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Title: Impact of individual nuclear masses on r -process abundances

Journal Article · · Physical Review C, Nuclear Physics
 [1];  [1];  [2];  [1];  [3];  [3];  [1]
  1. Univ. of Notre Dame, Notre Dame, IN (United States); Michigan State Univ., East Lansing, MI (United States)
  2. Michigan State Univ., East Lansing, MI (United States)
  3. Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)

We have performed for the first time a comprehensive study of the sensitivity of r-process nucleosynthesis to individual nuclear masses across the chart of nuclides. Using the latest version (2012) of the Finite-Range Droplet Model, we consider mass variations of ±0.5 MeV and propagate each mass change to all affected quantities, including Q values, reaction rates, and branching ratios. We find such mass variations can result in up to an order of magnitude local change in the final abundance pattern produced in an r-process simulation. As a result, we identify key nuclei whose masses have a substantial impact on abundance predictions for hot, cold, and neutron star merger r-process scenarios and could be measured at future radioactive beam facilities.

Research Organization:
Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
Sponsoring Organization:
USDOE
Grant/Contract Number:
PHY0822648; PHY1419765; SC0013039; AC52-06NA25396
OSTI ID:
1233554
Alternate ID(s):
OSTI ID: 1215769
Report Number(s):
LA-UR-15-24098; PRVCAN
Journal Information:
Physical Review C, Nuclear Physics, Vol. 92, Issue 3; ISSN 0556-2813
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 65 works
Citation information provided by
Web of Science

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Neutrino-driven wind simulations and nucleosynthesis of heavy elements text January 2012
Neutrino oscillations above black hole accretion disks: disks with electron-flavor emission text January 2012
Sensitivity of the r-process to nuclear masses text January 2012
Effect of a High Opacity on the Light Curves of Radioactively Powered Transients from Compact Object Mergers text January 2013
An r-Process Kilonova Associated with the Short-Hard GRB 130603B text January 2013
Sensitivity studies for r-process nucleosynthesis in three astrophysical scenarios text January 2013
Neutron-Capture Nucleosynthesis in the First Stars text January 2014
Comprehensive nucleosynthesis analysis for ejecta of compact binary mergers text January 2014
Transient Events from Neutron Star Mergers text January 1998
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Cited By (16)

Reverse engineering nuclear properties from rare earth abundances in the r process journal February 2017
r -process nucleosynthesis: connecting rare-isotope beam facilities with the cosmos journal July 2019
Using excitation-energy dependent fission yields to identify key fissioning nuclei in r -process nucleosynthesis journal April 2019
Influence of nuclear mass uncertainties on radiative neutron-capture rates journal August 2019
The Origin of r -process Elements in the Milky Way journal March 2018
β -delayed Fission in r -process Nucleosynthesis journal December 2018
Actinide Production in the Neutron-rich Ejecta of a Neutron Star Merger journal December 2018
Gamma Rays from Kilonova: A Potential Probe of r -process Nucleosynthesis journal February 2020
Impact of nuclear mass uncertainties on the $r$-process text January 2015
Reverse engineering nuclear properties from rare earth abundances in the $r$ process text January 2016
Refining mass formulas for astrophysical applications: a Bayesian neural network approach text January 2017
Validating neural-network refinements of nuclear mass models text January 2017
Precision mass measurements on neutron-rich rare-earth isotopes at JYFLTRAP - reduced neutron pairing and implications for the $r$-process calculations text January 2018
Using excitation-energy dependent fission yields to identify key fissioning nuclei in r-process nucleosynthesis text January 2018
Gamma-rays from kilonova: a potential probe of r-process nucleosynthesis text January 2019
Exploring the mass surface near the rare-earth abundance peak via precision mass measurements at JYFLTRAP text January 2019

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