Speaker
Description
Recent neutron-star merger observations have provided r-process abundance constraints, which has led to significant attention towards additional neutron-capture processes such as the i-process and n-process. Working between the rates and environmental neutron densities of the r-process and s-process, their reaction pathways and abundance contributions are not yet fully characterized. Operating in densities of 10
This contribution will review the β-Oslo analysis of
Your Email | bgreaves@uoguelph.ca |
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Supervisor | Carl Svensson |
Supervisor Email | sven@uoguelph.ca |
Funding Agency | NSERC |