References quoted in the XUNDL dataset: 27SI 26AL(D,NG):XUNDL-6
4 references found.
Clicking on a keynumber will list datasets that reference the given article.
Nucl.Phys. A291, 269 (1977)
W.A.Sterrenburg, G.van Middelkoop
Spectroscopy of 27Si with the 24Mg(α, nγ)27Si Reaction
NUCLEAR REACTIONS 24Mg(α, nγ), E=12.60, 12.90, 15.45, 16.35 MeV; measured nγ(θ), DSA, Eγ, Iγ. 27Si deduced levels, T1/2, J, π, δ, γ-branching. Enriched target.
doi: 10.1016/0375-9474(77)90319-0
Phys.Rev. C53, 1945 (1996)
R.B.Vogelaar, L.W.Mitchell, R.W.Kavanagh, A.E.Champagne, P.V.Magnus, M.S.Smith, A.J.Howard, P.D.Parker, H.A.O'Brien
Constraining 26Al + p Resonances using 26Al(3He, d)27Si
NUCLEAR REACTIONS 26Al(3He, d), E=20 MeV; measured σ(Ed), σ(θ); deduced implications for 26Al(p, γ) stellar reaction rate, model parameters. 27Si deduced levels, resonance, spectroscopic factors.
Phys.Rev.Lett. 102, 162502 (2009)
G.Lotay, P.J.Woods, D.Seweryniak, M.P.Carpenter, R.V.F.Janssens, S.Zhu
Identification of Key Astrophysical Resonances Relevant for the 26gAl(p, γ)27Si Reaction in Wolf-Rayet Stars, AGB stars, and Classical Novae
NUCLEAR REACTIONS 12C(16O, X)27Si, E=26 MeV; measured Eγ, Iγ, γγ-coin. 27Si; deduced resonance energies. 26Al(p, γ); calculated reaction rates at astrophysical energies.
doi: 10.1103/PhysRevLett.102.162502
Eur.Phys.J. A 52, 6 (2016)
A.Kankainen, P.J.Woods, F.Nunes, C.Langer, H.Schatz, V.Bader, T.Baugher, D.Bazin, B.A.Brown, J.Browne, D.T.Doherty, A.Estrade, A.Gade, A.Kontos, G.Lotay, Z.Meisel, F.Montes, S.Noji, G.Perdikakis, J.Pereira, F.Recchia, T.Redpath, R.Stroberg, M.Scott, D.Seweryniak, J.Stevens, D.Weisshaar, K.Wimmer, R.Zegers
Angle-integrated measurements of the 26Al (d, n) 27Si reaction cross section: a probe of spectroscopic factors and astrophysical resonance strengths
NUCLEAR REACTIONS 2H(26Al, n), E=30 MeV/nucleon; measured 511 keV γ-ray using GRETINA (Gamma-Ray Energy Tracking In-beam Nuclear Array), Si recoils, (Si)γ-coin; deduced Doppler-reconstructed γ-ray spectrum in coincidence with Si, σ, resonances, spectroscopic factors to discrete states; calculated σ using shell model.
doi: 10.1140/epja/i2016-16006-5