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Title: Properties of Nuclei up to A = 16 using Local Chiral Interactions

Journal Article · · Physical Review Letters
ORCiD logo [1]; ORCiD logo [2]; ORCiD logo [2];  [3];  [4];  [5];  [6]
  1. Michigan State Univ., East Lansing, MI (United States). Facility for Rare Isotope Beams; Los Alamos National Lab. (LANL), Los Alamos, NM (United States). Theoretical Division
  2. Los Alamos National Lab. (LANL), Los Alamos, NM (United States). Theoretical Division
  3. Technical Univ. of Darmstadt (Germany). Inst. of Nuclear Physics; GSI Helmholtz Centre for Heavy Ion Research, Darmstadt (Germandy). ExtreMe Matter Inst. (EMMI)
  4. Arizona State Univ., Tempe, AZ (United States). Dept. of Physics
  5. Technical Univ. of Darmstadt (Germany). Inst. of Nuclear Physics; GSI Helmholtz Centre for Heavy Ion Research, Darmstadt (Germandy). ExtreMe Matter Inst. (EMMI); Max-Planck Inst. for Nuclear Physics, Heidelberg (Germany)
  6. Huzhou Univ. (China). School of Science

Here, we report accurate quantum Monte Carlo calculations of nuclei up to A = 16 based on local chiral two- and three-nucleon interactions up to next-to-next-to-leading order. We examine the theoretical uncertainties associated with the chiral expansion and the cutoff in the theory, as well as the associated operator choices in the three-nucleon interactions. While in light nuclei the cutoff variation and systematic uncertainties are rather small, in 16O these can be significant for large coordinate-space cutoffs. Overall, we show that chiral interactions constructed to reproduce properties of very light systems and nucleon-nucleon scattering give an excellent description of binding energies, charge radii, and form factors for all these nuclei, including open-shell systems in A = 6 and 12.

Research Organization:
Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
Sponsoring Organization:
USDOE Office of Science (SC). Nuclear Physics (NP) (SC-26); European Research Council (ERC); German Federal Ministry of Education and Research (BMBF); National Science Foundation (NSF); National Natural Science Foundation of China (NSFC); Technical Univ. of Darmstadt (Germany)
Grant/Contract Number:
AC52-06NA25396; SC0013617; 307986; 05P15RDFN1; PHY-1404405; 11505056; U1732138; 11605054; AC02- 05CH11231
OSTI ID:
1432621
Alternate ID(s):
OSTI ID: 1427886
Report Number(s):
LA-UR-17-28568; PRLTAO; TRN: US1802529
Journal Information:
Physical Review Letters, Vol. 120, Issue 12; ISSN 0031-9007
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 63 works
Citation information provided by
Web of Science

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  • XIAMEN-CUSTIPEN WORKSHOP ON THE EQUATION OF STATE OF DENSE NEUTRON-RICH MATTER IN THE ERA OF GRAVITATIONAL WAVE ASTRONOMY, AIP Conference Proceedings https://doi.org/10.1063/1.5117799
conference January 2019
Exploring Bayesian parameter estimation for chiral effective field theory using nucleon–nucleon phase shifts journal February 2019
From the microscopic to the macroscopic world: from nucleons to neutron stars journal August 2019
Nonperturbative Extraction of the Effective Mass in Neutron Matter journal April 2019
Confronting gravitational-wave observations with modern nuclear physics constraints journal June 2019
Few- and many-nucleon systems with semilocal coordinate-space regularized chiral nucleon-nucleon forces text January 2018
Single- and two-nucleon momentum distributions for local chiral interactions text January 2018
Few- and many-nucleon systems with semilocal coordinate-space regularized chiral two- and three-body forces text January 2018
Non-perturbative Extraction of the Effective Mass in Neutron Matter text January 2019
From the microscopic to the macroscopic world: from nucleons to neutron stars text January 2019

Figures / Tables (5)