Isotopes are represented by element[nuclide index].
Special symbols D
 and
T
can be used for 2H and 3H.
Isotopes can be mixed within a formula, such as
DHO
 for partially deuterated water.
Use H[1]
 in formula for labile hydrogen.
These will be substituded with H and D in proportion with the D2O
fraction when computing the contrast match point of the sample.
 represents alanine with one labile hydrogen.
density
Mass density is needed to compute scattering factors for the material.
The density can be entered in the density field, or it can be given in
the formula by adding @value to the end.  Densities for the pure elements are
already known.
H2O@1
indicates that water has a density of 1 g/cm
3 
isotopic density
If the formula uses a mixture of isotopes, you can still use the density
of the material assuming natural abundance, but add an "n" to the value
to scale it to the isotope specific density.  If you already know the
isotopic density, use the value by itself and it will not be scaled.
D2O@1n
,
, and
all give the density of D
2O as 1.11 g/cm
3 
mole fractions
Using non-integer quantities, arbitrary concentration ratios can be
    be constructed.
    78.2H2O[16] + 21.8H2O[18] @1n
        represents water with 78.2% 
16O and 21.8% 
18O
    
 
mass fractions
Formulas can be mixed by mass, with each part starting with a percentage
    followed by formula followed by "//".  The first part must use "%wt" to
    indicate that it is a mass fraction.  The final part is the base, and it
    does not need a percentage since it makes up the rest of the material.
    50%wt Co // Ti
    is more descriptive than Co
0.552Ti
0.448 
    33%wt Co // 33% Fe // Ti
    builds a 1:1:1 mixture by mass of cobalt-iron-titanium
 
volume fractions
Volume fractions are like mass fractions, but they use "%vol" instead.
    Each component of the volume fraction must specify the density.
    20%vol (10%wt 
[email protected] // H2O@1) // D2O@1n
        is a 10% saline solution by weight mixed 20:80 by volume with
        D
2O, which is the same as
        
NaCl(H2O)29.1966(D2O)
[email protected] 
     
mass and volume mixtures
Specific amounts of materials can be mixed, with each part giving
    the quantity of material followed by "//".  Quantities can be masses
    (kg, g, mg, ug, or ng) or they can be volumes (L, mL, uL, nL).  Density
    is required for materials given by volume.  For scattering calculations
    density is required for the materials given by mass as well.
    5g NaCl // 50mL H2O@1
        is more descriptive than
        
NaCl(H2O)32.4407
     
    5g 
[email protected] // 50mL H2O@1
        computes the density as 1.05 g/cm
3.  Not useful in this
        case since 9%wt brine has a density of 1.0633 at ambient temperature.
    
 
    50 mL (45 mL H2O@1 // 5 g NaCl)@1.0707 // 20 mL D2O@1n
        uses the appropriate density for a 10%wt brine in the mixture.
    
 
layer thickness
Multilayer samples can specified as layer thickness and material separated
    by "//".  Thicknesses are in length units (cm, mm, um, nm).  The
    resulting material will compute activation for 1 cm2 of material.
    Density is required for each layer.
    1 cm Si // 5 nm Cr // 10 nm Au
     
biomolecules
    For FASTA sequences
    use "code:sequence", where code is "aa" for amino acid sequences, "dna" for
    DNA sequences, or "rna" for RNA sequences.  Density is estimated automatically.
    This calculation uses 1H for labile hydrogen, with substitution
    by H in natural abundance and pure D when computing contrast match point.
    β-casein amino acid sequence 
aa:RELEELNVPGEIVESLSSSEESITRINKKIEKFQSEEQQQTEDELQDKIHPFAQTQSLVYPFPGPIPNSLPQNIPPLTQTPVVVPPFLQPEVMGVSKVKEAMAPKHKEMPFPKYPVEPFTESQSLTLTDVENLHLPLPLLQSWMHQPHQPLPPTVMFPPQSVLSLSQSKVLPVPQKAVPYPQRDMPIQAFLLYQEPVLGPVRGPFPIIV
 
