NSR Query Results
Output year order : Descending NSR database version of March 21, 2024. Search: Author = G.Vancraeynest Found 14 matches. 2001GA59 Eur.Phys.J. A 11, 413 (2001) M.Gaelens, J.Andrzejewski, J.Camps, P.Decrock, M.Huyse, K.Kruglov, W.F.Mueller, A.Piechaczek, N.Severijns, J.Szerypo, G.Vancraeynest, P.Van Duppen, J.Wauters High-Precision Measurement of the 14O Half-Life using a Mass-Separated Radioactive Beam RADIOACTIVITY 14O(EC) [from 12C(3He, n), E=36 MeV]; measured Eγ, T1/2. Isotope Separator On-line method. Comparison with earlier data.
doi: 10.1007/s100500170053
2001LI56 Chin.Phys.Lett. 18, 1449 (2001) W.-P.Liu, M.Hellstrom, R.Collatz, J.Benlliure, L.Chulkov, D.Cortina Gil, F.Farget, H.Grawe, Z.Hu, N.Iwasa, M.Pfutzner, A.Piechaczek, R.Raabe, I.Reusen, E.Roeckl, G.Vancraeynest, A.Wohr Precise Determination of 40Ti Mass by Measuring the 40Sc Isospin Analogue State RADIOACTIVITY 40Ti(EC) [from 9Be(58Ni, X)]; measured β-delayed proton spectra. 40Sc deduced IAS energy. 40Ti deduced mass.
doi: 10.1088/0256-307X/18/11/307
1998BI06 Phys.Rev. C58, 754 (1998) N.Bijnens, P.Decrock, S.Franchoo, M.Gaelens, M.Huyse, H.-Y.Hwang, I.Reusen, J.Szerypo, J.von Schwarzenberg, G.Vancraeynest, P.Van Duppen, J.Wauters Study of 200,202Po Through β+ and Electron-Capture Decay and the Manifestation of Shape Coexistence in the Lighter Po Isotopes RADIOACTIVITY 200,202At(β+), (EC) [from Re(20Ne, X), E=200 MeV]; measured Eγ, Iγ, E(ce), I(ce), γγ-, (ce)γ-, (ce)(x-ray)-coin. 200,202Po deduced levels, J, π, multipolarity, configurations.
doi: 10.1103/PhysRevC.58.754
1998LI46 Phys.Rev. C58, 2677 (1998) W.Liu, M.Hellstrom, R.Collatz, J.Benlliure, L.Chulkov, D.Cortina Gil, F.Farget, H.Grawe, Z.Hu, N.Iwasa, M.Pfutzner, A.Piechaczek, R.Raabe, I.Reusen, E.Roeckl, G.Vancraeynest, A.Wohr β Decay of 40Ti and 41Ti and Implication for Solar-Neutrino Detection RADIOACTIVITY 40,41Ti(β+) [from 9Be(58Ni, X)]; measured Iβ, β-delayed proton spectra, γ spectra, pγ-coin, T1/2. 40,41Sc deduced levels, B(F)+B(GT) strength distributions. 40Ar deduced neutrino-induced events rates. FRS separator.
doi: 10.1103/PhysRevC.58.2677
1998VA08 Phys.Rev. C57, 2711 (1998) G.Vancraeynest, P.Decrock, M.Gaelens, M.Huyse, P.Van Duppen, C.R.Bain, T.Davinson, R.D.Page, A.C.Shotter, P.J.Woods, F.Binon, P.Duhamel, J.Vanhorenbeeck, R.Coszach, Th.Delbar, W.Galster, J.Graulich, P.Leleux, E.Lienard, P.Lipnik, C.Michotte, A.Ninane, J.Vervier, H.Herndl, H.Oberhummer, Cs.Sukosd, M.Wiescher 19Ne(p, γ)20Na and 19Ne(d, n)20Na Reactions and Its Astrophysical Implications for the Transition of the Hot CNO Cycle to the rp Process NUCLEAR REACTIONS 1H(19Ne, γ), E(cm)=0.6-1.8 MeV; 2H(19Ne, n), E(cm)=0.6-1.8 MeV; measured σ; deduced astrophysical reaction rates. 20Na deduced resonance properties. DWBA analysis. Radioactive beam.
