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!?5.><br />
binding energy than the second lightesto<br />
The most remarkable feature in the abundance distribution of these raider<br />
nuclides is, that, for wide ranges of mass numbers, their abundance values as a<br />
function of A seem to follow a law of "smoothness" of their own-<br />
In particular<br />
the abundances of Sn^^, Sn^^, Te^°, Xe''^^, Xe^^, Ba^°, etc., show this behavior<br />
in an impressive way-<br />
The conclusion seems inevitable that in these mass ranges<br />
a fraction of nuclear matter must have formed on the O^side of the energy valley<br />
in the region of the tuistabls neutron-deficient nuclear species, in a way that<br />
led to a "sBJOothed out" distribution of the stable species-<br />
Possibly, awcondary<br />
spallaticn processes may have led to the formation of these nuclides in the<br />
required proporticnso<br />
Magic nuEfeer effects in the higher mass i^gion<br />
Elsasaer (1933, 193k) was the first physicist who noticed that the abundance<br />
of nuclear species containing certain nujrfcers of neutrons or protons is excoptioneliy<br />
lai^e-<br />
Theae numbers, the so called "magic nurabers" ai^:<br />
2, 8, 20, 28, 50, 82^ 126 »<br />
They belong to two different arithmetical aeries:<br />
(1) 2, 8, 20, UO, 70, 112 » - - - -<br />
(2) 2, 6, lii, 28, 50, 82, 126 -<br />
The first series is significant at lower mass nunbersj, whil©<br />
the second<br />
series prodoainatea at mass nuiribers greater than kOo<br />
Magic number affects are<br />
rum well understood in terms of a shell structure of the nucleuso<br />
(Mayer and<br />
Jensen, 1955)<br />
A nagic nuiriber is signified by the sudden drop in the binding energy of the<br />
next nucleono<br />
Thti binding energy of the next nucleonj, however, is also a function