 
Thermal flux
Units: n/cm2/s
    Provide the thermal flux equivalent for the pre-sample beam configuration
    for the instrument. Because neutron capture cross sections are linear
    above 0.5 Å for most isotopes, simply scale the flux by λ/1.798 Å, where
    λ is the average wavelength at the sample weighted by spectral intensity.
    For non-linear isotopes activation may be underestimated
    (176Lu < 1.8 Å; 151Eu < 0.8 Å)
    or overestimated (33S < 11 Å; 204Hg < 20 Å).
    The neutron activation calculation follows (Shleien 1998).
    Activation is a function of isotope, not element.  When
    an element is used in a formula, the natural abundance of the individual
    isotopes is used to determine the total activation.  By default, the
    activation calculator uses values from the IAEA
    handbook (IAEA 1987), and the
    scattering calculator uses the IUPAC 2021 atomic weights and isotope composition
    database (CIAAW 2021).
    For very high fluences, e.g., more than 1016 n/cm2, the activation
    equations give erroneous results because of the precision limitations.
    If there is doubt simply do the calculation at a lower flux and
    proportion the result. This will not work for the cascade reactions,
    i.e., two neutron additions.
    Reaction = b  : This is the beta produced daughter of an activated parent.
    This is calculated only for the cases where the daughter is long lived
    relative to the parent. The calculated activity is through the end of
    exposure only. Contributions from the added decay of the parent after the
    end of irradiation are left for the user to determine, but are usually
    negligible for irradiations that are long relative to the parent halflife.
Calculation parameters are controlled by URL:
    - isotope abundance
 
    - 
    Use the following to select IUPAC 2021 isotopic abundance data rather than the IAEA 1987 data:
    index.html?abundance=IUPAC
    
 
    - activation cutoff
 
    - 
    The cutoff values for displaying activation data are set to 0.0005 μCi
    by default.  The full activation levels
    can be displayed using: index.html?cutoff=0
    
 
    - decay cutoff
 
    - The activation calculator determines the amount of time for the activation to decay to
    the cutoff level, or to 0.0005 μCi if cutoff is 0.  This can be set to a value
    such as 0.1 μCi using: index.html?decay=0.1
    
 
Notes on calculation:
- 
  For some numerical combinations with very large half-lives the numerical
  precision is inadequate and you get negative results. This can be
  corrected by reformulation or approximations but has not been done.
  Remember, the X in EXP(X) is limited to |X|<709
 - 
  Simplifications have been made as indicated in the comments column in
  data table
 - 
  Typically, for a decay chain where the daughter is also produced (isomers)
  the s of the parent has been added to that of the daughter when the
  daughter t1/2 is much longer (true for most cases) and the parent
  t1/2 is relatively short, e.g. less than 1 day, so that all the daughter
  will be made relatively promptly.
 - 
  In cases where the above condition is not met an * is put next to the
  nuclide name to warn that the daughter production has not been accounted
  for. In most cases the daughter is in a simple decay equilibrium.
 - 
  Where the decay product is a new nuclide a line has been added to the
  database to account for this. This production mode is indicated in
  the reaction column by 'b'. Where both m and g state contribute to daughter
  production it is simplified to a single parent, that with the greater
  cross-section or that with the longer half-life together with the sum
  of the cross-sections.
 - 
  In a few cases where the parent nuclide t1/2 is very short all production
  is assigned to the daughter and no entry is made for the parent, as
  noted in the comments column.
 - 
  No correction for neutron burn up has been made.
 - 
  Most cross-section data is from IAEA 273.
 - 
  Fast neutron data from NBSIR 85-3151, Compendium of Benchmark Neutron Fields
  is for reaction above the Cd cutooff, .4eV. Noted in comment column.
 - 
  Fast neutron reaction data from IAEA 273 has been weighted by a unit fluence
  fast maxwellian spectrum as described in NBSIR 85-3151, but no further
  weighting for a 1/v or thermal component has been made. Only selected
  reactions have been included.
 - 
   Reaction = b indicates production via decay from an activation produced parent.
 - 
  Notation on reaction product name:
  
 - m, m1, m2
  - 
    indicate metastable states. Decay may be the ground state or another nuclide.
  
