Phys.Rev. C 109, 054602 (2024)

F.Wamers, C.Lehr, J.Marganiec-Galkazka, F.Aksouh, Yu.Aksyutina, H.Alvarez-Pol, L.Atar, T.Aumann, S.Beceiro-Novo, C.A.Bertulani, K.Boretzky, M.J.G.Borge, C.Caesar, M.Chartier, A.Chatillon, L.V.Chulkov, D.Cortina-Gil, P.Diaz Fernandez, H.Emling, O.Ershova, L.M.Fraile, H.O.U.Fynbo, D.Galaviz, H.Geissel, M.Heil, M.Holl, H.T.Johansson, B.Jonson, C.Karagiannis, O.A.Kiselev, J.V.Kratz, R.Kulessa, N.Kurz, C.Langer, M.Lantz, T.Le Bleis, R.Lemmon, Yu.A.Litvinov, K.Mahata, C.Muntz, T.Nilsson, C.Nociforo, V.Panin, S.Paschalis, A.Perea, R.Plag, R.Reifarth, A.Richter, K.Riisager, C.Rodriguez-Tajes, D.Rossi, D.Savran, H.Scheit, G.Schrieder, H.Simon, J.Stroth, K.Summerer, O.Tengblad, S.Typel, H.Weick

New insight into knockout reactions from the two-proton halo nucleus ¹⁷Ne

NUCLEAR REACTIONS ¹H, ¹²C(¹⁷Ne, 2p)¹⁵O, (¹⁷Ne, p)¹⁶F, E=500 MeV/nucleon; measured reaction products, Eγ, Iγ, (particle)γ-coin; deduced σ, relative energy spectra, spectroscopic factors, σ of proton removal from ¹⁵O serving as core for ¹⁷Ne. ¹⁶F, ¹⁵O; deduced spectroscopic factors. Comparison to large-scale shell calculation performed with code KSHELL. R³B/LAND setup at the GSI Radioactive Beam Facility.

doi: 10.1103/PhysRevC.109.054602