Úloha intermediálních stavů při s- a p-procesu

Abstract

The goal of this bachelor thesis is to summarize the most important aspects of nucleosynthesis of elements in universe, with special focus on s- and p-process nucleosynthesis of isomeric state 180Tam. We had performed calculations of 180Tam synthesis under both stationary and dynamic stellar conditions, and made qualitative analysis of feasible stellar environments of 180Tam nucleosynthesis.

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Subject(s)

Nuclear physics, Astrophysics, Theoretical physics, Nucleosynthesis, Tantalum, s-Process, r-Process, p-Process, Supernovae

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