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Atoms neutron rich isotopes

Proton capture processes by heavy nuclei have already been briefly mentioned in several of the preceding sections. The (p,y) reaction can also be invoked to explain the presence of a number of proton-rich isotopes of lower abundance than those of nearby normal and neutron-rich isotopes (Fig. 1.5). Such isotopes would also result from expulsion of a neutron by a y-ray, i.e. (y,n). Such processes may again be associated with supernovae activity on a very short time scale. With the exceptions of " ln and " Sn, all of the 36 isotopes thought to be produced in this way have even atomic mass numbers the lightest is Se... [Pg.13]

Know that nuclear stability is best related to the neutron-to-proton ratio (n/p), which starts at about 1/1 for light isotopes and ends at about 1.5/1 for heavier isotopes with atomic numbers up to 83- All isotopes of atomic number greater than 84 are unstable and will commonly undergo alpha decay. Below atomic number 84, neutron-poor isotopes will probably undergo positron emission or electron capture, while neutron-rich isotopes will probably undergo beta emission. [Pg.267]

At the extremely high fluxes of a nuclear explosion, fast multiple neutron capture leads to very neutron-rich isotopes of U or Pu, respectively, changing rapidly into elements of appreciably higher atomic numbers by a quick succession of transmutations. This method of formation of heavier elements is also indicated in Fig. 14.5. The elements can be found in the debris of nuclear underground explosions. [Pg.284]

The combination of collinear fast-beam laser spectroscopy and P-RADOP (radiation-detected optical pumping) has been used to measure nuclear spins and moments of neutron-rich isotopes of the light alkali elements jLi [72-74] and Na [75]. Here, the optically pumped fast atomic beam is implanted into a single crystal placed in a static magnetic field. The NMR signal is destroying the nuclear polarization detected by measuring the p-decay asymmetry. [Pg.368]

Neutron-rich lanthanide isotopes occur in the fission of uranium or plutonium and ate separated during the reprocessing of nuclear fuel wastes (see Nuclearreactors). Lanthanide isotopes can be produced by neutron bombardment, by radioactive decay of neighboring atoms, and by nuclear reactions in accelerators where the rate earths ate bombarded with charged particles. The rare-earth content of solid samples can be determined by neutron... [Pg.541]

The silver white, shiny, metal-like semiconductor is considered a semimetal. The atomic weight is greater than that of the following neighbor (iodine), because tellurium isotopes are neutron-rich (compare Ar/K). Its main use is in alloys, as the addition of small amounts considerably improves properties such as hardness and corrosion resistance. New applications of tellurium include optoelectronics (lasers), electrical resistors, thermoelectric elements (a current gives rise to a temperature gradient), photocopier drums, infrared cameras, and solar cells. Tellurium accelerates the vulcanization of rubber. [Pg.139]

All elements with or more protons are unstable they eventually undergo decay. Other isotopes with fewer protons in their nucleus are also radioactive. The radioactivity corresponds to the neutron/proton ratio in the atom. If the neutron/proton ratio is too high (there are too many neutrons or too few protons), the isotope is said to be neutron rich and is, therefore, unstable. Likewise, if the neutron/proton ratio is too low (there are too few neutrons or too many protons), the isotope is unstable. The neutron/proton ratio for a certain element must fall within a certain range for the element to be stable. That s why some isotopes of an element are stable and others are radioactive. [Pg.68]

In December 1998 Russian scientists utiHzed a cyclotron at the Joint Institute for Nuclear Research in Dubna to produce some few atoms of element 114. They bombarded Pu with the neutron-rich Ca isotopes provided by the Lawrence Berkeley National Laboratory in California. In the target they could identify an isotope of the element 114 with a mass number of 289. Although the goal, mass number 298, was not attained, a surprisingly long half-hfe of 30 seconds was obtained [52.22]. [Pg.1212]


See other pages where Atoms neutron rich isotopes is mentioned: [Pg.18]    [Pg.445]    [Pg.34]    [Pg.7]    [Pg.122]    [Pg.125]    [Pg.136]    [Pg.155]    [Pg.279]    [Pg.303]    [Pg.11]    [Pg.13]    [Pg.411]    [Pg.360]    [Pg.313]    [Pg.136]    [Pg.885]    [Pg.887]    [Pg.905]    [Pg.2452]    [Pg.2486]    [Pg.2493]    [Pg.195]    [Pg.249]    [Pg.320]    [Pg.249]    [Pg.431]    [Pg.134]    [Pg.142]    [Pg.242]    [Pg.246]    [Pg.299]    [Pg.249]    [Pg.224]    [Pg.117]    [Pg.425]    [Pg.8]    [Pg.38]    [Pg.13]    [Pg.918]    [Pg.120]   
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Atoms isotopic

Isotopes atomic

Neutron atoms

Neutron rich

Neutrons isotopes

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