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The Theory of Stellar Evolution and Nucleosyntesis

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    0481858 - ASÚ 2018 RIV US eng C - Conference Paper (international conference)
    Klapp, J. C. - Bahena, David
    The Theory of Stellar Evolution and Nucleosyntesis.
    Proceedings of the 6th Mexican Nuclear Physics School. Melville: American Institute of Physics, 2010, s. 216-217. AIP Conference Proceedings, 1271. ISBN 9780735408203. ISSN 0094-243X.
    [Mexican Nuclear Physics School /6./. Mexico City (MX), 22.06.2009-03.07.2009]
    Institutional research plan: CEZ:AV0Z10030501
    Keywords : stellar evolution * nucleosynthesis * star formation
    OECD category: Atomic, molecular and chemical physics (physics of atoms and molecules including collision, interaction with radiation, magnetic resonances, Mössbauer effect)

    The structure and evolution of the stars is governed by the equations of hydrodynamics coupled to a nuclear reaction network and a detailed description of the relevant physics and chemist. In this work we present a simple and introductory description of the theory of stellar evolution and nucleosynthesis that could serve as a motivation to further study in this field of work.
    Permanent Link: http://hdl.handle.net/11104/0277323

     
     
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