E. Temanson

The $^{25} Al (p, γ)^{26} Si$ reaction is part of a reaction network with impact on the observed galactic $^{26}$ Al abundance. A new determination of the proton strength of th…

nucl-ex2021★ 9 cited

$^{50}$ Ti( $d$ , $p$ ) $^{51}$ Ti, single neutron energies in the $N = 29$ isotones and the $N = 32$ subshell closure

L. A. Riley, 1 J. M. Nebel-Crosson, 1 K. T. Macon +9

A measurement of the $^{50}$ Ti( $d$ , $p$ ) $^{51}$ Ti reaction at 16 MeV was performed using a Super Enge Split Pole Spectrograph to measure the magnitude of the $N = 32$ subshell gap in…

Measurement of the 25Al(d,n)26Si reaction and impact on the 25Al(p,γ)26Si reaction rate

50Ti(d,p)51Ti, single neutron energies in the N=29 isotones and the N=32 subshell closure

Measurement of the $^{25} Al (d, n)^{26} Si$ reaction and impact on the $^{25} Al (p, γ)^{26} Si$ reaction rate

$^{50}$ Ti( $d$ , $p$ ) $^{51}$ Ti, single neutron energies in the $N = 29$ isotones and the $N = 32$ subshell closure