Supernovae and Nucleosynthesis

Supernovae and Nucleosynthesis PDF

Author: David Arnett

Publisher: Princeton University Press

Published: 1996-03-24

Total Pages: 624

ISBN-13: 9780691011479

DOWNLOAD EBOOK →

This book investigates the question of how matter has evolved since its origin in the Big Bang, from the cosmological synthesis of hydrogen and helium to the generation of the complex set of nuclei that comprise our world and our selves. A central theme is the evolution of gravitationally contained thermonuclear reactors, otherwise known as stars. Our current understanding is presented systematically and quantitatively, by combining simple analytic models with new state-of-the-art computer simulations. The narrative begins with the clues (primarily the solar system abundance pattern), the constraining physics (primarily nuclear and particle physics), and the thermonuclear burning in the Big Bang itself. It continues with a step-by-step description of how stars evolve by nuclear reactions, a critical investigation of supernova explosion mechanisms and the formation of neutron stars and of black holes, and an analysis of how such explosions appear to astronomers (illustrated by comparison with recent observations). It concludes with a synthesis of these ideas for galactic evolution, with implications for nucleosynthesis in the first generation of stars and for the solar system abundance pattern. Emphasis is given to questions that remain open, and to active research areas that bridge the disciplines of astronomy, cosmochemistry, physics, and planetary and space science. Extensive references are given.

Supernovae and Nucleosynthesis

Supernovae and Nucleosynthesis PDF

Author: David Arnett

Publisher: Princeton University Press

Published: 2020-11-10

Total Pages: 598

ISBN-13: 0691221669

DOWNLOAD EBOOK →

This book investigates the question of how matter has evolved since its origin in the Big Bang, from the cosmological synthesis of hydrogen and helium to the generation of the complex set of nuclei that comprise our world and our selves. A central theme is the evolution of gravitationally contained thermonuclear reactors, otherwise known as stars. Our current understanding is presented systematically and quantitatively, by combining simple analytic models with new state-of-the-art computer simulations. The narrative begins with the clues (primarily the solar system abundance pattern), the constraining physics (primarily nuclear and particle physics), and the thermonuclear burning in the Big Bang itself. It continues with a step-by-step description of how stars evolve by nuclear reactions, a critical investigation of supernova explosion mechanisms and the formation of neutron stars and of black holes, and an analysis of how such explosions appear to astronomers (illustrated by comparison with recent observations). It concludes with a synthesis of these ideas for galactic evolution, with implications for nucleosynthesis in the first generation of stars and for the solar system abundance pattern. Emphasis is given to questions that remain open, and to active research areas that bridge the disciplines of astronomy, cosmochemistry, physics, and planetary and space science. Extensive references are given.

Supernovae, Neutron Star Physics and Nucleosynthesis

Supernovae, Neutron Star Physics and Nucleosynthesis PDF

Author: Debades Bandyopadhyay

Publisher: Springer Nature

Published: 2022-03-28

Total Pages: 221

ISBN-13: 3030951715

DOWNLOAD EBOOK →

This book deals with the interdisciplinary areas of nuclear physics, supernovae and neutron star physics. It addresses the physics and astrophysics of the spectacular supernova explosions, starting with the collapse of massive stars and ending with the birth of neutron stars or black holes. Recent progress in the understanding of core collapse supernova (CCSN) and observational aspects of future detections of neutrinos from CCSN explosions are discussed. The other main focus in this text is the novel phases of dense nuclear matter, its compositions and equation of state (EoS) from low to very high baryon density relevant to supernovae and neutron stars. The multi-messenger astrophysics of binary neutron star merger GW170817 and its relation to EoS through tidal deformability are also presented in detail. The synthesis of elements heavier than iron in the supernova and neutron star environment by the rapid (r)-process are treated here with special emphasis on the nucleosynthesis in the ejected material from GW170817. This monograph is written for graduate students and researchers in the field of nuclear astrophysics.

