Gespeichert in:
| Beteilige Person: | |
|---|---|
| Format: | Elektronisch E-Book |
| Sprache: | Englisch |
| Veröffentlicht: |
Princeton, NJ
Princeton University Press
[2020]
|
| Schriftenreihe: | Princeton Series in Astrophysics
55 |
| Schlagwörter: | |
| Links: | https://doi.org/10.1515/9780691221663?locatt=mode:legacy https://doi.org/10.1515/9780691221663?locatt=mode:legacy https://doi.org/10.1515/9780691221663?locatt=mode:legacy https://doi.org/10.1515/9780691221663?locatt=mode:legacy https://doi.org/10.1515/9780691221663?locatt=mode:legacy https://doi.org/10.1515/9780691221663?locatt=mode:legacy https://doi.org/10.1515/9780691221663 |
| Zusammenfassung: | 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 |
| Beschreibung: | Description based on online resource; title from PDF title page (publisher's Web site, viewed 06. Jan 2021) |
| Umfang: | 1 online resource 67 tables, 119 line drawings |
| ISBN: | 9780691221663 |
| DOI: | 10.1515/9780691221663 |
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| 520 | |a 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 | ||
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| 650 | 4 | |a valley of stability | |
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| id | DE-604.BV047111921 |
| illustrated | Not Illustrated |
| indexdate | 2025-02-18T19:09:33Z |
| institution | BVB |
| isbn | 9780691221663 |
| language | English |
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| physical | 1 online resource 67 tables, 119 line drawings |
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| publishDate | 2020 |
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| spelling | Arnett, David Verfasser aut Supernovae and Nucleosynthesis An Investigation of the History of Matter, from the Big Bang to the Present David Arnett Princeton, NJ Princeton University Press [2020] © 1996 1 online resource 67 tables, 119 line drawings txt rdacontent c rdamedia cr rdacarrier Princeton Series in Astrophysics 55 Description based on online resource; title from PDF title page (publisher's Web site, viewed 06. Jan 2021) 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 In English Kepler Lagrangian coordinates Ledoux criterion O shell burning absorption lines;accretion;alpha decay;angular momentum;backward differencing;baryogenesis;burning stages;chaos;Chandrasekhar mass;coulomb repulsion;curve of growth;deflagration;decoupling;deuterium;energy generation rate;expansional cooling;explosive time-scale;Fermi selection rules;freezeout;Galactic disk;gamma emission;gravitational contraction;helium burning hydrodynamics hydrogen burning ignition mass implicit differencing ionization lepton number magic numbers mass-luminosity relation mixing-length theory molecular clouds neutral currents numerical instability overproduction pairing energy photoelectric effect quartic radiation entropy radiation pressure shock emergence solar neighborhood spectral types stiff equations turbulent pressure uniform approximation valley of stability SCIENCE / Physics / Astrophysics bisacsh https://doi.org/10.1515/9780691221663 Verlag URL des Erstveröffentlichers Volltext |
| spellingShingle | Arnett, David Supernovae and Nucleosynthesis An Investigation of the History of Matter, from the Big Bang to the Present Kepler Lagrangian coordinates Ledoux criterion O shell burning absorption lines;accretion;alpha decay;angular momentum;backward differencing;baryogenesis;burning stages;chaos;Chandrasekhar mass;coulomb repulsion;curve of growth;deflagration;decoupling;deuterium;energy generation rate;expansional cooling;explosive time-scale;Fermi selection rules;freezeout;Galactic disk;gamma emission;gravitational contraction;helium burning hydrodynamics hydrogen burning ignition mass implicit differencing ionization lepton number magic numbers mass-luminosity relation mixing-length theory molecular clouds neutral currents numerical instability overproduction pairing energy photoelectric effect quartic radiation entropy radiation pressure shock emergence solar neighborhood spectral types stiff equations turbulent pressure uniform approximation valley of stability SCIENCE / Physics / Astrophysics bisacsh |
| title | Supernovae and Nucleosynthesis An Investigation of the History of Matter, from the Big Bang to the Present |
| title_auth | Supernovae and Nucleosynthesis An Investigation of the History of Matter, from the Big Bang to the Present |
| title_exact_search | Supernovae and Nucleosynthesis An Investigation of the History of Matter, from the Big Bang to the Present |
| title_full | Supernovae and Nucleosynthesis An Investigation of the History of Matter, from the Big Bang to the Present David Arnett |
| title_fullStr | Supernovae and Nucleosynthesis An Investigation of the History of Matter, from the Big Bang to the Present David Arnett |
| title_full_unstemmed | Supernovae and Nucleosynthesis An Investigation of the History of Matter, from the Big Bang to the Present David Arnett |
| title_short | Supernovae and Nucleosynthesis |
| title_sort | supernovae and nucleosynthesis an investigation of the history of matter from the big bang to the present |
| title_sub | An Investigation of the History of Matter, from the Big Bang to the Present |
| topic | Kepler Lagrangian coordinates Ledoux criterion O shell burning absorption lines;accretion;alpha decay;angular momentum;backward differencing;baryogenesis;burning stages;chaos;Chandrasekhar mass;coulomb repulsion;curve of growth;deflagration;decoupling;deuterium;energy generation rate;expansional cooling;explosive time-scale;Fermi selection rules;freezeout;Galactic disk;gamma emission;gravitational contraction;helium burning hydrodynamics hydrogen burning ignition mass implicit differencing ionization lepton number magic numbers mass-luminosity relation mixing-length theory molecular clouds neutral currents numerical instability overproduction pairing energy photoelectric effect quartic radiation entropy radiation pressure shock emergence solar neighborhood spectral types stiff equations turbulent pressure uniform approximation valley of stability SCIENCE / Physics / Astrophysics bisacsh |
| topic_facet | Kepler Lagrangian coordinates Ledoux criterion O shell burning absorption lines;accretion;alpha decay;angular momentum;backward differencing;baryogenesis;burning stages;chaos;Chandrasekhar mass;coulomb repulsion;curve of growth;deflagration;decoupling;deuterium;energy generation rate;expansional cooling;explosive time-scale;Fermi selection rules;freezeout;Galactic disk;gamma emission;gravitational contraction;helium burning hydrodynamics hydrogen burning ignition mass implicit differencing ionization lepton number magic numbers mass-luminosity relation mixing-length theory molecular clouds neutral currents numerical instability overproduction pairing energy photoelectric effect quartic radiation entropy radiation pressure shock emergence solar neighborhood spectral types stiff equations turbulent pressure uniform approximation valley of stability SCIENCE / Physics / Astrophysics |
| url | https://doi.org/10.1515/9780691221663 |
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