Improved $S$-factor of the $^{13}$C(p,$γ$)$^{14}$N reaction at $E_{mathrm{p}},=,$330-740 keV and parameters of resonances at 448 keV and 551 keV
Analysis
This article reports on improvements to the understanding of the $^{13}$C(p,$γ$)$^{14}$N reaction, a crucial process in nuclear astrophysics, specifically focusing on the S-factor and resonance parameters at specific energy levels. The research likely involves experimental measurements and analysis to refine the existing models of this reaction.
Key Takeaways
- •The research focuses on improving the understanding of the $^{13}$C(p,$γ$)$^{14}$N reaction.
- •The study investigates the S-factor and resonance parameters.
- •The energy range of interest is 330-740 keV.
Reference
“The article focuses on the $^{13}$C(p,$γ$)$^{14}$N reaction, the S-factor, and resonance parameters at 448 keV and 551 keV.”