doi: 10.1103/PhysRevC.57.2711
1997LI25 Z.Phys. A359, 1 (1997) W.Liu, M.Hellstrom, R.Collatz, J.Benlliure, L.Chulkov, D.Cortina Gil, F.Farget, H.Grawe, Z.Hu, N.Iwasa, M.Pfutzner, A.Piechaczek, R.Raabe, I.Reusen, E.Roeckl, G.Vancraeynest, A.Wohr β-Decay of 40Ti RADIOACTIVITY 40Ti(β+) [from 9Be(58Ni, X), E=550 MeV/nucleon]; measured T1/2, β-delayed Ep, Ip, Eγ, Iγ, pγ-coin. 40Sc levels deduced J, π, Iβ, Fermi, Gamow-Teller strength functions. 40Ar deduced neutrino absorption σ. 39Ca levels deduced proton branching.
doi: 10.1007/s002180050355
1997VA04 Nucl.Phys. A616, 107c (1997) G.Vancraeynest, C.R.Bain, F.Binon, R.Coszach, T.Davinson, P.Decrock, Th.Delbar, P.Duhamel, M.Gaelens, W.Galster, J.-S.Graulich, M.Huyse, P.Leleux, I.Licot, E.Lienard, P.Lipnik, C.Michotte, A.Ninane, R.D.Page, P.J.Sellin, A.C.Shotter, Cs.Sukosd, P.Van Duppen, J.Vanhorenbeeck, J.Vervier, M.Wiescher, P.J.Woods The 19Ne(p, γ)20Na Astrophysical Reaction Rate Determined from Measurements with a Radioactive Beam NUCLEAR REACTIONS 1H(19Ne, γ), E not given; 2H(19Ne, n), E(cm)=0.6-1.8 MeV; measured residual β-decay spectra, β-delayed α-decay characteristics; deduced 19Ne(p, γ) astrophysical reaction rate upper, lower limits, hot CNO cycle to rp-process transition in explosive hydrogen burning is probably governed by 15O(α, α) reactions. Inverse kinematics.
doi: 10.1016/S0375-9474(97)00079-1
1996BA29 Phys.Lett. 373B, 35 (1996) C.R.Bain, P.J.Woods, R.Coszach, T.Davinson, P.Decrock, M.Gaelens, W.Galster, M.Huyse, R.J.Irvine, P.Leleux, E.Lienard, M.Loiselet, C.Michotte, R.Neal, A.Ninane, G.Ryckewaert, A.C.Shotter, G.Vancraeynest, J.Vervier, J.Wauters Two Proton Emission Induced via a Resonance Reaction NUCLEAR REACTIONS 1H(13N, X), E=45 MeV; measured pp-coincidence associated energies, momenta; deduced reaction Q related features, emission mechanism. 14O level deduced 2p-decay branch width, Γ(2He).
doi: 10.1016/0370-2693(96)00109-8
1996MI12 Phys.Lett. 381B, 402 (1996) C.Michotte, C.R.Bain, F.Binon, R.Coszach, T.Davinson, P.Decrock, Th.Delbar, P.Duhamel, M.Gaelens, W.Galster, J.S.Graulich, M.Huyse, P.Leleux, E.Lienard, P.Lipnik, A.Ninane, A.C.Shotter, Cs.Sukosd, G.Vancraeynest, P.Van Duppen, J.Vanhorenbeeck, J.Vervier, M.Wiescher, P.J.Woods New Limits for the 19Ne(p, γ)20Na Astrophysical Reaction Rate from Direct Measurements using Radioactive Beams NUCLEAR REACTIONS, ICPND 2,1H(19Ne, γ), 2H(19Ne, n), E ≤ 20 MeV; measured σ(E); deduced 19Ne(p, γ) astrophysical reaction rate upper, lower limits, rp-process related features, 15O(α, γ) reaction role. Radioactive beam.
doi: 10.1016/0370-2693(96)00618-1
1995HU13 Nucl.Phys. A588, 313c (1995) M.Huyse, C.Bain, F.Binon, T.Davinson, P.Duhamel, P.Decrock, R.Coszach, Th.Delbar, M.Gaelens, W.Galster, P.Leleux, I.Licot, E.Lienard, P.Lipnik, M.Loiselet, C.Michotte, R.Page, G.Ryckewaert, P.J.Sellin, A.Shotter, Cs.Sukosd, G.Vancraeynest, P.Van Duppen, J.Vanhorenbeeck, J.Vervier, M.Wiescher, P.Woods Nuclear Reactions of Astrophysical Interest with Radioactive Beams NUCLEAR STRUCTURE 14O; 20Na; compiled, reviewed several reactions data. 20Na level deduced γ-decay, resonance strength features. NUCLEAR REACTIONS 1H(19Ne, γ), 2H(19Ne, n), E=11.4 MeV; measured β-delayed α-spectra following residual nucleus decay. 20Na level deduced γ-decay, resonance strength features. Inverse reactions, radioactive beam. RADIOACTIVITY 20Na(β+) [1H(19Ne, γ), 2H(19Ne, n), E=11.4 MeV]; measured β-delayed α-spectra. 20Na level deduced γ-decay, resonance strength features.
