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Protons positron production

E) Nuclides with too many neutrons per proton tend to undergo P-particle production. The net effect of P-particle production is to change a neutron to a proton. Positron production occurs for nuclides that are below the zone of stability (those nuclides whose neutron/proton ratios are too small). The net effect of positron emission is to change a proton to a neutron. An example of positron emission would be... [Pg.207]

A positron is a particle with the same mass as an electron but with the opposite charge. The net effect of positron production is to change a proton to a neutron. [Pg.227]

Te 5.10 alpha particles and 5 beta particles 7. Refer to Table 21.2 for potential radioactive decay processes. 17F and, 8F contain too many protons or too few neutrons. Electron capture or positron production are both possible decay mechanisms that increase the neu-tron-to-proton ratio. Alpha-particle production also increases the neu-tron-to-proton ratio, but it is not likely for these light nuclei. 21F contains too many neutrons or too few protons. Beta-particle production lowers the neutron-to-proton ratio, so we expect 21F to be a /3-emitter. 9. a. 2gCf + gO - fcIJSg + 4jn b. Rf 11. 6.35 X 1011 13. a. [Pg.1133]

Positional probability a type of probability that depends on the number of arrangements in space that yield a particular state. (17.1) Positron production a mode of nuclear decay in which a particle is formed having the same mass as an electron but opposite charge. The net effect is to change a proton to a neutron. (19.1)... [Pg.1099]

The first reaction is a fusion of two protons to produce a 2H nucleus, a positron (e+) and a neutrino (ve). The second reaction is a proton capture with the formation of 3He and a y-ray. In the third reaction two 3He nuclei fuse to give 4He and two protons. The total energy released in one cycle is 26.8 MeV or 4.30 x 10-12 J. An important product of this process is the neutrino and it should provide a neutrino flux from the Sun that is measurable at the surface of the Earth. However, the measured flux is not as big as calculated for the Sun - the so-called neutrino deficit... [Pg.92]

At very high temperatures, above 3 or 4 billion k, silicon is consumed so quickly that positron emission and electron capture reactions which might modify the n/p ratio are largely short-circuited. The weak interaction does not have time to convert any appreciable fraction of protons into neutrons during the brief period of thermonuclear combustion. It follows that, starting with matter that is initially dominated by nuclei containing equal numbers of neutrons and protons, such as oxygen-16 and silicon-28, the final products must conserve Z = N, unless they move away from nuclear stability beyond calcium-40, the last stable a element. [Pg.219]

The production of artificially produced radioactive elements dales back to the early work of Rutherford in 1919 when it was found that alpha particles reacted with nitrogen atoms to yield protons and oxygen atoms. Curie and Joliot found (1933) that when boron, magnesium, or aluminum were bombarded with alpha particles from polonium, the elements would emit neutrons, protons, and positrons. They also found that upon cessation... [Pg.332]

JOLIOT-CURIE. IRENE 11897-195ft. A French nuclear scientist who won the Nohel prize for chemistry with her husband Frederick Joliet-Curie. Their joint work involved production of artiliciul radioactive elements by using t/-rays to bombard boron. They discovered that hydrogen-containing material when exposed to what they considered p rays would emit protons. Tliev were involved in many firsts they gave Ihe first chemical proof of aitillcial transmutation and of capture of alpha particles, and were the firsi to prepare positron emitter. Her career started with a Sc.D. at the Univ ersity of Paris, and included scores of honors and awards. [Pg.894]

The apparatus used by Mills (1981) for the first observation of Ps was similar to that shown in Figure 8.2. Slow positrons were guided by an axial magnetic field onto a 40 A thick carbon film G2. The kinetic energy of the positrons was adjusted so that some could penetrate the foil and emerge bound to two electrons as Ps. The geometry and method are analogous to the production of H by proton bombardment of thin foils (see e.g. Allison, 1958). [Pg.364]


See other pages where Protons positron production is mentioned: [Pg.1127]    [Pg.1127]    [Pg.1141]    [Pg.1141]    [Pg.1147]    [Pg.862]    [Pg.738]    [Pg.1117]    [Pg.1117]    [Pg.476]    [Pg.8]    [Pg.364]    [Pg.24]    [Pg.9]    [Pg.10]    [Pg.32]    [Pg.843]    [Pg.98]    [Pg.215]    [Pg.412]    [Pg.965]    [Pg.952]    [Pg.32]    [Pg.180]   
See also in sourсe #XX -- [ Pg.894 ]




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