Y. Wang

The $^{13}$ C( $α$ , $n$ ) $^{16}$ O reaction is the main neutron source for the slow-neutron-capture (s-) process in Asymptotic Giant Branch stars and for the intermediate (i-) process.…

nucl-ex2018

Astrophysical $S_{E 2}$ factor of the $^{12} C (α, γ)^{16} O$ reaction through the $^{12} C (^{11} B,^{7} Li)^{16} O$ transfer reaction

Y. P. Shen, B. Guo, Z. H. Li +20

The $^{12} C (α, γ)^{16} O$ reaction plays a key role in the evolution of stars with masses of $M >$ 0.55 $M_{⊙}$ . The cross-section of the ${}^{12}\mathrm{C}(α…

nucl-ex2009

Asymptotic normalization coefficient from the 12C(7Li,6He)13N reaction and the astrophysical 12C(p,g)13N reaction rate

Z. H. Li, J. Su, B. Guo +15

Angular distribution of the 12C(7Li,6He)13N reaction at E(7Li) = 44.0 MeV was measured at the HI-13 tandem accelerator of Beijing, China. Asymptotic normalization coefficient (ANC)…

Deep underground laboratory measurement of 13C(α,n)16O in the Gamow windows of the s- and i-processes

Astrophysical SE2​ factor of the 12C(α,γ)16O reaction through the 12C(11B,7Li)16O transfer reaction

Asymptotic normalization coefficient from the 12C(7Li,6He)13N reaction and the astrophysical 12C(p,g)13N reaction rate

Deep underground laboratory measurement of $^{13}$ C( $α$ , $n$ ) $^{16}$ O in the Gamow windows of the $s$ - and $i$ -processes

Astrophysical $S_{E 2}$ factor of the $^{12} C (α, γ)^{16} O$ reaction through the $^{12} C (^{11} B,^{7} Li)^{16} O$ transfer reaction