doi: 10.1016/0375-9474(95)00155-T
1994CO12 Phys.Rev. C50, 1695 (1994) R.Coszach, Th.Delbar, W.Galster, P.Leleux, I.Licot, E.Lienard, P.Lipnik, C.Michotte, A.Ninane, J.Vervier, C.R.Bain, T.Davinson, R.D.Page, A.C.Shotter, P.J.Woods, D.Baye, F.Binon, P.Descouvemont, P.Duhamel, J.Vanhorenbeeck, M.Vincke, P.Decrock, M.Huyse, P.Van Duppen, G.Vancraeynest, F.C.Barker Resonant Scattering of Isobaric 19Ne and 19F Beams on an H Target NUCLEAR REACTIONS 1H(19Ne, 19Ne), (19F, 19F), E=0.5-0.9 MeV; measured σ(θ) vs E. 20Na deduced levels J, π.
doi: 10.1103/PhysRevC.50.1695
1994PA42 Phys.Rev.Lett. 73, 3066 (1994) R.D.Page, G.Vancraeynest, A.C.Shotter, M.Huyse, C.R.Bain, F.Binon, R.Coszach, T.Davinson, P.Decrock, Th.Delbar, P.Duhamel, M.Gaelens, W.Galster, P.Leleux, I.Licot, E.Lienard, P.Lipnik, C.Michotte, A.Ninane, P.J.Sellin, Cs.Sukosd, P.Van Duppen, J.Vanhorenbeeck, J.Vervier, M.Wiescher, P.J.Woods First Experimental Limit on the 19Ne(p, γ)20Na Resonance Strength, of Astrophysical Interest RADIOACTIVITY 20Na(β+) [from 1H(19Ne, γ), E=11.4 MeV]; measured β-delayed Eα, Iα; deduced stellar reaction rate implications. 20Na level deduced J, resonance strength. Polythylene targets. NUCLEAR REACTIONS 2H(19Ne, n), E=14-28 MeV; 1H(19Ne, γ), E=11.4 MeV; measured Eα, Iα following residual β-delayed α-decay; deduced stellar reaction rate implications. 20Na level deduced J, resonance strength. Polyethylene targets.
doi: 10.1103/PhysRevLett.73.3066
1993DE25 Phys.Rev. C48, 2057 (1993) P.Decrock, M.Gaelens, M.Huyse, G.Reusen, G.Vancraeynest, P.Van Duppen, J.Wauters, Th.Delbar, W.Galster, P.Leleux, I.Licot, E.Lienard, P.Lipnik, C.Michotte, J.Vervier, H.Oberhummer Study of the 13N(d, n)14O Reaction Cross Section and Its Astrophysical Implications for the 13N Proton Capture Reaction NUCLEAR REACTIONS, ICPND 2H(13N, n), E=8.2-28.5 MeV; measured Eγ, Iγ; deduced 13N(d, n) reaction σ(E), astrophysical implications. 14O level deduced spectroscopic factor. 13C, 13N(p, γ), E(cm) ≤ 1 MeV; calculated astrophysical S-factor.
doi: 10.1103/PhysRevC.48.2057
1992HU13 Nucl.Instrum.Methods Phys.Res. B70, 50 (1992) M.Huyse, P.Decrock, P.Dendooven, J.Gentens, G.Vancraeynest, P.Vandenberghe, P.Van Duppen Status Report of the Leuven Isotope Separator On-Line (LISOL) NUCLEAR REACTIONS 230,232Th(p, X), E=55 MeV; 233U(p, X), E=40 MeV; 231Pa(p, X), E=22 MeV; measured mass separated 227,226,225,224Pa, 225Th yields. Ion guide operation.
doi: 10.1016/0168-583X(92)95908-A
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