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An Introduction to Nuclear Astrophysics
by Richard N. Boyd
University of Chicago Press, 2008
eISBN: 978-0-226-06972-2 | Cloth: 978-0-226-06971-5
Library of Congress Classification QB464.B69 2007
Dewey Decimal Classification 523.0197

ABOUT THIS BOOK | AUTHOR BIOGRAPHY | REVIEWS | TOC | REQUEST ACCESSIBLE FILE
ABOUT THIS BOOK
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.  

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