Overview
ABSTRACT
This paper sets out the basics of nuclear physics that are directly useful for nuclear reactor studies. The principal definitions and concepts related to the atomic nucleus and its structure are presented together with its fundamental properties, including binding energy. The main radioactivity phenomena are described, with their important features. The isobaric transitions are also addressed as they occur inside the nuclear reactor core through the fission products. Radioactive equilibrium is discussed, calling on the two-body problem.
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Cheikh M'Backé DIOP: Research engineer - Commissariat à l'énergie atomique et aux énergies alternatives, CEA/Saclay, France
INTRODUCTION
The aim of nuclear reactor physics is to quantify, using physico-mathematical methods and calculation software (or calculation codes) – neutron codes and radiation protection codes in particular – relevant macroscopic quantities enabling respectively :
characterize the neutron state of a nuclear reactor core;
assess the effect of radiation on organic and inert matter (materials) and take appropriate measures to protect against it.
In the field of nuclear reactors, neutrons and gamma rays are the two main types of radiation to be considered from different angles: propagation in matter, induced radioactive phenomena and particles emitted by interaction with matter. The energy range concerned typically extends from 0 to 20 MeV.
We begin by placing nuclear physics in the context of nuclear reactor physics. We then present the main definitions of the atomic nucleus and its fundamental properties. The final part of the article is devoted to the phenomena of radioactivity, describing some of its most important properties.
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KEYWORDS
atomic nucleus | radioactivity | core physics | neutronics
Nuclear reactor physics – Basics of nuclear physics
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