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Nuclide reference — half-lives, emission lines, dose rates and shielding

Nuclide reference

One sheet per nuclide, for the 147 nuclides this site carries decay data for.

What is on each sheet, and how it is worked out

Each sheet gives the half-life, decay mode and specific activity, the photon, beta and alpha lines that the evaluated data records, and — where there are photons above the cutoff — the air kerma rate constant and the dose rate a given activity produces at a metre. None of it is copied from a published table of constants. The emission data come from the IAEA evaluated file and the photon interaction coefficients from NIST, and every derived quantity is recomputed from those two.

Emission probability is not dose contribution

A line's emission probability says how often it appears per hundred decays. Its share of the dose rate also carries its energy and the absorption coefficient of air at that energy, so the two rankings differ — a weak, hard line can outrank a strong, soft one. Each sheet prints both columns side by side and says how many lines it takes to account for ninety per cent of the dose rate. For most nuclides the answer is one or two out of a list of twenty or more.

Half-value layers are solved for the spectrum, not for one energy

The usual shortcut is to pick a representative energy, look the attenuation coefficient up, and divide. That is exact only for a nuclide with a single line. When there are several, each one is attenuated at its own rate, and the thickness that halves the total is not the thickness that halves any one of them. Sodium-22 shows the size of the error plainly: read from its strongest line at 1275 keV the lead half-value layer looks like 10.5 mm, but that line carries only 55% of the kerma and the rest is 511 keV annihilation radiation, so the real figure is 6.5 mm.

These sheets solve for the thickness that leaves half — then a tenth — of the whole spectrum's air kerma rate, line by line. The figures are narrow beam: scattered radiation is not added back, so a shield designed to these numbers will let more through than they suggest. The gamma shielding calculator takes a buildup factor when the answer has to be a design figure.

When half-value layers stop being additive

For a single energy the tenth-value layer is always 3.32 times the half-value layer, and stacking three half-value layers leaves an eighth. Neither holds for a broad spectrum. The first layer removes the soft part cheaply and what comes through is harder than what went in, so the second layer removes less than the first. Tin-113 is the extreme case here, with a tenth-value layer eighty-four times its half-value layer. Every sheet prints the ratio so the reader can see when the rule of thumb has stopped working.

Nuclides with no photon above the cutoff

51 of the 147 nuclides here have no photon line above the conventional 20 keV cutoff, so their air kerma rate constant is zero and no external dose rate can be quoted. They are not rare or exotic — they include tritium, carbon-14, nickel-63, strontium-90, technetium-99 and iodine-129, which is to say most of what matters in waste characterisation and decommissioning. Calculators built around a table of gamma constants either omit them or return zero without saying why. Their sheets give what does apply: beta endpoint and mean, range in common absorbers, bremsstrahlung yield against atomic number, and specific activity.

Beta shielding is a low-atomic-number job

Stopping a beta is a matter of enough material, and the range follows from the endpoint energy. What changes with the choice of material is how much of the beta energy leaves again as bremsstrahlung, which rises with atomic number. Shielding a strong beta emitter with lead converts a particle you could have stopped into a photon you now have to stop. Each beta sheet prints the yield in acrylic and in lead so the comparison is in front of the reader.

What these sheets do not tell you

Every figure here is an external quantity for a bare point source in air. Nothing on these sheets is an internal dose: committed effective dose per becquerel taken in depends on chemical form and biokinetics, and this site does not compute it. A real source has self-absorption, a capsule and a geometry, and each of those lowers what a meter would actually read. Shielding thicknesses are narrow beam, so scatter is not added back and a design needs more than they say. Where a nuclide emits betas, the range is an empirical fit and skin dose from a contamination is a different calculation again — it needs source geometry and a point kernel, which this site does not do. Each sheet repeats only the part of this that its own numbers make specific.

All 147 nuclides

96 emit photons above the cutoff; the rest are listed too. On a wide screen the table also carries the decay mode and Γ, the air kerma rate constant in mGy·m²/(GBq·h) at δ = 20 keV; on a narrow one both are on the sheet itself rather than squeezed into the list.

