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
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Edges energies:
Table of Isotopes, CD-ROM, 8th edition, Version 1.0, March 1996
Richard B Firestone
S Y Frank Chu, CD-ROM Editor
Virginia S Shirley, Editor
Wiley-Interscience
Total cross sections, fluorescent yields, jump ratios:
W.T. Elam, B.D. Ravel, J.R. Sieber,"A new database for X-Ray spectroscopic
calculations", Radiation Physics and Chemistry, 63, pp. 121-128, 2002.
Elastic scattering:
D.E. Cullen, J.H. Hubbell, J.H. Kissel, EPDL97: The evaluated photon
library, '97 Version. Lawrence Livermore National Laboratory Report
UCRL-50400, vol. 6 Rev 5.
Inelastic scattering:
J H Hubbell, W J Veigele, E A Briggs, R T Brown, D T Cromer, and R J
Howerton, "UD "Atomic form factors, incoherent scattering functions, and
photon scattering cross sections", J. Phys. Chem. Ref. Data, Vol. 4, No.
3, pag 471, 1975.
Coster-Kronig transition probability:
X-Ray Fluorescence Cross Sections for K and L X-Rays of the Elements
M.O. Krause, C.W. Nestor, Jr., C.J. Sparks, Jr. and E. Ricci
ORNL-5399, pag 120, 1978
fluor_lines.dat
===============
This x-ray transition table provides the energies (in eV) for K transitions connecting the K shell (n = 1) to the shells with principal quantum numbers n = 2 to 4 and L transitions connecting the L1, L2, and L3 shells (n = 2) to the shells with principal quantum numbers n = 3 and 4. The elements covered include Z = 10, neon to Z = 100, fermium.
Reference:
R.D. Deslattes, E.G. Kessler Jr., P. Indelicato, L. de Billy, E. Lindroth,
J. Anton, J.S. Coursey, D.J. Schwab, K. Olsen, and R.A. Dragoset (2003)
X-ray Transition Energies (version 1.0).
[Online] Available:
http://physics.nist.gov/XrayTrans
[2003, October 16]. National Institute of
Standards and Technology, Gaithersburg, MD.
Originally published as: R.D. Deslattes, E.G. Kessler, Jr., P. Indelicato, L. de Billy, E. Lindroth, and J. Anton, "X-ray transition energies: new approach to a comprehensive evaluation," Rev. Mod. Phys. 75, 35-99 (2003).
The data in this tabulation corresponds to the experimental values given in table 5 of the cited publication. If the experimental value is not available, it has been substituted by the theoretical value in the same table.
In addition, values for Z=3-9 for KL3 (Ka1) have been added from:
X-Ray Data Booklet
Section 1.2 X-RAY EMISSION ENERGIES
Jeffrey B. Kortright and Albert C. Thompson
http://xdb.lbl.gov/Section1/Sec_1-2.html
Column label: The x-ray transition in IUPAC Notation
radrate.dat
===========
X-ray emission rates for K and L shells
The data contained are in tables 13 and 14 of:
X-Ray Fluorescence Cross Sections for K and L X Rays of the elements
M. O. Krause, C. W. Nestor, C. J. Sparks and E. Ricci
ORNL-5399 (1978)
which cites:
[4] J.H. Scofield, Phys. Rev. A 9, 1041 (1974)
[5] J.H. Scofield, Phys. Rev. A 10, 1507 (1974)
[6] J.H. Scofield, Phys. Rev. A 12, 345 (1975)
[7] J.H. Scofield, in ATomic Intershell Processes, B, Crasemann,Ed.
vol. 1, Academic Press, 1975, chap. 6.
[8] Values for elements not listed in refs. 4-7 were interpolated
with the aid of Scofield's relativistic Hartree-Slater predictions [At. Data Nucl. Data Tables 14, 121 (1974)]
Labels are in iupac notation. Only radiation rates affecting single transition (not blended lines, ie. L1L23, L1O23 and L3N45 are present in Krause but they are not included in our tabulation) are used:
iupac siegbahn
K-shell:
KL3 Ka1
KL2 Ka2 (calculated as KL23-KL3 in the tables)
KM3 Kb1
KM2 Kb3 (calculated as KM23-KM3 in the tables)
L-shell:
L3M5 La1
L2M4 Lb1
L1M3 Lb3
L2N4 Lg1
L3M1 Ll
fi.dat
======
Anomalous scattering factor fi.
Taken from D.E. Cullen, J.H. Hubbell, J.H. Kissel, EPDL97: The evaluated photon
library, '97 Version. Lawrence Livermore National Laboratory Report
UCRL-50400, vol. 6 Rev 5.
kissel_pe.dat
=============
Partial and Total Photoelectric cross sections.
This data set contains data calculated by Lynn Kissel
(lkissel@llnl.gov). The original data is available from
ftp://www-phys.llnl.gov/rayleigh
and an interactive WWW interface is in
http://www-phys.llnl.gov/V_Div/scattering/elastic.html
For more information consult the references mentioned in the previous
paragraph.
Refractive indices
==================
The real (1-delta) and imaginary (beta) part of the refractive indices are calculated according to the formulas that can be found for example in the PhD thesises of Peter Cloetens, Carsten Raven and Timm Weitkamp
Compton profiles
================
Calculated by Biggs et al: Hartree-Fock Compton profiles for the elements
Atomic Data and Nuclear Data Tables 16, 201-309 (1975)
Taken from the LSCAT extension to the EGS4 program from Namito et al
Atomic level widths
===================
The data contained within atomiclevelswidth.dat were obtained from Campbell and Papp's paper "Widths of the atomic K-N7 levels", Atomic Data and Nuclear Data Tables (2001)
Non-radiative (Auger) rates
===========================
Taken from the EADL97 database. Originally published by Chen and Crasemann in their papers "Relativistic radiationless tranqition probabilities for atomic K- and L-shells", Atomic Data and Nulear Data Tables (1979) and "Relativistic M-shell radiationless transitions", Physical Review A (1980)
Crystal structures
==================
Taken from XOP with kind permissions from Manuel Sanchez del Rio.
CS_Energy.dat
=============
Mass energy-absorption coefficients. Values are taken from NIST (http://physics.nist.gov/PhysRefData/XrayMassCoef/tab3.html), as calculated by S.M. Seltzer (Radiation Research 136, 147 (1993)).
NIST compound composition database and element densities (densities.dat)
========================================================================
Taken from http://physics.nist.gov/cgi-bin/Star/compos.pl using the nist-compounds.pl script
Fluorescence yields and Coster-Kronig transition probabilities
==============================================================
Some of the values have been replaced by those from Campbell's paper "Fluorescence yields and Coster–Kronig probabilities for the atomic L subshells. Part II: The L1 subshell revisited", Atomic Data and Nulear Data Tables (2009)
Radionuclides
=============
Taken from http://ie.lbl.gov/toi using the nuclices.pl script
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