2006
DOI: 10.1086/500786
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r‐Process Nucleosynthesis in Magnetohydrodynamic Jet Explosions of Core‐Collapse Supernovae

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Cited by 128 publications
(178 citation statements)
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References 41 publications
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“…In the relatively cool regime of T < 9 ; 10 9 K, NSE breaks down and the chemical composition is calculated with a large nuclear reaction network (network B in Nishimura et al 2006). The network includes about 4000 nuclei from neutrons and protons up to fermium, whose atomic number Z = 100 (see Table 1 of Nishimura et al 2006).…”
Section: Nuclear Reaction Networkmentioning
confidence: 99%
“…In the relatively cool regime of T < 9 ; 10 9 K, NSE breaks down and the chemical composition is calculated with a large nuclear reaction network (network B in Nishimura et al 2006). The network includes about 4000 nuclei from neutrons and protons up to fermium, whose atomic number Z = 100 (see Table 1 of Nishimura et al 2006).…”
Section: Nuclear Reaction Networkmentioning
confidence: 99%
“…Nearly all models in the current literature with a rapid freezeout (including the MHDJ [38][39][40][41][42][43][44]) show this underproduction if the final abundances are normalized to the abundance peaks. It was pointed out in [27], however, that a solution to the underproduction of nuclei above and below the r-process abundance peaks can be obtained if one considers that a fission recycling environment (e.g.…”
Section: Current Models For the R-processmentioning
confidence: 99%
“…In the magneto-hydrodynamic jet (MHDJ) supernova model [38][39][40] magnetic turbulence leads the ejection of neutron rich material into a jet. As the jet transports this neutron-rich material away from the star it can undergo r-process nucleosynthesis in a way that avoids the problems associated with neutrino interactions in the NDW model.…”
Section: Current Models For the R-processmentioning
confidence: 99%
“…Optical and near-infrared observations of such an event, accompanying the short-duration GRB130603B have been reported [71] (see also [4]). After the first detailed nucleosynthesis predictions (following ideas of [33]) of such an event [13], many more and more sophisticated investigations have been undertaken, involving quite a number of authors [5,12,16,17,27,32,39,42,51,56,61,78] as well as the black hole accretion disk system after the formation of a central black hole [27,70,78,82].…”
Section: Neutron Star Mergersmentioning
confidence: 99%