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Radioactivity Beta (β)



How Nature correct an excess of protons or neutrons

Beta (β) radioactivity was first observed in the form of a mysterious ray that was deflected by electromagnetic fields in the opposite direction from alpha radiation. The radiation was therefore known to consist of negatively charged particles. After J.J. Thomson discovered (a little before in 1897), the fundamental carrier of negative electric charge, the electron, beta radiation was quickly found to be made up of the same particles.

Il fallut attendre la découverte en 1932 de l'électron positif appelé positon, puis celle de la radioactivité artificielle en 1934, pour mettre en évidence un rayonnement semblable, mais véhiculé par des électrons positifs. On distingue les deux variantes de radioactivité bêta sous les noms de radioactivité bêta-moins et bêta-plus.

Example of a beta-negative decay
A cobalt 60 nucleus, containing 33 neutrons and 27 protons, has an excess of 6 neutrons – shown in blue. To even the balance, one of these neutrons transforms into a proton (shown in red) to form a stable nucleus of nickel 60 with 28 protons (one more than before) and 32 neutrons (one fewer than before). At the time of the decay, two other particles are created: an electron and an antineutrino which is able to pass undetected.
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At the origin of this type of radiation is a force within the nucleus capable of transforming one type of nucleon into another (a proton into a neutron, or vice versa): the so-called 'weak' forces. This transformation does not change the total number of nucleons, but is accompanied by the emission of an electron (or a positron) to compensate the change of electric charge. The electron is expelled together with a kind of neutral positron – an antineutrino - while a positron is expelled with a neutrino, the neutral counterpart of the electron.

Beta decays are observed in Nature, when the process release energy, which is the case for beta emitteurs. The alternative to correct an excess of one type of nucleons - the direct expulsion of a proton or neutron from the nucleus - cost generally energy and occurs only for very unstable nuclei produced in reactors with a large excess of neutrons.

Beta-minus radiation, the emission of an electron and an anti-neutrino, occurs when a neutron transforms into a proton. The reverse process, whereby a proton becomes a neutron through the emission of a positron and a neutrino, is the source of beta-positive radiation. The neutrinos and antineutrinos are tiny, almost massless particles that are virtually impossible to detect.

The energy produced in beta decay is split among the three bodies involved: the recoiling nucleus, the electron (or positron) and the antineutrino (or neutrino). The nucleus, whose mass is by far the greatest, takes away comparatively little energy. The two light particles share practically the energy released in the decay. The electron (or positron) usually takes away a little less than half of this energy.

Three-body beta kinematics
When beta decay takes place, the energy released is shared between the recoiling nucleus, the electron and its antineutrino. As the nucleus was initially at rest, the sum of the three momentum vectors must be equal to zero (for the nucleus, the momentum is equal to the mass times the velocity v). Shown above is the 120° case where all three momenta have equal values. We can see that the kinetic energy T and speed of the recoiling nucleus are negligible compared to the two other particles, which shared the decay energy (1.16 MeV in the decay of bismuth 210).
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A proton excess is rare in nature, and we are indebted to Irene and Frederic Joliot-Curie for synthesizing the first beta-plus emitters after their discovery of artificial radioactivity in 1934 (*). Today beta-plus emitters are produced by small accelerators such as cyclotrons for medical applications, an exemple being fluorine-18 which is used in positron emission tomography for cancer screening

The radioactive half-lives of beta emitters are much more shorter, with a few exceptions, than half-lives of alpha emitters. Sometimes they can be very short. Energies released in beta decays variy from a few keV in the case of tritium to around 1 MeV. They are furthermore shared between electrons and antineutrinos. They are far below the energies of alpha particles that are above 4 MeV.

A few beta-emitters exist in nature, tritium and carbon-14 produced in the atmosphere by cosmic rays or potassium-40 a long-lived isotope of potassium responsible of 4000 decays per second in the human body. Others, such as bismuth-210 are descendants of uranium and thorium nuclei. In reactors, the products of nuclear fission that inherit of the neutron excess in uranium or plutonium nuclei are also beta emitters. The best known are iodine-131 and caesium-137.

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