r-Process Nucleosynthesis in Black Hole-Neutron Star Mergers
- Union College
- North Carolina State University
- University of Edinburgh
- Max Planck Institut fur Astrophysik (MPA), Germany
- ORNL
Compact object mergers have long been speculated to be a possible site of r-process nucleosynthesis. While most attention has been focused on the cold decompression of neutron star matter ejected from the merger, other sites within the merger likely contribute to its nucleosynthetic output. Here we consider hot outflows from the accretion disk that forms around the black hole following a black hole- neutron star merger. We begin with the results of a three-dimensional numerical merger model and carefully calculate the neutrino and antineutrino fluxes emitted from the accretion disk. We find that neutrino interactions on free nucleons in the outflowing material result in neutron excesses such that at least a weak r-process is produced and in some cases a main r-process as well. Additionally, we find that the weak r-process pattern calculated for certain trajectories compares favorably to the pattern observed in a weak r-process-enhanced halo star.
- Research Organization:
- Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States). Holifield Radioactive Ion Beam Facility (HRIBF)
- Sponsoring Organization:
- USDOE Office of Science (SC)
- DOE Contract Number:
- DE-AC05-00OR22725
- OSTI ID:
- 958942
- Resource Relation:
- Conference: Nuclei in the Cosmos X, Mackinac Island, MI, USA, 20080727, 20080801
- Country of Publication:
- United States
- Language:
- English
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