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Interaction of Electromagnetic Radiation and Charged Particles with Matter

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The Physics of Nuclear Reactors

Abstract

All nuclear reactions are associated with the emission of radiation. This radiation contributes in part to the release of nuclear energy by interacting with materials in the reactor core, and more generally, poses problems of radioprotection. Similarly, a large number of particles is created during operation of the reactor, in particular, charged particles such as α particles, as well as electrons and positrons as a result of β radioactivity. All of these particles interact with matter and release energy that contributes to the thermal balance of the pile. They also pose radioprotection problems for staff and can damage the reactor structures through the cumulative effects of collision. In this chapter, we examine the fundamentals needed to understand the phenomena of interaction between charged particles and matter.

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Notes

  1. 1.

    Concerning polarization, see (Filippi 1965, p. 101) and the work of the French physicist Etienne Malus (1808).

  2. 2.

    An illustration is provided by way of the x-ray applications used by the Department of Military Applications of CEA described in the journal CHOCS No 9 (December 1993). For the technical aspect of sensors, see Samueli et al. (1968).

  3. 3.

    Heinrich Rudolf Hertz (1857–1894) was a German physicist known for his work on electromagnetic radiation, including light. Born into a comfortably-off family in Hamburg, at the age of 6 years he entered the demanding School of Dr. Richard Lange. In 1872, he entered the prestigious Johanneum Gymnasium and obtained the Abitur in 1875. He then entered a construction engineering school but after reflection, signed up in for the University of Munich, where his mathematics teacher, Von Jolly, introduced him to the rigor of mathematics. He then studied under Von Helmholtz and de Kirchhoff in Berlin. Thanks to Von Helmholtz’s training, he was awarded the gold medal of the Faculty of Philosophy for a study on electrical inertia. He defended his thesis on electrical induction: Über die induction in rotirenden kugeln (On the induction of rotating balls) in February 1880. He analyzed the problem of contact between two elastically and linearly deformable balls, a problem known as Hertzian contact stress. He then worked for 3 years as assistant to Von Helmholtz. He obtained a teaching position in Kiel for 2 years, after which he moved to Karlsruhe to become the assistant of future Nobel prizewinner, Karl Ferdinand Braun, and it was here that he carried out studies to verify that light is indeed a form of electromagnetic radiation. On November 13, 1886, he created the first wireless link using electromagnetic radiation produced by an oscillator and showed that these waves also travel at the speed of light. In 1887, he turned his attention to the photoelectric effect discovered empirically by Antoine Becquerel, but he is rightly considered to be the principal investigator in this field. These experiments, then those of his assistant, Wilhelm Hallwachs, are central to Einstein’s theory of quanta of light and that of the photoelectric effect (initially known as the Hallwachs effekt). He died at a mere 37 years through septicemia that was doubtless caused by recurrent mastoiditis, before he had time to understand the significance of his experimental discoveries [Sources: article by R. Haidar in Photoniques No 56, pp. 21–23 (2011), “Heinrich Hertz, a Short Life” by Charles Susskind, San Francisco Press (1995)] (Public domain and the Marguet collection).

    Heinrich Hertz

  4. 4.

    The term “photon” is derived from the Greek word for light. It was first used in 1926 by chemist Gilbert N. Lewis (1875–1946) in a theory. Although the theory was not confirmed, the term itself was immediately adopted by the scientific community.

  5. 5.

    William Henry Bragg was the father of William Laurence Bragg , cited earlier, with whom he shared the 1915 Nobel Prize in Physics “for their services in the analysis of crystal structure by means of X-rays.

  6. 6.

    Arthur Holly Compton (1892–1962) was an American physicist who obtained his doctorate in physics from the University of Princeton in 1916. He worked and taught at various universities, including Chicago (1923–1945), then Saint-Louis (1945–1961). His experimental and theoretical work on x-rays was considerable, earning him the 1927 Nobel Prize in Physics for discovery of the effect that bears his name.

    figure e

    (the Marguet collection)

  7. 7.

    There is an amusing anecdote about the fine structure constant. A journalist was interviewing Enrico Fermi one day and wished to take a photograph of the Master. In order to make the pose more credible, he asked Fermi to pretend to be writing an equation on the blackboard. Fermi played along graciously, but feeling uninspired, he wrote the formula for fine structure with the numerator and the nominator reversed and he mischievously mixed up the units α =  2/ec ! The picture incorporated this error in backstage, and we see Fermi smiling and drawing a vague geometric figure in which he inserts angle θ where he fancies, and clearly visible on the blackboard above his head sits the erroneous formula. That would have been fine, except that the United States Post Office later decided to create a stamp using this very photo in honor of Fermi after his death. The mistake was spotted too late and the stamp was issued. In a panic, the image on the stamp was corrected in order to limit the damage. As Rutherford famously quipped: “All science is either physics or stamp collecting”.

