The following milestones were defined to keep track on the experiment progress and define the products of the experiment.
Milestones:
M1 (Q1 2018): Finalise design
M2 (Q1 2019): experiment emplaced and non-active circulation started
M3 (Q1 2020): start of circulation of radionuclides
M4 (Q1 2022): Decision to overcore and distribute samples to laboratories or to continue circulation
M5 (End 2022): end of the first phase of the CIM project
Figure 3: Current project organisation- Organisation
The working programme comprises of the following steps:
Step 1: Finalise experimental design
Step 2: Drill needed boreholes and install initial condition monitoring
Step 3: Develop and construct the experimental equipment (packer system, surface equipment)
Step 4: Emplace circulation interval
Step 5: Start circulation and monitoring
Step 6: Overcore and post-mortem analysis
The project relies largely on experience acquired with previous projects using radionuclides at GTS (LTD, CFM) and will benefit from the lessons learned of these projects with respect to borehole and surface equipment and sampling.
Table 1: Isotopes (radioactive and stable) foreseen for the circulation in the CIM experiment.
Isotope | Species |
C-14 | Formate HCOO- |
I-129 | Iodide I- |
H-3 | HTO |
Cl-36 | Cl- |
Cs-134 | Cs+ |
Ba-133 | Ba2+ |
Four vertical or slightly inclined boreholes resulting from the overcoring of the HPF experiment at GTS have been backfilled with OPC mortar in 2004 (Figure 2).
One of these boreholes is being used as circulation borehole for the CIM experiment. The borehole and the depth of the circulation interval was selected in order to position the latter in an area of dense matrix with no distinct water conducting features. The selection was based on available geological logs from the HPF project. Three monitoring boreholes were drilled at short distance (ca 15 cm) from the source borehole.
Figure 1: Setup of the circulation in a sub-vertical borehole
Figure 2: Schematic 3D view of the HPF and planned CIM borehole relative to the AU-126 shear zone and AU tunnel at the GTS
Carbon-14 and Iodine-129 released from repositories of L/ILW and TRU wastes typically contribute most to dose rates over the long-term (i.e. 10 ka to 100 ka) according to performance assessment (PA) calculations. This is primarily due to the combination of (i) high solubility and (ii) low sorption properties of the chemical forms that the two radionuclides are expected to exist in. In the case of C-14, experimental work on the speciation of carbon during corrosion of activated and un-activated steel under anoxic conditions similar to that of an emplacement tunnel showed the formation of oxygenated and reduced hydrocarbons, including carboxylic acids and CH4.
Methane is not expected to react with cementitious material or with the host rock. Uncertainties remain, however, on the retardation of carboxylic acids in clay and cementitious materials. In the case of formic acid, so far no retardation was expected in near-neutral environments; however laboratory experiments at PSI showed evidence of weak sorption of formic acid on cementitious material.
I-129 originates largely from reprocessed waste and is expected to occur mostly as iodide. Although it is planned that large amounts of cementitious material will be used in L/ILW and TRU waste repositories, there remains much uncertainty on both the release and in-situ retardation of I-129 as well as C-14 species in cementitious materials, especially in naturally aged cement on the field scale.
The following aims were developed based on the wishes from the current partners (NUMO, RWM, SURAO and Nagra):
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