Origin of the Chemical Elements

@article{Rauscher2011OriginOT,
  title={Origin of the Chemical Elements},
  author={Thomas Rauscher and Andr{\'a}s Patk{\'o}s},
  journal={arXiv: Solar and Stellar Astrophysics},
  year={2011},
  pages={611}
}
This review provides the necessary background from astrophysics, nuclear, and particle physics to understand the cosmic origin of the chemical elements. It reflects the year 2009 state of the art in this extremely quickly developing interdisciplinary research direction. The discussion summarizes the nucleosynthetic processes in the course of the evolution of the Universe and the galaxies contained within, including primordial nucleosynthesis, stellar evolution, and explosive nucleosynthesis in… 
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References

SHOWING 1-10 OF 165 REFERENCES
Nucleosynthesis and Chemical Evolution of Galaxies
This chapter deals with a brief presentation of the nucleosynthesis processes which are responsible for the formation of the observed chemical elements : the primordial nucleosynthesis occurring just
Stellar Structure and Evolution
This book introduces the theory of the internal structure of stars and their evolution in time. It presents the basic physics of stellar interiors, methods for solving the underlying equations, and
Nucleosynthesis in stellar and supernova environments
This article provides a review of the present status of research in nucleosynthesis, with emphasis on problems of nucleosynthesis in stellar and supernova environments. The authors begin by surveying
Stellar production rates of carbon and its abundance in the universe.
TLDR
It is shown that outside a narrow window of 0.5 and 4% of the values of the strong and Coulomb forces, respectively, the stellar production of carbon or oxygen is reduced by factors of 30 to 1000.
Synthesis of the Elements in Stars
Man inhabits a universe composed of a great variety of elements and their isotopes. In Table I,1 a count of the stable and radioactive elements and isotopes is listed. Ninety elements are found
The physics of stars
Basic Concepts in Astrophysics. Properties of Matter and Radiation. Heat Transfer in Stars. Thermonuclear Fusion in Stars. Stellar Structure. The Endpoints of Stellar Evolution. Helioseismology.
s-process nucleosynthesis-nuclear physics and the classical model
Among the various processes responsible for the formation of the heavy elements in stars, the slow neutron capture process (s-process) is distinguished by the fact that it involves mostly stable
CURRENT QUESTS IN NUCLEAR ASTROPHYSICS AND EXPERIMENTAL APPROACHES
▪ Abstract This review summarizes current problems and questions in experimental nuclear astrophysics. It focuses on the present need for experimental data, emphasizing novel methods and approaches.
...
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