References quoted in the XUNDL dataset: 12C 12C(P,P'):XUNDL-57
3 references found.
Clicking on a keynumber will list datasets that reference the given article.
Nucl.Instrum.Methods Phys.Res. A589, 202 (2008)
T.Kibedi, T.W.Burrows, M.B.Trzhaskovskaya, P.M.Davidson, C.W.Nestor, Jr.
Evaluation of theoretical conversion coefficients using BrIcc
COMPILATION Z=5-110; compiled and evaluated ICC data. BrICC database.
doi: 10.1016/j.nima.2008.02.051
Nucl.Phys. A968, 71 (2017)
J.H.Kelley, J.E.Purcell, C.G.Sheu
Energy levels of light nuclei A = 12
COMPILATION 12He, 12Li, 12Be, 12B, 12C, 12N, 12O; compiled data on energy levels, J, π, γ transitions, other structure data.
doi: 10.1016/j.nuclphysa.2017.07.015
Phys.Rev. C 102, 024320 (2020)
T.K.Eriksen, T.Kibedi, M.W.Reed, A.E.Stuchbery, K.J.Cook, A.Akber, B.Alshahrani, A.A.Avaa, K.Banerjee, A.C.Berriman, L.T.Bezzina, L.Bignell, J.Buete, I.P.Carter, B.J.Coombes, J.T.H.Dowie, M.Dasgupta, L.J.Evitts, A.B.Garnsworthy, M.S.M.Gerathy, T.J.Gray, D.J.Hinde, T.H.Hoang, S.S.Hota, E.Ideguchi, P.Jones, G.J.Lane, B.P.McCormick, A.J.Mitchell, N.Palalani, T.Palazzo, M.Ripper, E.C.Simpson, J.Smallcombe, B.M.A.Swinton-Bland, T.Tanaka, T.G.Tornyi, M.O.de Vries
Improved precision on the experimental E0 decay branching ratio of the Hoyle state
NUCLEAR REACTIONS 12C(p, p'), E=10.5 MeV; measured electron-positron pairs for E0 transition from the first excited 0+ Hoyle state, and for E2 transition from the first 2+ state, Eγ, (ce)(ce)- and (ce)γ-coin, γ(θ), E(p), I(p) using the superconducting solenoid Super-e pair spectrometer and Si(Li) detector array for electrons and positrons, HPGe detector for γ radiation, and ANU BALiN double sided silicon strip detector array for scattered protons at the 14 UD pelletron tandem accelerator of Australian National University; deduced E0 branching ratio ΓE0π/Γ, reduction in radiative width. Comparison with previous experimental measurements; calculated 3α reaction rate within the temperature range of helium burning red giant stars using the NACRE library value. Possible impact on astrophysical calculations.
doi: 10.1103/PhysRevC.102.024320