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 2013 — a three-hour open-book examination in which any
non-communicating calculator is permitted. The cover page states that all seven
questions must be attempted (no choose-N-of-M here) for a total of 100 points, and
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(c) (the
photon-production law assumed for the current change) and Question 5(a) (the numeric value
behind the news item's "five times the acceptable exposure" claim).
Reference texts. K. S. Krane, Introductory Nuclear Physics
(nuclear masses and binding energy, radioactive decay, fission); F. H. Attix,
Introduction to Radiological Physics and Radiation Dosimetry (X-ray production and
bremsstrahlung spectra, photon interactions — photoelectric effect, Compton
scattering, pair production, gamma detectors); J. R. Cember and T. E. Johnson,
Introduction to Health Physics, 5th ed. (dose equivalent, internal dosimetry and
effective half-life, shielding, fission-product hazards); J. E. Turner, Atoms,
Radiation, and Radiation Protection, 3rd ed. (radiation interactions with matter,
health-physics standards).
Question 5: Radiation Safety and Standards (15 marks)
Given. $T_{1/2}({}^{90}\text{Sr})=29.1$ yr, decaying by $\beta^-$ to
${}^{90}$Y ($T_{1/2}=64$ h, then stable Zr); $T_{1/2}({}^{137}\text{Cs})=30$ yr, decaying by
$\beta^-/\gamma$ to ${}^{137m}$Ba; the "practically vanished" activity criterion (10
half-lives, activity down to $2^{-10}\approx0.098\%$ of its initial value) applied
consistently across (e)(i) and (f)(ii).
Find. (a) the numeric occupational dose implied by "5× the
acceptable exposure"; (e)(i) the time for ${}^{90}$Sr to practically vanish; (f)(ii) the
fraction of ${}^{137}$Cs remaining at that same elapsed time.
Approach. Use the standard annual occupational effective-dose limit as
the "acceptable exposure" baseline for (a); apply the standard 10-half-life "practically
vanished" convention to (e)(i), then apply that same elapsed time as the argument of
${}^{137}$Cs's own decay law for (f)(ii); answer the remaining conceptual sub-parts from
fission-product half-life/yield, chemistry-of-uptake, and gamma-vs-beta detectability
arguments.
Part (a) — the implied dose value. The commonly cited annual
occupational effective-dose limit for nuclear workers is $\approx 20$ mSv/year (the ICRP recommendation, averaged over five years; in Canada the CNSC limit for a Nuclear
Energy Worker is 50 mSv in any one year and 100 mSv over a five-year dosimetry period, i.e.
the same 20 mSv/yr average); five times that
figure is
$$\boxed{5 \times 20\text{ mSv} = 100\text{ mSv (in one hour, at the point measured)}}$$
consistent with contemporaneous reporting of the actual Fukushima measurement.
Part (b) — why Sr-90 and Cs-137 are named. Among the hundreds of
fission products, ${}^{90}$Sr and ${}^{137}$Cs stand out because they combine a
moderate half-life (29.1 and 30 years respectively) — long enough to persist
in the environment for decades, short enough to carry substantial activity per unit mass
(specific activity $\propto 1/T_{1/2}$) — with a relatively high fission yield
and problematic biochemistry (Sr mimics calcium, Cs mimics potassium, so both are readily
taken up biologically). Fission products with much shorter half-lives decay away within
days to weeks of an accident; those with much longer half-lives (like ${}^{129}$I) have such
low specific activity that they contribute comparatively little dose rate per becquerel of
mass present.
Part (c) — why ${}^{129}$I and ${}^{131}$I are absent from the report.
${}^{131}$I has a short 8-day half-life, so by August 2013 — roughly 2.5 years (over 110
half-lives) after the March 2011 accident — essentially none of the originally
released ${}^{131}$I remains; it is simply gone. ${}^{129}$I, conversely, has an enormously long
half-life ($\approx 1.57\times10^7$ years), so even though some inventory remains, its
specific activity (Bq per gram) is minuscule, contributing negligible dose rate compared to
the moderate-half-life ${}^{90}$Sr and ${}^{137}$Cs highlighted in the report.
Part (d) — source of tritium. Tritium ($^3$H) is not itself a
fission product in significant yield, but reactors produce it two ways: (i)
ternary fission, in which roughly 1 in every $10^4$ fission events splits
into three fragments rather than two, occasionally yielding a light nucleus such as
tritium directly, and (ii) neutron activation of light nuclides present in
the coolant or control materials — for example ${}^{10}\text{B}(n,2\alpha)^3\text{H}$
from boron used in control/shutdown systems, or $^6\text{Li}(n,\alpha)^3\text{H}$ where
lithium is present, plus ${}^2\text{H}(n,\gamma)^3\text{H}$ capture on the deuterium
naturally present in the cooling water itself. All of these mechanisms operate continuously during reactor operation, so
tritium accumulates in reactor water independent of any fresh fission-product release.
Part (e)(i) — time for ${}^{90}$Sr to practically vanish. Using the
standard "practically gone" convention of 10 half-lives (activity down to
$2^{-10}\approx0.098\%$):
$$\boxed{t = 10 \times T_{1/2}({}^{90}\text{Sr}) = 10 \times 29.1 = 291\text{ years}}$$
Part (e)(ii) — why ${}^{90}$Sr is still a hazard. The soil-shielding
argument only removes the external beta hazard. ${}^{90}$Sr is chemically almost
identical to calcium, so plants and animals take it up through the food chain and deposit it
in bone (a "bone-seeker"), exactly where calcium goes. Once incorporated, its beta particles
(and its daughter ${}^{90}$Y's, which are even more energetic) are emitted inside the
body, directly irradiating adjacent bone marrow at short range with no soil, skin, or
clothing to stop them — making ${}^{90}$Sr predominantly an internal
(ingestion) radiological hazard rather than an external one.
Part (f)(i) — validity of the whole-body-counting statement.Valid. Whole-body counters detect gamma rays escaping the body from
outside; ${}^{137}$Cs's daughter ${}^{137m}$Ba emits a strong, easily detected 662 keV gamma, so
whole-body Cs-137 burdens are readily quantified externally. ${}^{90}$Sr and its daughter
${}^{90}$Y are essentially pure beta emitters with no significant gamma line,
and beta particles cannot escape the body to reach an external detector — whole-body
(gamma) counting is blind to ${}^{90}$Sr, which instead requires bioassay methods (urine or
fecal sampling) to quantify.
Part (f)(ii) — remaining ${}^{137}$Cs after 291 years. Applying
${}^{137}$Cs's own decay law over the same 291-year interval found in (e)(i):
$$n_{\text{half-lives}} = \frac{291}{30} = 9.7, \qquad
\text{fraction remaining} = 2^{-9.7}$$
$$\boxed{\text{fraction remaining} = 2^{-9.7} \approx 1.20\times10^{-3} \approx 0.12\%}$$
Roughly one part in 830 of the original ${}^{137}$Cs activity is still present — small,
but not yet at the same "practically vanished" threshold as ${}^{90}$Sr, since ${}^{137}$Cs's
half-life is marginally longer.
Question 5 — results
Quantity
Value
(a) Implied dose value
≈ 100 mSv (5 × 20 mSv/yr occupational limit)
(e)(i) Time for ${}^{90}$Sr to practically vanish
291 years (10 half-lives)
(f)(ii) ${}^{137}$Cs fraction remaining at t = 291 yr