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NSR database version of May 10, 2024.

Search: Author = T.Woodruff

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2020AN02      Phys.Rev. C 101, 025801 (2020)

T.Anderson, M.Skulski, L.Callahan, A.Clark, A.Nelson, P.Collon, G.Chmiel, T.Woodruff, M.Caffee

Measurement of ³⁴S(³He, p)³⁶Cl cross sections for nuclide enrichment in the early solar system

NUCLEAR REACTIONS ³He(³⁴S, p)³⁶Cl, E=1.11-2.36 MeV/nucleon; measured production σ(E) for ³⁶Cl at NSL, University of Notre Dame, ³⁶Cl atoms by accelerator mass spectroscopy (AMS) at NSL and at PRIME laboratory, Purdue University. Comparison with predictions from TALYS and other models. Discussed astrophysical implications of ³⁶Cl in terms of presence of short-lived radionuclides (SLRs) at the time of the formation of the solar system.

doi: 10.1103/PhysRevC.101.025801
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2455.

2017AN08      Phys.Rev. C 96, 015803 (2017)

T.Anderson, M.Skulski, A.Clark, A.Nelson, K.Ostdiek, P.Collon, G.Chmiel, T.Woodruff, M.Caffee

Re-measurement of the ³³S (α, p)³⁶Cl cross section for early solar system nuclide enrichment

NUCLEAR REACTIONS ⁴He(³³S, ³⁶Cl), E=0.78-1.52 MeV/nucleon; measured ³⁶Cl/Cl concentrations by AMS technique, integrated σ(E) at the Tandem accelerator of the NSL, University of Notre Dame. Comparison with previous experimental measurements and with Hauser-Feshbach code TALYS. Systematically lower cross sections obtained in the present work than in the originally reported ones, thus resolving the discrepancy with theoretical calculations.

doi: 10.1103/PhysRevC.96.015803
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2268.