4.5 Article

Accurate nuclear radii and binding energies from a chiral interaction

Journal

PHYSICAL REVIEW C
Volume 91, Issue 5, Pages -

Publisher

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevC.91.051301

Keywords

-

Funding

  1. U.S. Department of Energy, Office of Science, Office of Nuclear Physics [DEFG02-96ER40963, DE-SC0008499, DE-SC0008511]
  2. Oak Ridge National Laboratory
  3. National Science Foundation [1404159]
  4. Swedish Foundation for International Cooperation in Research and Higher Education (STINT) [IG2012-5158]
  5. European Research Council [ERC-StG-240603]
  6. Research Council of Norway [ISP-Fysikk/216699]
  7. NSERC [401945-2011]
  8. National Research Council Canada
  9. Office of Science of the Department of Energy [DE-AC05-00OR22725]
  10. National Institute for Computational Sciences
  11. Swedish National Infrastructure for Computing (SNIC)
  12. Notur project in Norway
  13. Division Of Physics
  14. Direct For Mathematical & Physical Scien [1404159] Funding Source: National Science Foundation

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With the goal of developing predictive ab initio capability for light and medium-mass nuclei, two-nucleon and three-nucleon forces from chiral effective field theory are optimized simultaneously to low-energy nucleon-nucleon scattering data, as well as binding energies and radii of few-nucleon systems and selected isotopes of carbon and oxygen. Coupled-cluster calculations based on this interaction, named NNLOsat, yield accurate binding energies and radii of nuclei up to Ca-40, and are consistent with the empirical saturation point of symmetric nuclear matter. In addition, the low-lying collective J(pi) = 3(-) states in O-16 and 40Ca are described accurately, while spectra for selected p- and sd-shell nuclei are in reasonable agreement with experiment.

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