  - +
  - 
    indicates radioactive daughter production already included in daughter listing
    several parent t1/2's required to acheive calculated daughter activity.
    All activations are assigned at end of irradiation.
    In most cases the added activity to the daughter is small.
  
  - *
  - 
    indicates radioactive daughter production NOT calculated, approx
    secular equilibrium.
  
  - s
  - 
    indicates radioactive daughter of this nuclide in secular equilibrium
    after several daughter t1/2's.
  
  - t
  - 
    indicates transient equilibrium via beta decay. Accumulation of that nuclide
    during irradiation is separately calculated.
  
  
 
 
    Cadmium ratio
    Units: none
    
    Samples in the rabbit tubes can be shielded with cadmium to reduce the thermal
    flux while leaving the epithermal flux mostly unchanged.  The cadmium ratio
    determines the degree of reduction in the scattering cross sections, corresponding
    to the reduced flux.  This value is unitless.  Use a value of 0 for beamline
    experiments.
    
 
    Thermal/fast ratio
    Units: none
    
    When performing neutron activation analysis in a rabbit tube, the additional
    fast neutron activations need to be determined.  The thermal/fast ratio is
    used to determine the fast neutron flux from the thermal flux equivalent for
    the given rabbit tube.  The resulting fast flux is (thermal flux)/(thermal/fast ratio).
    This value is unitless.  Use a value of 0 for beamline experiments.
    
 
    Material mass
    Units: g, kg, mg or ug
    
    The total neutron activation depends on the mass of the individual
    isotopes in the sample and the total time in the beam.  All activation
    calculations assume a thin plate sample, with all parts of the sample
    exposed to full flux during activation, and no self-shielding when
    estimating the activation level outside the beam.
    
 
    Exposure
    Units: h m s d w y
    
    Exposure is the duration of the exposure at the given flux. Activation
    will be accumulated over that time, with decay beginning the moment the
    sample is activated. Time defaults to hours, but can be set to
    hours, minutes, seconds, days, weeks or years by adding h, m, s, d, w, or y
    to the value respectively.
    
 
    Decay
    Units: h m s d w y OR yyyy-mm-dd hh:mm:ss
    
    The sample begins to decay immediately, even while it is being activated.
    The decay field allows you to specify how long since the sample
    was removed from the beam.  The default is hours, but can be set to
    hours, minutes, seconds, days, weeks or years by adding h, m, s, d, w, or y
    to the value respectively.
    We always compute the activation level when the sample is removed from the beam,
    and at 1 hour, 1 day and 15 days post activation.
    
    
    Instead of saying how long the sample activation has decayed, you can use
    the time that the sample was removed from the beam. Times are given as
        year-month-day hour:minute:second.
    Approximate times are allowed, such as 2010-03 for March, 2010.  This is
    equivalent to 2010-03-31 23:59:59, which is the end of March so that the
    activation estimate will be conservative.  This is the most activation
    consistent with the sample being on the beam sometime in March, 2010.
    Times are specified in US/Eastern.  Add "Z" after the time of day to
    indicate universal coordinated time (UTC), or add a timezone offset such
    as "+01" for +1 hours in France in winter, when daylight savings time is
    not in effect.
    
    
    
    | If you type: | This is equivalent to: | 
    | 2 m | 2 minutes ago | 
    | 1 | 1 hour ago | 
    | 2.5w | 2 and a half weeks ago | 
    | 3 y | 3 years ago | 
    | 2015-01-02 21:45:00 | January 2, 2015 at 9:45 PM US/Eastern | 
    | 2010-03 | March 31, 2010 at 11:59:59 PM US/Eastern | 
    | 2010-7-5 12:23 | July 5, 2010 at 12:23:59 PM US/Eastern | 
    | 2015-01-02 21:45:00Z | January 2, 2015 at 9:45 PM UTC | 
    | 2015-01-02 21:45:00-0600 | January 2, 2015 at 9:45 PM US/Central | 
    | 2015-08-02 21:45:00-0500 | August 2, 2015 at 9:45 PM US/Central | 
     |  | 
    
 
    Mass density
    Units: g/cm3 or A3
    
    Density is used to compute absorption, transmission and scattering.
    
