K. Hatanaka

The $^{22}$ Ne( $α$ ,n) $^{25}$ Mg reaction is the dominant neutron source for the slow neutron capture process ( $s$ -process) in massive stars and contributes, together with the $^{13}$ …

nucl-ex2011★ 70 cited

The $^{150}$ Nd( $^{3}$ He, $t$ ) and $^{150}$ Sm( $t$ , $^{3}$ He) reactions with applications to $β β$ decay of $^{150}$ Nd

C. J. Guess, T. Adachi, H. Akimune +40

The $^{150}$ Nd( $^{3}$ He, $t$ ) reaction at 140 MeV/u and $^{150}$ Sm( $t$ , $^{3}$ He) reaction at 115 MeV/u were measured, populating excited states in $^{150}$ Pm. The transitions studied po…

Probing astrophysically important states in 26Mg nucleus to study neutron sources for the s-Process

The 150Nd(3He,t) and 150Sm(t,3He) reactions with applications to ββ decay of 150Nd

Probing astrophysically important states in $^{26}$ Mg nucleus to study neutron sources for the $s$ -Process

The $^{150}$ Nd( $^{3}$ He, $t$ ) and $^{150}$ Sm( $t$ , $^{3}$ He) reactions with applications to $β β$ decay of $^{150}$ Nd