Issue |
EPJ Nuclear Sci. Technol.
Volume 2, 2016
|
|
---|---|---|
Article Number | 31 | |
Number of page(s) | 6 | |
DOI | https://doi.org/10.1051/epjn/2016024 | |
Published online | 17 June 2016 |
https://doi.org/10.1051/epjn/2016024
Regular Article
Dose and temperature distribution in spent fuel containing material
1 Research Centre Řež, Ltd., Hlavní 130, 250 68 Řež near Prague, Czech Republic
2 ÚJV Řež, a.s., Hlavní 130, 250 68 Řež near Prague, Czech Republic
⁎ e-mail: ladislav.viererbl@cvrez.cz, vie@cvrez.cz
Received:
13
October
2015
Accepted:
31
May
2016
Published online: 17 June 2016
Spent fuel containing material (SFCM) can arise during severe nuclear reactor accident by melting of a reactor core and surrounding material (corium) or during accident in spent fuel storage. It consists of nuclear fuel, fission products, activation products and materials from fuel cladding, concrete, etc. The paper deals with dose and temperature characteristics inside the SFCM after transition of the molten mixture to solid state. Calculations were made on simplified spherical models, without connection to some specific nuclear accident. The dose rate was estimated for alpha, beta and gamma radiation in times over the course of 30 years from the end of the fission chain reaction. Concentration of helium generated in the material by alpha decay was calculated. For the dose rate values estimation, computation code ORIGEN 2.2 with dosimetric library ENDF/B-IV were used. Temperature distribution inside the solid SFCM was calculated by FLUENT code. As source of heating, energy of radioactive decays was taken. Estimated dose and temperature characteristics can be used, e.g. for evaluation of radiation damage and temperature behaviour of SFCM or for radiation test design of corium simulating materials.
© L. Viererbl et al., published by EDP Sciences, 2016
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
1 Introduction
Spent fuel containing material (SFCM) can arise during severe nuclear reactor accident by melting of a reactor core and surrounding material (it is called corium in this case) or during accident in spent fuel storage. It consists of nuclear fuel, fission products, activation products and materials from fuel control rods, fuel cladding, concrete and other structural material [1]. Other compounds arise from products of their chemical reaction with air and water. The molten reactor core can release volatile elements and compounds. After a reactor or spent fuel storage accident, SFCM remains in a molten phase for some time, mainly due to fission products decay heating. When this heating decreases and/or cooling is applied, the SFCM changes to a solid state. The composition of SFCM at the time of solidification depends on reactor type, the nature of the accident, and many other factors.
This paper deals with dose characteristics inside the SFCM after transition of the molten mixture to a solid state. For calculations, simplified models of SFCM were used. The purpose of the calculation is not to describe some specific nuclear accident but estimated dose and temperature characteristics can be used, e.g. for evaluation of radiation damage and temperature behaviour of SFCM or for radiation test design of corium simulating materials [2].
2 Time dependence of dose rate and helium generation in SFCM
2.1 Calculation model
In the real event, SFCM composition, shape and dimensions could vary from case to case. For time dependence of dose rate calculations, a simplified model with the following assumptions was used:
- –
the SFCM is homogenous;
- –
the dose is equal to the decay energy (without neutrinos) released in unit mass (more details in Sect. 3);
- –
the dose rate is produced by alpha, beta and gamma radiation (contributions for example from neutrons and fission fragments are neglected);
- –
10% of SFCM mass is uranium with fission and activation products created during irradiation. Uranium enrichment was 4.5% before fission. The remaining 90% is some “passive” material, e.g. Fe, SiO2. For this part of the calculation, the precise content is not important;
- –
uranium was irradiated in four reactor cycles per year as follows: 25% of the uranium was irradiated with neutrons for one year, 25% for two years, 25% for three years and 25% for four years. This corresponds to a situation where every year 25% of the fuel is changed and the end of chain fission (time of accident) is end of a reactor cycle;
- –
neutron fluence and spectrum of irradiation agree with PWR type reactors.
Dose rate, dose and helium production values are given for 10% uranium content. For other content levels, the values can be simply recalculated because in this simplified model they are proportional to uranium content.
2.2 Radionuclide activities
For radionuclide activities estimation, computation code ORIGEN 2.2 [3] with dosimetric library ENDF/B-IV was used. ORIGEN is a computer code system for calculating the build-up, decay, and processing of radioactive materials. ORIGEN 2.2 is a revised version that incorporates updates of reactor models, cross-sections, fission product yields, and decay data. This, not the newest version, was chosen for his simplicity of result outputs and sufficient precision for the given estimation.
Calculations were performed for 23 time points from 0 to 109 s (32 years) after end of chain fission. Activities for about 1000 fission product radionuclides and 100 actinide radionuclides were calculated using the assumptions in Section 2.1. As an example, Table 1 provides a list of more important radionuclides in SFCM.
