References quoted in the XUNDL dataset: 27SI 12C(16O,NG):XUNDL-1

6 references found.

Clicking on a keynumber will list datasets that reference the given article.

Return to 12C(16O,NG):XUNDL-1

1990EN08

Nucl.Phys. A521, 1 (1990); Errata and Addenda Nucl.Phys. A529, 763 (1991); Errata Nucl.Phys. A564, 609 (1993)

P.M.Endt

Energy Levels of A = 21-44 Nuclei (VII)

COMPILATION A=21-44; compiled, evaluated structure data.

doi: 10.1016/0375-9474(90)90598-G

2003AU03

Nucl.Phys. A729, 337 (2003)

G.Audi, A.H.Wapstra, C.Thibault

The AME2003 atomic mass Evaluation (II). Tables, graphs, and references

COMPILATION A=1-293; compiled, evaluated atomic mass data.

doi: 10.1016/j.nuclphysa.2003.11.003

2009LO01

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

2009LO05

Phys.Rev. C 80, 055802 (2009), Erratum Phys.Rev. C 81, 029903 (2010)

G.Lotay, P.J.Woods, D.Seweryniak, M.P.Carpenter, R.V.F.Janssens, S.Zhu

γ-ray spectroscopy study of states in ²⁷Si relevant for the ²⁶Al^m(p, γ)²⁷Si reaction in novae and supernovae

NUCLEAR REACTIONS ¹²C(¹⁶O, n), E=26 MeV; measured Eγ, γγ-coin, γ(θ), and half-lives by DSA using Gammasphere array. ²⁷Si; deduced levels, J, π, and proton resonances. ^26mAl(p, γ)²⁷Si; deduced stellar reaction rates.

doi: 10.1103/PhysRevC.80.055802

2011AUZZ

Priv.Comm. (2011)

G.Audi, W.Meng

Atomic Mass Evaluation 2011

2011LO21

Phys.Rev. C 84, 035802 (2011); Pub Note Phys.Rev. C 84, 039901 (2011)

G.Lotay, P.J.Woods, D.Seweryniak, M.P.Carpenter, H.M.David, R.V.F.Janssens, S.Zhu

Identification of analog states in the T = 1/2 A = 27 mirror system from low excitation energies to the region of hydrogen burning in the ²⁶Al^{g, m}(p, γ)²⁷Si reactions

NUCLEAR REACTIONS ¹²C(¹⁶O, p), E=26 MeV; measured Eγ, Iγ, γγ-coin, γ(θ), level half-lives by DSA method using Gammasphere array. ²⁷Al; deduced levels, J, π, multipolarities, mirror energy differences. Comparison with shell-model calculations, and with level structure of ²⁷Si mirror nucleus. Relevance to ²⁶Al(p, γ)²⁷Si and ^26mAl(p, γ)²⁷Si reactions for galactic abundance of the cosmic ^26gAl, and for the excess abundance of ²⁶Mg in presolar grains.

doi: 10.1103/PhysRevC.84.035802