Stellar Explosions

Stellar Explosions PDF

Author: Jordi Jose

Publisher: CRC Press

Published: 2016-01-05

Total Pages: 472

ISBN-13: 1439853088

DOWNLOAD EBOOK →

Stars are the main factories of element production in the universe through a suite of complex and intertwined physical processes. Such stellar alchemy is driven by multiple nuclear interactions that through eons have transformed the pristine, metal-poor ashes leftover by the Big Bang into a cosmos with 100 distinct chemical species. The products of

Principles of Stellar Evolution and Nucleosynthesis

Principles of Stellar Evolution and Nucleosynthesis PDF

Author: Donald D. Clayton

Publisher: University of Chicago Press

Published: 1983

Total Pages: 634

ISBN-13: 0226109534

DOWNLOAD EBOOK →

Donald D. Clayton's Principles of Stellar Evolution and Nucleosynthesis remains the standard work on the subject, a popular textbook for students in astronomy and astrophysics and a rich sourcebook for researchers. The basic principles of physics as they apply to the origin and evolution of stars and physical processes of the stellar interior are thoroughly and systematically set out. Clayton's new preface, which includes commentary and selected references to the recent literature, reviews the most important research carried out since the book's original publication in 1968.

Nucleosynthesis and Chemical Evolution of Galaxies

Nucleosynthesis and Chemical Evolution of Galaxies PDF

Author: Bernard Ephraim Julius Pagel

Publisher: Cambridge University Press

Published: 2009-01-15

Total Pages: 485

ISBN-13: 0521840309

DOWNLOAD EBOOK →

A lucid introduction for advanced undergraduates and graduate students, and an authoritative overview for researchers and professional scientists.

Supernovae

Supernovae PDF

Author: Albert G. Petschek

Publisher: Springer Science & Business Media

Published: 2012-12-06

Total Pages: 304

ISBN-13: 1461232864

DOWNLOAD EBOOK →

For millennia mankind has watched as the heavens move in their stately progression from night to night and from year to year, presaging with their changes the changing seasons. The sun, the moon, and the planets move in what appears to be an unchanging firmament, except occasionally when a new "star" appears. Among the new stars there are comets, novae, and finally supernovae, the subject of this book. Superstitious mankind regarded these events as significant portents and recorded them carefully so that we have records of supernovae that may reach back as far as 1300 B. C. (Clark and Stephenson, 1977; Murdin and Murdin, 1985). The Cygnus Loop, believed to be a 15,000-year-old supernova remnant at a distance of only 800 pc (Chevalier and Seward, 1988), must have awed our ancestors. Tycho's supernova of 1572, at a distance of 2500 pc, had a magnitude of -4. 0, comparable to Venus at its brightest, and Kepler's supernova of 1604 had a magnitude of - 3 or so. Thus the Cygnus Loop supernova might have had a magnitude of - 6 or so, and should have been readily visible in daytime. A supernova in Vela, about 8000 B. C. was comparably close, as was SN 1006, whose magnitude may have been -9. While most of the supernova records come from the Old World, the supernova of 1054 is recorded in at least one petroglyph in the American West.

Stellar Evolution, Nuclear Astrophysics, and Nucleogenesis

Stellar Evolution, Nuclear Astrophysics, and Nucleogenesis PDF

Author: A. G. W. Cameron

Publisher: Courier Corporation

Published: 2013-02-20

Total Pages: 210

ISBN-13: 0486498557

DOWNLOAD EBOOK →

Along with classic papers byFowler, Hoyle, and the Burbidges,this work stands as a key foundationin the development of nuclear astrophysics. Long out ofprint and very hard to find, this remarkable work has beenedited and re-typeset by an atomic expert. Now availablein an affordable paperback edition for the very first time,it addresses interrelated questions — What are stars? Howdoes the sun shine? Why is gold so rare, and Where did theelements come from? — that have puzzled observers fromtime immemorial.Edited and re-typeset reprint of the original Atomic Energy ofCanada, Ltd., 1957 edition.

Stellar Evolution and Nucleosynthesis

Stellar Evolution and Nucleosynthesis PDF

Author: Sean G. Ryan

Publisher: Cambridge University Press

Published: 2010-01-07

Total Pages: 244

ISBN-13: 9780521196093

DOWNLOAD EBOOK →

An ideal bridging text for astrophysics and physics majors looking to move on from the introductory texts.