The two lowest T = 3/2 levels in 21Na have been studied in the 19F(3He, n), 20Ne (p,p) and 20Ne (p,p’) reactions, and their excitation energies, spins, parities and widths have been determined. In a separate investigation, branching ratios were measured for the isospin-nonconserving particle decays of the lowest T = 3/2 levels in 17O and 17F to the ground state and first two excited states of 16O, by studying the 15N(3He,n) 17F*(p) 16O and 18O(3He, α)17O*(n) 16O reactions. The 19F(3He,n) 21Na reaction was studied at incident energies between 4.2 and 5.9 MeV using a pulsed-beam neutron-time-of-flight spectrometer. Two T = 3/2 levels were identified at excitation energies of 8.99 ± 0.05 MeV (J > ½) and 9.22 ± 0.015 MeV (J π = ½+, Γ ˂ 40 ...
A powerful method of investigating proton-unbound nuclear states by tracking their decay products in...
A method has been developed that can provide beams of many short-lived nuclei of interest in nucleos...
The 17F(p, γ)18 reaction is important in stellar explosions, but its rate has been uncertain because...
We discuss new results concerning the investigation of the 19F(p,α 0)16O and 10B(p,α 0)7Be reactions...
The nuclear structure of 19Ne near the proton threshold is of interest for understanding the rates o...
We have employed (^3He, n) double-stripping reactions to locate low-lying T = 3/2 and T = 2 states i...
We have employed (^3He, n) double-stripping reactions to locate low-lying T = 3/2 and T = 2 states i...
(18O, 19N) and (18O, 21O) nuclear reactions on a 18O target provide measurements of excited state en...
The 19F(p,α0)16O and 19F(p,απ)16O reactions can be fruitfully exploited to probe natural parity stat...
The rate of destruction of 18F via the 18F + p reactions is of importance in both novae and X-ray b...
A good understanding of the level structure of 19Ne around the proton threshold is critical to estim...
Proton and alpha widths for a 3/2+ ( l p = 0) state in 19Ne at Ex-7.1 MeV have been extracted using ...
In explosive astrophysical environments such as novae, X-ray bursters and supernovae, conditions of...
Proton and two proton emission from light neutron deficient nuclei around A=20 have been studied. A ...
The investigation of the 19F(p, α0) reaction at low bombarding energies allows the study of the spec...
A powerful method of investigating proton-unbound nuclear states by tracking their decay products in...
A method has been developed that can provide beams of many short-lived nuclei of interest in nucleos...
The 17F(p, γ)18 reaction is important in stellar explosions, but its rate has been uncertain because...
We discuss new results concerning the investigation of the 19F(p,α 0)16O and 10B(p,α 0)7Be reactions...
The nuclear structure of 19Ne near the proton threshold is of interest for understanding the rates o...
We have employed (^3He, n) double-stripping reactions to locate low-lying T = 3/2 and T = 2 states i...
We have employed (^3He, n) double-stripping reactions to locate low-lying T = 3/2 and T = 2 states i...
(18O, 19N) and (18O, 21O) nuclear reactions on a 18O target provide measurements of excited state en...
The 19F(p,α0)16O and 19F(p,απ)16O reactions can be fruitfully exploited to probe natural parity stat...
The rate of destruction of 18F via the 18F + p reactions is of importance in both novae and X-ray b...
A good understanding of the level structure of 19Ne around the proton threshold is critical to estim...
Proton and alpha widths for a 3/2+ ( l p = 0) state in 19Ne at Ex-7.1 MeV have been extracted using ...
In explosive astrophysical environments such as novae, X-ray bursters and supernovae, conditions of...
Proton and two proton emission from light neutron deficient nuclei around A=20 have been studied. A ...
The investigation of the 19F(p, α0) reaction at low bombarding energies allows the study of the spec...
A powerful method of investigating proton-unbound nuclear states by tracking their decay products in...
A method has been developed that can provide beams of many short-lived nuclei of interest in nucleos...
The 17F(p, γ)18 reaction is important in stellar explosions, but its rate has been uncertain because...