References quoted in the XUNDL dataset: 19F 18O(3HE,D):XUNDL-15

7 references found.

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

Return to 18O(3HE,D):XUNDL-15

1970GR04

Nucl.Phys. A142, 137 (1970)

L.L.Green, C.O.Lennon, I.M.Naqib

A Nuclear Structure Study of ¹⁹F Levels from the ¹⁸O(³He, d)¹⁹F Reaction

NUCLEAR REACTIONS ¹⁸O(³He, d), E=11 MeV; measured σ(E;Ed, θ). ¹⁹F levels deduced S. Enriched target.

doi: 10.1016/0375-9474(70)90480-X

1970SC25

Nucl.Phys. A155, 644 (1970)

C.Schmidt, H.H.Duhm

The ¹⁸O(³He, d)¹⁹F Reaction at E = 16 MeV

NUCLEAR REACTIONS ¹⁸O(³He, d), E(³He)=16 MeV;measured σ(θ). ¹⁹F deduced levels, J, π, L-values, S.

doi: 10.1016/0375-9474(70)90918-8

1980WI17

Nucl.Phys. A349, 165 (1980)

M.Wiescher, H.W.Becker, J.Gorres, K.-U.Kettner, H.P.Trautvetter, W.E.Kieser, C.Rolfs, R.E.Azuma, K.P.Jackson, J.W.Hammer

Nuclear and Astrophysical Aspects of ¹⁸O(p, γ)¹⁹F

NUCLEAR REACTIONS ¹⁸O(p, γ), E=80-2200 keV; measured Ep, Eγ, Iγ(E, θ). ¹⁹F deduced levels, absolute γ-transition strength, Γ, J, π, δ, γ-branching ratios, S, astrophysical reaction rate. Enriched target, Ge(Li) detectors.

doi: 10.1016/0375-9474(80)90451-0

1995TI05

Phys.Rev. C52, 1145 (1995)

R.Timmermans, Th.A.Rijken, J.J.de Swart

Reply to ' Comment on ' Antiproton-Proton Partial-Wave Analysis Below 925 MeV/c ' '

NUCLEAR REACTIONS ¹H(p-bar, p-bar), E at < 925 MeV/c; analyzed partial wave analyses; deduced parameter extraction justifications.

doi: 10.1103/PhysRevC.52.1145

1995TI07

Nucl.Phys. A595, 1 (1995)

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

Energy Levels of Light Nuclei A = 18-19

COMPILATION ¹⁸Be, ^18,19B, ^18,19C, ^18,19N, ^18,19O, ^18,19F, ^18,19Ne, ^18,19Na; compiled, evaluated structure data.

doi: 10.1016/0375-9474(95)00338-1

2012BU16

Phys.Rev. C 86, 065804 (2012)

M.Q.Buckner, C.Iliadis, J.M.Cesaratto, C.Howard, T.B.Clegg, A.E.Champagne, S.Daigle

Thermonuclear reaction rate of ¹⁸O(p, γ)¹⁹F

NUCLEAR REACTIONS ¹⁸O(p, γ)¹⁹F, E=95 keV; measured Eγ, Iγ, γγ-coin; deduced resonance strength, direct capture S factor using LENA facility. Improved thermonuclear reaction rates.

doi: 10.1103/PhysRevC.86.065804

2019BU17

Eur.Phys.J. A 55, 114 (2019)

V.Burjan, Z.Hons, V.Kroha, J.Mrazek, S.Piskor, A.M.Mukhamedzhanov, L.Trache, R.E.Tribble, M.La Cognata, L.Lamia, R.G.Pizzone, S.Romano, C.Spitaleri, A.Tumino

The determination of the astrophysical S-factor of the direct ¹⁸O(p, γ)¹⁹F capture by the ANC method

doi: 10.1140/epja/i2019-12801-8