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dc.contributor.authorThielemann, Friedrich-Karl
dc.contributor.authorFroehlich, Carla
dc.contributor.authorHirschi, R.
dc.contributor.authorLiebendoerfer, M.
dc.contributor.authorDillmann, I.
dc.contributor.authorMocelj, D.
dc.contributor.authorRauscher, T.
dc.contributor.authorMartinez-Pinedo, G.
dc.contributor.authorLanganke, K.
dc.contributor.authorFarouqi, K.
dc.contributor.authorKratz, K.L.
dc.contributor.authorPfeiffer, B.
dc.contributor.authorPanov, I.
dc.contributor.authorNadyozhin, D. K.
dc.contributor.authorBlinnikov, S.
dc.contributor.authorBravo, E.
dc.contributor.authorHix, W. R.
dc.contributor.authorHoflich, P.
dc.contributor.authorZinner, N. T.
dc.date.accessioned2014-12-04T09:44:37Z
dc.date.available2014-12-04T09:44:37Z
dc.date.issued2007
dc.identifier.citationThielemann , F-K , Froehlich , C , Hirschi , R , Liebendoerfer , M , Dillmann , I , Mocelj , D , Rauscher , T , Martinez-Pinedo , G , Langanke , K , Farouqi , K , Kratz , K L , Pfeiffer , B , Panov , I , Nadyozhin , D K , Blinnikov , S , Bravo , E , Hix , W R , Hoflich , P & Zinner , N T 2007 , Production of intermediate-mass and heavy nuclei . in Progress in Particle and Neclear Physics . Progress in Particle and Nuclear Physics , no. 1 , vol. 59 , Elsevier , pp. 74-93 , International Workshop on Nuclear Physics/28th Course Radioactive Beams, Nuclear Dynamics and Astrophysics , Erice , Italy , 16/09/06 . https://doi.org/10.1016/j.ppnp.2006.12.019
dc.identifier.citationconference
dc.identifier.issn0146-6410
dc.identifier.otherPURE: 1624361
dc.identifier.otherPURE UUID: fc8df63c-4660-4e6e-b5c0-1b56c7567ec8
dc.identifier.otherWOS: 000248204700008
dc.identifier.otherScopus: 34248367435
dc.identifier.urihttp://hdl.handle.net/2299/14877
dc.description.abstractNucleosynthesis is the science related to all astrophysical processes which are responsible for the abundances of the elements and their isotopes in the universe. The astrophysical sites are the big bang and stellar objects. The working of nucleosynthesis processes is presented in a survey of events which act as abundance sources. For intermediate-mass and heavy elements, these are stellar evolution, type la and core collapse supernovae as well as hypernovae. We discuss successes and failures of existing processes and possible solutions via new (hitherto unknown) processes. Finally an analysis of their role is given in the puzzle to explain the evolution of the elemental and isotopic compositions found in galaxies, and especially the mixture found in the solar system. Different timescales due to the progenitor mass dependence of the endpoints of stellar evolution (type II supemova. explosions - SNe II vs. planetary nebulae) or single vs. binary stellar systems (the latter being responsible for novae, type la supernovae - SNe la, or X-ray bursts) are the keys to understand galactic evolution. At very early times, the role of explosion energies of events, polluting pristine matter with a composition originating only from the big bang, might also play a role. We also speculate on the role of very massive stars not undergoing SN II explosions but rather causing "hypernovae" after the formation of a central black hole via core collapse. @ 2007 Published by Elsevier B.V.en
dc.format.extent20
dc.language.isoeng
dc.publisherElsevier
dc.relation.ispartofProgress in Particle and Neclear Physics
dc.relation.ispartofseriesProgress in Particle and Nuclear Physics
dc.subjectTHERMONUCLEAR REACTION-RATES
dc.subjectSTATISTICAL-MODEL CALCULATIONS
dc.subjectBIG-BANG NUCLEOSYNTHESIS
dc.subjectR-PROCESS NUCLEOSYNTHESIS
dc.subjectIA SUPERNOVAE
dc.subjectMETAL-POOR STARS
dc.subjectASTROPHYSICAL REACTION-RATES
dc.subjectNEUTRINO-DRIVEN WINDS
dc.subjectCORE-COLLAPSE SUPERNOVAE
dc.subjectGALACTIC CHEMICAL EVOLUTION
dc.titleProduction of intermediate-mass and heavy nucleien
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research
rioxxterms.versionofrecordhttps://doi.org/10.1016/j.ppnp.2006.12.019
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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