Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008phdt........21b&link_type=abstract
Proquest Dissertations And Theses 2008. Section 0155, Part 0606 103 pages; [Ph.D. dissertation].United States -- North Carolina
Astronomy and Astrophysics
Astrophysics
Neutrinos, Neutron Capture, Fission Cycling, Supernova, Nucleosynthesis
Scientific paper
A long-standing problem in the field of nuclear astrophysics is the question of which astrophysical environment(s) serves as a host to the elemental production process known as the r -process. The r -process is the sequence of nuclear reactions that is responsible for producing the heaviest elements in nature and generates about half of the solar system abundance of nuclei with A >= 100. While the basic recipe for generating r -process elements is understood, the production of heavy nuclei through repetitions of neutron capture and b-decay, determining the astrophysical production site of the r -process has remained elusive. We examine how the r -process environment would be affected by the presence of a sterile neutrino, and we find that the resulting conditions yield an r -process that can reproduce the observed r -process abundance pattern more closely than other models of the r -process. We explore the r -process under conditions where both fission cycling and steady-b flow obtain and find that these mechanisms can jointly operate in the r -process to yield an abundance pattern that reproduces the features of the halo star data. We have examined the role that individual neutron capture cross sections play in the r -process and, contrary to conventional wisdom, find that the evolution of the r -process is sensitive to the neutron capture cross sections of certain, critical nuclei.
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