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Capture of neutrons

Secondary ionization caused by the capture of neutrons is important in the detection of neutrons. Neutrons will interact with B-10 to produce Li-7 and He-4. [Pg.33]

The main mechanism by which nuclides beyond the iron peak are produced is by neutron capture. The basic processes involved in neutron capture were laid out by Burbidge, Burbidge, Hoyle, and Fowler (1957) (this classic paper is commonly known as B2FH). The common ingredient in these processes is the capture of a neutron by a nucleus, increasing the atomic mass by one unit. If the resulting nucleus is stable, it remains an isotope of the original element. If not, the atom P-decays (a neutron emits an electron and becomes a proton) and becomes an isotope of the next heavier element. Any isotope, whether stable or unstable, can capture another neutron. The rate of capture compared to the rate of decay leads to two basic end-member processes, the -process and the r-proccss. The s-process is capture of neutrons on a time scale that is slow compared to the rate of P-decay. The r-process is neutron capture on such a rapid time scale that many neutrons can be captured before P-decay occurs. [Pg.77]

Studies of the effect of neutron irradiation are divided into three groups slow or thermal neutrons, fission products and reactor neutrons. The slow neutrons are obtained from a radioactive source or high energy neutrons that are produced by deuterium bombardment of a beryllium target in a cyclotron and slowed down passing thru a thick paraffin wax block. The fission products in one case are produced when a desired sample is mixed or coated with uranium oxide and subsequently irradiated with slow neutrons. The capture of neutrons by U23S leads... [Pg.30]

Reactor fuel elements are contained in cans. In early British reactors, these were made of aluminium or aluminium/magnesium alloy to minimise capture of neutrons in the canning material. Nowadays, uranium fuel is enriched with respect to the 235U content, and the extra reactivity enables steel or zirconium cans to be used. In the original... [Pg.66]

The inventory of this stable nuclide is based on its atmospheric inventory, which includes an appreciable contribution from crustal degassing of He. Based on atmospheric Kr/Kr ratio of (5.2 0.4) X 10. Based on atmospheric Ar/Ar ratio of (0.107 0.004) dpm 1 Ar (STP). Includes a rough estimate of C1 produced by the capture of neutrons at the Earth s surface. [Pg.2173]

Natural lithium consists of 7.42% Ti and 92.58% Ti. Much of the tritium (fH) used in experiments with fusion reactions is made by the capture of neutrons by Ti atoms. [Pg.821]

Earth s atmosphere is constantly being bombarded by cosmic rays of extremely high penetrating power. These rays, which originate in outer space, consist of electrons, neutrons, and atomic nuclei. One of the important reactions between the atmosphere and cosmic rays is the capture of neutrons by atmospheric nitrogen (nitrogen-14 isotope) to produce the radioactive carbon-14 isotope and hydrogen. The unstable carbon atoms eventually form C02, which mixes with the ordinary carbon dioxide ( C02) in the air. As the carbon-14 isotope decays, it emits f3 particles (electrons). The rate of decay (as measured by the number of electrons emitted per second) obeys first-order kinetics. It is customary in the study of radioactive decay to write the rate law as... [Pg.527]

Such a process is known as the slowy or s-process. While the reaction probability for the capture of neutrons increases with the atomic number of the element, the relative amoimt of the elements in the star will decrease with increasing atomic number, because of the successive higher order of reaction ( 15.3). The result is the observed flattening of the abundance curve for A > 100, see Figures 17.2a and 17.7b. [Pg.458]

Some amount of Cl appears at the impact of the cosmic rays on minerals of groxmd surface through capture of neutrons by isotopes Cl (neutrons emerge at radioactive decay) and forms a low and relatively stable level of backgroxmd Cl content in groxmd water. [Pg.406]

Because of its neuronic, mechanical, and physical properties, hafnium is an excellent control material for water-cooled, water-moderated reactors. It is found together with zirconium, and the process that produces pure zirconium produces hafnium as a by-product. Hafnium is resistant to corrosion by high-temperature water, has adequate mechanical strength, and can be readily fabricated. Hafnium consists of four isotopes, each of which has appreciable neutron absorption cross sections. The capture of neutrons by the isotope hafnium-177 leads to the formation of hafnium-178 the latter forms hafnium-179, which leads to hafnium-180. The first three have large resonance-capture cross sections, and hafnium-180 has a moderately large cross section. Thus, the element hafnium in its natural form has a long, useful lifetime as a neutron absorber. Because of the limited availability and high cost of hafnium, its use as a control material in civilian power reactors has been restricted. [Pg.177]

The capture of neutrons above thermal energies is described rather well by the Breit-Wigner formulas, and an analysis of the case, assuming that one resonance level predominates, is given by Anderson. A more accurate analysis was given subsequently by S. Dancoff and M. Ginsburg. [Pg.179]


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Neutron capture

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