Following nuclei through nucleosynthesis: a novel tracing technique
arXiv:2008.06075 · doi:10.1103/PhysRevC.104.015803
Abstract
Astrophysical nucleosynthesis is a family of diverse processes by which atomic nuclei undergo nuclear reactions and decays to form new nuclei. The complex nature of nucleosynthesis, which can involve as many as tens of thousands of interactions between thousands of nuclei, makes it difficult to study any one of these interactions in isolation using standard approaches. In this work, we present a new technique, nucleosynthesis tracing, that we use to quantify the specific role of individual nuclear reaction, decay, and fission processes in relationship to nucleosynthesis as a whole. We apply this technique to study fission and -decay as they occur in the rapid neutron capture () process of nucleosynthesis.
18 pages, 10 figures
References in corpus (15)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Multi-messenger Observations of a Binary Neutron Star Merger
- The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models
- Current Status of r-Process Nucleosynthesis
- SkyNet: A modular nuclear reaction network library
- Dynamical r-process studies within the neutrino-driven wind scenario and its sensitivity to the nuclear physics input
- Uncertainty Quantification for Nuclear Density Functional Theory and Information Content of New Measurements
- Quantified limits of the nuclear landscape
- Primary fission fragment mass yields across the chart of nuclides
- Cold r-Process in Neutrino-Driven Winds
- Neutron-gamma competition for -delayed neutron emission
- Estimation of M1 scissors mode strength for deformed nuclei in the medium to heavy mass region by statistical Hauser-Feshbach model calculations
- Fission Cycling in a Supernova r-process
- Co-production of light and heavy -process elements via fission deposition
- Efficient method for estimation of fission fragment yields of r-process nuclei
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