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Nuclear Astrophysics: Evolution of Stars from Hydrogen Burning to Supernova Explosion

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Solar, Stellar and Galactic Connections Between Particle Physics and Astrophysics

Part of the book series: Astrophysics and Space Science Proceedings ((ASSSP))

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Abstract

Nuclear astrophysics has developed in the last twenty years into one of the most important subfields of ‘applied’ nuclear physics. It is a truly interdisciplinary field, concentrating on primordial and stellar nucleosynthesis, stellar evolution, and the interpretation of cataclysmic stellar events like novae and supernovae.

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Author information

Authors and Affiliations

  1. Gesellschaft für Schwerionenforschung, Technische Universität Darmstadt, D-64291, Darmstadt, Germany

    K. Langanke

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  1. K. Langanke
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Editor information

Editors and Affiliations

  1. Instituto Nacional de Astofísica, Óptica y Electrónica, Tonantzintla, México

    Alberto Carramiñana

  2. Instituto de Física y Matemáticas, Universidad Michoacana de San Nicolás de Hidalgo, México

    Francisco Siddhartha Guzmán

  3. Centro de Investigación y Estudios Avanzados del IPN, México DF, México

    Tonatiuh Matos

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Langanke, K. (2007). Nuclear Astrophysics: Evolution of Stars from Hydrogen Burning to Supernova Explosion. In: Carramiñana, A., Guzmán, F.S., Matos, T. (eds) Solar, Stellar and Galactic Connections Between Particle Physics and Astrophysics. Astrophysics and Space Science Proceedings. Springer, Dordrecht. https://doi.org/10.1007/978-1-4020-5575-1_1

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