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Supernovae and Nucleosynthesis: An Investigation of the History of Matter, from the Big Bang to the Present - David Arnett
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ISBN: 9780691011479

ID: 978069101147

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. David Arnett, Books, Science and Nature, Supernovae and Nucleosynthesis: An Investigation of the History of Matter, from the Big Bang to the Present Books>Science and Nature, Princeton University Press

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Supernovae and Nucleosynthesis : An Investigation of the History of Matter, from the Big Bang to the Present - David Arnett
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ISBN: 0691011478

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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. astronomy,astronomy and astrophysics,astronomy and space science,astrophysics and space science,evolution,physics,science,science and math,science and math,science and scientists Evolution, Princeton University Press

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Supernovae and Nucleosynthesis: An Investigation of the History of Matter, from the Big Bang to the Present - Arnett, David
Vergriffenes Buch, derzeit bei uns nicht verfügbar.
(*)
Arnett, David:
Supernovae and Nucleosynthesis: An Investigation of the History of Matter, from the Big Bang to the Present - gebrauchtes Buch

ISBN: 9780691011479

ID: 2544126

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: An Investigation of the History of Matter, from the Big Bang to the Present Arnett, David, Princeton University Press

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Supernovae and Nucleosynthesis
Vergriffenes Buch, derzeit bei uns nicht verfügbar.
(*)
Supernovae and Nucleosynthesis - neues Buch

ISBN: 9780691011479

ID: 9780691011479

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. Books, [PU: Princeton University Press]

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Supernovae and Nucleosynthesis: An Investigation of the History of Matter, from the Big Bang to the Present (Princeton Series in Astrophysics (Paperback)) - Arnett, David
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Arnett, David:
Supernovae and Nucleosynthesis: An Investigation of the History of Matter, from the Big Bang to the Present (Princeton Series in Astrophysics (Paperback)) - Taschenbuch

1996, ISBN: 9780691011479

, Taschenbuch, [PU: Princeton Series in Astrophysi], [SC: 2.2]

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Details zum Buch
Supernovae and Nucleosynthesis: An Investigation of the History of Matter, from the Big Bang to the Present

This book is intended to be what was well described by Prof. S. Chandrasekhar in reference to his own goals for scientific books: '...a certain viewpoint of the field, written by one who has been an active participant in its development...' The subject is the synthesis and evolution of atomic nuclei, by thermonuclear reactions, from the Big Bang to the present.

Detailangaben zum Buch - Supernovae and Nucleosynthesis: An Investigation of the History of Matter, from the Big Bang to the Present


EAN (ISBN-13): 9780691011479
ISBN (ISBN-10): 0691011478
Taschenbuch
Erscheinungsjahr: 1996
Herausgeber: PRINCETON UNIV PR
496 Seiten
Gewicht: 0,853 kg
Sprache: eng/Englisch

Buch in der Datenbank seit 06.01.2007 11:13:47
Buch zuletzt gefunden am 02.07.2018 23:05:17
ISBN/EAN: 9780691011479

ISBN - alternative Schreibweisen:
0-691-01147-8, 978-0-691-01147-9


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