{"paper":{"title":"Halo nucleus Be-11: A spectroscopic study via neutron transfer","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"nucl-ex","authors_text":"A. Bey, A. N. Villano, A. Roberts, B. Moazen, C. Matei, C. Nesaraja, D. Matyas, D. Shapira, D. W. Bardayan, D. W. Stracener, F. M. Nunes, G. L. Wilson, I. Spassova, J. A. Cizewski, J. C. Blackmon, J. F. Liang, J. F. Shriner Jr, J. J. Kolata, K. A. Chipps, K. I. Hahn, K. L. Jones, K. T. Schmitt, K. Y. Chae, M. Mato\\v{s}, M. S. Smith, P. D. O'Malley, R. L. Kozub, S. D. Pain, S. H. Ahn, S. M. Brown, S. T. Pittman, W. A. Peters","submitted_at":"2012-03-14T13:24:39Z","abstract_excerpt":"The best examples of halo nuclei, exotic systems with a diffuse nuclear cloud surrounding a tightly-bound core, are found in the light, neutron-rich region, where the halo neutrons experience only weak binding and a weak, or no, potential barrier. Modern direct reaction measurement techniques provide powerful probes of the structure of exotic nuclei. Despite more than four decades of these studies on the benchmark one-neutron halo nucleus Be-11, the spectroscopic factors for the two bound states remain poorly constrained. In the present work, the Be-10(d,p) reaction has been used in inverse ki"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1203.3081","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}