
b_c = self.b_c
sigma_s = self.total
sigma_a = self.absorption/ABSORPTION_WAVELENGTH*wavelength
number_density = self._number_density*1e-24
# PAK 2017-04-21: compute incoherent cross section from total cross section
sigma_c = 4*pi/100 * b_c**2
sigma_i = max(sigma_s - sigma_c, 0.)
# Compute SLD
sld_re = number_density * b_c * 10
sld_im = number_density * sigma_a / (2 * wavelength) * 0.01
sld_inc = number_density * sqrt(sigma_i / (4*pi/100)) * 10
return sld_re, sld_im, sld_inc
@require_keywords
def scattering(self, wavelength=ABSORPTION_WAVELENGTH):
r"""
Returns neutron scattering information for the element at natural
abundance and density.
:Parameters:
*wavelength* : float | |Ang|
:Returns:
*sld* : (float, float, float) | |1e-6/Ang^2|
(*real*, -*imaginary*, *incoherent*) scattering length density
*xs* : (float, float, float) | |1/cm|
(*coherent*, *absorption*, *incoherent*) cross sections.
*penetration* : float | cm
1/e penetration length.
.. Note:
Values may not be correct when the element or isotope has
*is_energy_dependent=True*
See :func:`neutron_scattering` for details.
"""
# Compute number and absorption density assuming isotope has
# same structure as the bulk element
if not self.has_sld():
return None, None, None
b_c = self.b_c
sigma_s = self.total
sigma_a = self.absorption*wavelength/ABSORPTION_WAVELENGTH
number_density = self._number_density*1e-24
# PAK 2017-04-21: compute incoherent cross section from total cross section
sigma_c = 4*pi/100 * b_c**2
sigma_i = max(sigma_s - sigma_c, 0.)
# Compute SLD
sld_re = number_density * b_c * 10
sld_im = number_density * sigma_a / (2 * wavelength) * 0.01
sld_inc = number_density * sqrt(sigma_i / (4*pi/100)) * 10
# Compute scattering cross section per unit volume
total_xs = number_density * sigma_s
coh_xs = number_density * sigma_c
abs_xs = number_density * sigma_a
inc_xs = number_density * sigma_i
# Compute 1/e length
penetration = 1/(abs_xs + total_xs)
return (sld_re, sld_im, sld_inc), (coh_xs, abs_xs, inc_xs), penetration
def init(table, reload=False):
"""
Loads the Rauch table from the neutron data book.
"""
if 'neutron' in table.properties and not reload:
return
table.properties.append('neutron')
assert ('density' in table.properties and 'mass' in table.properties), \
"Neutron table requires mass and density properties"
# Defaults for missing neutron information
missing = Neutron()
Isotope.neutron = missing
Element.neutron = missing
for line in nsftable.split('\n'):
columns = line.split(',')
nsf = Neutron()
p = columns[1]
spin = columns[2]
nsf.b_c, nsf.bp, nsf.bm = [fix_number(a) for a in columns[3:6]]
nsf.is_energy_dependent = (columns[6] == 'E')
nsf.coherent, nsf.incoherent, nsf.total, nsf.absorption \
= [fix_number(a) for a in columns[7:]]
parts = columns[0].split('-')
Z = int(parts[0])
symbol = parts[1]
isotope_number = int(parts[2]) if len(parts) == 3 else 0
# Fetch element from the table and check that the symbol matches
element = table[Z]
assert element.symbol == symbol, \
"Symbol %s does not match %s" % (symbol, element.symbol)
# Plug the default number density for the element into the nsf so
# it can calculate sld.
nsf._number_density = element.number_density
# For new elements, clear out 'neutron' attribute for isotopes
# This protects against isotope using the element data when
# they don't have any specific neutron data.
#if isotope_number == 0 or not hasattr(element,'neutron'):
# for iso in element: iso.neutron = None
if isotope_number == 0:
# Bulk values using laboratory abundances of isotopes
element.neutron = nsf
else:
# Values for the individual isotope
isotope = element.add_isotope(isotope_number)
isotope.neutron = nsf
isotope.nuclear_spin = spin
# p column contains either abundance(uncertainty) or "half-life Y"
isotope.neutron.abundance = fix_number(p) if ' ' not in p else 0
# If the element is not yet initialized, copy info into the atom.
# This serves to set the element info for elements with only
# one isotope.
if element.neutron is missing:
element.neutron = nsf
for line in nsftableI.split('\n'):
columns = line.split(',')
# Fetch the nsf record
parts = columns[0].split('-')
Z = int(parts[0])
symbol = parts[1]
isotope_number = int(parts[2]) if len(parts) == 3 else 0
element = table[Z]
if isotope_number == 0:
nsf = element.neutron
else:
nsf = element[isotope_number].neutron
# Read imaginary values
nsf.b_c_i, nsf.bp_i, nsf.bm_i = [fix_number(a) for a in columns[1:]]
# Xe total cross section is missing from the table
# put it in even though it has not been independently measured
if table.Xe.neutron.total is None:
table.Xe.neutron.total = table.Xe.neutron.coherent + table.Xe.neutron.incoherent
# Note: docs and function prototype are reproduced in __init__
@require_keywords
def neutron_scattering(compound, density=None,
wavelength=ABSORPTION_WAVELENGTH, energy=None,
natural_density=None):
r"""
Computes neutron scattering cross sections for molecules.
:Parameters:
*compound* : Formula initializer
Chemical formula
*density* : float | |g/cm^3|
Mass density
*natural_density* : float | |g/cm^3|
Mass density of formula with naturally occuring abundances
*wavelength* 1.798 : float | |Ang|
Neutron wavelength.
*energy* : float | meV
Neutron energy. If energy is specified then wavelength is ignored.
:Returns:
*sld* : (float, float, float) | |1e-6/Ang^2|
(*real*, -*imaginary*, *incoherent*) scattering length density.
*xs* : (float, float, float) | |1/cm|
(*coherent*, *absorption*, *incoherent*) cross sections.
*penetration* : float | cm
1/e penetration depth of the beam
:Raises:
*AssertionError* : density is missing.
.. Note:
Values may not correct if any element or isotope has
*is_energy_dependent=True*
The coherent and incoherent cross sections are calculated from the
bound scattering lengths for nuclei. The actual cross sections depend
on the incoming neutron energy and sample temperature, especially for
light elements. For low energy neutrons (cold neutrons), the tabulated
cross sections are generally a lower limit. The measured incoherent
scattering from hydrogen, for example, can be considerably larger
(by more than 20%) than its bound value. For example, the incoherent
scattering cross section of H2O is 5.621/cm as computed from these tables
compared to ~7.0/cm as measured with 5 meV neutrons at 290K. [#May1982]_
The scattering factor tables are not self consistent. The following
functions show discrepencies between the various measurements of the
scattering potential:
:func:`absorption_comparison_table`
:func:`coherent_comparison_table`
:func:`total_comparison_table`
To compute the neutron cross sections we first need to average
quantities for the unit cell of the molecule.
Molar mass *m* (g/mol) is the sum of the masses of each component:
.. math::
m = \sum{n_i m_i}\ {\rm for\ each\ atom}\ i=1,2,\ldots
Cell volume $V$ (|Ang^3|/molecule) is molar mass $m$ over density
$rho$, with a correction based on Avogadro's number $N_A$ (atoms/mol)
and the length conversion $10^8$ |Ang|/cm:
.. math::
V = m/\rho \cdot 1/N_A \cdot (10^8)^3
Number density $N$ is the number of scatterers per unit volume:
.. math::
N = \left.\sum{n_i} \right/ V
Coherent scattering cross section $\sigma_c$ of the molecule is computed
from the average scattering length of its constituent atoms, weighted by
their frequency.
.. math::
b_c = \left.\sum n_i b_c \right/ \sum n_i
This is converted to a scattering cross section and scaled
by 1 barn = 100 |fm^2|:
.. math::
\sigma_c = \left. 4 \pi b_c^2 \right/ 100
Similarly, the absorption cross section $\sigma_a$, the incoherent cross
section $\sigma_i$, and the total cross section $\sigma_s$ can be computed
from the corresponding cross sections of the constituent elements,\ [#Sears1999]_
already expressed in barns:
.. math::
\sigma_a &= \left. \sum n_j \sigma_{aj} \right/ \sum n_j \\
\sigma_i &= \left. \sum n_j \sigma_{ij} \right/ \sum n_j \\
\sigma_s &= \left. \sum n_j \sigma_{sj} \right/ \sum n_j
The neutron cross sections are tabulated at wavelength 1.798 |Ang|.
In the thermal neutron energy range most absorption cross sections
scale linearly with wavelength,\ [#Lynn1990]_ and can be adjusted
with a simple multiplication:
.. math::
\sigma_a = \sigma_a \lambda / \lambda_o = \sigma_a \lambda / 1.798
If *isotope.neutron.is_energy_dependent()* is true for any part of
the material, then this relation may not hold, and the returned values
are only valid for 1.798 |Ang|.
From the scattering cross sections, the scattering length for a material
$b = b' - i b''$ can be computed using the following relations:[#Sears1999]_
.. math::
\sigma_c &= 4 \pi |b_c|^2 \\
\sigma_a &= \left. 4 \pi \left< b'' \right> \right/k \ {\rm for} \ k=2\pi / \lambda \\
\sigma_i &= 4 \pi |b_i|^2 \\
\sigma_s &= 4 \pi \left< |b|^2 \right>
Transforming we get:
.. math::
b'' &= \left. \sigma_a \right/ (2 \lambda) \\
b_i &= \sqrt{ \sigma_i / (4 \pi) }
The incoherent scattering length $b_i$ can be treated primarily
as an absorption length in large scale structure calculations, with the
complex scattering length approximated by $b = b_c - i (b'' + b_i)$.