NuclideHalf-lifeEmissions
Ac-227 21.772 years beta, alpha
Am-241 432.6 years photon, alpha
Am-243 7364 years alpha
Ar-39 268 years beta
Au-198 2.6941 days photon
Au-198m 2.272 days photon
Ba-133 10.551 years photon
Ba-133m 38.93 hours photon
Ba-137m 2.552 minutes photon
Bi-210 5.012 days beta
C-14 5700 years beta
Ca-41 9.94 × 10⁴ years none recorded
Ca-45 162.61 days beta
Cd-109 461.9 days photon
Cd-109m1 11.8 microseconds photon
Cd-109m2 10.6 microseconds photon
Ce-139 137.63 days photon
Ce-139m 57.58 seconds photon
Ce-141 32.504 days photon
Ce-144 284.91 days photon, beta
Cf-249 351 years alpha
Cf-252 2.647 years alpha
Cl-36 3.013 × 10⁵ years photon, beta
Cm-242 162.88 days alpha
Cm-243 29.1 years alpha
Cm-244 18.11 years photon, alpha
Cm-245 8423 years alpha
Cm-246 4706 years alpha
Co-57 271.74 days photon
Co-60 1925.28 days photon, beta
Co-60m 10.467 minutes photon
Cr-51 27.704 days photon
Cs-134 2.0652 years photon
Cs-134m 2.912 hours photon
Cs-135 2.3 × 10⁶ years beta
Cs-137 30.08 years photon
Eu-152 13.517 years photon
Eu-152m1 9.3116 hours photon
Eu-152m2 96 minutes photon
Eu-154 8.601 years photon
Eu-154m 46.3 minutes photon
F-18 109.77 minutes photon
Fe-55 2.744 years X-ray only
Fe-59 44.490 days photon
Ga-67 3.2617 days photon
Ga-68 67.71 minutes photon
Gd-148 71.1 years alpha
Ge-68 270.93 days X-ray only
H-3 12.32 years beta
Hg-203 46.610 days photon
Hg-203m 22.1 microseconds photon
Ho-166 26.824 hours beta
I-125 59.407 days photon
I-129 1.57 × 10⁷ years beta
I-131 8.0252 days photon, beta
In-111 2.8047 days photon
In-111m 7.7 minutes photon
Ir-192 73.829 days photon
Ir-192m1 1.45 minutes photon
Ir-192m2 241 years photon
K-40 1.248 × 10⁹ years photon
Kr-85 10.739 years photon, beta
Kr-85m 4.480 hours photon
Lu-177 6.6443 days photon
Lu-177m 160.4 days photon
Mn-54 312.20 days photon
Mo-99 65.924 hours photon, beta
Na-22 2.6018 years photon
Na-24 14.956 hours photon
Na-24m 20.18 milliseconds photon
Nb-95 34.991 days photon
Nb-95m 3.61 days photon
Ni-59 7.6 × 10⁴ years none recorded
Ni-63 100.8 years beta
Np-237 2.144 × 10⁶ years alpha
P-32 14.268 days beta
P-33 25.38 days beta
Pa-231 32570 years alpha
Pb-210 22.20 years photon, beta
Pm-147 2.6234 years photon, beta
Po-210 138.376 days alpha
Pr-144 17.28 minutes beta
Pu-238 87.7 years photon, alpha
Pu-239 24110 years photon, alpha
Pu-240 6561 years photon, alpha
Pu-241 14.329 years X-ray only, beta
Pu-242 3.73 × 10⁵ years alpha
Pu-244 8.13 × 10⁷ years alpha
Ra-223 11.43 days photon, alpha
Ra-224 3.6316 days alpha
Ra-226 1600 years photon, alpha
Ra-228 5.75 years none recorded
Re-188 17.005 hours photon
Re-188m 18.59 minutes photon
Rh-106 30.07 seconds photon, beta
Rh-106m 131 minutes photon
Ru-106 371.8 days beta
S-35 87.37 days beta
Sb-124 60.20 days photon
Sb-124m1 93 seconds photon
Sb-124m2 20.2 minutes photon
Sb-125 2.75856 years photon
Sc-46 83.79 days photon
Sc-46m 18.75 seconds photon
Se-75 119.78 days photon
Se-79 3.27 × 10⁵ years beta
Si-32 157 years beta
Sm-147 1.073 × 10¹¹ years alpha
Sm-151 90 years beta
Sm-153 46.284 hours photon
Sm-153m 10.6 milliseconds photon
Sn-113 115.09 days photon
Sn-113m 21.4 minutes photon
Sr-85 64.849 days photon
Sr-85m 67.63 minutes photon
Sr-89 50.563 days photon, beta
Sr-90 28.91 years beta
Ta-182 114.74 days photon
Ta-182m1 283 milliseconds X-ray only
Ta-182m2 15.84 minutes photon
Tc-99 2.111 × 10⁵ years beta
Tc-99m 6.0072 hours photon
Th-228 1.9116 years photon, alpha
Th-229 7880 years alpha
Th-230 75584 years alpha
Th-232 1.40 × 10¹⁰ years photon, alpha
Tl-201 3.0420 days photon
Tl-201m 2.11 milliseconds photon
Tl-204 3.783 years beta
U-232 68.9 years alpha
U-233 1.5919 × 10⁵ years alpha
U-234 2.455 × 10⁵ years photon, alpha
U-235 7.04 × 10⁸ years photon, alpha
U-236 2.342 × 10⁷ years alpha
U-238 4.468 × 10⁹ years photon, alpha
U-238m 280 ns photon
Xe-133 5.2475 days photon
Xe-133m 2.198 days photon
Y-88 106.626 days photon
Y-88m1 0.301 milliseconds photon
Y-88m2 13.98 milliseconds photon
Y-90 64.05 hours X-ray only, beta
Y-90m 3.19 hours photon
Y-91 58.51 days beta
Zn-65 243.93 days photon
Zr-93 1.61 × 10⁶ years beta
Zr-95 64.032 days photon

Decay data from the IAEA Nuclear Data Section — Livechart API (ENSDF); attenuation coefficients from the NIST X-Ray Mass Attenuation Coefficients. Both are harvested once and committed to the source repository, so these figures do not change between visits. The derivations, their validation and the citations for both upstream datasets are on the methods page.

For a handful of nuclides the endpoint on the page is not the one that decides the shield: a short-lived daughter carries a harder beta, and the source contains both. Nuclides whose daughter sets the shield lists them with the factor by which the parent figure understates the thickness.