No-core shell-model calculations in light nuclei with three-nucleon forces. Barrett, B. R., Navrátil, P., Nogga, A., Ormand, W. E., & Vary, J. P. Nuclear Physics A, 746(1-4 SPEC.ISS.):579–582, 2004. doi abstract bibtex 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. First results show that NN plus 3N interactions based on chiral perturbation theory lead to a realistic description of 6Li. \textcopyright 2004 Elsevier B.V. All rights reserved.
@article{Barrett2004,
abstract = {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. First results show that NN plus 3N interactions based on chiral perturbation theory lead to a realistic description of 6Li. {\textcopyright} 2004 Elsevier B.V. All rights reserved.},
author = {Barrett, B. R. and Navr{\'{a}}til, P. and Nogga, A. and Ormand, W. E. and Vary, J. P.},
doi = {10.1016/j.nuclphysa.2004.09.137},
issn = {03759474},
journal = {Nuclear Physics A},
number = {1-4 SPEC.ISS.},
pages = {579--582},
title = {{No-core shell-model calculations in light nuclei with three-nucleon forces}},
volume = {746},
year = {2004}
}
Downloads: 0
{"_id":"XHWx9kurWXqyRNMfS","bibbaseid":"barrett-navrtil-nogga-ormand-vary-nocoreshellmodelcalculationsinlightnucleiwiththreenucleonforces-2004","author_short":["Barrett, B. R.","Navrátil, P.","Nogga, A.","Ormand, W. E.","Vary, J. P."],"bibdata":{"bibtype":"article","type":"article","abstract":"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. First results show that NN plus 3N interactions based on chiral perturbation theory lead to a realistic description of 6Li. \\textcopyright 2004 Elsevier B.V. All rights reserved.","author":[{"propositions":[],"lastnames":["Barrett"],"firstnames":["B.","R."],"suffixes":[]},{"propositions":[],"lastnames":["Navrátil"],"firstnames":["P."],"suffixes":[]},{"propositions":[],"lastnames":["Nogga"],"firstnames":["A."],"suffixes":[]},{"propositions":[],"lastnames":["Ormand"],"firstnames":["W.","E."],"suffixes":[]},{"propositions":[],"lastnames":["Vary"],"firstnames":["J.","P."],"suffixes":[]}],"doi":"10.1016/j.nuclphysa.2004.09.137","issn":"03759474","journal":"Nuclear Physics A","number":"1-4 SPEC.ISS.","pages":"579–582","title":"No-core shell-model calculations in light nuclei with three-nucleon forces","volume":"746","year":"2004","bibtex":"@article{Barrett2004,\nabstract = {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. First results show that NN plus 3N interactions based on chiral perturbation theory lead to a realistic description of 6Li. {\\textcopyright} 2004 Elsevier B.V. All rights reserved.},\nauthor = {Barrett, B. R. and Navr{\\'{a}}til, P. and Nogga, A. and Ormand, W. E. and Vary, J. P.},\ndoi = {10.1016/j.nuclphysa.2004.09.137},\nissn = {03759474},\njournal = {Nuclear Physics A},\nnumber = {1-4 SPEC.ISS.},\npages = {579--582},\ntitle = {{No-core shell-model calculations in light nuclei with three-nucleon forces}},\nvolume = {746},\nyear = {2004}\n}\n","author_short":["Barrett, B. R.","Navrátil, P.","Nogga, A.","Ormand, W. E.","Vary, J. P."],"key":"Barrett2004","id":"Barrett2004","bibbaseid":"barrett-navrtil-nogga-ormand-vary-nocoreshellmodelcalculationsinlightnucleiwiththreenucleonforces-2004","role":"author","urls":{},"metadata":{"authorlinks":{}}},"bibtype":"article","biburl":"https://cloud.swalk.xyz/bebop/bibtex.bib","dataSources":["7fTi5NtYYKwjPXfpu"],"keywords":[],"search_terms":["core","shell","model","calculations","light","nuclei","three","nucleon","forces","barrett","navrátil","nogga","ormand","vary"],"title":"No-core shell-model calculations in light nuclei with three-nucleon forces","year":2004}