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This volume covers a variety of modern aspects of the observational, experimental and theoretical studies on the origin, evolution and distribution of the elements in the Universe. The topics include “Early Universe and Primordial Nucleosynthesis”, “Evolution of Galaxies”, “Nucleosynthesis in Novae and Supernovae”, “Neutron Stars and Hadronic Matter”, and “Nuclear Astrophysics”.
This book focuses on current topics in astronomy, astrophysics and nuclear astrophysics. The areas covered are: origin of the universe and nucleosynthesis; chemical and dynamical evolution of galaxies; nova/supernova and evolution of stars; astrophysical nuclear reaction; structure of nuclei with unstable nuclear beams; origin of the heavy element and age of the universe; neutron star and high density matter; observation of elements; high energy cosmic rays; neutrino astrophysics.
The Proceedings cover the interdisciplinary field related to nuclear physics, particle physics, astronomy and astrophysics. The conference aimed to understand the origin of the elements in the universe and the evolution of galaxies through the discussions and collaborations of nuclear physicists and astronomers studying various processes of astrophysical nucleosynthesis.
All papers have been peer-reviewed. Chemical elements are fundamental matter to comprise the universe and hold a great deal of interest for astronomers and nuclear physicists, for these play an important role in understanding the dawn of the universe to the formation of solar system. This volume contains the proceedings of the symposium that aims to understand the origin and evolution of the universe through the current knowledge of nuclear astrophysics.