The most active fission products and actinide radionuclides ordered by mass activity for a time of 107 s (116 days) after end of chain fission in SFCM.
2.3 Dose rate
For dose rate calculations, 89 fission products and 17 actinide radionuclides were chosen. The selection was made according to activities at different time points. Radionuclides (elements) with a boiling point of less than 200 °C were not used due to supposed evaporation.
For selected radionuclides, energy released per decay was determined as the sum of products of Energy × Intensity of the lines for alpha, beta and/or gamma radiation (including X-radiation) using NuDat [4] and Nucleonica [5] databases. By multiplying by activity and summing over selected radionuclides, final dose rates were given (Fig. 1). Absorbed doses can be obtained by integration of dose rates. Doses were calculated from a time of 100 s after the end of chain fission (Fig. 2). From these values, doses for chosen time interval can be obtained. For example, the total absorbed dose from all radiation types from 104 s to 108 s (2.8 hours to 3.2 years) is equal to 1.5 × 108 Gy.
Fig. 1 Time dependences of dose rates for alpha, beta and gamma radiation in SFCM. |
Fig. 2 Time dependences of doses in SFCM calculated from time of 100 s after the end of chain fission. |
2.4 Helium production
Similarly as for dose rates, helium production was calculated from the count rate of alpha particles generated in alpha decays of actinides. Alpha particles make consecutively helium atoms. The count rate has similar shape as alpha dose rate. Integral count of helium atoms generated in unit mass of SFCM is in Figure 3.
With similar calculation as for dose, e.g. from 104 s to 108 s number of helium atoms generated in 1 kg of SFCM would be 6 × 1018 atoms/kg.
The total uncertainty of the calculated values of dose rates, doses and helium concentration was estimated to be from 10 to 30%, depending on the type of radiation, quantity, etc.
Fig. 3 Time dependence of helium atoms generated in SFCM from a time of 100 s after end of chain fission. |
3 Spatial distribution of dose rate in SFCM
3.1 Calculation model
In Section 2 it was assumed that the dose is equal to the decay energy released from a unit mass, i.e. released energy is in equilibrium with absorbed energy. In other words, it was assumed that the SFCM has infinite dimensions. This is quite true for the inner part of an object that is large in comparison with the particle range in the material. For alpha particles, the typical range is in tens of μm and for beta particle less than one cm in SFCM. For gamma radiation, the typical half-value shield thickness is a few cm depending on radiation energy and SFCM composition. Gamma radiation is then most interesting with regards to the spatial distribution of dose rate. To illustrate this complex aspect, a few simple model examples were calculated.
Simplified models with following the assumptions were used for the calculations:
- (a)
the SFCM is homogenous;
- (b)
10% of the mass is uranium and the remaining 90% is SiO2;
- (c)
a spherical shape;
- (d)
the dose rate is produced by a homogenous monoenergetic gamma radiation source.
MCNP(X) [6] computer code with ENDF/B-VII.0 nuclear data library was used for calculation. The absorbed dose was computed using Type 3 mesh mode (energy absorption in volume) for spheres of diameters 6, 10, 30, 60, and 100 cm. Source energies of 300 keV, 661 keV, and 3000 keV were also considered. These energies cover the possible range of emission energies of real isotopes.
3.2 Results
Spatial distributions of relative dose rates in SFCM for different energies and different diameters are shown in Figures 4 and 5. Relative values are normalized to released energy in a mass unit, i.e. 100% corresponds to values used in Section 2.
The results confirm that assumption (b) in Section 2 (decay energy = absorbed energy) is a good approximation for material dimensions above tens of centimetres even in case of high gamma energies. Uncertainty of the calculated values in this section for given assumptions was estimated to be 5%.
Fig. 4 Spatial distribution of relative dose rate for gamma energy of 300 keV and different SFCM sphere diameters d. |
Fig. 5 Spatial distribution of relative dose rate for gamma energy of 3000 keV and different SFCM sphere diameters d. |
4 Temperature distribution in the SFCM
4.1 Calculation model
To estimate the temperature field inside the SFCM, a simplified model was chosen with a homogenous spherical shape. The energy source was radiation heating taken from the dose rate calculation in Section 2. Perfect cooling was presumed on the sphere's surface. Geometry and calculation nets were created using GAMBIT 2.4.6 code, and thermal calculations were performed using ANSYS FLUENT 12 code [7] with some simplified assumptions.
A series of temperature distribution calculations in the SFCM sphere was performed, where the four variable input parameters were sphere surface temperature TS, sphere radius R, specific heat Q, and SFCM material (the effect of spent fuel with radionuclides in the SFCM on thermal parameters was neglected). Table 2 shows the various parameter values considered. Specific heat values were derived from dose rates in the SFCM (see Sect. 2.2) at different times after the end of the fission chain reaction (Tab. 3). Baseline values were chosen as follows (bold values in Tab. 2): TS = 20 °C, R = 50 cm, Q = 3.41 W/kg, and ZrO2 material. During each calculation, only one of the parameters was varied from baseline values.
