An Introduction to Nuclear Astrophysics

An Introduction to Nuclear Astrophysics

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Nuclear astrophysics is the study of how all naturally occurring elements formed and evolved into our present universe via nuclear processes, beginning with the Big Bang and continuing today in astrophysical objects such as stars, x-ray bursters, and supernovae. Emerging from traditional studies in astrophysics and particle research, this cross-disciplinary field touches upon astronomy, astrophysics, cosmology, and particle physics. In An Introduction to Nuclear Astrophysics, author Richard Boyd includes basic nomenclature and information so that students from astronomy or physics can quickly orient themselves in the material. Subsequent chapters describe earthbound and space born instruments operating in service to nuclear astrophysics worldwide; background topics such as nuclear and neutrino physics, scattering formalism, and thermonuclear reaction rates; and information on galactic chemical evolution, solar nucleosynthesis, s- and r-processes, and gamma-ray bursts. Each chapter includes problem sets against which students may test their knowledge before moving ahead, and the author has included copious references intended to guide students to further study. An Introduction to Nuclear Astrophysics is an essential textbook for undergraduate and graduate students in astronomy and astrophysics. It is also an invaluable overview of the subject for researchers in nuclear astrophysics and related fields.The Hertzsprung-Russell (HR) diagram. The curved diagonal line that moves from the upper left to the lower right is known as the main sequence; most stars, roughly 90 % of them, are found to lie along that line. The group of stars that starts atanbsp;...

Title:An Introduction to Nuclear Astrophysics
Author:Richard N. Boyd
Publisher:University of Chicago Press - 2007


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