    The historic photo on the left (Public domain) and the US postal stamp containing the error issued in 2001 on the right (The Marguet collection).

  8. 8.

    This methodology was used in the GRACE code for the calculation of the attenuation of photons and the heating of the surrounding shielding of reactors, coded in Fortran on IBM 709 in 1959 by D.S. Duncan and A.B. Speir (Atomics International).

  9. 9.

    Y. Sakamoto, S.I. Tanaka, Interpolation of gamma-ray build-up factors for point isotropic source with respect to atomic number, Nuclear Science and Engineering, 100, p. 33–42 (1988).

  10. 10.

    A. Assad , M. Chiron , J.C. Nimal , C. Diop , P. Ridoux : A new approximating formula for calculating gamma-ray buildup factors for multilayer shields, Nuclear Science and Engineering, 132, p. 203–216 (1999).

  11. 11.

    Thanks to the work of Andréas Schumm (EDF/R&D) on the MODERATO code.

  12. 12.

    On photoneutron cross sections, see: Rudy Lee Van Hemert : Threshold Phtoneutron Cross sections for light nuclei, PhD, University of California, 1968.

  13. 13.

    L.V. Spencer : Energy dissipation by fast electrons, National Bureau of Standards, USA, 1959.

  14. 14.

    O. Blunck, K. Westphal: ”Zum energieverlust enrigiereicher elektronen in dünnen schichten” Zeitung Physik 130, p. 641 (1951).

  15. 15.

    Patrick Maynard Stuart Blackett (1897–1974) spent a great deal of time working on the characterization of cosmic rays and he was awarded the Nobel Prize for his work in 1948. After completing his studies at Cambridge in 1921, he conducted many experiments. He became President of the Royal Society in 1965, and was made a baron in 1965.

  16. 16.

    Russian physicist Pavel Cherenkov (1904–1990), who won the Nobel prize in Physics in 1958, together with I. Tamm and I. Franck for their physical explanation of the Cherenkov effect.

    Lucien Mallet (1885–1981) was one of the first radiologists in France. In particular, he developed radiotherapy in the field of cancer, going on to write a book on the subject: Les applications biologiques des corps radioactifs artificiels [Biological applications of artificial radioactive bodies]. In 1921, he worked with Dr. Robert Proust of the Hôpital Tenon in Paris on the development of a treatment for certain cancers involving radiotherapy. In 1926, he described the luminous radiation produced by a source of radium irradiating water which he attributed to the inexact nature of direct photons. He showed in 1928 that this radiation is continuous in energy. A Mallet prize was created in 1985 and is awarded by the “Fondation de France” for deserving work in the field of oncological radiotherapy.

    figure i

    Two stamps celebrating the Russian physicist, Pavel Cherenkov (The Marguet collection).

    figure j

    (The Marguet collection) Plaque from the Paris Mint

  17. 17.

    Johannes (Hans) Wilhelm Geiger (1882–1945). German physicist. After his doctorate in 1906 in Erlangen, he left for England and studied terrestrial magnetism at Manchester University. It was here that he met Rutherford and became his assistant for experimental work. In 1912, he returned to Germany and worked at the National Institute of Science and Technology in Berlin on the detection of charged particles. It was in Kiel, from 1925 onwards, that together with his doctoral student, Walther Müller, he developed the famous proportional Geiger-Müller counter, whose clicking indicates the intensity of radiation being measured. In 1936, he was appointed director of the Technische Hochschule in Berlin. He was one of the key signatories of the Heisenberg-Wien-Geiger Memorandum of 1936, signed by many German scientists in protest against the poor image of theoretical physics in Nazi propaganda, which they attributed to the disdain of students for this subject. This memorandum ended such attacks and incited the regime to use physicists in the war effort rather than discouraging them. Indeed, Geiger, whether or not favorable to the regime, was a member of the German team that worked on developing the atomic bomb alongside Heisenberg.

    figure k

    (Public domain)

  18. 18.

    Ernest Marsden (1882–1970). New Zealand physicist. A compatriot of Rutherford, under whom he studied at Manchester, Marsden worked with Geiger on the α-particle diffusion experiments. He returned to New Zealand in 1914, where in 1926 he founded the Department of Industrial and Scientific Research. During the Second World War, he worked on the development of radars.

    figure l

    (Public domain)

  19. 19.

    Hans Geiger, Ernest Marsden: “On a Diffuse Reflection of the α-Particles”, Proceedings of the Royal Society, Vol. 82, pp. 495–500 (1909).

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Marguet, S. (2017). Interaction of Electromagnetic Radiation and Charged Particles with Matter. In: The Physics of Nuclear Reactors. Springer, Cham. https://doi.org/10.1007/978-3-319-59560-3_3

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