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S - process production in the central helium burning of large masses ( M ⩾ 15 M⊙ )

  • II. Stellar Evolution, Nucleosynthesis and Isotopic Anomalies in Meteorites
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Nuclear Astrophysics

Part of the book series: Lecture Notes in Physics ((LNP,volume 287))

Abstract

From these computations one gets some general indications:

  1. 1)

    If the hypothesis of the B.P.is true, they may increase the s-process production by a factor of 4 – 5 in the range ofmass number 60 : 70 (in the 15 Me Y = 0.28 and Z = 0.02).

  2. 2)

    Theeffect of the newC 12 (a,7)rate is again to slightly increase the production of s-elements in the range of mass number 60 - 70 by a factor of 2 (in the 25 Me Y = 0.25 Z = 0.003).

We are now computing models of different masses and chemical composition to obtain more detailed information on the effect of this new physics on the production of s - elements.

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Wolfgang Hillebrandt Rudolf Kuhfuß Ewald Müller James W. Truran

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© 1987 Springer-Verlag

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Bencivenni, D., Castellani, V., Chieffi, A. (1987). S - process production in the central helium burning of large masses ( M ⩾ 15 M⊙ ). In: Hillebrandt, W., Kuhfuß, R., Müller, E., Truran, J.W. (eds) Nuclear Astrophysics. Lecture Notes in Physics, vol 287. Springer, Berlin, Heidelberg. https://doi.org/10.1007/BFb0016581

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  • DOI: https://doi.org/10.1007/BFb0016581

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-18279-5

  • Online ISBN: 978-3-540-47869-0

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