NSR Query Results

Output year order : Descending
Format : Normal

NSR database version of April 27, 2024.

Search: Author = J.Saiz

Found 2 matches.

Back to query form

2021KE04      Phys.Rev. C 103, 035805 (2021)

A.R.L.Kennington, G.Lotay, D.T.Doherty, D.Seweryniak, C.Andreoiu, K.Auranen, M.P.Carpenter, W.N.Catford, C.M.Deibel, K.Hadynska-Klek, S.Hallam, D.Hoff, T.Huang, R.V.F.Janssens, S.Jazrawi, J.Jose, F.G.Kondev, T.Lauritsen, J.Li, A.M.Rogers, J.Saiz, G.Savard, S.Stolze, G.L.Wilson, S.Zhu

Level structure of the T_z = -1 nucleus ³⁴Ar and its relevance for nucleosynthesis in ONe novae

NUCLEAR REACTIONS ¹²C(²⁴Mg, 2n)³⁴Ar, (²⁴Mg, 2p)³⁴S, E=95 MeV; measured reaction products, Eγ, Iγ, (³⁴Ar)γ- and (³⁴S)γ-coin, γγ-coin, γ(θ) using GRETINA array for detection of high-energy γ rays, and Fragment mass analyzer (FMA) for recoils at ATLAS-ANL facility. ³⁴Ar, ³⁴S; deduced levels, proton-unbound levels of astrophysical significance, J, π, mirror symmetry, ³³S/³²S and ³⁴S/³²S ratios to search for nova presolar grains, and compared with previous experimental data. ³⁴Cl(p, γ), T=0.1-0.8 GK; calculated stellar reaction rate. Comparison of levels structures in ³⁴Ar and ³⁴S with data from the ENSDF database, and with shell-model calculations using USDA Hamiltonian, within the sd shell-model space for even-parity states, and using WBP Hamiltonian, within the sd-pf space for odd-parity levels.

doi: 10.1103/PhysRevC.103.035805
Citations: PlumX Metrics
Data from this article have been entered in the XUNDL database. For more information, click here.

2020KE03      Phys.Rev.Lett. 124, 252702 (2020)

A.R.L.Kennington, G.Lotay, D.T.Doherty, D.Seweryniak, C.Andreoiu, K.Auranen, M.P.Carpenter, W.N.Catford, C.M.Deibel, K.Hadynska-Klek, S.Hallam, D.E.M.Hoff, T.Huang, R.V.F.Janssens, S.Jazrawi, J.Jose, F.G.Kondev, T.Lauritsen, J.Li, A.M.Rogers, J.Saiz, G.Savard, S.Stolze, G.L.Wilson, S.Zhu

Search for Nova Presolar Grains: γ-Ray Spectroscopy of ³⁴Ar and its Relevance for the Astrophysical ³³Cl(p, γ) Reaction

NUCLEAR REACTIONS ¹²C(²⁴Mg, X)³⁴Ar, E=95 MeV; measured reaction products, Eγ, Iγ. ³⁴Cl, ³⁴S; deduced γ-ray energies, intensities, J, π, contribution of individual resonances to the stellar reaction rate.

doi: 10.1103/PhysRevLett.124.252702
Citations: PlumX Metrics
Data from this article have been entered in the XUNDL database. For more information, click here.