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Author: David Arnett
Publisher: Princeton University Press
ISBN: 0691221669
Category : Science
Languages : en
Pages : 598
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Book Description
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.
Author: David Arnett
Publisher: Princeton University Press
ISBN: 0691221669
Category : Science
Languages : en
Pages : 598
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Book Description
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.
Author: Bernard Ephraim Julius Pagel
Publisher: Cambridge University Press
ISBN: 0521840309
Category : Science
Languages : en
Pages : 485
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Book Description
A lucid introduction for advanced undergraduates and graduate students, and an authoritative overview for researchers and professional scientists.
Author: A. G. W. Cameron
Publisher: Courier Corporation
ISBN: 0486498557
Category : Science
Languages : en
Pages : 210
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Book Description
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.
Author: Donald D. Clayton
Publisher: University of Chicago Press
ISBN: 0226109534
Category : Science
Languages : en
Pages : 634
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Book Description
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.
Author: Athem W. Alsabti
Publisher:
ISBN: 9783319207940
Category : Supernovae
Languages : en
Pages :
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Book Description
Author: Sean G. Ryan
Publisher: Cambridge University Press
ISBN: 9780521196093
Category : Nature
Languages : en
Pages : 244
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Book Description
An ideal bridging text for astrophysics and physics majors looking to move on from the introductory texts.
Author: Alba Formicola
Publisher: Springer Nature
ISBN: 3030138763
Category : Science
Languages : en
Pages : 495
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Book Description
These peer-reviewed NIC XV conference proceedings present the latest major advances in nuclear physics, astrophysics, astronomy, cosmochemistry and neutrino physics, which provide the necessary framework for a microscopic understanding of astrophysical processes. The book also discusses future directions and perspectives in the various fields of nuclear astrophysics research. In addition, it also includes a limited number of section of more general interest on double beta decay and dark matter.
Author: Jacco Vink
Publisher: Springer Nature
ISBN: 3030552314
Category : Science
Languages : en
Pages : 532
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Book Description
Written by a leading expert, this monograph presents recent developments on supernova remnants, with the inclusion of results from various satellites and ground-based instruments. The book details the physics and evolution of supernova remnants, as well as provides an up-to-date account of recent multiwavelength results. Supernova remnants provide vital clues about the actual supernova explosions from X-ray spectroscopy of the supernova material, or from the imprints the progenitors had on the ambient medium supernova remnants are interacting with - all of which the author discusses in great detail. The way in which supernova remnants are classified, is reviewed and explained early on. A chapter is devoted to the related topic of pulsar wind nebulae, and neutron stars associated with supernova remnants. The book also includes an extended part on radiative processes, collisionless shock physics and cosmic-ray acceleration, making this book applicable to a wide variety of astronomical sub-disciplines. With its coverage of fundamental physics and careful review of the state of the field, the book serves as both textbook for advanced students and as reference for researchers in the field.
Author: Richard Boyd
Publisher: Springer Science & Business Media
ISBN: 146141332X
Category : Science
Languages : en
Pages : 223
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Book Description
Where were the amino acids, the molecules of life, created: perhaps in a lightning storm in the early Earth, or perhaps elsewhere in the cosmos? This book argues that at least some of them must have been produced in the cosmos, and that the fact that the Earthly amino acids have a specific handedness provides an important clue for that explanation. The book discusses several models that purport to explain the handedness, ultimately proposing a new explanation that involves cosmic processing of the amino acids produced in space. The book provides a tour for laypersons that includes a definition of life, the Big Bang, stellar nucleosynthesis, the electromagnetic spectrum, molecules, and supernovae and the particles they produce.
Author: Jordi Jose
Publisher: CRC Press
ISBN: 1439853088
Category : Science
Languages : en
Pages : 467
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Book Description
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
