Actions for No-Core Shell Model Calculations in Light Nuclei with Three-Nucleon Forces [electronic resource].

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No-Core Shell Model Calculations in Light Nuclei with Three-Nucleon Forces [electronic resource].

Published
Washington, D.C. : United States. Dept. of Energy, 2004.
Oak Ridge, Tenn. : Distributed by the Office of Scientific and Technical Information, U.S. Dept. of Energy.
Physical Description
PDF-file: 6 pages; size: 0.4 Mbytes
Additional Creators
Lawrence Berkeley National Laboratory, United States. Department of Energy, and United States. Department of Energy. Office of Scientific and Technical Information
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Summary
The ab initio No-Core Shell Model (NCSM) has recently been expanded to include nucleon-nucleon (NN) and three-nucleon (3N) interactions at the three-body cluster level. Here it is used to predict binding energies and spectra of p-shell nuclei based on realistic NN and 3N interactions. It is shown that 3N force (3NF) properties can be studied in these nuclear systems. First results show that interactions based on chiral perturbation theory lead to a realistic description of ⁶Li.
Report Numbers
E 1.99:ucrl-proc-201751
ucrl-proc-201751
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Note
Published through SciTech Connect.
01/08/2004.
"ucrl-proc-201751"
Presented at: The Sixth International Conference on Radioactive Nuclear Beams (RNB6), Argonne, IL, United States, Sep 22 - Sep 26, 2003.
Ormand, W E; Navratil, P; Barrett, B R; Vary, J P; Nogga, A.
Funding Information
W-7405-ENG-48
View MARC record | catkey: 14668793