Actinide Production in the Neutron-rich Ejecta of a Neutron Star Merger
Journal Article
·
· The Astrophysical Journal (Online)
- Univ. of Notre Dame, IN (United States); Joint Inst. for Nuclear Astrophysics (JINA), East Lansing, MI (United States)
- Univ. of Notre Dame, IN (United States)
- Joint Inst. for Nuclear Astrophysics (JINA), East Lansing, MI (United States); Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
- Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
The rapid neutron-capture ("r-") process is responsible for synthesizing many of the heavy elements observed in both the solar system and Galactic metal-poor halo stars. Simulations of r-process nucleosynthesis can reproduce abundances derived from observations with varying success, but so far they fail to account for the observed overenhancement of actinides, present in about 30% of r-process-enhanced stars. In this work, we investigate actinide production in the dynamical ejecta of a neutron star merger (NSM) and explore whether varying levels of neutron-richness can reproduce the actinide boost. We also investigate the sensitivity of actinide production on nuclear physics properties: fission distribution, β-decay, and mass model. For most cases, the actinides are overproduced in our models if the initial conditions are sufficiently neutron-rich for fission cycling. Here, we find that actinide production can be so robust in the dynamical ejecta that an additional lanthanide-rich, actinide-poor component is necessary in order to match observations of actinide-boost stars. We present a simple actinide-dilution model that folds in estimated contributions from two nucleosynthetic sites within a merger event. Our study suggests that while the dynamical ejecta of an NSM are likely production sites for the formation of actinides, a significant contribution from another site or sites (e.g., the NSM accretion disk wind) is required to explain abundances of r-process-enhanced, metal-poor stars.
- Research Organization:
- Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
- Sponsoring Organization:
- National Science Foundation (NSF); USDOE National Nuclear Security Administration (NNSA); USDOE Office of Science (SC). Nuclear Physics (NP)
- Grant/Contract Number:
- 89233218CNA000001; AC52-06NA25396; AC52-07NA27344; SC0013039; SC0018232
- OSTI ID:
- 1768516
- Report Number(s):
- LA-UR--18-29300
- Journal Information:
- The Astrophysical Journal (Online), Journal Name: The Astrophysical Journal (Online) Journal Issue: 1 Vol. 870; ISSN 1538-4357
- Publisher:
- Institute of Physics (IOP)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
Similar Records
Contribution of neutron star mergers to the r-process chemical evolution in the hierarchical galaxy formation
MeV Gamma Rays from Fission: A Distinct Signature of Actinide Production in Neutron Star Mergers
Actinide-rich and Actinide-poor r -process-enhanced Metal-poor Stars Do Not Require Separate r -process Progenitors
Journal Article
·
Thu Oct 20 00:00:00 EDT 2016
· Astrophysical Journal
·
OSTI ID:22868589
MeV Gamma Rays from Fission: A Distinct Signature of Actinide Production in Neutron Star Mergers
Journal Article
·
Thu Oct 22 20:00:00 EDT 2020
· The Astrophysical Journal. Letters (Online)
·
OSTI ID:1736327
Actinide-rich and Actinide-poor r -process-enhanced Metal-poor Stars Do Not Require Separate r -process Progenitors
Journal Article
·
Mon Aug 05 20:00:00 EDT 2019
· The Astrophysical Journal (Online)
·
OSTI ID:1565905