The scattering potential is often expressed as a scattering length
density (SLD). This is just the number density of the scatterers times
their scattering lengths, with a correction for units.
.. math::
\rho_{\rm re} &= 10 N b_c \\
\rho_{\rm im} &= -N b'' / 100 \\
\rho_{\rm inc} &= 10 N b_i
with the factors of 10 chosen to give SLD in units of $\AA^{-2}$. The
resulting $\rho = \rho_{\rm re} + i \rho_{\rm im}$ can be used in the
scattering equations. Treatment of the incoherent scattering $\rho_{\rm inc}$
will depend on the equation. For example, it can be treated as an absorption
in specular reflectivity calculations since the incoherently scattered neutrons
are removed from the multilayer recurrence calculation.
Similarly, scattering cross section includes number density:
.. math::
\Sigma_{\rm coh} &= N \sigma_c \\
\Sigma_{\rm inc} &= N \sigma_i \\
\Sigma_{\rm abs} &= N \sigma_a \\
\Sigma_{\rm s} &= N \sigma_s
The 1/e penetration depth *t_u* represents the the depth into the sample at
which the unscattered intensity is reduced by a factor of $e$:
.. math::
t_u = \left. 1 \right/ (\Sigma_{\rm s} + \Sigma_{\rm abs})
Note that the calculated penetration depth includes the effects of both
absorption and incoherent scattering (which spreads the beam in the
full $4\pi$ spherical surface, and so it looks like absorption with
respect to the beam), as well as the coherent scattering from the sample.
If you instead want to calculate the effective shielding of the sample,
you should recalculate penetration depth without the coherent scattering.
Transmission rate can be computed from $e^{-d/t_u}$ for penetration i
depth $t_u$ and sample thickness $d$.
In general, the total scattering cross section is not the sum of the
coherent and incoherent cross sections,
$\Sigma_{\rm s} \ne \Sigma_{\rm coh}+\Sigma_{\rm inc}$.\ [#Glinka2011]_
Instead, we compute $\Sigma_{\rm inc} = \Sigma_{\rm s} - \Sigma_{\rm coh}$
in accordance with Sect. 4.4.4 of the Internation Tables for Crystallography
Volume C.
Including unit conversion with $\mu=10^{-6}$ the full scattering equations
are:
.. math::
\rho_{\rm re}\,(\mu/\AA^2) &= (N/\AA^3)
\, (b_c\,{\rm fm})
\, (10^{-5} \AA/{\rm\,fm})
\, (10^6\,\mu) \\
\rho_{\rm im}\,(\mu/\AA^2) &= (N/\AA^3)
\, (\sigma_a\,{\rm barn})
\, (10^{-8}\,\AA^2/{\rm barn}) / (2 \lambda\, \AA)
\, (10^6\,\mu) \\
\rho_{\rm inc}\,(\mu/\AA^2) &= (N/\AA^3)
\, \sqrt{(\sigma_i\, {\rm barn})/(4 \pi)
\, (100\, {\rm fm}^2/{\rm barn})}
\, (10^{-5}\, \AA/{\rm fm})
\, (10^6\, \mu) \\
\Sigma_{\rm coh}\,(1/{\rm cm}) &= (N/\AA^3)
\, (\sigma_c\, {\rm barn})
\, (10^{-8}\, \AA^2/{\rm barn})
\, (10^8\, \AA/{\rm cm}) \\
\Sigma_{\rm inc}\,(1/{\rm cm}) &= (N/\AA^3)
\,(\sigma_i\, {\rm barn})
\, (10^{-8}\, \AA^2/{\rm barn})
\, (10^8\, \AA/{\rm cm}) \\
\Sigma_{\rm abs}\,(1/{\rm cm}) &= (N/\AA^3)
\,(\sigma_a\,{\rm barn})
\, (10^{-8}\, \AA^2/{\rm barn})
\, (10^8\, \AA/{\rm cm}) \\
\Sigma_{\rm s}\,(1/{\rm cm}) &= (N/\AA^3)
\,(\sigma_s\,{\rm barn})
\, (10^{-8}\, \AA^2/{\rm barn})
\, (10^8\, \AA/{\rm cm}) \\
t_u\,({\rm cm}) &= 1/(\Sigma_{\rm s}\, 1/{\rm cm}
\,+\, \Sigma_{\rm abs}\, 1/{\rm cm})
"""
from . import formulas
compound = formulas.formula(compound, density=density,
natural_density=natural_density)
assert compound.density is not None, "scattering calculation needs density"
if energy is not None:
wavelength = neutron_wavelength(energy)
assert wavelength is not None, "scattering calculation needs energy or wavelength"
# Sum over the quantities
molar_mass = num_atoms = 0
sigma_s = sigma_a = b_c = 0
is_energy_dependent = False
for element, quantity in compound.atoms.items():
if not element.neutron.has_sld():
return None, None, None
#print element,quantity,element.neutron.b_c,element.neutron.absorption,element.neutron.total
molar_mass += element.mass*quantity
num_atoms += quantity
sigma_a += quantity * element.neutron.absorption
sigma_s += quantity * element.neutron.total
b_c += quantity * element.neutron.b_c
is_energy_dependent |= element.neutron.is_energy_dependent
# If nothing to sum, return values for a vacuum. This might be because
# the material has no atoms or it might be because the density is zero.
if molar_mass*compound.density == 0:
return (0, 0, 0), (0, 0, 0), inf
# Turn sums into scattering factors
b_c /= num_atoms
sigma_s /= num_atoms
sigma_a *= wavelength/ABSORPTION_WAVELENGTH/num_atoms
# Compute number density
cell_volume = (molar_mass/compound.density)/avogadro_number*1e24 # (10^8 A/cm)^3
number_density = num_atoms / cell_volume
# PAK 2017-04-21: compute incoherent cross section from total cross section
sigma_c = 4*pi/100 * b_c**2 # = 4 pi |b_c/10|^2
sigma_i = max(sigma_s - sigma_c, 0.0)
# Compute SLD
sld_re = number_density * b_c * 10
sld_im = number_density * sigma_a / (2 * wavelength) * 0.01
sld_inc = number_density * sqrt(sigma_i / (4*pi/100)) * 10
# Compute scattering cross section per unit volume
total_xs = number_density * sigma_s
coh_xs = number_density * sigma_c
abs_xs = number_density * sigma_a
inc_xs = number_density * sigma_i
# Compute 1/e length
penetration = 1/(abs_xs + total_xs)
return (sld_re, sld_im, sld_inc), (coh_xs, abs_xs, inc_xs), penetration
def neutron_sld(*args, **kw):
"""
Computes neutron scattering length densities for molecules.
:Parameters:
*compound* : Formula initializer
Chemical formula
*density* : float | |g/cm^3|
Mass density
*natural_density* : float | |g/cm^3|
Mass density of formula with naturally occuring abundances
*wavelength* : float | |Ang|
Neutron wavelength.
*energy* : float | meV
Neutron energy. If energy is specified then wavelength is ignored.
:Returns:
*sld* : (float, float, float) | |1e-6/Ang^2|
(*real*, -*imaginary*, *incoherent*) scattering length density.
:Raises:
*AssertionError* : density is missing.
Returns the scattering length density of the compound.
See :func:`neutron_scattering` for details.
"""
return neutron_scattering(*args, **kw)[0]
def neutron_sld_from_atoms(*args, **kw):
r"""
.. deprecated:: 0.91
:func:`neutron_sld` now accepts dictionaries of \{atom\: count\} directly.
"""
return neutron_scattering(*args, **kw)[0]
def _sum_piece(wavelength, compound):
"""
Helper for neutron_composite_sld which precomputes quantities of interest
for material fragments in a composite formula.
"""
# Sum over the quantities
molar_mass = num_atoms = 0
sigma_a = sigma_s = b_c = 0
is_energy_dependent = False
for element, quantity in compound.atoms.items():
#print element,quantity,element.neutron.b_c,element.neutron.absorption,element.neutron.total
molar_mass += element.mass*quantity
num_atoms += quantity
sigma_a += quantity * element.neutron.absorption
sigma_s += quantity * element.neutron.total
b_c += quantity * element.neutron.b_c
is_energy_dependent |= element.neutron.is_energy_dependent
return num_atoms, molar_mass, b_c, sigma_s, sigma_a
def neutron_composite_sld(materials, wavelength=ABSORPTION_WAVELENGTH):
"""
Create a composite SLD calculator.
:Parameters:
*materials* : [Formula]
List of materials
*wavelength* = 1.798: float OR [float] | |Ang|
Probe wavelength(s).
:Returns:
*calculator* : f(w, density=1) -> (*real*, -*imaginary*, *incoherent*)
The composite calculator takes a vector of weights and returns the
scattering length density of the composite. This is useful for operations
on large molecules, such as calculating a set of contrasts or fitting
a material composition.
Table lookups and partial sums and constants are precomputed so that
the calculation consists of a few simple array operations regardless
of the size of the material fragments.
