References quoted in the XUNDL dataset: 17O 13C(7LI,T):XUNDL-17

3 references found.

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1993TI07

Nucl.Phys. A564, 1 (1993)

D.R.Tilley, H.R.Weller, C.M.Cheves

Energy Levels of Light Nuclei A = 16-17

COMPILATION ¹⁶He, ^17,16Be, ^17,16B, ^17,16C, ^17,16N, ^17,16O, ^17,16F, ^17,16Ne, ¹⁷Na; compiled, evaluated structure data.

doi: 10.1016/0375-9474(93)90073-7

2008PE09

Phys.Rev. C 77, 042801 (2008)

M.G.Pellegriti, F.Hammache, P.Roussel, L.Audouin, D.Beaumel, P.Descouvemont, S.Fortier, L.Gaudefroy, J.Kiener, A.Lefebvre-Schuhl, M.Stanoiu, V.Tatischeff, M.Vilmay

Indirect study of the ¹³C(α, n)¹⁶O reaction via the ¹³C(⁷Li, t)¹⁷O transfer reaction

NUCLEAR REACTIONS ¹³C(⁷Li, t), (⁷Li, ⁷Li), E=28, 34 MeV; measured σ(θ). ¹⁷O; deduced levels, J, α spectroscopic factors, asymptotic normalization factors. ¹²C(⁷Li, t), (⁷Li, ⁷Li), E=28 MeV; measured yields. ¹³C(α, n); deduced astrophysical S-factor, reaction rates. Comparison with recommended values. DWBA analysis.

doi: 10.1103/PhysRevC.77.042801

2020ME09

Phys.Rev. C 102, 035803 (2020)

A.Meyer, N.de Sereville, A.M.Laird, F.Hammache, R.Longland, T.Lawson, M.Pignatari, L.Audouin, D.Beaumel, S.Fortier, J.Kiener, A.Lefebvre-Schuhl, M.G.Pellegriti, M.Stanoiu, V.Tatischeff

Evaluation of the ¹³N(α, p)¹⁶O thermonuclear reaction rate and its impact on the isotopic composition of supernova grains

NUCLEAR REACTIONS ¹³C(⁷Li, t)¹⁷O^*, E=34 MeV; measured E(t), I(t), σ(θ) using Enge Split-Pole magnetic spectrometer at the Tandem-ALTO facility in Orsay. ¹⁷O; deduced levels, resonances, J, π, L-transfers from analysis of angular distributions with finite-range distorted wave Born approximation (DWBA) calculations, Γ_α, α-spectroscopic factors, and compared with previous experimental data, and evaluated data in the ENSDF database. ¹⁷O, ¹⁷F; comparison of levels resonances, spin-parities, and resonance parameters in mirror nuclei. ¹³N(α, p)¹⁶O, E(cm)=0.05-3.0 MeV; deduced astrophysical S-factor by R-matrix calculations using AZURE2 code, Monte-Carlo reaction rates from 0.01-10 GK, isotopic abundances in the He-shell ejecta of a supernova model, production factors of stable isotopes, in the mass region between ¹²C and ⁵⁰V.

doi: 10.1103/PhysRevC.102.035803