{"paper":{"title":"Beta-delayed gamma decay of 26P: Possible evidence of a proton halo","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"nucl-ex","authors_text":"10, 10), (10) Joint Institute for Nuclear Astrophysics, 11), (11) Department of Physics, 12), (12) Department of Electrical Engineering, 13), (13) Geology, 14), (14) Department of Physics, 2, 2), (2) Department of Physics, 3), (3) Department of Chemistry, 4), (4) Physics Department, (5) Department of Physics, (6) Department of Physics, 7, (7) Physics Division, 8), (8) Department of Physics, (9) Department of Physics, A. A. Chen (5), A. Bowe (1, A. Simon (1, A. Spyrou (1, Astronomy, B. A. Brown (1, C. J. Prokop (1, Colorado School of Mines, C. Wrede (1, D. Irvine (9), D. P\\'erez-Loureiro (1), E. McNeice (9), E. Thiagalingam (5) ((1) National Superconducting Cyclotron Laboratory, F. Montes (1, F. Naqvi (9), Joint Institute for Nuclear Astrophysics, J. Pereira (1, J. Quaglia (1, J. Sakstrup (1, K. A. Chipps (6, Kalamazoo College, M. B. Bennett (1, McMaster University, Michigan State University, M. Santia (1, N. Cooper (9), Oak Ridge National Laboratory, Physics Department, R. Ortez (1, S. B. Schwartz (1, S. D. Pain (7), S. J. Quinn (1, S.N. Liddick (3), S. Shanab (1, University of Notre Dame), University of Southern Indiana, University of Tennessee, University of Washington, Wright Nuclear Structure Laboratory, Yale University","submitted_at":"2016-06-21T21:08:38Z","abstract_excerpt":"Background: Measurements of $\\beta$ decay provide important nuclear structure information that can be used to probe isospin asymmetries and inform nuclear astrophysics studies. Purpose: To measure the $\\beta$-delayed $\\gamma$ decay of $^{26}$P and compare the results with previous experimental results and shell-model calculations. Method: A $^{26}$P fast beam produced using nuclear fragmentation was implanted into a planar germanium detector. Its $\\beta$-delayed $\\gamma$-ray emission was measured with an array of 16 high-purity germanium detectors. Positrons emitted in the decay were detected "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1606.06770","kind":"arxiv","version":1},"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"}