"""
parts = [_sum_piece(wavelength, m) for m in materials]
V = [numpy.array(v) for v in zip(*parts)]
num_atoms_parts, molar_mass_parts, b_c_parts, sigma_s_parts, sigma_a_parts = V
def _compute(weights, density=1):
# Sum over the quantities
molar_mass = numpy.sum(weights*molar_mass_parts)
num_atoms = numpy.sum(weights*num_atoms_parts)
sigma_a = numpy.sum(weights*sigma_a_parts)
sigma_s = numpy.sum(weights*sigma_s_parts)
b_c = numpy.sum(weights*b_c_parts)
# If nothing to sum, return values for a vacuum. This might be because
# the material has no atoms or it might be because the density is zero.
if molar_mass*density == 0:
return 0, 0, 0
# Turn sums into scattering factors
b_c /= num_atoms
sigma_a *= wavelength/ABSORPTION_WAVELENGTH/num_atoms # at tabulated wavelength
sigma_s /= num_atoms
# Compute number density
cell_volume = (molar_mass/density)/avogadro_number*1e24
number_density = num_atoms / cell_volume
# PAK 2017-04-21: compute incoherent cross section from total cross section
sigma_c = 4*pi/100 * b_c**2
sigma_i = max(sigma_s - sigma_c, 0.0)
# Compute SLD
sld_re = number_density * b_c * 10
sld_im = number_density * sigma_a / (2 * wavelength) * 0.01
sld_inc = number_density * sqrt(sigma_i / (4*pi/100)) * 10
return sld_re, sld_im, sld_inc
return _compute
def sld_plot(table=None):
"""
Plots SLD as a function of element number.
:Parameters:
*table* : PeriodicTable
The default periodictable unless a specific table has been requested.
:Returns: None
"""
from .plot import table_plot
table = default_table(table)
SLDs = dict((el, el.neutron.sld()[0])
for el in table
if el.neutron.has_sld())
SLDs[table.D] = table.D.neutron.sld()[0]
table_plot(SLDs, label='Scattering length density ($10^{-6}$ Nb)',
title='Neutron SLD for elements in natural abundance')
# We are including the complete original table here in case somebody in
# future wants to extract uncertainties or other information.
#
# Z-Symbol-A
# This is the atomic number, the symbol and the isotope.
# If Z-Symbol only, the line represents an element with scattering determined
# by the natural abundance of the isotopes in laboratory samples. If there
# is only one isotope, then there is no corresponding element definition.
# concentration/half-life
# This is the natural abundance of the isotope expressed as a percentage, or
# it is the half-life in years (number Y) or seconds (number S).
# spin I
# For isotopes, the nuclear spin.
# b_c, bp, bm
# Bound coherent scattering length in fm
# b+/b- if present are spin dependent scattering for I+1/2 and I-1/2
# respectively
# c
# 'E' if there is a strong energy dependency.
# '+/-' if separate b+/b- values are available [doesn't seem true -PAK]
# coherent, incoherent, total
# The coherent and incoherent scattering cross-sections in barns.
# absorption
# The thermal absorption cross section in barns at 1.798 Angstroms/25.30 meV.
#
# Numbers in parenthesis represents uncertainty.
# Numbers followed by '*' are estimated.
# Numbers may be given as limit, e.g., <1.0e-6
#
# Formatting corrections by Paul Kienzle
nsftable = """\
0-n-1,618 S,1/2,-37.0(6),0,-37.0(6),,43.01(2),,43.01(2),0
1-H,,,-3.7409(11),,,,1.7568(10),80.26(6),82.02(6),0.3326(7)
1-H-1,99.985,1/2,-3.7423(12),10.817(5),-47.420(14),+/-,1.7583(10),80.27(6),82.03(6),0.3326(7)
1-H-2,0.0149,1,6.674(6),9.53(3),0.975(60),,5.592(7),2.05(3),7.64(3),0.000519(7)
1-H-3,12.26 Y,1/2,4.792(27),4.18(15),6.56(37),,2.89(3),0.14(4),3.03(5),<6.0E-6
2-He,,,3.26(3),,,,1.34(2),0,1.34(2),0.00747(1)
2-He-3,0.013,1/2,5.74(7),4.7(5),8.8(1.4),E,4.42(10),1.6(4),6.0(4),5333.0(7.0)
2-He-4,99.987,0,3.26(3),,,,1.34(2),0,1.34(2),0
3-Li,,,-1.90(3),,,,0.454(10),0.92(3),1.37(3),70.5(3)
3-Li-6,7.5,1,2.0(1),0.67(14),4.67(17),+/-,0.51(5),0.46(5),0.97(7),940.0(4.0)
3-Li-7,92.5,3/2,-2.22(2),-4.15(6),1.00(8),+/-,0.619(11),0.78(3),1.40(3),0.0454(3)
4-Be-9,100,3/2,7.79(1),,,,7.63(2),0.0018(9),7.63(2),0.0076(8)
5-B,,,5.30(4),,,,3.54(5),1.70(12),5.24(11),767.0(8.0)
5-B-10,19.4,3,-0.2(4),-4.2(4),5.2(4),,0.144(6),3.0(4),3.1(4),3835.0(9.0)
5-B-11,80.2,3/2,6.65(4),5.6(3),8.3(3),,5.56(7),0.21(7),5.77(10),0.0055(33)
6-C,,,6.6484(13),,,,5.551(2),0.001(4),5.551(3),0.00350(7)
6-C-12,98.89,0,6.6535(14),,,,5.559(3),0,5.559(3),0.00353(7)
6-C-13,1.11,1/2,6.19(9),5.6(5),6.2(5),+/-,4.81(14),0.034(11),4.84(14),0.00137(4)
7-N,,,9.36(2),,,,11.01(5),0.50(12),11.51(11),1.90(3)
7-N-14,99.635,1,9.37(2),10.7(2),6.2(3),,11.03(5),0.50(12),11.53(11),1.91(3)
7-N-15,0.365,1/2,6.44(3),6.77(10),6.21(10),,5.21(5),0.00005(10),5.21(5),0.000024(8)
8-O,,,5.805(4),,,,4.232(6),0.000(8),4.232(6),0.00019(2)
8-O-16,99.75,0,5.805(5),,,,4.232(6),0,4.232(6),0.00010(2)
8-O-17,0.039,5/2,5.6(5),5.52(20),5.17(20),,4.20(22),0.004(3),4.20(22),0.236(10)
8-O-18,0.208,0,5.84(7),,,,4.29(10),0,4.29(10),0.00016(1)
9-F-19,100,1/2,5.654(12),5.632(10),5.767(10),+/-,4.017(14),0.0008(2),4.018(14),0.0096(5)
10-Ne,,,4.566(6),,,,2.620(7),0.008(9),2.628(6),0.039(4)
10-Ne-20,90.5,0,4.631(6),,,,2.695(7),0,2.695(7),0.036(4)
10-Ne-21,0.27,3/2,6.66(19),,,,5.6(3),0.05(2),5.7(3),0.67(11)
10-Ne-22,9.2,0,3.87(1),,,,1.88(1),0,1.88(1),0.046(6)
