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17-Phys-B1 Radiation Physics · December 2016

Question 1 of 7: Fukushima Cooling-Water Isotopes and Caesium's Effective Half-Life

Nivaar worked solution (AI-drafted; not reviewed by a licensed engineer)

Notes on this paper

Paper format. 98-Phys-B1 Radiation Physics, National Examination December 2016 — a three-hour open-book examination in which any non-communicating calculator is permitted (the candidate must record the calculator's make and model on the first sheet). The cover page states the exam has 7 questions worth a total of 87 points, of which only 80 points' worth need be answered for full marks; every question and sub-part is nonetheless answered in full below so the paper remains a complete study resource. The cover page's own marking-scheme summary (13+9+8+10+19+10+18 = 87) is internally consistent with the stated total. The cover page also invites the candidate to submit a written statement of any assumptions made where a question is open to interpretation — this licence is used below in Question 2 (ICRP-60 neutron weighting factors are assumed for the thermal/fast neutron energy brackets, since none are given explicitly), Question 4 (the source's printed comparison wavelength "10 pm" for a carbon-dioxide laser photon is read as the real CO2-laser wavelength, 10 μm, since no laser emits at 10 picometres), Question 5(f) (shield thicknesses are order-of-magnitude illustrative estimates, since the source gives no source strength/dose-rate target to size against), and Question 5(g) (the fission-energy-distribution percentages are standard textbook illustrative values, since the source gives no numeric data of its own to compute them from).

Reference texts. K. S. Krane, Introductory Nuclear Physics (nuclear reaction equations, fission energetics, mass–energy conservation); F. H. Attix, Introduction to Radiological Physics and Radiation Dosimetry (photon/EM interactions, non-ionizing radiation, shielding); J. R. Cember and T. E. Johnson, Introduction to Health Physics, 5th ed. (internal dosimetry, radiation weighting factors, MIRD absorbed-fraction formalism, ALARA); J. E. Turner, Atoms, Radiation, and Radiation Protection, 3rd ed. (neutron detection/shielding, Compton scattering, radiation protection tenets).

Question 1: Fukushima Cooling-Water Isotopes and Caesium's Effective Half-Life (13 marks)

Question text not reproduced: the examination questions are © Engineers and Geoscientists BC. Open the official past paper (linked at the top of this page) to read the question, then follow the worked solution below.

Given. Fukushima Daiichi is light-water cooled; discarded cooling water has been treated to remove caesium and strontium but not tritium; caesium's biological half-life $T_b=70$ days, physical half-life $T_p=30.17$ years.

Find. (a)–(f) qualitative explanations of isotope production, hazard and treatment choices; (g) the effective half-life $T_{\text{eff}}$ of caesium in the body.

Approach. Classify each isotope by its production mechanism (direct fission product vs. neutron-activation product), use each isotope's decay mode/half-life/chemical behaviour to identify the dominant hazard isotope and its removal difficulty, then combine biological and physical clearance in part (g) via the reciprocal-half-life rule.