    - from formula
 
    - Leave the density field blank and add
    
@
 + density
    to the end of the formula, where density is in g/cm3.
    For compounds with specific isotopes, you can use the density of the
    naturally occurring compound as
    @
 + density + n
    and the isotope specific density will be computed.  Density defaults to
    1 g/cm3, or for pure elements, the natural density given in
    the periodic table is used.
    
     
    - g/cm3
 
    - Enter the density by itself, which will be interpreted as g/cm3, or
    equivalently, kg/L.  No units are needed.  If the value is
    density + 
n
 then it is density of the the
    naturally occuring compound and the isotopic density will be computed.
    D
2O has a natural density of
    
1n
 and an isotopic density of
    
1.11
 
     
    - cell volume
 
    - Enter a number followed by A3 for Å3.  Be sure that your
    formula contains the correct number of atoms for the unit cell, possibly by
    using n(formula), where n is 6 for hexagonal close packed, 4 for face centered
    cells, 2 for body centered and base centered cells, or 1 for simple cells.
    
4NaCl has a cell volume of
    
179.4 A3
 
     
    - crystal lattice parameters
 
    - Enter lattice parameters "a:n b:n c:n alpha:n beta:n gamma:n"
    where a, b, c are in Å and α, β, γ are in degrees.
    If not specified, b and c default to a.  Ratios can also be used,
    so that "b/a:n" gives b=n*a, and "c/a:n" gives c=n*a.  Angles
    α, β, and γ default to 90°.  Be sure that the
    formula contains the correct number of atoms for the unit cell.
    
4NaCl has a cubic lattice with
    
a:5.6402
 
     
    
 
    Thickness
    Units: cm
    
    The material thickness in cm is used to determine sample transmission,
    or how much beam will be absorbed by the sample or scattered incoherently.
    Leave it at 1 cm if you do not need this information.
    
 
    Source neutrons
    Units: Ang, meV or m/s
    
    The energy of the source neutrons will affect the absorption cross section
    and hence the penetration depth and sample attenuation.  Energy can be
    expressed as wavelength in Å, as energy in meV, or as neutron
    velocity in m/s.
    Neutron cross sections are tabulated
    at 1.798 Å = 25.3 meV = 2200 m/s, with an assumed 1/v dependence for
    the absorption cross section (Rauch 2003,
    Sears 2006).
    
    For heavier isotopes (Cd, Hf, rare earths) and/or shorter wavelengths
    (below 1 Å) there are neutron resonances
    in the thermal range. For common rare-earth isotopes the energy-dependent
    coherent and absorption cross sections tabulated in
    Lynn and Seeger 1992 are used.
    Incoherent scattering will be understimated for these elements.
    Resonances for 113Cd and 180Ta are ignored.
    
    There is also a wavelength dependence for single phonon interactions which
    gives rise to significant inelastic scattering for lighter isotopes (H, D)
    and/or longer wavelengths (above 5 Å). This factor is both
    temperature and material dependent and will not be included
    in the scattering calculations. In particular, penetration length and
    transmitted flux are going to be significantly overestimated.
    
 
    Source X-rays
    Units: Ang, keV or Ka
    
    X-ray absorption and scattering are computed from the energy dependent
    atomic scattering factors (Henke 1993).
    Energy can be expressed as wavelength in Å, as energy in keV, or
    using an element name for the Kα emission line2 for
    that element (Deslattes 2003).
    
 
    References
    
    - 
        CIAAW. Isotopic compositions of the elements 2021. Available online
        at www.ciaaw.org
        Bölke, et al. (2005).
        [atomic weights,
        isotopic abundance]
    
 
    - 
        Deslattes, R.D.; Kessler, Jr., E.G.; Indelicato, P.; de Billy, L.; Lindroth, E. and Anton, J. (2003).
        Rev. Mod. Phys. 75, 35-99.
        [xray emission lines]
    
 
    - 
        Henke, B.L.; Gullikson, E.M. and Davis, J.C. (1993).
        X-ray interactions:
        photoabsorption, scattering, transmission, and reflection at E=50-30000 eV, Z=1-92,
        Atomic Data and Nuclear Data Tables Vol. 54 (no.2), 181-342.
        [xray cross sections]
    