11-Na-23,100,3/2,3.63(2),6.42(4),-1.00(6),+/-,1.66(2),1.62(3),3.28(4),0.530(5)
12-Mg,,,5.375(4),,,,3.631(5),0.08(6),3.71(4),0.063(3)
12-Mg-24,78.99,0,5.49(18),,,,4.03(4),0,4.03(4),0.050(5)
12-Mg-25,10,5/2,3.62(14),4.73(30),1.76(20),+/-,1.65(13),0.28(4),1.93(14),0.19(3)
12-Mg-26,11,0,4.89(15),,,,3.00(18),0,3.00(18),0.0382(8)
13-Al-27,100,5/2,3.449(5),3.67(2),3.15(2),,1.495(4),0.0082(6),1.503(4),0.231(3)
14-Si,,,4.15071(22),,,,2.1633(10),0.004(8),2.167(8),0.171(3)
14-Si-28,92.2,0,4.106(6),,,,2.120(6),0,2.120(6),0.177(3)
14-Si-29,4.7,1/2,4.7(1),4.50(15),4.7(4),+/-,2.78(12),0.001(2),2.78(12),0.101(14)
14-Si-30,3.1,0,4.58(8),,,,2.64(9),0,2.64(9),0.107(2)
15-P-31,100,1/2,5.13(1),,,+/-,3.307(13),0.005(10),3.312(16),0.172(6)
16-S,,,2.847(1),,,,1.0186(7),0.007(5),1.026(5),0.53(1)
16-S-32,95,0,2.804(2),,,,0.9880(14),0,0.9880(14),0.54(4)
16-S-33,0.74,3/2,4.74(19),,,+/-,2.8(2),0.3(6),3.1(6),0.54(4)
16-S-34,4.2,0,3.48(3),,,,1.52(3),0,1.52(3),0.227(5)
16-S-36,0.02,0,3.0(1.0)*,,,,1.1(8),0,1.1(8),0.15(3)
17-Cl,,,9.5792(8),,,,11.528(2),5.3(5),16.8(5),33.5(3)
17-Cl-35,75.77,3/2,11.70(9),16.3(2),4.0(3),+/-,17.06(6),4.7(6),21.8(6),44.1(4)
17-Cl-37,24.23,3/2,3.08(6),3.10(7),3.05(7),+/-,1.19(5),0.001(3),1.19(5),0.433(6)
18-Ar,,,1.909(6),,,,0.458(3),0.225(5),0.683(4),0.675(9)
18-Ar-36,0.34,0,24.9(7),,,,77.9(4),0,77.9(4),5.2(5)
18-Ar-38,0.07,0,3.5(3.5),,,,1.5(3.1),0,1.5(3.1),0.8(5)
18-Ar-40,99.59,0,1.7,,,,0.421(3),0,0.421(3),0.660(9)
19-K,,,3.67(2),,,,1.69(2),0.27(11),1.96(11),2.1(1)
19-K-39,93.3,3/2,3.79(2),5.15,1.51,+/-,1.76(2),0.25(11),2.01(11),2.1(1)
19-K-40,0.012,4,3.1(1.0)*,,,,1.1(6),0.5(5)*,1.6(9),35.0(8.0)
19-K-41,6.7,3/2,2.69(8),,,,0.91(5),0.3(6),1.2(6),1.46(3)
20-Ca,,,4.70(2),,,,2.78(2),0.05(3),2.83(2),0.43(2)
20-Ca-40,96.94,0,4.78(5),,,,2.90(2),0,2.90(2),0.41(2)
20-Ca-42,0.64,0,3.36(10),,,,1.42(8),0,1.42(8),0.68(7)
20-Ca-43,0.13,7/2,-1.56(9),,,,0.31(4),0.5(5),0.8(5),6.2(6)
20-Ca-44,2.13,0,1.42(6),,,,0.25(2),0,0.25(2),0.88(5)
20-Ca-46,0.003,0,3.55(21),,,,1.6(2),0,1.6(2),0.74(7)
20-Ca-48,0.18,0,0.39(9),,,,0.019(9),0,0.019(9),1.09(14)
21-Sc-45,100,7/2,12.1(1),6.91(22),18.99(28),+/-,19.0(3),4.5(3),23.5(6),27.5(2)
22-Ti,,,-3.370(13),,,,1.485(2),2.87(3),4.35(3),6.09(13)
22-Ti-46,8,0,4.72(5),,,,3.05(7),0,3.05(7),0.59(18)
22-Ti-47,7.5,5/2,3.53(7),0.46(23),7.64(13),,1.66(11),1.5(2),3.2(2),1.7(2)
22-Ti-48,73.7,0,-5.86(2),,,,4.65(3),0,4.65(3),7.84(25)
22-Ti-49,5.5,7/2,0.98(5),2.6(3),-1.2(4),,0.14(1),3.3(3),3.4(3),2.2(3)
22-Ti-50,5.3,0,5.88(10),,,,4.80(12),0,4.80(12),0.179(3)
23-V,,,-0.443(14),,,,0.01838(12),5.08(6),5.10(6),5.08(4)
23-V-50,0.25,6,7.6(6)*,,,,7.3(1.1),0.5(5)*,7.8(1.0),60.0(40.0)
23-V-51,99.75,7/2,-0.402(2),4.93(25),-7.58(28),+/-,0.0203(2),5.07(6),5.09(6),4.9(1)
24-Cr,,,3.635(7),,,,1.660(6),1.83(2),3.49(2),3.05(6)
24-Cr-50,4.35,0,-4.50(5),,,,2.54(6),0,2.54(6),15.8(2)
24-Cr-52,83.8,0,4.914(15),,,,3.042(12),0,3.042(12),0.76(6)
24-Cr-53,9.59,3/2,-4.20(3),1.16(10),-13.0(2),,2.22(3),5.93(17),8.15(17),18.1(1.5)
24-Cr-54,2.36,0,4.55(10),,,,2.60(11),0,2.60(11),0.36(4)
25-Mn-55,100,5/2,-3.750(18),-4.93(46),-1.46(33),,1.75(2),0.40(2),2.15(3),13.3(2)
26-Fe,,,9.45(2),,,,11.22(5),0.40(11),11.62(10),2.56(3)
26-Fe-54,5.8,0,4.2(1),,,,2.2(1),0,2.2(1),2.25(18)
26-Fe-56,91.7,0,10.1(2),,,,12.42(7),0,12.42(7),2.59(14)
26-Fe-57,2.19,1/2,2.3(1),,,,0.66(6),0.3(3)*,1.0(3),2.48(30)
26-Fe-58,0.28,0,15(7),,,,28.0(26.0),0,28.0(26.0),1.28(5)
27-Co-59,100,7/2,2.49(2),-9.21(10),3.58(10),+/-,0.779(13),4.8(3),5.6(3),37.18(6)
28-Ni,,,10.3(1),,,,13.3(3),5.2(4),18.5(3),4.49(16)
28-Ni-58,67.88,0,14.4(1),,,,26.1(4),0,26.1(4),4.6(3)
28-Ni-60,26.23,0,2.8(1),,,,0.99(7),0,0.99(7),2.9(2)
28-Ni-61,1.19,3/2,7.60(6),,,,7.26(11),1.9(3),9.2(3),2.5(8)
28-Ni-62,3.66,0,-8.7(2),,,,9.5(4),0,9.5(4),14.5(3)
28-Ni-64,1.08,0,-0.37(7),,,,0.017(7),0,0.017(7),1.52(3)
29-Cu,,,7.718(4),,,,7.485(8),0.55(3),8.03(3),3.78(2)
29-Cu-63,69.1,3/2,6.477(13),,,+/-,5.2(2),0.006(1),5.2(2),4.50(2)
29-Cu-65,30.9,3/2,10.204(20),,,+/-,14.1(5),0.40(4),14.5(5),2.17(3)
30-Zn,,,5.680(5),,,,4.054(7),0.077(7),4.131(10),1.11(2)
30-Zn-64,48.9,0,5.23(4),,,,3.42(5),0,3.42(5),0.93(9)
30-Zn-66,27.8,0,5.98(5),,,,4.48(8),0,4.48(8),0.62(6)
30-Zn-67,4.1,5/2,7.58(8),5.8(5),10.1(7),+/-,7.18(15),0.28(3),7.46(15),6.8(8)
30-Zn-68,18.6,0,6.04(3),,,,4.57(5),0,4.57(5),1.1(1)
30-Zn-70,0.62,0,6.9(1.0)*,,,,4.5(1.5),0,4.5(1.5),0.092(5)
31-Ga,,,7.288(2),,,,6.675(4),0.16(3),6.83(3),2.75(3)
31-Ga-69,60,3/2,8.043(16),6.3(2),10.5(4),+/-,7.80(4),0.091(11),7.89(4),2.18(5)
31-Ga-71,40,3/2,6.170(11),5.5(6),7.8(1),+/-,5.15(5),0.084(8),5.23(5),3.61(10)
32-Ge,,,8.185(20),,,,8.42(4),0.18(7),8.60(6),2.20(4)
32-Ge-70,20.7,0,10.0(1),,,,12.6(3),0,12.6(3),3.0(2)
32-Ge-72,27.5,0,8.51(10),,,,9.1(2),0,9.1(2),0.8(2)
32-Ge-73,7.7,9/2,5.02(4),8.1(4),1.2(4),,3.17(5),1.5(3),4.7(3),15.1(4)
32-Ge-74,36.4,0,7.58(10),,,,7.2(2),0,7.2(2),0.4(2)
32-Ge-76,7.7,0,8.2(1.5),,,,8.0(3.0),0,8.0(3.0),0.16(2)
33-As-75,100,3/2,6.58(1),6.04(5),7.47(8),+/-,5.44(2),0.060(10),5.50(2),4.5(1)
34-Se,,,7.970(9),,,,7.98(2),0.32(6),8.30(6),11.7(2)
34-Se-74,0.9,0,0.8(3.0),,,,0.1(6),0,0.1(6),51.8(1.2)
34-Se-76,9,0,12.2(1),,,,18.7(3),0,18.7(3),85.0(7.0)
