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Title: Reverse engineering nuclear properties from rare earth abundances in the r process

Journal Article · · Journal of Physics. G, Nuclear and Particle Physics
ORCiD logo [1];  [2];  [3]; ORCiD logo [4]
  1. Los Alamos National Lab. (LANL), Los Alamos, NM (United States)
  2. North Carolina State Univ., Raleigh, NC (United States). Dept. of Physics
  3. Univ. of Notre Dame, IN (United States). Dept. of Physics
  4. Univ. of Tennessee, Knoxville, TN (United States). Dept. of Physics and Astronomy; Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States). Physics Division

The bulk of the rare earth elements are believed to be synthesized in the rapid neutron capture process or r process of nucleosynthesis. The solar r-process residuals show a small peak in the rare earths around $$A\sim 160$$, which is proposed to be formed dynamically during the end phase of the r process by a pileup of material. This abundance feature is of particular importance as it is sensitive to both the nuclear physics inputs and the astrophysical conditions of the main r process. We explore the formation of the rare earth peak from the perspective of an inverse problem, using Monte Carlo studies of nuclear masses to investigate the unknown nuclear properties required to best match rare earth abundance sector of the solar isotopic residuals. When nuclear masses are changed, we recalculate the relevant β-decay properties and neutron capture rates in the rare earth region. The feedback provided by this observational constraint allows for the reverse engineering of nuclear properties far from stability where no experimental information exists. We investigate a range of astrophysical conditions with this method and show how these lead to different predictions in the nuclear properties influential to the formation of the rare earth peak. We conclude that targeted experimental campaigns in this region will help to resolve the type of conditions responsible for the production of the rare earth nuclei, and will provide new insights into the longstanding problem of the astrophysical site(s) of the r process.

Research Organization:
Los Alamos National Laboratory (LANL), Los Alamos, NM (United States); Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States)
Sponsoring Organization:
USDOE Office of Science (SC), Nuclear Physics (NP); National Science Foundation (NSF); USDOE National Nuclear Security Administration (NNSA)
Grant/Contract Number:
AC52-06NA25396; SC0013039; FG02-02ER41216; PHY1554876; PHY0822648; PHY1419765
OSTI ID:
1419747
Alternate ID(s):
OSTI ID: 1460177
Report Number(s):
LA-UR-16-27225; TRN: US1801383
Journal Information:
Journal of Physics. G, Nuclear and Particle Physics, Vol. 44, Issue 3; ISSN 0954-3899
Publisher:
IOP PublishingCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 28 works
Citation information provided by
Web of Science

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The r-process of stellar nucleosynthesis: Astrophysics and nuclear physics achievements and mysteries text January 2007
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The impact of individual nuclear masses on $r$-process abundances text January 2015
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Impact of nuclear mass uncertainties on the $r$-process text January 2015
The link between rare earth peak formation and the astrophysical site of the $r$ process text January 2016
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Spectroscopic Studies of Very Metal-Poor Stars with the Subaru High Dispersion Spectrograph. III. Light Neutron-Capture Elements text January 2005
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Microscopic mass formulae text January 1994
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Cited By (9)

Exploring the mass surface near the rare-earth abundance peak via precision mass measurements at JYFLTRAP journal March 2020
Masses and β -Decay Spectroscopy of Neutron-Rich Odd-Odd Eu 160 , 162 Nuclei: Evidence for a Subshell Gap with Large Deformation at N = 98 journal May 2018
r -process nucleosynthesis: connecting rare-isotope beam facilities with the cosmos journal July 2019
β -delayed Fission in r -process Nucleosynthesis journal December 2018
Influence of nuclear mass uncertainties on radiative neutron-capture rates journal August 2019
Precision Mass Measurements on Neutron-Rich Rare-Earth Isotopes at JYFLTRAP: Reduced Neutron Pairing and Implications for r -Process Calculations journal June 2018
Precision Mass Measurements of Neutron-Rich Neodymium and Samarium Isotopes and Their Role in Understanding Rare-Earth Peak Formation journal June 2018
Precision mass measurements on neutron-rich rare-earth isotopes at JYFLTRAP - reduced neutron pairing and implications for the $r$-process calculations text January 2018
Exploring the mass surface near the rare-earth abundance peak via precision mass measurements at JYFLTRAP text January 2019