NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = S.Ghelberg Found 9 matches. 2007PA15 J.Radioanal.Nucl.Chem. 272, 243 (2007) M.Paul, A.Valenta, I.Ahmad, D.Berkovits, C.Bordeanu, S.Ghelberg, Y.Hashimoto, A.Hershkowitz, S.Jiang, T.Nakanishi, K.Sakamoto An upper limit to interstellar 244Pu abundance as deduced from radiochemical search in deep-sea sediment: An account
doi: 10.1007/s10967-007-0508-3
2006AH10 Phys.Rev.C 74, 065803 (2006) I.Ahmad, J.P.Greene, E.F.Moore, S.Ghelberg, A.Ofan, M.Paul, W.Kutschera Improved measurement of the 44Ti half-life from a 14-year long study RADIOACTIVITY 44Ti(EC) [from 45Sc(p, 2n)]; measured Eγ, Iγ, T1/2.
doi: 10.1103/PhysRevC.74.065803
2006NA02 Phys.Rev.Lett. 96, 041102 (2006) H.Nassar, M.Paul, I.Ahmad, Y.Ben-Dov, J.Caggiano, S.Ghelberg, S.Goriely, J.P.Greene, M.Hass, A.Heger, A.Heinz, D.J.Henderson, R.V.F.Janssens, C.L.Jiang, Y.Kashiv, B.S.Nara Singh, A.Ofan, R.C.Pardo, T.Pennington, K.E.Rehm, G.Savard, R.Scott, R.Vondrasek 40Ca(α, γ)44Ti Reaction in the Energy Regime of Supernova Nucleosynthesis NUCLEAR REACTIONS 4He(40Ca, γ), E(cm) ≈ 0.6-1.2 MeV/nucleon; measured yield. 40Ca(α, γ), E=low; deduced astrophysical reaction rate. Accelerator mass spectrometry.
doi: 10.1103/PhysRevLett.96.041102
2005NA08 Phys.Rev.Lett. 94, 092504 (2005) H.Nassar, M.Paul, I.Ahmad, D.Berkovits, M.Bettan, P.Collon, S.Dababneh, S.Ghelberg, J.P.Greene, A.Heger, M.Heil, D.J.Henderson, C.L.Jiang, F.Kappeler, H.Koivisto, S.O'Brien, R.C.Pardo, N.Patronis, T.Pennington, R.Plag, K.E.Rehm, R.Reifarth, R.Scott, S.Sinha, X.Tang, R.Vondrasek Stellar (n, γ) Cross Section of 62Ni NUCLEAR REACTIONS 62Ni(n, γ), E=spectrum; measured total σ. Fast-neutron activation, accelerator mass spectrometry. Astrophysical implications discussed.
doi: 10.1103/PhysRevLett.94.092504
2005NA30 Nucl.Phys. A758, 411c (2005) H.Nassar, M.Paul, S.Ghelberg, A.Ofan, N.Trubnikov, Y.Ben-Dov, M.Hass, B.S.Nara Singh Study of the supernova nucleosynthesis 40Ca(α, γ)44Ti reaction: progress report NUCLEAR REACTIONS 4He(40Ca, γ), E=72 MeV; measured yields. Radiochemical separation, accelerator mass spectrometry. Astrophysical implications discussed.
doi: 10.1016/j.nuclphysa.2005.05.075
2004NA39 Nucl.Phys. A746, 613c (2004) H.Nassar, S.Ghelberg, M.Paul, S.Dababneh, M.Heil, F.Kappeler, R.Plag, I.Ahmad, J.P.Greene, D.J.Henderson, C.L.Jiang, R.C.Pardo, T.Pennington, K.E.Rehm, R.Scott, S.Sinha, X.Tang, R.Vondrasek, H.Koivisto, D.Berkovits, M.Bettan, R.Reifarth, P.Collon, S.O'Brien, N.Patronis Production and isobaric separation of 63Ni ions for determination of the 62Ni(n, γ)63Ni reaction cross section at stellar temperatures NUCLEAR REACTIONS 62Ni(n, γ), E=fast; measured yields.
doi: 10.1016/j.nuclphysa.2004.09.140
2003PA34 Nucl.Phys. A718, 239c (2003) M.Paul, C.Feldstein, I.Ahmad, D.Berkovits, C.Bordeanu, J.Caggiano, S.Ghelberg, J.Goerres, J.Greene, M.Hass, A.Heinz, D.Henderson, S.K.Hui, R.V.F.Janssens, C.L.Jiang, S.Jiang, Y.Nirel, R.C.Pardo, T.Pennington, K.E.Rehm, G.Savard, G.Verri, R.Vondrasek, I.Wiedenhover, M.Wiescher Counting 44Ti Nuclei from the 40Ca(α, γ)44Ti Reaction NUCLEAR REACTIONS 4He(40Ca, X)44Ti, E=70.9 MeV; measured yield. 44Ti deduced resonance strength. Chemical separation, accelerator mass spectrometry.
doi: 10.1016/S0375-9474(03)00720-6
2003PA37 Nucl.Phys. A719, 29c (2003) M.Paul, A.Valenta, I.Ahmad, D.Berkovits, C.Bordeanu, S.Ghelberg, Y.Hashimoto, A.Hershkowitz, S.Jiang, T.Nakanishi, K.Sakamoto A window on nucleosynthesis through detection of short-lived radionuclides
doi: 10.1016/S0375-9474(03)00954-0
2000HU16 Nucl.Instrum.Methods Phys.Res. B172, 642 (2000) S.K.Hui, M.Paul, D.Berkovits, E.Boaretto, S.Ghelberg, M.Hass, A.Hershkowitz, E.Navon 44Ti Atom Counting for Nuclear Astrophysics NUCLEAR REACTIONS 12C(34S, 2n), E=20 MeV; measured production σ. 40Ca(α, γ), E=low; calculated yields. Accelerator mass spectrometry.
doi: 10.1016/S0168-583X(00)00101-4
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