34-Se-77,7.5,0,8.25(8),,,,8.6(2),0.05(25),8.65(16),42.0(4.0)
34-Se-78,23.5,0,8.24(9),,,,8.5(2),0,8.5(2),0.43(2)
34-Se-80,50,0,7.48(3),,,,7.03(6),0,7.03(6),0.61(5)
34-Se-82,8.84,0,6.34(8),,,,5.05(13),0,5.05(13),0.044(3)
35-Br,,,6.79(2),,,,5.80(3),0.10(9),5.90(9),6.9(2)
35-Br-79,50.49,3/2,6.79(7),,,+/-,5.81(2),0.15(6),5.96(13),11.0(7)
35-Br-81,49.31,3/2,6.78(7),,,+/-,5.79(12),0.05(2),5.84(12),2.7(2)
36-Kr,,,7.81(2),,,,7.67(4),0.01(14),7.68(13),25.0(1.0)
36-Kr-78,0.35,0,,,,,,0,,6.4(9)
36-Kr-80,2.5,0,,,,,,0,,11.8(5)
36-Kr-82,11.6,0,,,,,,0,,29.0(20.0)
36-Kr-83,11.5,9/2,,,,,,,,185.0(30.0)
36-Kr-84,57,0,,,,,,0,6.6,0.113(15)
36-Kr-86,17.3,0,8.07(26),,,,8.2(4),0,8.2(4),0.003(2)
37-Rb,,,7.08(2),,,,6.32(4),0.5(4),6.8(4),0.38(1)
37-Rb-85,72.17,5/2,7.07(10),,,,6.2(2),0.5(5)*,6.7(5),0.48(1)
37-Rb-87,27.83,3/2,7.27(12),,,,6.6(2),0.5(5)*,7.1(5),0.12(3)
38-Sr,,,7.02(2),,,,6.19(4),0.06(11),6.25(10),1.28(6)
38-Sr-84,0.56,0,5.0(2.0),,,,6.0(2.0),0,6.0(2.0),0.87(7)
38-Sr-86,9.9,0,5.68(5),,,,4.04(7),0,4.04(7),1.04(7)
38-Sr-87,7,9/2,7.41(7),,,,6.88(13),0.5(5)*,7.4(5),16.0(3.0)
38-Sr-88,82.6,0,7.16(6),,,,6.42(11),0,6.42(11),0.058(4)
39-Y-89,100,1/2,7.75(2),8.4(2),5.8(5),+/-,7.55(4),0.15(8),7.70(9),1.28(2)
40-Zr,,,7.16(3),,,,6.44(5),0.02(15),6.46(14),0.185(3)
40-Zr-90,51.48,0,6.5(1),,,,5.1(2),0,5.1(2),0.011(59
40-Zr-91,11.23,5/2,8.8(1),7.9(2),10.1(2),+/-,9.5(2),0.15(4),9.7(2),1.17(10)
40-Zr-92,17.11,0,7.5(2),,,,6.9(4),0,6.9(4),0.22(6)
40-Zr-94,17.4,0,8.3(2),,,,8.4(4),0,8.4(4),0.0499(24)
40-Zr-96,2.8,0,5.5(1),,,,3.8(1),0,3.8(1),0.0229(10)
41-Nb-93,100,9/2,7.054(3),7.06(4),7.35(4),+/-,6.253(5),0.0024(3),6.255(5),1.15(6)
42-Mo,,,6.715(20),,,,5.67(3),0.04(5),5.71(4),2.48(4)
42-Mo-92,15.48,0,6.93(8),,,,6.00(14),0,6.00(14),0.019(2)
42-Mo-94,9.1,0,6.82(7),,,,5.81(12),0,5.81(12),0.015(2)
42-Mo-95,15.72,5/2,6.93(7),,,,6.00(10),0.5(5)*,6.5(5),13.1(3)
42-Mo-96,16.53,0,6.22(6),,,,4.83(9),0,4.83(9),0.5(2)
42-Mo-97,9.5,5/2,7.26(8),,,,6.59(15),0.5(5)*,7.1(5),2.5(2)
42-Mo-98,23.78,0,6.60(7),,,,5.44(12),0,5.44(12),0.127(6)
42-Mo-100,9.6,0,6.75(7),,,,5.69(12),0,5.69(12),0.4(2)
43-Tc-99,210000 Y,9/2,6.8(3),,,,5.8(5),0.5(5)*,6.3(7),20.0(1.0)
44-Ru,,,7.02(2),,,,6.21(5),0.4(1),6.6(1),2.56(13)
44-Ru-96,5.8,0,,,,,,0,,0.28(2)
44-Ru-98,1.9,0,,,,,,0,,<8.0
44-Ru-99,12.7,5/2,,,,,,,,6.9(1.0)
44-Ru-100,12.6,0,,,,,,0,,4.8(6)
44-Ru-101,17.07,5/2,,,,,,,,3.3(9)
44-Ru-102,31.61,0,,,,,,0,,1.17(7)
44-Ru-104,18.58,0,,,,,,0,,0.31(2)
45-Rh-103,100,1/2,5.90(4),8.15(6),6.74(6),,4.34(6),0.3(3)*,4.6(3),144.8(7)
46-Pd,,,5.91(6),,,,4.39(9),0.093(9),4.48(9),6.9(4)
46-Pd-102,1,0,7.7(7)*,,,,7.5(1.4),0,7.5(1.4),3.4(3)
46-Pd-104,11,0,7.7(7)*,,,,7.5(1.4),0,7.5(1.4),0.6(3)
46-Pd-105,22.33,5/2,5.5(3),,,+/-,3.8(4),0.8(1.0),4.6(1.1),20.0(3.0)
46-Pd-106,27.33,0,6.4(4),,,,5.1(6),0,5.1(6),0.304(29)
46-Pd-108,26.71,0,4.1(3),,,,2.1(3),0,2.1(3),8.5(5)
46-Pd-110,11.8,0,7.7(7)*,,,,7.5(1.4),0,7.5(1.4),0.226(31)
47-Ag,,,5.922(7),,,,4.407(10),0.58(3),4.99(3),63.3(4)
47-Ag-107,51.8,1/2,7.555(11),8.14(9),5.8(3),+/-,7.17(2),0.13(3),7.30(4),37.6(1.2)
47-Ag-109,48.2,1/2,4.165(11),3.24(8),6.9(2),+/-,2.18(1),0.32(5),2.50(5),91.0(1.0)
48-Cd,,,4.83(5),,,E,3.04(6),3.46(13),6.50(12),2520.0(50.0)
48-Cd-106,1.2,0,5.0(2.0)*,,,,3.1(2.5),0,3.1(2.5),1.0(2.0)
48-Cd-108,0.9,0,5.31(24),,,,3.7(1),0,3.7(1),1.1(3)
48-Cd-110,12.39,0,5.78(8),,,,4.4(1),0,4.4(1),11.0(1.0)
48-Cd-111,12.75,1/2,6.47(8),,,,5.3(2),0.3(3)*,5.6(4),24.0(5.0)
48-Cd-112,24.07,0,6.34(6),,,,5.1(2),0,5.1(2),2.2(5)
48-Cd-113,12.36,1/2,-8.0(1),,,E,12.1(4),0.3(3)*,12.4(5),20600.0(400.0)
48-Cd-114,28.86,0,7.48(5),,,,7.1(2),0,7.1(2),0.34(2)
48-Cd-116,7.58,0,6.26(9),,,,5.0(2),0,5.0(2),0.075(13)
49-In,,,4.065(20),,,,2.08(2),0.54(11),2.62(11),193.8(1.5)
49-In-113,4.28,9/2,5.39(6),,,,3.65(8),0.000037(5),3.65(8),12.0(1.1)
49-In-115,95.72,9/2,4.00(3),2.1(1),6.4(4),,2.02(2),0.55(11),2.57(11),202.0(2.0)
50-Sn,,,6.225(2),,,,4.871(3),0.022(5),4.892(6),0.626(9)
50-Sn-112,1,0,6.0(1.0)*,,,,4.5(1.5),0,4.5(1.5),1.00(11)
50-Sn-114,0.66,0,6.0(3),,,,4.8(5),0,4.8(5),0.114(30)
50-Sn-115,0.35,1/2,6.0(1.0)*,,,,4.5(1.5),0.3(3)*,4.8(1.5),30.0(7.0)
50-Sn-116,14.3,0,6.10(1),,,,4.42(7),0,4.42(7),0.14(3)
50-Sn-117,7.61,1/2,6.59(8),0.22(10),-0.23(10),,5.28(8),0.3(3)*,5.6(3),2.3(5)
50-Sn-118,24.03,0,6.23(4),,,,4.63(8),0,4.63(8),0.22(5)
50-Sn-119,8.58,1/2,6.28(3),0.14(10),0.0(1),,4.71(8),0.3(3)*,5.0(3),2.2(5)
50-Sn-120,32.86,0,6.67(4),,,,5.29(8),0,5.29(8),0.14(3)
50-Sn-122,4.72,0,5.93(3),,,,4.14(7),0,4.14(7),0.18(2)
50-Sn-124,5.94,0,6.15(3),,,,4.48(8),0,4.48(8),0.133(5)
51-Sb,,,5.57(3),,,,3.90(4),0.00(7),3.90(6),4.91(5)
51-Sb-121,57.25,5/2,5.71(6),5.7(2),5.8(2),,4.10(9),0.0003(19),4.10(19),5.75(12)
51-Sb-123,42.75,7/2,5.38(7),5.2(2),5.4(2),,3.64(9),0.001(4),3.64(9),3.8(2)
52-Te,,,5.68(2),,,,4.23(4),0.09(6),4.32(5),4.7(1)
52-Te-120,0.09,0,5.3(5),,,,3.5(7),0,3.5(7),2.3(3)
52-Te-122,2.4,0,3.8(2),,,,1.8(2),0,1.8(2),3.4(5)
52-Te-123,0.87,1/2,-0.05(25),-1.2(2),3.5(2),,0.002(3),0.52(5),0.52(5),418.0(30.0)
52-Te-124,4.61,0,7.95(10),,,,8.0(2),0,8.0(2,6.8(1.3)
52-Te-125,6.99,1/2,5.01(8),4.9(2),5.5(2),,3.17(10),0.008(8),3.18(10),1.55(16)
52-Te-126,18.71,0,5.55(7),,,,3.88(10),0,3.88(10),1.04(15)
