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AbstractAbstract
[en] A statistical equilibrium theory describing the abundances of elements in universe is presented. The distribution of light and heavier nuclei is generated in a dense nuclear matter at high temperature as it exists in early stages of star formation. Clustering of nucleons in heavier structures is dominated both by simple combinatorial considerations as well as by intrinsic properties of the structures, mainly the binding energies. The present model takes into account both aspects. An extension to non extensive statistics is also discussed. (author)
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Oancea, Margareta; Sandu, Doina; Calboreanu, Rodica (Documentation and Publishing Office, Horia Hulubei, National Institute for Physics and Nuclear Engineering, PO Box MG-6, RO-76900 Bucharest-Magurele (Romania)); Romanian Physical Society, PO Box MG-6, RO-76900 Bucharest-Magurele (Romania); 126 p; 2000; p. 22; National Physics Conference; National Physics Conference; Constanta (Romania); 21-23 Sep 2000; Available from author(s) or Documentation and Publishing Office, Horia Hulubei National Institute for Physics and Nuclear Engineering, PO Box MG-6, RO-76900 Bucharest-Magurele (RO); Available from Documentation and Publishing Office, Horia Hulubei National Institute for Physics and Nuclear Engineering, PO Box MG-6, RO-76900 Bucharest-Magurele (RO); Short communication
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Miscellaneous
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Conference
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