K. Kemper

In the Ge-Sr mass region, isotopes with neutron number $N \leq 40$ are known to feature rapid shape changes with both nucleon number and angular momentum. To gain new insights into…

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-ex2014★ 60 cited

Constraining the 6.05 MeV 0 $^{+}$ and 6.13 MeV 3 $^{-}$ cascade transitions in the $^{12}$ C( $α$ , $γ$ ) $^{16}$ O reaction using the Asymptotic Normalization Coefficients

M. L. Avila, G. V. Rogachev, E. Koshchiy +7

Background. The $^{12}$ C $(α, γ)^{16}$ O reaction plays a fundamental role in astrophysics and needs to be known with accuracy better than 10%. Cascade $γ$ transitions through the exc…

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…

Hexadecapole strength in the rare isotopes 74,76Kr

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

Constraining the 6.05 MeV 0+ and 6.13 MeV 3− cascade transitions in the 12C(α,γ)16O reaction using the Asymptotic Normalization Coefficients

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

Hexadecapole strength in the rare isotopes $^{74, 76}$ Kr

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

Constraining the 6.05 MeV 0 $^{+}$ and 6.13 MeV 3 $^{-}$ cascade transitions in the $^{12}$ C( $α$ , $γ$ ) $^{16}$ O reaction using the Asymptotic Normalization Coefficients