References quoted in the XUNDL dataset: 19F 4HE(15N,A):XUNDL-14

3 references found.

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


1962YA03

J.Phys.Soc.Japan 17, 595 (1962)

K.Yagi, K.Katori, H.Ohnuma, Y.Hashimoto, Y.Nogami

NUCLEAR REACTIONS 18O(p, p), E=600-1450 keV; measured reaction products. 19F; deduced levels, J, π, nuclear properties, σ(θ).

doi: 10.1143/JPSJ.17.595


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


2019LA08

Phys.Rev. C 99, 034301 (2019)

M.La Cognata, M.Fisichella, A.Di Pietro, P.Figuera, V.Z.Goldberg, S.Cherubini, J.P.Fernandez-Garcia, M.Gulino, L.Lamia, D.Lattuada, M.Lattuada, R.G.Pizzone, G.G.Rapisarda, S.Romano, R.Sparta, C.Spitaleri, D.Torresi, A.Tumino, M.Zadro

Observation of 15N α resonant structures in 19F using the thick target in inverse kinematics scattering method

NUCLEAR REACTIONS 4He(15N, α), E=40.23 MeV; measured Eα, Iα, differential σ(θ) using ΔE-E silicon telescopes for α detection and surface barrier detectors for 15N-like recoils at the LNL-Catania Tandem accelerator facility. 19F; deduced levels, resonances, J, π, α-widths, proton widths and potential α-cluster states using R-matrix analysis using AZURE2 code. Comparison with previous experimental data, and with literature data for mirror nucleus 19Ne. Relevance to models of stars in different evolutionary stages, such as the asymptotic giant branch (AGB) stars asymptotic giant branch (AGB).

doi: 10.1103/PhysRevC.99.034301