Curium-244
Cm-244 · Curium, Z = 96, A = 244
Curium-244 decays by alpha decay, half-life 18.11 years. Specific activity is 2.99e+12 Bq/g (80.9 Ci/g), so a gigabecquerel comes to 334 µg — weighable, but on an analytical balance. Over a year the activity falls to 96.24%, and over forty years to 21.63%.
The air kerma rate constant is small — 0.00000336 mGy·m²/(GBq·h), 2.6e+4× less than Cs-137 and 1.0e+5× less than Co-60, ranking 94 of 96 by Γ — near the bottom of the photon emitters, but above the cutoff, which 51 nuclides in this dataset are not. 1 GBq at 1 m reads 0.00000336 mGy/h, and 1 Ci at the same distance 0.000124 mGy/h. It takes 5.95 TBq at a metre to reach 20 µSv/h from the photons alone.
3 lines clear the 20 keV cutoff, but one of them carries 90% of the dose rate. The leading one is 42.8 keV at 90.1% of the total — its emission probability is 0.02635%, which is also the highest.
Shielding barely arises: 0.0558 mm of lead halves the air kerma rate and 0.207 mm takes it to a tenth, thicknesses a source capsule is likely to exceed on its own. Steel does the halving in 0.335 mm. At 1 GBq and a metre it is already under 20 µSv/h with nothing in the way. The tenth-value layer runs 3.7 times the half-value layer, not the 3.32 a single energy would give.
Alpha emission is led by 5.805 MeV at 76.9%, one of 3 recorded lines. None of it reaches through skin, so the alpha is an intake hazard rather than an external one — the photon figures above are the separate question.
Half-life, specific activity and dose rate
| Half-life | 18.11 years (5.715e+8 s) |
| Decay mode | alpha decay |
| Specific activity | 2.99e+12 Bq/g (80.9 Ci/g) |
| Air kerma rate constant Γ (δ = 20 keV) | 0.00000336 mGy·m²/(GBq·h) |
| Dose rate, 1 GBq at 1 m | 0.00000336 mGy/h |
| Dose rate, 1 Ci at 1 m | 0.000124 mGy/h |
| Kerma-weighted mean photon energy | 51.35 keV |
42.8 keV carries 90% of the dose rate
1 further line below the 20 keV cutoff, the highest at 17.60 keV and 9.04% emission probability in all, is excluded here and from Γ. Why the two columns rank differently.
| Energy (keV) | Emission probability (%) | Share of dose rate (%) |
|---|---|---|
| 42.82 | 0.02635 | 90.05 |
| 152.63 | 0.00105 | 5.48 |
| 98.86 | 0.00142 | 4.46 |
0.0558 mm of lead halves this spectrum
Solved numerically across all 3 lines, narrow beam. Why not one representative energy.
| Material | HVL (mm) | TVL (mm) | TVL / HVL |
|---|---|---|---|
| lead | 0.0558 | 0.207 | 3.71 |
| tungsten | 0.0441 | 0.162 | 3.68 |
| iron | 0.335 | 1.47 | 4.40 |
| copper | 0.221 | 0.991 | 4.49 |
| concrete | 7.31 | 26.1 | 3.57 |
| water | 28.4 | 95.8 | 3.38 |
| aluminum | 5.66 | 20.5 | 3.63 |
A single energy would give 3.32. What a spread of energies does instead.
3 alpha lines, strongest 5.805 MeV
3 recorded lines from 5.664 to 5.805 MeV, the strongest 5.805 MeV at 76.9% of 100.0% total alpha emission.
| Energy (MeV) | Emission probability (%) |
|---|---|
| 5.8048 | 76.9 |
| 5.7626 | 23.1 |
| 5.6640 | 0.0204 |
Activity over decades and centuries
Ten half-lives is 181 years, which puts decay storage out of reach: 21.63% survives forty years. The mean life 1/λ, the quantity that enters an integrated dose, is 26.1 years.
| Elapsed | Fraction remaining |
|---|---|
| 1 half-life | 50.0 % |
| 2 half-lives | 25.0 % |
| 5 half-lives | 3.12 % |
| 10 half-lives | 0.0977 % |
| Time to fall to 10 % of today's activity | 60.2 years |
| Time to fall to 1 % | 120 years |
| Time to fall to 0.1 % | 180 years |
Limits — intake, not external dose
- 0.00000336 mGy/h at a metre — bare point source, no capsule, no self-absorption.
- 0.0558 mm of lead halves this spectrum, narrow beam, scatter not added back.
- Γ excludes 1 line under 20 keV, carrying 9.04% of all emissions.
- Alpha reaches nothing through skin — Cm-244 is an intake problem, not an external one.
- What every sheet leaves out, internal dose included.
Gamma and decay calculators for Cm-244
Other Curium nuclides: Cm-242, Cm-243, Cm-245, Cm-246
Computed from the IAEA Nuclear Data Section — Livechart API (ENSDF) and the NIST X-Ray Mass Attenuation Coefficients. Derivations and citations.