 
    - 
        IAEA (1987).
        Handbook on Nuclear Activation Data.
        TR 273 (International Atomic Energy Agency, Vienna, Austria).
        [tech report]
    
 
    
    - 
        Kienzle, P. A. (2008).
        Extensible periodic table
        [Computer Software].
        https://periodictable.readthedocs.io.
        [calculator source,
        web service source]
    
 
    - 
        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.
        doi:10.1016/0092-640X(90)90013-A
        [rare earth scattering lengths]
    
 - 
        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.
        [booklet,
        neutron cross sections]
    
 
    - 
        Sears, V. F. (2006). "Scattering lengths for neutrons" In Prince, E. Ed.
        International Tables for Crystallography Volume C: Mathematical, Physical and Chemical Tables"
        Kluwer Academic Publishers, pp 444-454.
        doi:10.1107/97809553602060000103
        [scattering calculations]
    
 
    - 
        Shleien, B.; Slaback, L.A. and Birky, B.K. (1998).
        Handbook of health physics and radiological health.
        Williams & Wilkins, Baltimore.
        [activation data]
    
 
    
 
    History
    
    - 2025-04-23 v2.0.0
 
        - Fix sort by half-life with units of ky, My, Gy.
 
    - 2025-02-28 v2.0.0
 
        - Use standard year as 365 rather than 365.2425 days when reporting decay time.
    
 
    - 2024-12-03 v2.0.0
 - Update mass and abundance tables, and physical constant values
        
neutron cross section updates for H, He, C, O, Zn, Kr, Sn, Xe, Sm, Eu, Ir, Pb, Bi
        
X-ray cross section updates for Pt, Cr, Nb, Y, Er
        
208Pb activation scaled by 0.001 (value was reported in mbarns but added as barns)
     
    - 2024-03-22 v1.7.0
 - Mixture formulas allow wt% and vol%.
        
Formulas allow unicode subscripts such as H₂O.
        
FASTA sequences (aa: rna: dna:) allowed as mixture components.
        
FASTA calculations updated.
        
Use correct halflife for Tm-171, Ho-163 and W-188 activation products.
        
Improve numerical precision of activation calculations.
     
    - 2021-04-21 v1.6.0
 - Support energy-dependent rare earth elements.
        
Use complex scattering length bc when computing
              σc = 4π |bc|2/100 and
              σi = σs - σc.
     
    - 2020-10-29 v1.5.3
 - Change field labels from 'time on/off beam' to 'exposure/decay duration'.
 
    - 2020-01-22
 - Restore support for Internet Explorer 10 and 11.
 
    - 2019-12-02
 - Fix cutoff=0 handling in URL.
 
    - 2019-11-14 v1.5.2
 - Correct units on activity table: nCi becomes uCi.
        
Elemental carbon density changed to 2.2 to match CXRO, CRC and RSC.
     
    - 2019-11-04
 - Update neutron refs with links to ILL data book and Table for Crystallography.
 
    - 2019-09-16
 - Improve help system: can now scroll between sections.
 
    - 2019-09-11 v1.5.1
 - Include notes on activation calculation.
 
    - 2019-08-27
 - Change default cutoff to 0.5 nCi.
 
    - 2018-01-12
 - Make activation table sortable.
 
    - 2017-05-11 v1.5.0
 - Improved support for printing tables.
        
Support for biomolecules with labile hydrogen (FASTA format).
        
Mixture by mass and volume, e.g., 5 g NaCl // 50 mL H2O@1
        
Multi-layer materials, e.g., 5 um Si // 3 nm Cr // 8 nm Au
        
Compute incoherent cross section from coherent and total.
     
    - 2016-12-07
 - Use exponential notation for all activity levels.
 
    - 2015-10-20
 - Allow decay time to be calculated from timestamp..
 
    - 2014-03-20 v1.4.1
 - Default to isotopic density.
 
    - 2013-11-05
 - Support for X-ray scattering.
 
    - 2013-04-17 v1.3.8
 - Initial release.