52-Te-128,31.79,0,5.88(8),,,,4.36(10),0,4.36(10),0.215(8)
52-Te-130,34.48,0,6.01(7),,,,4.55(11),0,4.55(11),0.29(6)
53-I-127,100,5/2,5.28(2),6.6(2),3.4(2),,3.50(3),0.31(6),3.81(7),6.15(6)
54-Xe,,,4.69(4),,,,3.04(4),0,,23.9(1.2)
54-Xe-124,0.1,0,,,,,,0,,165.0(20.0)
54-Xe-126,0.09,0,,,,,,0,,3.5(8)
54-Xe-128,1.9,0,,,,,,0,,<8.0
54-Xe-129,26.14,1/2,,,,,,,,21.0(5.0)
54-Xe-130,3.3,0,,,,,,0,,<26.0
54-Xe-131,21.18,3/2,,,,,,,,85.0(10.0)
54-Xe-132,26.89,0,,,,,,0,,0.45(6)
54-Xe-134,10.4,0,,,,,,0,,0.265(20)
54-Xe-136,8.9,0,,,,,,0,,0.26(2)
55-Cs-133,100,7/2,5.42(2),,,+/-,3.69(15),0.21(5),3.90(6),29.0(1.5)
56-Ba,,,5.07(3),,,,3.23(4),0.15(11),3.38(10),1.1(1)
56-Ba-130,0.1,0,-3.6(6),,,,1.6(5),0,1.6(5),30.0(5.0)
56-Ba-132,0.09,0,7.8(3),,,,7.6(6),0,7.6(6),7.0(8)
56-Ba-134,2.4,0,5.7(1),,,,4.08(14),0,4.08(14),2.0(1.6)
56-Ba-135,6.59,3/2,4.66(10),,,,2.74(12),0.5(5)*,3.2(5),5.8(9)
56-Ba-136,7.81,0,4.90(8),,,,3.03(10),0,3.03(10),0.68(17)
56-Ba-137,11.32,3/2,6.82(10),,,,5.86(17),0.5(5)*,6.4(5),3.6(2)
56-Ba-138,71.66,0,4.83(8),,,,2.94(10),0,2.94(19),0.27(14)
57-La,,,8.24(4),,,,8.53(8),1.13(19),9.66(17),8.97(2)
57-La-138,0.09,5,8.0(2.0)*,,,,8.0(4.0),0.5(5)*,8.5(4.0),57.0(6.0)
57-La-139,99.91,7/2,8.24(4),11.4(3),4.5(4),+/-,8.53(8),1.13(15),9.66(17),8.93(4)
58-Ce,,,4.84(2),,,,2.94(2),0.00(10),2.94(10),0.63(4)
58-Ce-136,0.19,0,5.76(9),,,,4.23(13),0,4.23(13),7.3(1.5)
58-Ce-138,0.26,0,6.65(9),,,,5.64(15),0,5.64(15),1.1(3)
58-Ce-140,88.48,0,4.81(9),,,,2.94(11),0,2.94(11),0.57(4)
58-Ce-142,11.07,0,4.72(9),,,,2.84(11),0,2.84(11),0.95(5)
59-Pr-141,100,5/2,4.58(5),,,+/-,2.64(6),0.015(3),2.66(6),11.5(3)
60-Nd,,,7.69(5),,,,7.43(19),9.2(8),16.6(8),50.5(1.2)
60-Nd-142,27.11,0,7.7(3),,,,7.5(6),0,7.5(6),18.7(7)
60-Nd-143,12.17,7/2,14.0(2.0)*,,,,25.0(7.0),55.0(7.0),80.0(2.0),337.0(10.0)
60-Nd-144,23.85,0,2.8(3),,,,1.0(2),0,1.0(2),3.6(3)
60-Nd-145,8.5,7/2,14.0(2.0)*,,,,25.0(7.0),5.0(5.0)*,30.0(9.0),42.0(2.0)
60-Nd-146,17.22,0,8.7(2),,,,9.5(4),0,9.5(4),1.4(1)
60-Nd-148,5.7,0,5.7(3),,,,4.1(4),0,4.1(4),2.5(2)
60-Nd-150,5.6,0,5.28(20),,,,3.5(3),0,3.5(3),1.2(2)
61-Pm-147,2.62 Y,7/2,12.6(4),,,,20.0(1.3),1.3(2.0),21.3(1.5),168.4(3.5)
62-Sm,,,0.00(5),,,E,0.422(9),39.0(3.0),39.4(3.0),5922.0(56.0)
62-Sm-144,3.1,0,-3.0(4.0)*,,,,1.0(3.0),0,1.0(3.0),0.7(3)
62-Sm-147,15,7/2,14.0(3.0),,,,25.0(11.0),14.0(19.0.),39.0(16.0),57.0(3.0)
62-Sm-148,11.2,0,-3.0(4.0)*,,,,1.0(3.0),0,1.0(3.0),2.4(6)
62-Sm-149,13.8,7/2,18.7(28),,,E,63.5(6),137.0(5.0),200.0(5.0),42080.0(400.0)
62-Sm-150,7.4,0,14.0(3.0),,,,25.0(11.0),0,25.0(11.0),104.0(4.0)
62-Sm-152,26.7,0,-5.0(6),,,,3.1(8),0,3.1(8),206.0(6.0)
62-Sm-154,22.8,0,8.0(1.0),,,,11.0(2.0),0,11.0(2.0),8.4(5)
63-Eu,,,5.3(3),,,E,6.57(4),2.5(4),9.2(4),4530.0(40.0)
63-Eu-151,47.8,5/2,,,,E,5.5(2),3.1(4),8.6(4),9100.0(100.0)
63-Eu-153,52.8,5/2,8.22(12),,,,8.5(2),1.3(7),9.8(7),312.0(7.0)
64-Gd,,,9.5(2),,,E,29.3(8),151.0(2.0),180.0(2.0),49700.0(125.0)
64-Gd-152,0.2,0,10.0(3.0)*,,,,13.0(8.0),0,13.0(8.0),735.0(20.0)
64-Gd-154,2.2,0,10.0(3.0)*,,,,13.0(8.0),0,13.0(8.0),85.0(12.0)
64-Gd-155,14.9,3/2,13.8(3),,,E,40.8(4),25.0(6.0),66.0(6.0),61100.0(400.0)
64-Gd-156,20.6,0,6.3(4),,,,5.0(6),0,5.0(6),1.5(1.2)
64-Gd-157,15.7,3/2,4.0(2.0),,,E,650.0(4.0),394.0(7.0),1044.0(8.0),259000.0(700.0)
64-Gd-158,24.7,0,9.0(2.0),,,,10.0(5.0),0,10.0(5.0),2.2(2)
64-Gd-160,21.7,0,9.15(5),,,,10.52(11),0,10.52(11),0.77(2)
65-Tb-159,100,3/2,7.34(2),6.8(2),8.1(2),+/-,6.84(6),0.004(3),6.84(6),23.4(4)
66-Dy,,,16.9(3),,,,35.9(8),54.4(1.2),90.3(9),994.0(13.0)
66-Dy-156,0.06,0,6.1(5),,,,4.7(8),0,4.7(8),33.0(3.0)
66-Dy-158,0.1,0,6.0(4.0)*,,,,5.0(6.0),0,5.(6.),43.0(6.0)
66-Dy-160,2.3,0,6.7(4),,,,5.6(7),0,5.6(7),56.0(5.0)
66-Dy-161,18.9,5/2,10.3(4),,,,13.3(1.0),3.0(1.0),16.0(1.0),600.0(25.0)
66-Dy-162,25.5,0,-1.4(5),,,,0.25(18),0,0.25(18),194.0(10.0)
66-Dy-163,24.9,5/2,5.0(4),6.1(5),3.5(5),,3.1(5),0.21(19),3.3(5),124.0(7.0)
66-Dy-164,28.2,0,49.4(5),,,,307.0(3.0),0,307.0(3.0),2840.0(40.0)
67-Ho-165,100,7/2,8.44(3),6.9(2),10.3(2),+/-,8.06(8),0.36(3),8.42(16),64.7(1.2)
68-Er,,,7.79(2),,,,7.63(4),1.1(3),8.7(3),159.0(4.0)
68-Er-162,0.14,0,9.01(11),,,,9.7(4),0,9.7(4),19.0(2.0)
68-Er-164,1.6,0,7.95(14),,,,8.4(4),0,8.4(4),13.0(2.0)
68-Er-166,33.4,0,10.51(19),,,,14.1(5),0,14.1(5),19.6(1.5)
68-Er-167,22.9,7/2,3.06(5),5.3(3),0.0(3),,1.1(2),0.13(6),1.2(2),659.0(16.0)
68-Er-168,27,0,7.43(8),,,,6.9(7),0,6.9(7),2.74(8)
68-Er-170,15,0,9.61(6),,,,11.6(1.2),0,11.6(1.2),5.8(3)
69-Tm-169,100,1/2,7.07(3),,,+/-,6.28(5),0.10(7),6.38(9),100.0(2.0)
70-Yb,,,12.41(3),,,,19.42(9),4.0(2),23.4(2),34.8(8)
70-Yb-168,0.14,0,-4.07(2),,,E,2.13(2),0,2.13(2),2230.0(40.0)
70-Yb-170,3,0,6.8(1),,,,5.8(2),0,5.8(2),11.4(1.0)
70-Yb-171,14.3,1/2,9.7(1),6.5(2),19.4(4),,11.7(2),3.9(2),15.6(3),48.6(2.5)
70-Yb-172,21.9,0,9.5(1),,,,11.2(2),0,11.2(2),0.8(4)
70-Yb-173,16.3,5/2,9.56(10),2.5(2),13.3(3),,11.5(2),3.5,15,17.1(1.3)
70-Yb-174,31.8,0,19.2(1),,,,46.8(5),0,46.8(5),69.4(5.0)
70-Yb-176,12.7,0,8.7(1),,,,9.6(2),0,9.6(2),2.85(5)
71-Lu,,,7.21(3),,,,6.53(5),0.7(4),7.2(4),74.0(2.0)
71-Lu-175,97.4,7/2,7.28(9),,,,6.59(5),0.6(4),7.2(4),21.0(3.0)
71-Lu-176,2.6,7,6.1(2),,,,4.7(2),1.2(3),5.9,2065.(35.)
