Abstract
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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Röpke, G., Blaschke, D. & Schulz, H. Quantum statistical cluster abundances in hot nuclear matter and elemental composition of cosmic-ray sources. Astrophys Space Sci 95, 417–423 (1983). https://doi.org/10.1007/BF00653644
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DOI: https://doi.org/10.1007/BF00653644