eBook PDF / e-Pub Stellar Evolution Physics: Volume 1, Physical Processes in Stellar Interiors

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Title:Stellar Evolution Physics: Volume 1, Physical Processes in Stellar Interiors
Format Type:Ebook
Author:
Publisher:Cambridge University Press
ISBN:1139786393
ISBN 13:
Number of Pages:864
Category:Manga

Stellar Evolution Physics: Volume 1, Physical Processes in Stellar Interiors by Icko Iben Jr.

PDF, EPUB, MOBI, TXT, DOC Stellar Evolution Physics: Volume 1, Physical Processes in Stellar Interiors This text describes the microscopic physics operating in stars and demonstrates how stars respond from formation through hydrogen burning phases up to the onset of helium burning Intended for beginning graduate students and senior undergraduates with a solid background in physics it illustrates the intricate interplay between the microscopic physical processes and the stars macroscopic responses The volume starts with the gravitationally contracting phase which carries the star from formation to the core hydrogen burning main sequence through the main sequence phase through shell hydrogen burning phases as a red giant up to the onset of core helium burning Particular emphasis is placed on describing the gravothermal responses of stars to nuclear transformations in the interior and energy loss from the surface responses which express the very essence of stellar evolution The volume is replete with many illustrations and detailed numerical solutions to prepare the reader to program and calculate evolutionary models

  • Stellar Evolution Physics

    This book Home of eBook - Stellar Evolution Physics - This text describes the microscopic physics operating in stars and demonstrates how stars respond from formation through hydrogen burning phases up to the onset...

    Read Online
  • Stellar Evolution Physics: Volume 2, Advanced Evolution of Single Stars

    This book Home of eBook - Stellar Evolution Physics: Volume 2, Advanced Evolution of Single Stars - This volume explains the microscopic physics operating in stars in advanced stages of their evolution and describes with many numerical examples and illustratio...

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  • Stellar Evolution Physics: Volume 1, Physical Processes in Stellar Interiors

    This book Home of eBook - Stellar Evolution Physics: Volume 1, Physical Processes in Stellar Interiors - This text describes the microscopic physics operating in stars and demonstrates how stars respond from formation through hydrogen burning phases up to the onset...

    Read Online
  • Stellar Evolution Physics 2 Volume Set

    This book Home of eBook - Stellar Evolution Physics 2 Volume Set - In Stellar Evolution Physics Icko Iben describes the microscopic physics operating in stars and how stars respond macroscopically showing the intricate interpla...

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Stellar Evolution Physics: Volume 2, Advanced Evolution of Single Stars, Stellar Evolution Physics 2 Volume Set, Stellar Evolution Physics: Volume 1, Physical Processes in Stellar Interiors, Stellar Evolution Physics
In Stellar Evolution Physics Icko Iben describes the microscopic physics operating in stars and how stars respond macroscopically showing the intricate interplay between these processes Volume intended for graduate students with a solid background in physics covers the processes up to the onset of helium burning Volume builds on these principles covering models of low and intermediate mass stars the AGB phase the final cooling white dwarf phase and a model for a massive star Particular attention is given to the gravothermal responses to nuclear reaction induced transformations in the interior and energy loss from the surface responses at the heart of stellar evolution The volumes include over illustrations and many numerical solutions in order to prepare the reader to program and calculate evolutionary models for themselves Taken together the two volumes will prepare a graduate student for professional level research in this key area of astrophysics, This volume explains the microscopic physics operating in stars in advanced stages of their evolution and describes with many numerical examples and illustrations how they respond to this microphysics Models of low and intermediate mass are evolved through the core helium burning phase the asymptotic giant branch phase alternating shell hydrogen and helium burning and through the final cooling white dwarf phase A massive model is carried from the core helium burning phase through core and shell carbon burning phases Gravothermal responses to nuclear reaction induced transformations and energy loss from the surface are described in detail Written for senior graduate students and researchers who have mastered the principles of stellar evolution as developed in the first volume of Stellar Evolution Physics sufficient attention is paid to how numerical solutions are obtained to enable the reader to engage in model construction on a professional level, This text describes the microscopic physics operating in stars and demonstrates how stars respond from formation through hydrogen burning phases up to the onset of helium burning Intended for beginning graduate students and senior undergraduates with a solid background in physics it illustrates the intricate interplay between the microscopic physical processes and the stars macroscopic responses The volume starts with the gravitationally contracting phase which carries the star from formation to the core hydrogen burning main sequence through the main sequence phase through shell hydrogen burning phases as a red giant up to the onset of core helium burning Particular emphasis is placed on describing the gravothermal responses of stars to nuclear transformations in the interior and energy loss from the surface responses which express the very essence of stellar evolution The volume is replete with many illustrations and detailed numerical solutions to prepare the reader to program and calculate evolutionary models, This text describes the microscopic physics operating in stars and demonstrates how stars respond from formation through hydrogen burning phases up to the onset of helium burning Intended for beginning graduate students and senior undergraduates with a solid background in physics it illustrates the intricate interplay between the microscopic physical processes and the stars macroscopic responses The volume starts with the gravitationally contracting phase which carries the star from formation to the core hydrogen burning main sequence through the main sequence phase through shell hydrogen burning phases as a red giant up to the onset of core helium burning Particular emphasis is placed on describing the gravothermal responses of stars to nuclear transformations in the interior and energy loss from the surface responses which express the very essence of stellar evolution The volume is replete with many illustrations and detailed numerical solutions to prepare the reader to program and calculate evolutionary models