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Electrons from unstable isotopes

The product nuclei as initially formed are highly unstable isotopes and emit delayed neutrons as well as electrons and gamma photons while settling down into their stable configurations, which ate usually isotopes of different elements from those first formed. The neutrons, both prompt and delayed, continue the reaction by encountering other fissionable nuclei... [Pg.501]

The important phenomenon of exponential decay is the prototype first-order reaction and provides an informative introduction to first-order kinetic principles. Consider an important example from nuclear physics the decay of the radioactive isotope of carbon, carbon-14 (or C). This form of carbon is unstable and decays over time to form nitrogen-14 ( N) plus an electron (e ) the reaction can be written as... [Pg.110]

Termination in autoxidations is rather more complex than in the chain reactions we have considered so far. As we have noted briefly earlier (Section 9.2, p. 488), the peroxy radicals first combine to an unstable tetroxide, ROOOOR.124 The existence of these compounds when R is tertiary is inferred from isotope tracer studies,125 and the equilibrium 9.72 is observable by electron... [Pg.500]

Radioactivity is the spontaneous emission of radiation from an unstable nucleus. Alpha (a) radiation consists of helium nuclei, small particles containing two protons and two neutrons (fHe). Beta (p) radiation consists of electrons ( e), and gamma (y) radiation consists of high-energy photons that have no mass. Positron emission is the conversion of a proton in the nucleus into a neutron plus an ejected positron, e or /3+, a particle that has the same mass as an electron but an opposite charge. Electron capture is the capture of an inner-shell electron by a proton in the nucleus. The process is accompanied by the emission of y rays and results in the conversion of a proton in the nucleus into a neutron. Every element in the periodic table has at least one radioactive isotope, or radioisotope. Radioactive decay is characterized kinetically by a first-order decay constant and by a half-life, h/2, the time required for the... [Pg.978]

All isotopes of Tc are unstable toward fi decay or electron capture, and traces exist in nature only as fragments from the spontaneous fission of U. Thus, while it is not a member of the actinide series, it is radioactive and, therefore, the role of photocatalysis in control of its valence state will be briefly considered here. [Pg.467]

The " N nucleus (1 = 1, 99.6%) has a moderately large magnetic moment and hyperfine splittings from this nucleus are a distinctive feature of the ESR spectra. For example, the thermally unstable S4N4 " radical anion has been identified by its characteristic nine-line ESR spectrum. For S (/ = 3/2, 0.76%), isotopic labeling is usually necessary to obtain information on electron spin density at sulfur. [Pg.4646]

Hydrogen is the most abundant element in the universe more than 90% of all atoms are hydrogen. Hydrogen is the simplest atom and element number 1, consisting of one proton and one electron only. Apart from this ordinary isotope called protium, a small fraction of hydrogen atoms exist as deuterium (1 proton, 1 neutron, 1 electron) and an even smaller fraction as unstable tritium (1 proton, 2 neutrons, 1 electron). [Pg.1]

Nuclear reactions may lead to stable or unstable (radioactive) products. In general, (n, y), (n, p), and (d, p) reactions give radionuclides on the right-hand side of the line of p stability that exhibit decay, whereas (p, n), (d,2n), (n, 2n), (y, n), (d, n) and (p, y) reactions lead to radionuclides on the left-hand side of the line of p stability that exhibit p decay or electron capture (e). (n, y), (d, p), (n, 2n) and (y, n) reactions give isotopic nuclides, and these cannot be separated from the target nuclides by chemical methods, except for the application of the chemical effects of nuclear transformations which will be discussed in chapter 9. [Pg.147]


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See also in sourсe #XX -- [ Pg.291 ]




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Unstability

Unstable

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