72-Hf,,,7.77(14),,,,7.6(3),2.6(5),10.2(4),104.1(5)
72-Hf-174,0.184,0,10.9(1.1),,,,15.0(3.0),0,15.0(3.0),561.0(35.0)
72-Hf-176,5.2,0,6.61(18),,,,5.5(3),0,5.5(3),23.5(3.1)
72-Hf-177,18.5,0,0.8(1.0)*,,,,0.1(2),0.1(3),0.2(2),373.0(10.0)
72-Hf-178,27.2,0,5.9(2),,,,4.4(3),0,4.4(3),84.0(4.0)
72-Hf-179,13.8,9/2,7.46(16),,,,7.0(3),0.14(2),7.1(3),41.0(3.0)
72-Hf-180,35.1,0,13.2(3),,,,21.9(1.0),0,21.9(1.0),13.04(7)
73-Ta,,,6.91(7),,,,6.00(12),0.01(17),6.01(12),20.6(5)
73-Ta-180,0.012,9,7.0(2.0)*,,,,6.2(3.5),0.5(5)*,7.0(4.0),563.0(60.0)
73-Ta-181,99.98,7/2,6.91(7),,,+/-,6.00(12),0.011(2),6.01(12),20.5(5)
74-W,,,4.755(18),,,,2.97(2),1.63(6),4.60(6),18.3(2)
74-W-180,0.13,0,5.0(3.0)*,,,,3.0(4.0),0,3.0(4.0),30.0(20.0)
74-W-182,26.3,1/2,7.04(4),,,,6.10(7),0,6.10(7),20.7(5)
74-W-183,14.3,1/2,6.59(4),6.3(4),7.0(4),,5.36(7),0.3(3)*,5.7(3),10.1(3)
74-W-184,30.7,0,7.55(6),,,,7.03(11),0,7.03(11),1.7(1)
74-W-186,28.6,0,-0.73(4),,,,0.065(7),0,0.065(7),37.9(6)
75-Re,,,9.2(2),,,,10.6(5),0.9(6),11.5(3),89.7(1.0)
75-Re-185,37.5,5/2,9.0(3),,,,10.2(7),0.5(9),10.7(6),112.0(2.0)
75-Re-187,62.5,5/2,9.3(3),,,,10.9(7),1.0(6),11.9(4),76.4(1.0)
76-Os,,,10.7(2),,,,14.4(5),0.3(8),14.7(6),16.0(4.0)
76-Os-184,0.02,0,10.0(2.0)*,,,,13.0(5.0),0,13.0(5.0),3000.0(150.0)
76-Os-186,1.6,0,12.0(1.7),,,,17.0(5.0),0,17.0(5.0),80.0(13.0)
76-Os-187,1.6,1/2,10.0(2.0)*,,,,13.0(5.0),0.3(3)*,13.0(5.0),320.0(10.0)
76-Os-188,13.3,0,7.8(3),,,,7.3(6),0,7.3(6),4.7(5)
76-Os-189,16.1,3/2,11.0(3),,,,14.4(8),0.5(5)*,14.9(9),25.0(4.0)
76-Os-190,26.4,0,11.4(3),,,,15.2(8),0,15.2(8),13.1(3)
76-Os-192,41,0,11.9(4),,,,16.6(1.2),0,16.6(1.2),2.0(1)
77-Ir,,,10.6(3),,,,14.1(8),0.0(3.0),14.0(3.0),425.0(2.0)
77-Ir-191,37.4,3/2,,,,,,,,954.0(10.0)
77-Ir-193,62.6,3/2,,,,,,,,111.0(5.0)
78-Pt,,,9.60(1),,,,11.58(2),0.13(11),11.71(11),10.3(3)
78-Pt-190,0.01,0,9.0(1.0),,,,10.0(2.0),0,10.0(2.0),152.0(4.0)
78-Pt-192,1.78,0,9.9(5),,,,12.3(1.2),0,12.3(1.2),10.0(2.5)
78-Pt-194,32.9,0,10.55(8),,,,14.0(2),0,14.0(2),1.44(19)
78-Pt-195,33.8,1/2,8.91(9),9.5(3),7.2(3),+/-,9.8(2),0.13(4),9.9(2),27.5(1.2)
78-Pt-196,25.3,0,9.89(8),,,,12.3(2),0,12.3(2),0.72(4)
78-Pt-198,7.2,0,7.8(1),,,,7.6(2),0,7.6(2),3.66(19)
79-Au-197,100,3/2,7.90(7),6.26(10),9.90(14),+/-,7.32(12),0.43(5),7.75(13),98.65(9)
80-Hg,,,12.595(45),,,,20.24(5),6.6(1),26.8(1),372.3(4.0)
80-Hg-196,0.15,0,30.3(1.0),,,E,115.0(8.0),0,115.0(8.0),3080.0(180.0)
80-Hg-198,10.1,0,,,,,,0,,2.0(3)
80-Hg-199,16.9,0,16.9(4),,,E,36.0(2.0),30.0(3.0),66.0(2.0),2150.0(48.0)
80-Hg-200,23.1,0,,,,,,0,,<60.0
80-Hg-201,13.2,3/2,,,,,,,,7.8(2.0)
80-Hg-202,29.7,0,11.002(43),,,,15.2108(2),0,15.2108(2),4.89(5)
80-Hg-204,6.8,0,,,,,,0,,0.43(10)
81-Tl,,,8.776(5),,,,9.678(11),0.21(15),9.89(15),3.43(6)
81-Tl-203,29.5,1/2,8.51(8),9.08(10),6.62(10),,6.14(28),0.14(4),6.28(28),11.4(2)
81-Tl-205,70.5,1/2,8.87(7),5.15(10),9.43(10),+/-,11.39(17),0.007(1),11.40(17),0.104(17)
82-Pb,,,9.401(2),,,,11.115(7),0.0030(7),11.118(7),0.171(2)
82-Pb-204,1.4,0,10.893(78),,,,12.3(2),0,12.3(2),0.65(7)
82-Pb-206,24.1,0,9.221(78),,,,10.68(12),0,10.68(12),0.0300(8)
82-Pb-207,22.1,1/2,9.286(16),,,+/-,10.82(9),0.002(2),10.82(9),0.699(10)
82-Pb-208,52.4,0,9.494(30),,,,11.34(5),0,11.34(5),0.00048(3)
83-Bi-209,100,9/2,8.532(2),8.26(1),8.74(1),,9.148(4),0.0084(19),9.156(4),0.0338(7)
88-Ra-226,1620 Y,0,10.0(1.0),,,,13.0(3.0),0,13.0(3.0),12.8(1.5)
90-Th-232,100,0,10.31(3),,,,13.36(8),0,13.36(8),7.37(6)
91-Pa-231,32500 Y,3/2,9.1(3),,,,10.4(7),0.1(3.3),10.5(3.2),200.6(2.3)
92-U,,,8.417(5),,,,8.903(11),0.005(16),8.908(11),7.57(2)
92-U-233,159000 Y,5/2,10.1(2),,,,12.8(5),0.1(6),12.9(3),574.7(1.0)
92-U-234,0.005,0,12.4(3),,,,19.3(9),0,19.3(9),100.1(1.3)
92-U-235,0.72,7/2,10.50(3),,,,13.78(11),0.2(2),14.0(2),680.9(1.1)
92-U-238,99.27,0,8.407(7),,,,8.871(11),0,8.871(11),2.68(2)
93-Np-237,2140000 Y,5/2,10.55(10),,,,14.0(3),0.5(5)*,14.5(6),175.9(2.9)
94-Pu-239,24400 Y,1/2,7.7(1),,,,7.5(2),0.2(6),7.7(6),1017.3(2.1)
94-Pu-240,6540 Y,0,3.5(1),,,,1.54(9),0,1.54(9),289.6(1.4)
94-Pu-242,376000 Y,0,8.1(1),,,,8.2(2),0,8.2(2),18.5(5)
95-Am-243,7370 Y,5/2,8.3(2),,,,8.7(4),0.3(2.6),9.0(2.6),75.3(1.8)
96-Cm-244,17.9 Y,0,9.5(3),,,,11.3(7),0,11.3(7),16.2(1.2)
96-Cm-246,4700 Y,0,9.3(2),,,,10.9(5),0,10.9(5),1.36(17)
96-Cm-248,340000 Y,0,7.7(2),,,,7.5(4),0,7.5(4),3.00(26)\
"""
# Imaginary values for select isotopes
# isotope, b_c_i, bp_i, bm_i
nsftableI = """\
2-He-3,-1.48,,-5.925
3-Li-6,-0.26,-0.08(1),-0.62(2)
5-B,-0.21,,
47-Ag-107,-0.01,,
47-Ag-109,-0.025,,
48-Cd,-1.2,,
48-Cd-113,-12,,
49-In,-0.054,,
49-In-115,-0.056,,
52-Te-123,-0.1,,
62-Sm,-1.5,,
62-Sm-149,-11,,
64-Gd,-13.6,,
64-Gd-155,-10.3,,
71-Lu-176,-0.57(2),,
80-Hg-196,-0.8,,\
"""
# Excluding the following because the measurements for the real parts
# were not used in nsftable table.
# 63-Eu-151,-2.46,,
# 64-Gd-157,-47,-75,
def fix_number(str):
"""
Converts strings of the form e.g., 35.24(2)* into numbers without
uncertainty. Also accepts a limited range, e.g., <1e-6, which is
converted as 1e-6. Missing values are set to 0.
"""
if str == '':
return None
idx = str.find('(')
if idx >= 0:
str = str[0:idx]
if str[0] == '<':
str = str[1:]
return float(str)
def sld_table(wavelength=1, table=None, isotopes=True):
"""
Scattering length density table for wavelength 4.75 |Ang|.
:Parameters:
*table* : PeriodicTable
If *table* is not specified, use the common periodic table.
*isotopes* = True : boolean
Whether to consider isotopes or not.
:Returns: None
Example
>>> sld_table(wavelength=4.75) # doctest: +ELLIPSIS, +NORMALIZE_WHITESPACE
Neutron scattering length density table
atom mass density sld imag incoh
H 1.008 0.071 -1.582 0.000 10.691
1-H 1.008 0.071 -1.583 0.000 10.691
D 2.014 0.141 2.823 0.000 1.705
T 3.016 0.212 2.027 0.000 0.453
He 4.003 0.122 0.598 0.000 0.035
3-He 3.016 0.092 1.054 0.272 0.706 *
4-He 4.003 0.122 0.598 0.000 0.035
...
