K. Kemper

most cited

^{50}

Ti(

d

p

)

^{51}

Ti, single neutron energies in the

N = 29

isotones and the

N = 32

subshell closure

9 citations · 9 across the 2 of their papers we have counts for

collaborators

2 papers

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…

nucl-ex2006

Astrophysical factor for the neutron generator 13C(alpha,n)16O reaction in the AGB stars

E. D. Johnson, G. V. Rogachev, A. M. Mukhamedzhanov +15

The reaction 13C(alpha,n) is considered to be the main source of neutrons for the s-process in AGB stars. At low energies the cross section is dominated by the 1/2+ 6.356 MeV sub-t…

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

Astrophysical factor for the neutron generator 13C(alpha,n)16O reaction in the AGB stars

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