J. Su

The solar composition problem has puzzled astrophysicists for more than 20 years. Recent measurements of carbon-nitrogen-oxygen (CNO) neutrinos by the Borexino experiment show a $\…

nucl-ex2023★ 24 cited

Isospin-dependence of the charge-changing cross-section shaped by the charged-particle evaporation process

J. W. Zhao, B. -H. Sun, I. Tanihata +26

We present the charge-changing cross sections (CCCS) of $^{11 - 15}$ C, $^{13 - 17}$ N, and $^{15, 17 - 18}$ O at around 300 MeV/nucleon on a carbon target, which extends to $p$ -shell isotop…

nucl-ex2022★ 39 cited

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

B. Gao, T. Y. Jiao, Y. T. Li +71

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-ex2021★ 22 cited

Advancement of Photospheric Radius Expansion and Clocked Type-I X-Ray Burst Models with the New $^{22}$ Mg $(α, p)^{25}$ Al Reaction Rate Determined at Gamow Energy

J. Hu, H. Yamaguchi, Y. H. Lam +34

We report the first (in)elastic scattering measurement of $^{25} Al + p$ with the capability to select and measure in a broad energy range the proton resonances in $^{26}$ Si…

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…

Enhanced S-factor for the 14N(p,γ)15O reaction and its impact on the solar composition problem

Isospin-dependence of the charge-changing cross-section shaped by the charged-particle evaporation process

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

Advancement of Photospheric Radius Expansion and Clocked Type-I X-Ray Burst Models with the New 22Mg(α,p)25Al Reaction Rate Determined at Gamow Energy

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

Enhanced $S$ -factor for the $^{14}$ N $(p, γ)^{15}$ O reaction and its impact on the solar composition problem

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

Advancement of Photospheric Radius Expansion and Clocked Type-I X-Ray Burst Models with the New $^{22}$ Mg $(α, p)^{25}$ Al Reaction Rate Determined at Gamow Energy

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