References quoted in the XUNDL dataset: 19NE 18F(P,P),(P,A):XUNDL-7

3 references found.

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2001BA49

Phys.Rev. C63, 065802 (2001)

D.W.Bardayan, J.C.Blackmon, W.Bradfield-Smith, C.R.Brune, A.E.Champagne, T.Davinson, B.A.Johnson, R.L.Kozub, C.S.Lee, R.Lewis, P.D.Parker, A.C.Shotter, M.S.Smith, D.W.Visser, P.J.Woods

Destruction of ¹⁸F via ¹⁸F(p, α)¹⁵O Burning Through the E_c.m. = 665 keV Resonance

NUCLEAR REACTIONS ¹H(¹⁸F, p), (¹⁸F, α), E=10-14 MeV; measured particle spectra, σ(θ), σ. ¹⁸F(p, α), E(cm)=663 keV; deduced σ. ¹⁹Ne deduced resonance energy, width, proton branching ratio. Astrophysical implications discussed.

doi: 10.1103/PhysRevC.63.065802

2011AUZZ

Priv.Comm. (2011)

G.Audi, W.Meng

Atomic Mass Evaluation 2011

2012MO03

Phys.Rev. C 85, 022801 (2012)

D.J.Mountford, A.StJ.Murphy, N.L.Achouri, C.Angulo, J.R.Brown, T.Davinson, F.de Oliveira Santos, N.de Sereville, P.Descouvemont, O.Kamalou, A.M.Laird, S.T.Pittman, P.Ujic, P.J.Woods

Resonances in ¹⁹Ne with relevance to the astrophysically important ¹⁸F(p, α)¹⁵O reaction

NUCLEAR REACTIONS ¹H(¹⁸F, α), (¹⁸F, p), [secondary ¹⁸F beam from C(²⁰Ne, X), E=95 MeV/nucleon primary reaction], E(cm)=0.5-1.9 MeV; measured particle spectra, time of flight, differential cross sections at GANIL-SPIRAL facility. ¹⁹Ne; deduced resonance energies, J, π, α and proton partial widths, covariance matrix, astrophysical S factor for ¹⁸F(p, α)¹⁵O reaction. R-matrix analysis. Astrophysical implications. Comparison with previous experimental results.

doi: 10.1103/PhysRevC.85.022801