A new method for nuclear-reaction network analysis, element production in S-Cl region during the He and C burning in 25 Ms stars

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dc.creatorSzalanski, P.
dc.creatorPadureanu, I.
dc.creatorStepinski, M.
dc.creatorGledenov, Yu. M.
dc.creatorSedyshev, P. V.
dc.creatorMachrafi, R.
dc.creatorOprea, A.
dc.creatorAranghel, D.
dc.creatorMarganiec, J.
dc.date2002-11-27
dc.date2002-12-09
dc.date.accessioned2026-07-07T02:06:34Z
dc.date.available2026-07-07T02:06:34Z
dc.descriptionThis paper presents the results of calculation of element overproduction in the S-Cl region during helium and carbon burning in massive stars (25 Ms). Calculations for a given set of differential equations were performed using integrated mathematical systems. The authors think that this method may be successfully adopted for other physical problems in which solving nuclear-reaction network play an important role, in particular for the problem of transmutation of heavy elements and chemical kinetics.
dc.description8 pages, 3 figures, X International Seminar on Interaction of Neutrons with Nuclei (ISINN-10) "Neutron Spectroscopy, Nuclear Structure and Related Topics", Dubna (Russia), May 22-25, 2002
dc.identifierhttps://arxiv.org/abs/astro-ph/0211595
dc.identifierhttp://arxiv.org/abs/astro-ph/0211595
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5408
dc.subjectAstrophysics
dc.titleA new method for nuclear-reaction network analysis, element production in S-Cl region during the He and C burning in 25 Ms stars
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