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NSR database version of April 11, 2024.

Search: Author = S.Ancelin

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2015AS03      Eur.Phys.J. A 51, 11 (2015)

M.Assie, B.Le Crom, B.Genolini, M.Chabot, D.Mengoni, J.A.Duenas, S.Ancelin, D.Beaumel, Y.Blumenfeld, N.de Sereville, J.-J.Dormard, T.Faul, J.Guillot, A.Jallat, V.Le Ven, I.Martel, E.Rauly, D.Suzuki, A.-S.Torrento

Characterization of light particles (Z ≤ 2) discrimination performances by pulse shape analysis techniques with high-granularity silicon detector

doi: 10.1140/epja/i2015-15011-6
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2014BE12      Phys.Rev. C 89, 065805 (2014)

S.Benamara, N.de Sereville, A.M.Laird, F.Hammache, I.Stefan, P.Roussel, S.Ancelin, M.Assie, A.Coc, I.Deloncle, S.P.Fox, J.Kiener, L.Lefebvre, A.Lefebvre-Schuhl, G.Mavilla, P.Morfouace, A.M.Sanchez-Benitez, L.Perrot, M.Sinha, V.Tatischeff, M.Vandebrouck

Nucleosynthesis of ²⁶Al in massive stars: New ²⁷Al states above α and neutron emission thresholds

NUCLEAR REACTIONS ²⁷Al(p, p'), E=18 MeV; measured E(p), I(p), using Enge split-pole spectrometer at Tandem-Alto facility in Orsay. ²⁷Al; deduced levels, resonances above neutron and alpha thresholds. Relevance to ²⁶Al nucleosynthesis in massive stars and estimates of thermonuclear reaction rates.

doi: 10.1103/PhysRevC.89.065805
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Data from this article have been entered in the XUNDL database. For more information, click here.

2013HA39      Phys.Rev. C 88, 062802 (2013)

F.Hammache, A.Coc, N.de Sereville, I.Stefan, P.Roussel, S.Ancelin, M.Assie, L.Audouin, D.Beaumel, S.Franchoo, B.Fernandez-Dominguez, S.Fox, C.Hamadache, J.Kiener, A.Laird, B.Le Crom, A.Lefebvre-Schuhl, L.Lefebvre, I.Matea, A.Matta, G.Mavilla, J.Mrazek, P.Morfouace, F.de Oliveira Santos, A.Parikh, L.Perrot, A.M.Sanchez-Benitez, D.Suzuki, V.Tatischeff, P.Ujic, M.Vandebrouck

Search for new resonant states in ¹⁰C and ¹¹C and their impact on the cosmological lithium problem

NUCLEAR REACTIONS ¹⁰B(³He, t)¹⁰C, ¹¹B(³He, t)¹¹C, E=35 MeV; measured E(t), I(t), σ(θ), light fragments using split-pole magnetic spectrometer, proportional gas counter, and plastic scintillator at Orsay-ALTO tandem accelerator facility. ^10,11C; deduced levels, resonances, widths. ¹²C, ¹²N, ¹⁶F; deduced levels from impurities. Discussed ⁷Li abundance and deficit Big-Bang nucleosynthesis (BBN).

doi: 10.1103/PhysRevC.88.062802
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Data from this article have been entered in the XUNDL database. For more information, click here.