4.7 Article

N3LO NN interaction adjusted to light nuclei in ab exitu approach

Journal

PHYSICS LETTERS B
Volume 761, Issue -, Pages 87-91

Publisher

ELSEVIER SCIENCE BV
DOI: 10.1016/j.physletb.2016.08.006

Keywords

NN interaction; Ab initionuclear structure; No-core shell model; Light nuclei

Funding

  1. U.S. Department of Energy (SciDAC/NUCLEI) [DESC0008485, DE-FG02-87ER40371]
  2. US National Science Foundation [1516096]
  3. Russian Foundation for Basic Research [15-02-06604-a]
  4. U.S. Department of Energy [DE-AC02-07CH11358]
  5. Iowa State University
  6. Rare Isotope Science Project of Institute for Basic Science - Ministry of Science, ICT and Future Planning
  7. National Research Foundation of Korea [2013M7A1A1075764]
  8. Office of Science of the U.S. Department of Energy [DE-AC02-05CH11231]
  9. Office of Advanced Cyberinfrastructure (OAC)
  10. Direct For Computer & Info Scie & Enginr [1516096] Funding Source: National Science Foundation
  11. National Research Foundation of Korea [2013M7A1A1075764] Funding Source: Korea Institute of Science & Technology Information (KISTI), National Science & Technology Information Service (NTIS)

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We use phase-equivalent transformations to adjust off-shell properties of similarity renormalization group evolved chiral effective field theory NN interaction (Idaho N3LO) to fit selected binding energies and spectra of light nuclei in an ab exitu approach. We then test the transformed interaction on a set of additional observables in light nuclei to verify that it provides reasonable descriptions of these observables with an apparent reduced need for three- and many-nucleon interactions. (C) 2016 The Authors. Published by Elsevier B.V.

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