References quoted in the XUNDL dataset: 12C 12C(P,P'):XUNDL-54
5 references found.
Clicking on a keynumber will list datasets that reference the given article.
Phys.Rev.Lett. 105, 022501 (2010)
M.Chernykh, H.Feldmeier, T.Neff, P.von Neumann-Cosel, A.Richter
Pair Decay Width of the Hoyle State and its Role for Stellar Carbon Production
NUCLEAR REACTIONS 12C(e, e'), E=29-78 MeV; measured reaction products; deduced transition form factors, charge density, pair decay width of the Hoyle state.
doi: 10.1103/PhysRevLett.105.022501
J.Phys.:Conf.Ser. 312, 042026 (2011)
P.von Neumann-Cosel, M.Chernykh, H.Feldmeier, T.Neff, A.Richter
Pair decay width of the Hoyle state and carbon production in stars
NUCLEAR REACTIONS 12C(e, e'), E=73 MeV; measured Ee, Ie; deduced transition charge density for transition in from ground to the Hoyle state, formfactor at low q, pair decay widths.
doi: 10.1088/1742-6596/312/4/042026
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
Phys.Rev.Lett. 125, 182701 (2020)
T.Kibedi, B.Alshahrani, A.E.Stuchbery, A.C.Larsen, A.Gorgen, S.Siem, M.Guttormsen, F.Giacoppo, A.I.Morales, E.Sahin, G.M.Tveten, F.L.Bello Garrote, L.Crespo Campo, T.K.Eriksen, M.Klintefjord, S.Maharramova, H.-T.Nyhus, T.G.Tornyi, T.Renstrom, W.Paulsen
Radiative Width of the Hoyle State from γ-Ray Spectroscopy
NUCLEAR REACTIONS 12C(p, p'), E=10.7 MeV; measured reaction products, Eγ, Iγ, γ-γ-p coin.; deduced γ-ray energies, resonances, radiative branching ratio, radiative widths. Comparison with available data.
doi: 10.1103/PhysRevLett.125.182701