Z. An

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★ 17 cited

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-th2016★ 9 cited

New Astrophysical Reaction Rate for the $^{12} C (α, γ)^{16} O$ Reaction

Z. D. An, Y. G. Ma, G. T. Fan +3

A new astrophysical reaction rate for $^{12}$ C( $α, γ$ ) $^{16}$ O has been evaluated on the basis of a global R-matrix fitting to the available experimental data. The reaction rates of…

nucl-th2015★ 23 cited

Astrophysical S factor of { $^{12}$ C( $α, γ$ ) $^{16}$ O} Calculated with the Reduced R-matrix Theory

Zhen-Dong An, Zhen-Peng Chen, Yu-Gang Ma +7

Determination of the accurate astrophysical S factor of { $^{12}$ C( $α, γ$ ) $^{16}$ O} reaction has been regarded as a holy grail of nuclear astrophysics for decades. In current stellar…

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

New Astrophysical Reaction Rate for the 12C(α,γ)16O Reaction

Astrophysical S factor of {12C(α,γ)16O} Calculated with the Reduced R-matrix Theory

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

New Astrophysical Reaction Rate for the $^{12} C (α, γ)^{16} O$ Reaction

Astrophysical S factor of { $^{12}$ C( $α, γ$ ) $^{16}$ O} Calculated with the Reduced R-matrix Theory