Parameter variants for calculation.
Specific radiation heat versus times t after the end of the fission chain reaction.
4.2 Results
Figure 6 shows the calculated temperature distribution in the SFCM sphere for the baseline variant. Naturally, the distribution is spherically symmetrical with the maximum temperature TC in the sphere's centre. The distribution shape is similar for different variants and varies mainly in the temperature difference ΔT between the sphere's centre and the sphere's surface, ΔT = TC − TS. This value is therefore given as the only parameter characterizing the temperature distribution for a variant. Then, for example for the baseline variant with surface temperature TS = 20 °C and centre temperature TC = 424 °C, the difference ΔT = 404 K. For varying surface temperature TS, a constant difference ΔT is used for calculation approximation. Thus for example for TS = 120 °C, we would have TC = 524 °C (R, Q and material as in the baseline variant). For values of ΔT for varying R, Q, and material, see Tables 4–6. When temperatures obtained by simplifying formal calculations are above the material's melting point, the values are given in brackets.
Fig. 6 Temperature distribution in the sphere for the baseline variant. TS = 20 °C, R = 50 cm, Q = 3.41 W/kg and ZrO2 material. |
Temperature difference for varying sphere radius R.
Temperature difference for varying specific heat Q.
Temperature difference for varying materials.
5 Discussion and conclusion
The estimated calculation uncertainties in dosimetry parameters for spent fuel containing material (up to 30% in Sect. 2 and 5% in Sect. 3) are sufficient because uncertainties in composition and other SFCM parameters would in reality be much greater. Thermal calculations confirmed that due to radiation heating, temperature inside a larger SFCM volume may reach relatively high values even if the SFCM surface is cooled intensively. These results can help to explain corium behaviour during cooling.
Estimated absorbed dose characteristics can be used to evaluate radiation damage and temperature behaviour of SFCM. These dose values can be also used for radiation test design of corium simulating materials. The typical total dose absorbed in the material over a few years after the end of chain fission was estimated on the order of 108 Gy. This dose can be achieved with irradiation in a middle power research reactor over 1–100 days, depending on proximity to the reactor core and other irradiation conditions. The results were used for radiation tests design with corium simulating materials, which were made in LVR-15 research reactor and which are described in reference [2].
Acknowledgments
This work was performed within the scope of research project LH12224, KONTAKT II, the Ministry of Education, Youth and Sports.
References
- C. Journeau, P. Piluso, K.N. Frolov, Corium physical properties for severe accident, R&D, in Proceedings of ICAPP’04, Pittsburgh, PA, USA, June 13–17, 2004 (2004), Paper 4140 [Google Scholar]
- Z. Lahodová, L. Viererbl, M. Vinš, A. Voljanskij, M. Kiselová, Irradiation of materials intended for chemical and thermal stabilization of molten nuclear fuel, in TopFuel 2015 Conference, Zurich, Switzerland, September 13–17, 2015 (2015) [Google Scholar]
- ORIGEN 2.2, RSICC Computer Code Collection, Oak Ridge National Laboratory, 2002 [Google Scholar]
- NuDat, National Nuclear Data Centre, 1997 [Google Scholar]
- Nucleonica GmbH, Nucleonica Nuclear Science Portal (www.nucleonica.com), Version 3.0.11, Karlsruhe, 2014 [Google Scholar]
- MCNPX user manual, Version 2.7.0, LA-CP-11-00438, 2011 [Google Scholar]
- ANSYS FLUENT 12.0 Theory Guide, ANSYS, Inc., 2009 [Google Scholar]
Cite this article as: Ladislav Viererbl, Zdena Lahodová, Jelena Zmítková, Miroslav Vinš, Jiří Šrank, Dose and temperature distribution in spent fuel containing material, EPJ Nuclear Sci. Technol. 2, 31 (2016)
All Tables
The most active fission products and actinide radionuclides ordered by mass activity for a time of 107 s (116 days) after end of chain fission in SFCM.
Specific radiation heat versus times t after the end of the fission chain reaction.
All Figures
Fig. 1 Time dependences of dose rates for alpha, beta and gamma radiation in SFCM. |
|
In the text |
Fig. 2 Time dependences of doses in SFCM calculated from time of 100 s after the end of chain fission. |
|
In the text |
Fig. 3 Time dependence of helium atoms generated in SFCM from a time of 100 s after end of chain fission. |
|
In the text |
Fig. 4 Spatial distribution of relative dose rate for gamma energy of 300 keV and different SFCM sphere diameters d. |
|
In the text |
Fig. 5 Spatial distribution of relative dose rate for gamma energy of 3000 keV and different SFCM sphere diameters d. |
|
In the text |
Fig. 6 Temperature distribution in the sphere for the baseline variant. TS = 20 °C, R = 50 cm, Q = 3.41 W/kg and ZrO2 material. |
|
In the text |
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