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- W1635249150 abstract "We give an overview of explosive burning and the role which neutron and/or proton separation energies play. We focus then on the rapid neutron capture process (r-process) which encounters unstable nuclei with neutron separation energies in the range 1-4 MeV, and the rapid proton capture process (rp-process), operating close to the proton drip-line. The site of the rp-process is related to hydrogen accreting neutron stars in binary stellar systems. Explosive II-burning produces nuclei as heavy as A=100, powering events observable as X-ray bursts. The r-process abundances witness nuclear structure far from beta-stability as well as the conditions in the appropriate astrophysical environment. But there is a remaining lack in the full understanding of its astrophysical origin, ranging from the high entropy neutrino wind, blown from hot neutron star surfaces after a supernova explosion, to low entropy ``cold decompresssion`` of neutron star matter ejected in mergers of binary neutron star systems." @default.
- W1635249150 created "2016-06-24" @default.
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- W1635249150 date "1998-11-01" @default.
- W1635249150 modified "2023-09-27" @default.
- W1635249150 title "EXPLOSIVE NUCLEOSYNTHESIS CLOSE TO THE DRIP LINES" @default.
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