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Beyond one million years: The intrinsic radiation hazard of high-level nuclear wastes Cover

Beyond one million years: The intrinsic radiation hazard of high-level nuclear wastes

Open Access
|Nov 2024

Figures & Tables

Fig. 1.

Radioactive decay over time of spent CANDU fuel upon discharge from the reactor. It uses natural uranium in comparison and shows that it will take up to 10 million years before the spent fuel goes back to the same overall radioactivity levels as the original ore equivalent. The same chart can be applied qualitatively to any kind of uranium-based SF.

Fig. 2.

Decay of VHLW from reprocessing of 1 ton of spent fuel [4].

Fig. 3.

Radiological dose rate in Sv/h from two French HLW drill cores. C2 is VHLW; CU1 is SF (p. 25 in Ref. [2] and p. 533 in Ref. [7]).

Fig. 4.

Accrued, external dose from drill cores of several kinds of present and future French VHLW after a 10-min exposure, 40 cm from the drill core, and as a function of time [9].

Table 1.

Gamma dose rate (mSv/h) at three distances from a POLLUX-8 cask loaded with 8 UO2 fuel assemblies, neglecting the shielding of the cask

Decay time (million years)Next to surface (4 cm)40 cm (extrapolated)10 m
16.560.6970.0279
102.770.2900.0116
1002.680.2820.0113
10002.310.2430.00974
Table 2a.

Main contributors to the gamma dose rate from SF as a function of time 4 in million years for the configuration of Table 1. The (4n + 2) elements are denoted in bold and the (4n + 1) elements are denoted in italics

0.1 My1 My10 My100 My1000 My
Bi-214Bi-214Bi-214Bi-214Bi-214
Sb-126mPa-233Pb-214Pb-214Pb-214
Pb-214Th-229Pa-234mPa-234mPa-234m
Pa-233Bi-213Pa-233Bi-210Bi-210
Sb-126Pb-214Th-229U-235Th-234
Th-229Tl-209Bi-213Ra-223
Np-237Np-237Bi-210
Bi-213Fr-221U-235
Bi-210Ac-225Ra-223
Tl-209Ra-225Tl-209

4 The original calculations were based on LWR fuel but, for the past 105 years, say, they apply to any U-fuel, as the differences among uranium fuel types smooth out.

Table 2b.

Highest gamma energies in the (4n + 2) and (4n + 1) chains. The weighted averages values are based on the data obtained from Japan Atomic Energy Agency [15,16,17,18]

RadionuclideWeighted average gamma energy per emission (keV)
Bi-214944.00
Pb-214318.38
Pa-233311.86
Th-22947.96
Table 3.

Relative contributions from the three actinide chains to the gamma dose from a block of unshielded eight UO2 fuel assemblies (same assemblies as mentioned in Table 1)

Decay time (million years)U-238 chain (%)Np-237 chain (%)Excess U-234 chain (%)Total, surface dose rate (mSv/h)
141.1232.1026.786.56
262.4135.162.414.32
477.2822.713.49
692.317.692.92
895.734.272.81
1096.293.722.77
1498.861.142.72
2099.830.172.69
1001002.68
10001002.31
Table 4.

Exposure time in hours for getting the annual ICRP dose constraint of 0.3 mSv as a function of time at three distances from POLLUX-8 cask assemblies, neglecting the shielding of the cask

Decay time (million years)Exposure (h) at contactExposure (h) at 40 cmExposure (h) at 10 m
10.0460.43010.8
100.1081.03425.9
1000.1121.06426.6
10000.1301.23430.8
Table 5.

Elemental activity ratios (at 10 000 years) and chain activity ratios (at one million years) for French VHLW

Time (years)Np-237/(U-234 + U-238)Np-237/U-238U-234/U-238
10 000576.7319 220.6232.34
1 000 0004672.9313 896.101.97
Fig. 5.

The dose rate 2 cm away from the full-size C2 VHLW cylinder as a function of time (source: ANDRA).

Table A1.1.

Density and HVL for various materials depending on the energy of the gamma rays

MaterialDensity (g/cm3)HVL (cm) for 0.3 MeVHVL (cm) for 0.6 MeVHVL (cm) for 1.0 MeVHVL (cm) for 1.5 MeV
Concrete2.32.084.026.697.70
R7T7 glass2.62.224.105.926.50
UO210.970.260.490.791.33
Table A1.2.

Transmission factors for energies 0.944 MeV and 0.312 MeV in R7T7 glass waste forms of radii 21 cm and 5 cm

Energy (MeV)Cylinder radius (cm)HVL (cm)Transmission factor (%)
0.944213.7578.53
0.312211.5760.28
0.94453.75756.80
0.31251.57627.90
Table A2.1.

Dose rate computation coefficients for the German spent fuel of Table 1

Ai (mSv/h)λi (1/106 years)
U-2382.6971.55 × 10−4
Np-2372.9100.324
U-23429.6702.820
DOI: https://doi.org/10.2478/nuka-2024-0029 | Journal eISSN: 1508-5791 (formerly 0029-5922) | Journal ISSN: 0029-5922
Language: English
Page range: 215 - 224
Submitted on: Jul 24, 2024
Accepted on: Sep 23, 2024
Published on: Nov 20, 2024
Published by: Institute of Nuclear Chemistry and Technology
In partnership with: Paradigm Publishing Services
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© 2024 Claudio Pescatore, published by Institute of Nuclear Chemistry and Technology
This work is licensed under the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 License.