References quoted in the XUNDL dataset: 11C 10B(P,A):XUNDL-11
7 references found.
Clicking on a keynumber will list datasets that reference the given article.
Phys.Rev. C28, 1431 (1983)
M.Wiescher, R.N.Boyd, S.L.Blatt, L.J.Rybarcyk, J.A.Spizuoco, R.E.Azuma, E.T.H.Clifford, J.D.King, J.Gorres, C.Rolfs, A.Vlieks
11C Level Structure via the 10B(p, γ) Reaction
NUCLEAR REACTIONS, ICPND 10B(p, γ), E=0.07-2.2 MeV; measured Eγ, Iγ, γ yield, capture σ vs E, γ(θ); deduced direct capture contributions. 11C deduced resonances, J, π, Γ, γ-branching ratios, Γγ/Γ.
Nucl.Phys. A533, 321 (1991)
M.Youn, H.T.Chung, J.C.Kim, H.C.Bhang, K.-H.Chung
The 10B(p, α0)7Be Reaction in the Thermonuclear Energy Region
NUCLEAR REACTIONS, ICPND 10B(p, α), E=120-480 keV; measured σ(E, θ); deduced σ(E), astrophysical S-factor, thermonuclear reaction rate.
doi: 10.1016/0375-9474(91)90493-P
Z.Phys. A345, 231 (1993)
C.Angulo, S.Engstler, G.Raimann, C.Rolfs, W.H.Schulte, E.Somorjai
The Effects of Electron Screening and Resonances in (p, α) Reactions on 10B and 11B at Thermal Energies
NUCLEAR REACTIONS, ICPND 11,10B(p, α), E(cm)=17-134 keV; measured spectra, α yield. 11B(p, γ), E=140-260 keV; 1H(19F, αγ), E ≈ 6.23-7.83; measured thick target yield; deduced absolute astrophysical S-factor vs E, electron screening role.
Z.Phys. A345, 333 (1993)
C.Angulo, W.H.Schulte, D.Zahnow, G.Raimann, C.Rolfs
Astrophysical S(E) Factor of 10B(p, α1)7Be at Low Energies
NUCLEAR REACTIONS, ICPND 10B(p, α), E(cm)=48-159 keV; measured absolute fusion σ, astrophysical S-factor vs E. γ-spectroscopic techniques.
Nucl.Instrum.Methods Phys.Res. B184, 309 (2001)
M.Chiari, L.Giuntini, P.A.Mando, N.Taccetti
Proton Elastic Scattering Cross-Section on Boron from 0.5 to 3.3 MeV
NUCLEAR REACTIONS B, 10,11B(p, p), E=0.5-3.3 MeV; measured σ(θ). Comparison with previous results.
doi: 10.1016/S0168-583X(01)00787-X
Phys.Rev. C 95, 044617 (2017)
M.Wiescher, R.J.deBoer, J.Gorres, R.E.Azuma
Low energy measurements of the 10B (p, α) 7Be reaction
NUCLEAR REACTIONS 10B(p, p), (p, α), E=80-1440 keV; measured Eα, Iα σ(θ, E) at incident E(p)=400-1000 keV, and Eγ, Iγ at E(p)=80-1440 keV for the yield of the 429 keV radiation from the reaction at the University of Notre Dame; deduced total S-factor, Legendre polynomial fit parameters from angular distributions. R-matrix analysis. Comparison with previous experimental data.
doi: 10.1103/PhysRevC.95.044617
Phys.Rev. C 105, 055802 (2022)
B.Vande Kolk, K.T.Macon, R.J.deBoer, T.Anderson, A.Boeltzig, K.Brandenburg, C.R.Brune, Y.Chen, A.M.Clark, T.Danley, B.Frentz, R.Giri, J.Gorres, M.Hall, S.L.Henderson, E.Holmbeck, K.B.Howard, D.Jacobs, J.Lai, Q.Liu, J.Long, K.Manukyan, T.Massey, M.Moran, L.Morales, D.Odell, P.O'Malley, S.N.Paneru, A.Richard, D.Schneider, M.Skulski, N.Sensharma, C.Seymour, G.Seymour, D.Soltesz, S.Strauss, A.Voinov, L.Wustrich, M.Wiescher
Investigation of the 10B (p, α)7Be reaction from 0.8 to 2.0 MeV
NUCLEAR REACTIONS 10B(p, α), (p, p), E=0.8-2.0 MeV; measured Eα, Iα, Ep, Ip; deduced σ(θ), σ(E) S-factor, resonance parameters of 10B+p system - energy, spin, partial (p0, α0, α1) and total width. 10B(p, γ), E=0 .1-2.0 MeV; deduced σ(θ). 11C; deduced levels, J, π. R-matrix analysis. Measurements were made at the University of Notre Dame (UND) Nuclear Science Laboratory (NSL) using a degrader foil method, while those at the Edwards AcceleratorLaboratory at Ohio University (OU) were performed using the time-of-flight (ToF)technique. Comparison with other experimental data.
doi: 10.1103/PhysRevC.105.055802