NSR Query Results

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NSR database version of April 11, 2024.

Search: Author = A.Ofan

Found 3 matches.

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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
Citations: PlumX Metrics

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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC1406.

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
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