Element abundance in the solar system and element formation in the Galaxy

Computer Science

Scientific paper

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Abundance, Galactic Evolution, Heavy Nuclei, Nuclear Fusion, Solar System, Milky Way Galaxy, Stellar Evolution, Stellar Temperature, Thermonuclear Explosions

Scientific paper

Questions concerning the significance of the greater abundance of elements with an even number of protons compared to those with an odd number are considered along with the characteristics of thermonuclear element synthesis, the s-process component of the heavy nuclei, and the synthesis of neutron-rich and proton-rich heavy nuclei. Aspects regarding the time and place of origin of the heavy elements are discussed. The hypotheses of galactic nucleosynthesis of the elements include a hypothesis of an element synthesis in stars and a hypothesis which considers a further processing of primary matter, which was possibly formed in galactic explosions, by the s process.

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