References quoted in the XUNDL dataset: 26SI 26P EC DECAY:43.7 MS:XUNDL-15
6 references found.
Clicking on a keynumber will list datasets that reference the given article.
Eur.Phys.J. A 21, 419 (2004)
J.C.Thomas, L.Achouri, J.Aysto, R.Beraud, B.Blank, G.Canchel, S.Czajkowski, P.Dendooven, A.Ensallem, J.Giovinazzo, N.Guillet, J.Honkanen, A.Jokinen, A.Laird, M.Lewitowicz, C.Longour, F.de Oliveira Santos, K.Perajarvi, M.Stanoiu
Beta-decay properties of 25Si and 26P
RADIOACTIVITY 25Si, 26P(EC) [from 12C(36Ar, X)]; measured β-delayed Eγ, Ep, T1/2; deduced log ft, Gamow-Teller strength distributions, proton-decay and two-proton decay branching ratios. 24Mg, 25Al, 26Si deduced levels, feeding intensities, mirror asymmetry parameters. Comparison with shell-model predictions.
doi: 10.1140/epja/i2003-10218-8
Phys.Rev. C 75, 062801 (2007)
D.Seweryniak, P.J.Woods, M.P.Carpenter, T.Davinson, R.V.F.Janssens, D.G.Jenkins, T.Lauritsen, C.J.Lister, J.Shergur, S.Sinha, A.Woehr
Level structure of 26Si and its implications for the astrophysical reaction rate of 25Al(p, γ)26Si
NUCLEAR REACTIONS 12C(16O, 2n), E=58 MeV; measured Eγ, Iγ, γγ-coinc using the Gammasphere. 26Si deduced levels, J, π. Compared results to model calculations and discussed astrophysical implications.
doi: 10.1103/PhysRevC.75.062801
Phys.Rev. C 79, 032801 (2009)
P.N.Peplowski, L.T.Baby, I.Wiedenhover, S.E.Dekat, E.Diffenderfer, D.L.Gay, O.Grubor-Urosevic, P.Hoflich, R.A.Kaye, N.Keeley, A.Rojas, A.Volya
Lowest l=0 proton resonance in 26Si and implications for nucleosynthesis of 26Al
NUCLEAR REACTIONS 2H(25Al, n)26Si, E=91.5 MeV; 2H(24Mg, n)25Al, E=140 MeV; measured decay proton spectra, resonances, excitation energies, σ, proton and γ widths. 26Si; deduced levels, resonances, J, π; 25Al(p, γ)26Si; deduced reaction rate.
doi: 10.1103/PhysRevC.79.032801
Phys.Rev. C 79, 035803 (2009)
C.Wrede
Thermonuclear 25Al(p, γ)26Si reaction rate in classical novae and Galactic 26Al
NUCLEAR REACTIONS 25Al(p, γ); analyzed thermonuclear reaction rates. 26Si; deduced level, resonance, J, π. Discussed implications for nova contribution to galactic 26Al.
doi: 10.1103/PhysRevC.79.035803
Chin.Phys.C 36, 1603 (2012)
M.Wang, G.Audi, A.H.Wapstra, F.G.Kondev, M.MacCormick, X.Xu, B.Pfeiffer
The AME2012 atomic mass evaluation (II). Tables, graphs and references
COMPILATION A=1-295; compiled, evaluated atomic mass data.
Phys.Rev.Lett. 111, 232503 (2013)
M.B.Bennett, C.Wrede, K.A.Chipps, J.Jose, S.N.Liddick, M.Santia, A.Bowe, A.A.Chen, N.Cooper, D.Irvine, E.McNeice, F.Montes, F.Naqvi, R.Ortez, S.D.Pain J.Pereira, C.Prokop, J.Quaglia, S.J.Quinn, S.B.Schwartz, S.Shanab, A.Simon, A.Spyrou, E.Thiagalingam
Classical-Nova Contribution to the Milky Way's 26Al Abundance: Exit Channel of the Key 25Al(p, γ)26Si Resonance
RADIOACTIVITY 26P(β+) [from Be(36Ar, X)26P, E=150 MeV/nucleon]; measured Eβ, Iβ, Eγ, Iγ, βγ- and βγγ-coin.; deduced resonances energy, J, π. Astrophysical implications.
doi: 10.1103/PhysRevLett.111.232503