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17-Phys-B1 Radiation Physics · December 2016

Question 4 of 7: Inverse Compton Scattering — Generating 10 MeV Photons

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 4: Inverse Compton Scattering — Generating 10 MeV Photons (10 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.

Check: the source prints the comparison wavelength as "10 pm"; no laser operates at 10 picometres (that is a hard X-ray wavelength), while the real carbon-dioxide laser line is 10.6 μm — this is read as "10 μm" (micrometre), per the exam's own invitation to state assumptions. The form of equation (1) reproduced above is the one consistent with the printed $\lambda_0$ definition and with the simplified equation (2) the question itself supplies.

Given. $\lambda_0=2h/m_ec$; incident photon $\lambda_i=10\ \mu\text{m}$ (CO$_2$ laser); target final photon energy $E_f=10$ MeV; $m_ec^2=0.511$ MeV.

Find. (a) dimensional proof; (b) numeric comparison $\lambda_0$ vs. $\lambda_i$; (c) the condition for the approximation (2); (d) electron speed $v$; (e) total electron energy; (f) electron kinetic energy; (g) accelerating voltage.

Approach. Part (a)–(c) are dimensional/limiting-case analysis of the given formula. For (d)–(g), use the ultra-relativistic limit of equation (2) ($\lambda_f/\lambda_i=(1-\beta)/(1+\beta)\to1/4\gamma^2$ as $\beta\to1$) together with $E_f/E_i=\lambda_i/\lambda_f$ to solve for the Lorentz factor $\gamma$, then read off $v$, total energy, kinetic energy, and the equivalent accelerating voltage.

  1. Part (a) — dimensions of $\lambda_0=2h/m_ec$. $[h]=\text{J}\cdot\text{s} =\text{kg}\,\text{m}^2\text{s}^{-1}$, $[m_e]=\text{kg}$, $[c]=\text{m}\,\text{s}^{-1}$, so $$[\lambda_0] = \frac{\text{kg}\,\text{m}^2\text{s}^{-1}}{\text{kg}\cdot\text{m}\,\text{s}^{-1}} = \text{m}$$ $$\boxed{[\lambda_0]=\text{m} \ \ \text{(a length, consistent with a wavelength)}}$$
  2. Part (b) — numeric value of $\lambda_0$ vs. the CO$_2$ laser line. $$\lambda_0 = \frac{2h}{m_ec} = \frac{2(6.626\times10^{-34})}{(9.109\times10^{-31})(2.998\times10^{8})}$$ $$\boxed{\lambda_0 \approx 4.85\times10^{-12}\ \text{m} = 4.85\ \text{pm}}$$ Compared with the CO$_2$ laser's $\lambda_i=10\ \mu\text{m}=1\times10^{4}$ pm, $$\frac{\lambda_i}{\lambda_0} = \frac{10\ \mu\text{m}}{4.85\ \text{pm}} \approx 2.1\times10^{6}$$ i.e. $\lambda_0$ is about two million times smaller than the incident laser wavelength — utterly negligible by comparison.
  3. Part (c) — condition for the simplified equation (2). In equation (1), the $\lambda_0$ term is added directly to $\lambda$ (both multiplied by the same $(1-\beta)/(1+\beta)$ factor), so it can be dropped whenever $$\boxed{\lambda \gg \lambda_0 = 2h/m_ec}$$ i.e. whenever the incident photon's wavelength is much larger than the (fixed, $\sim$5 pm) Compton-like length scale $\lambda_0$. Part (b) shows this holds by six orders of magnitude for a CO$_2$-laser photon, which is exactly why the approximation (2) is safe to use for the rest of this question.
  4. Part (d) — electron velocity $v$ to generate 10 MeV photons. Using equation (2) and $E\propto1/\lambda$ (so $E_f/E_i=\lambda_i/\lambda_f$): $$\frac{E_f}{E_i} = \frac{\lambda_i}{\lambda_f} = \frac{1+\beta}{1-\beta}, \qquad \beta=v/c$$ The incident photon energy is $E_i=hc/\lambda_i=1240\ \text{eV}\cdot\text{nm}/10{,}000\ \text{nm} \approx0.124$ eV. For an ultra-relativistic electron ($\beta\to1$), $1-\beta\approx1/2\gamma^2$ and $1+\beta\approx2$, so $(1+\beta)/(1-\beta)\approx4\gamma^2$: $$4\gamma^2 \approx \frac{E_f}{E_i} = \frac{10\times10^{6}\ \text{eV}}{0.124\ \text{eV}} \approx 8.07\times10^{7}$$ $$\gamma \approx \sqrt{\frac{8.07\times10^7}{4}} \approx 4490$$ $$\beta = \sqrt{1-1/\gamma^2} \approx 0.99999998,\qquad \boxed{v = \beta c \approx 2.99792\times10^{8}\ \text{m/s}}$$ (the electron falls short of $c$ by only about 7.4 m/s — an extreme but physically ordinary regime, the same one used in real Compton-backscatter gamma-ray sources).
  5. Part (e) — total electron energy at $v$. $$E_{\text{tot}} = \gamma m_ec^2 = 4490\times0.511\ \text{MeV}$$ $$\boxed{E_{\text{tot}} \approx 2295\ \text{MeV} \approx 2.29\ \text{GeV}}$$
  6. Part (f) — kinetic energy at $v$. $$KE = (\gamma-1)m_ec^2 = E_{\text{tot}} - m_ec^2 = 2295 - 0.511$$ $$\boxed{KE \approx 2294\ \text{MeV}}$$ (the 0.511 MeV rest-mass energy is a negligible correction at this $\gamma$).
  7. Part (g) — accelerating voltage. An electron accelerated through potential difference $V$ gains kinetic energy $KE=eV$, so numerically $V$ in volts equals $KE$ in eV: $$\boxed{V = \frac{KE}{e} \approx 2.29\times10^{9}\ \text{V} = 2.29\ \text{GV}}$$ (in practice such an electron beam is built up over many accelerating stages, e.g. a linac or synchrotron, rather than a single 2.3 GV potential — the voltage quoted is the energy equivalent, not a literal single-gap design value).
Question 4 — results
PartResult
(a)$[\lambda_0]=\text{m}$
(b)$\lambda_0\approx4.85$ pm $\approx\lambda_i/(2.1\times10^6)$
(c)valid when $\lambda\gg\lambda_0$
(d) $v$$\approx2.99792\times10^8$ m/s ($\gamma\approx4490$)
(e) $E_{\text{tot}}$$\approx2295$ MeV
(f) $KE$$\approx2294$ MeV
(g) $V$$\approx2.29$ GV