  1. Part (a) — production mechanisms. Caesium (134Cs, 137Cs) and strontium (90Sr) are direct fission products: when a 235U nucleus splits, the two mid-mass fragments land in the mass regions around $A\approx90$–100 (Sr) and $A\approx134$–137 (Cs), either directly or after a short chain of $\beta^-$ decays from the primary (more neutron-rich) fragment. Tritium (3H), by contrast, is not a fission product of that mass region; in a light-water reactor it arises from (i) rare ternary fission (roughly 1 in $10^4$ fissions ejects a third light fragment, occasionally 3H), and (ii) neutron activation — $(n,\alpha)$ capture on trace 10B/6Li in control materials and coolant chemistry, and $(n,\gamma)$ capture on the small natural abundance of deuterium already present in ordinary water. Both routes make far less tritium than a heavy-water reactor, but the volumes of coolant and years of operation still accumulate a measurable inventory.
  2. Part (b) — isotope of caesium of greatest concern. 137Cs ($T_{1/2}=30.17$ y) is of most concern, not 134Cs ($T_{1/2}=2.06$ y). Its long physical half-life means it persists in the environment and in stored water for decades rather than decaying away within a few years; it is also a strong photon emitter (via its short-lived daughter 137mBa, 662 keV gamma) and, chemically, caesium behaves like potassium, so it is readily taken up and distributed through soft tissue if ingested.
  3. Part (c) — isotope of strontium of greatest concern. 90Sr ($T_{1/2}=28.8$ y) is of greatest concern. Strontium is chemically similar to calcium, so 90Sr is a classic "bone-seeker": once ingested it substitutes for calcium in bone mineral and is retained there for years, delivering a prolonged internal beta dose directly to the bone marrow — a far more damaging exposure pathway than a similarly-sized dose to soft tissue that clears quickly.
  4. Part (d) — why iodine is absent from the report. Radioiodine (131I, $T_{1/2}=8.02$ days) was indeed released in the accident, but by April 2016 — more than five years and over 200 physical half-lives after the March 2011 accident — its activity has decayed to a physically negligible fraction ($2^{-200}$) of its original value. There is simply no detectable 131I left to report in water stored and treated years later; its short half-life is precisely why it is an acute, not a long-term, hazard.
  5. Part (e) — why tritium survives the cleansing. The treatment system (ALPS, an ion-exchange/co-precipitation train) removes caesium and strontium because they exist as dissolved cations (Cs$^+$, Sr$^{2+}$) chemically distinct from the water molecule itself, so they can be captured on exchange resins. Tritium instead exists as tritiated water (HTO) — the tritium atom has replaced a hydrogen atom in the water molecule, so it is chemically indistinguishable from ordinary water. No conventional filtration or ion-exchange process can separate HTO from H$_2$O; only expensive, large-scale isotope separation (e.g. cryogenic distillation) could, which is impractical at the volume involved.
  6. Part (f) — tritium's hazard mechanism. 3H decays by $\beta^-$ emission (${}^{3}\text{H}\rightarrow{}^{3}\text{He}+\beta^-+\bar\nu$) with a very low average beta energy ($\sim$5.7 keV, 18.6 keV maximum) and a range in tissue of only tens of micrometres — too short to penetrate the skin's outer dead layer, so tritium poses essentially no external hazard. Its danger is entirely internal: because it is chemically identical to hydrogen, HTO is freely taken up by ingestion, inhalation or skin absorption and distributes through the body's water (∼60% of body mass), irradiating tissue from within at short range. Its 12.32-year physical half-life is long, but its biological half-life as body water ($\sim$10 days) is short, so a single intake clears relatively quickly — the real hazard from a leak like Fukushima's is chronic, repeated intake, not one large dose.
  7. Part (g) — effective half-life of caesium. The physical and biological clearance processes act in parallel, so their rate constants add: $$\frac{1}{T_{\text{eff}}} = \frac{1}{T_b} + \frac{1}{T_p}$$ Converting $T_p=30.17$ y to days ($30.17\times365.25=11{,}019.6$ d) and substituting $T_b=70$ d: $$\frac{1}{T_{\text{eff}}} = \frac{1}{70} + \frac{1}{11{,}019.6} = 0.014286 + 0.0000908 = 0.014376\ \text{d}^{-1}$$ $$\boxed{T_{\text{eff}} = \frac{1}{0.014376} \approx 69.6\ \text{days}}$$ Because $T_p\gg T_b$ here, $T_{\text{eff}}$ is dominated by (and lands close to, but slightly below) the biological half-life $T_b=70$ d — physically, the body clears caesium almost as fast as it would clear any chemically similar, non-radioactive tracer, since 30 years of physical decay barely registers over a 70-day biological residence.
Question 1 — results
PartResult
(a)Cs, Sr: direct fission products; H-3: ternary fission + neutron activation
(b)$^{137}$Cs (30.17 y, persistent, strong γ emitter, K-like uptake)
(c)$^{90}$Sr (28.8 y, bone-seeker, Ca-like uptake)
(d)$^{131}$I ($T_{1/2}=8$ d) has decayed away (>200 half-lives by 2016)
(e)Tritium is chemically part of the water molecule itself (HTO); ion-exchange cannot remove it
(f)Internal-only hazard: low-energy $\beta^-$, 12.32 yr physical / ∼10 d biological half-life
(g) $T_{\text{eff}}$$\approx 69.6$ days
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