Quantum statistical cluster abundances in hot nuclear matter and elemental composition of cosmic-ray sources

Details Quantum statistical cluster abundances in hot nuclear matter and elemental composition of cosmic-ray sources Quantum statistical cluster abundances in hot nuclear matter and elemental composition of cosmic-ray sources

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..95..417r&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 95, no. 2, Sept. 1983, p. 417-423.

Statistics

1

Abundance, Cosmic Rays, High Temperature Plasmas, Quantum Statistics, Supernovae, Astronomical Models, Coulomb Collisions, Dense Plasmas, Equations Of State, Fermi Liquids, Gravitational Collapse, Interstellar Matter, Radiation Sources

Scientific paper

Cluster abundances of a hot nuclear medium are determined within a quantum statistical model calculation for symmetric matter. It is suggested that differences between the elemental abundances of the cosmic-ray source and those of the solar system may be characterized in terms of different freeze-out thermodynamic parameters. The possible energy dependence of these parameters is discussed.

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