248-Cm 248.072 13.569 2.536 0.000 0.207
* Energy dependent cross sections
"""
table = default_table(table)
# Table for comparison with scattering length density calculators
# b_c for Sc, Te, Xe, Sm, Eu, Gd, W, Au, Hg are different from Neutron News
# The Rauch data have cited references to back up the numbers
# (see doc directory), though it is not clear what criteria are
# used to select amongst the available measurements.
print(" Neutron scattering length density table")
print("%-7s %7s %7s %7s %7s %7s"
%('atom', 'mass', 'density', 'sld', 'imag', 'incoh'))
for el in table:
if el.neutron.has_sld():
coh, jcoh, inc = el.neutron.sld(wavelength=wavelength)
print("%-7s %7.3f %7.3f %7.3f %7.3f %7.3f%s"
%(el, el.mass, el.density, coh, jcoh, inc,
' *' if el.neutron.is_energy_dependent else ''))
if isotopes:
isos = [iso for iso in el if iso.neutron != None and iso.neutron.has_sld()]
else:
isos = []
for iso in isos:
coh, jcoh, inc = iso.neutron.sld(wavelength=wavelength)
print("%-7s %7.3f %7.3f %7.3f %7.3f %7.3f%s"
%(iso, iso.mass, iso.density, coh, jcoh, inc,
' *' if iso.neutron.is_energy_dependent else ''))
print("* Energy dependent cross sections")
def energy_dependent_table(table=None):
"""
Prints a table of energy dependent isotopes.
:Parameters:
*table* : PeriodicTable
If *table* is not specified, use the common periodic table.
:Returns: None
Example
>>> energy_dependent_table()
Elements and isotopes with energy dependent absorption:
He-3
Cd Cd-113
Sm Sm-149
Eu Eu-151
Gd Gd-155 Gd-157
Yb-168
Hg-196 Hg-199
"""
table = default_table(table)
# List of energy dependent elements and isotopes
print("Elements and isotopes with energy dependent absorption:")
for el in table:
if not hasattr(el, 'neutron'):
continue
dep = []
if el.neutron.is_energy_dependent:
dep += [str(el)]
dep += [str(el)+'-'+str(iso.isotope)
for iso in el
if iso.neutron != None and iso.neutron.is_energy_dependent]
if len(dep) > 0:
print(" " + " ".join(dep))
def _diff(iso, a, b, tol=0.01):
if None in (a, b):
if a is not None or b is not None:
if a is None and b > tol:
print("%10s %8s %8.2f"%(iso, "----", b))
elif b is None and a > tol:
print("%10s %8.2f %8s"%(iso, a, "----"))
elif abs(a - b) > tol:
print("%10s %8.2f %8.2f %5.1f%%"
% (iso, a, b, (100*(a-b)/b if b != 0 else inf)))
def compare(fn1, fn2, table=None, tol=0.01):
table = default_table(table)
for el in table:
try:
res1 = fn1(el)
except Exception:
res1 = None
try:
res2 = fn2(el)
except Exception:
res2 = None
_diff(el, res1, res2, tol=tol)
for iso in el:
try:
res1 = fn1(iso)
except Exception:
res1 = None
try:
res2 = fn2(iso)
except Exception:
res2 = None
_diff(iso, res1, res2, tol=tol)
def absorption_comparison_table(table=None, tol=None):
r"""
Prints a table comparing absorption to the imaginary bound coherent
scattering length b_c_i. This is used to checking the integrity
of the data and formula.
The relationship between absorption and b_c_i is:
.. math::
\sigma_a = -2 \lambda b_i \cdot 1000
The wavelength $\lambda = 1.798 \AA$ is the neutron wavelength at which
the absorption is tallied. The factor of 1000 transforms from
|Ang|\ |cdot|\ fm to barn.
:Parameters:
*table* : PeriodicTable
The default periodictable unless a specific table has been requested.
*tol* = 0.01 : float | barn
Show differences greater than this amount.
:Returns: None
Example
>>> absorption_comparison_table (tol=0.5) # doctest: +ELLIPSIS, +NORMALIZE_WHITESPACE
Comparison of absorption and (-2000 lambda b_c_i)
3-He 5333.00 5322.08 0.2%
Li 70.50 ----
6-Li 940.00 934.96 0.5%
B 767.00 755.16 1.6%
10-B 3835.00 ----
N 1.90 ----
...
"""
print("Comparison of absorption and (-2000 lambda b_c_i)")
compare(lambda el: el.neutron.absorption,
lambda el: -2000*el.neutron.b_c_i*ABSORPTION_WAVELENGTH,
table=table, tol=tol)
return
def coherent_comparison_table(table=None, tol=None):
r"""
Prints a table of $4 \pi b_c^2/100$ and coherent for each isotope.
This is useful for checking the integrity of the data and formula.
The table only prints where b_c exists.
:Parameters:
*table* : PeriodicTable
The default periodictable unless a specific table has been requested.
*tol* = 0.01 : float | barn
Amount of difference to show
:Returns: None
Example
>>> coherent_comparison_table (tol=0.5) # doctest: +ELLIPSIS, +NORMALIZE_WHITESPACE
Comparison of (4 pi b_c^2/100) and coherent
n 172.03 43.01 300.0%
1-n 172.03 43.01 300.0%
Sc 18.40 19.00 -3.2%
45-Sc 18.40 19.00 -3.2%
65-Cu 13.08 14.10 -7.2%
70-Zn 5.98 4.50 33.0%
84-Sr 3.14 6.00 -47.6%
...
"""
print("Comparison of (4 pi b_c^2/100) and coherent")
compare(lambda el: 4*pi/100*el.neutron.b_c**2,
lambda el: el.neutron.coherent,
table=table, tol=tol)
def total_comparison_table(table=None, tol=None):
"""
Prints a table of neutron.total and sum coh,inc for each
isotope where these exist. This is used to checking the integrity
of the data and formula.
:Parameters:
*table* : PeriodicTable
The default periodictable unless a specific table has been requested.
*tol* = 0.01 : float | barn
Amount of difference to show
:Returns: None
Example
>>> total_comparison_table (tol=0.1)
Comparison of total cross section to (coherent + incoherent)
n 43.01 ----
1-n 43.01 ----
84-Kr 6.60 ----
149-Sm 200.00 200.50 -0.2%
Eu 9.20 9.07 1.4%
Gd 180.00 180.30 -0.2%
155-Gd 66.00 65.80 0.3%
161-Dy 16.00 16.30 -1.8%
180-Ta 7.00 6.70 4.5%
187-Os 13.00 13.30 -2.3%
"""
print("Comparison of total cross section to (coherent + incoherent)")
compare(lambda el: el.neutron.total,
lambda el: el.neutron.coherent+el.neutron.incoherent,
table=table, tol=tol)
def incoherent_comparison_table(table=None, tol=None):
"""
Prints a table of incoherent computed from total and b_c with incoherent.
:Parameters:
*table* : PeriodicTable
The default periodictable unless a specific table has been requested.
*tol* = 0.01 : float | barn
Amount of difference to show
:Returns: None
Example
>>> incoherent_comparison_table (tol=0.5) # doctest: +ELLIPSIS, +NORMALIZE_WHITESPACE
Comparison of incoherent and (total - 4 pi b_c^2/100)
Sc 4.50 5.10 -11.8%
45-Sc 4.50 5.10 -11.8%
65-Cu 0.40 1.42 -71.7%
70-Zn 0.00 -1.48 -100.0%
84-Sr 0.00 2.86 -100.0%
113-Cd 0.30 4.36 -93.1%
...
"""
print("Comparison of incoherent and (total - 4 pi b_c^2/100)")
compare(lambda el: el.neutron.incoherent,
lambda el: el.neutron.total - 4*pi/100*el.neutron.b_c**2,
table=table, tol=tol)
def print_scattering(compound, wavelength=ABSORPTION_WAVELENGTH):
"""
Print the scattering for a single compound.
"""
from . import formulas
compound = formulas.formula(compound)
density = compound.density if compound.density is not None else 1.0
sld, xs, penetration = neutron_scattering(compound, wavelength=wavelength,
density=density)
print("%s at %g Ang (density=%g g/cm^3)"
% (str(compound), wavelength, density))
print(" sld: %g + %g j (%g incoherent) 1e-6/Ang^2"%sld)
print(" sigma_c: %g sigma_i: %g sigma_a: %g 1/cm"%sld)
print(" mu: %g 1/cm 1/e penetration: %g cm"%(1/penetration, penetration))
def main():
"""
Simple command line interface, showing the predicted neutron scattering.
Usage::
python -m periodictable.nsf [-Lwavelength] compound@density compound@density ...
For example::
$ python -m periodictable.nsf XeF6@3.56
scattering for XeF6 at 1.798 Ang (density=3.56 g/cm^3)
sld: 3.37503 + 0.000582313 j (0.402605 incoherent) 1e-6/Ang^2
sigma_c: 3.37503 sigma_i: 0.000582313 sigma_a: 0.402605 1/cm
1/e penetration: 2.23871 cm
"""
import sys
compounds = sys.argv[1:]
if compounds[0].startswith('-L'):
wavelength = float(compounds[0][2:])
compounds = compounds[1:]
else:
wavelength = ABSORPTION_WAVELENGTH
for c in compounds:
print_scattering(c, wavelength)
if __name__ == "__main__":
main()
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