References quoted in the XUNDL dataset: 26SI 28SI(P,T):XUNDL-3

4 references found.

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


2002BA25

Phys.Rev. C65, 032801 (2002)

D.W.Bardayan, J.C.Blackmon, A.E.Champagne, A.K.Dummer, T.Davinson, U.Greife, D.Hill, C.Iliadis, B.A.Johnson, R.L.Kozub, C.S.Lee, M.S.Smith, P.J.Woods

Astrophysically Important 26Si States Studied with the 28Si(p, t)26Si Reaction

NUCLEAR REACTIONS 28Si(p, t), E=40, 42 MeV; measured triton spectra, σ(θ). 26Si deduced levels, J, π. Astrophysical implications discussed.

doi: 10.1103/PhysRevC.65.032801


2003BA85

Nucl.Phys. A718, 505c (2003)

D.W.Bardayan, J.C.Blackmon, A.E.Champagne, A.K.Dummer, T.Davinson, U.Greife, D.Hill, C.Iliadis, B.A.Johnson, R.L.Kozub, C.S.Lee, M.S.Smith, P.J.Woods

Study of 26Si States Important for 26Al Nucleosynthesis in Novae

NUCLEAR REACTIONS 28Si(p, t), E=40, 42 MeV; measured σ(E, θ). 26Si deduced levels, J, π. Astrophysical implications discussed.

doi: 10.1016/S0375-9474(03)00825-X


2004PA42

Phys.Rev. C 70, 065805 (2004); Erratum Phys.Rev. C 73, 049907 (2006)

Y.Parpottas, S.M.Grimes, S.Al-Quraishi, C.R.Brune, T.N.Massey, J.E.Oldendick, A.Salas, R.T.Wheeler

Astrophysically important 26Si states studied with the (3He, n) reaction and the 25Al(p, γ)26Si reaction rates in explosive hydrogen burning environments

NUCLEAR REACTIONS 24Mg(3He, n), E=7.9, 8.11, 10.0 MeV; measured En, σ(θ). 26Si deduced levels, J, π. 25Al(p, γ), E=low; calculated astrophysical reaction rates.

doi: 10.1103/PhysRevC.70.065805


2006BA65

Phys.Rev. C 74, 045804 (2006)

D.W.Bardayan, J.A.Howard, J.C.Blackmon, C.R.Brune, K.Y.Chae, W.R.Hix, M.S.Johnson, K.L.Jones, R.L.Kozub, J.F.Liang, E.J.Lingerfelt, R.J.Livesay, S.D.Pain, J.P.Scott, M.S.Smith, J.S.Thomas, D.W.Visser

Astrophysically important 26Si states studied with the 28Si(p, t)26Si reaction. II. Spin of the 5.914-MeV 26Si level and galactic 26Al production

NUCLEAR REACTIONS 28Si(p, t), (p, d), E=40 MeV; measured particle spectra, angular distributions. 26Si level deduced J, π. 25Al(p, γ), E=low; deduced astrophysical reaction rate.

doi: 10.1103/PhysRevC.74.045804


Note: Additional references listed in dataset: 2006BA85,. See dataset contents for details.