Nucleosynthesis of solar system matter

Details Nucleosynthesis of solar system matter Nucleosynthesis of solar system matter

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991geokh......926l&link_type=abstract

Geokhimiia (ISSN 0016-7525), July 1991, p. 926-935. In Russian.

Astronomy and Astrophysics

Astrophysics

2

Astronomical Models, Chemical Composition, Nuclear Astrophysics, Nuclear Fusion, Solar System Evolution, Big Bang Cosmology, High Energy Interactions, Stellar Physics, Supernova Remnants

Scientific paper

The paper examines two basic problems that prevail in the theory of nucleosynthesis of solar-system matter: finding an adequate model for the process and finding astrophysical bodies in which the nucleosynthetic processes can be studied. It is shown that the distribution of elements in the solar system matter cannot be explained by multiple repetitions of supernova explosions in the Galaxy disk. The paper presents a hypothesis on the origin of the most probable objects and the number of stages in the nucleosynthesis process in solar system matter. This model does not require cosmological synthesis of D, He-3, and Li-7.

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