More Like this

1. $\alpha$ -unbound levels in ${}^{34}\mathrm{Ar}$ from ${}^{36}\mathrm{Ar}(p,t){}^{34}\mathrm{Ar}$ reaction measurements and implications for the astrophysical ${}^{30}\mathrm{S}(\alpha ,p){}^{33}\mathrm{Cl}$ reaction rate

   https://doi.org/10.1103/PhysRevC.97.054613  

   Long, A. M.; Adachi, T.; Beard, M.; Berg, G. P.; Couder, M.; deBoer, R. J.; Dozono, M.; Görres, J.; Fujita, H.; Fujita, Y.; et al (May 2018, Physical Review C)
2. ${}^{11}\mathrm{B}$ states above the $\alpha$ -decay threshold via the ${}^{10}\mathrm{B}(d,p){}^{11}\mathrm{B}$ reaction

   https://doi.org/10.1103/PhysRevC.110.054319  

   Kuchera, A N; Ryan, G; Selby, G; Snider, D; Anderson, S; Almaraz-Calderon, S; Baby, L T; Brown, B A; Hanselman, K; Lopez-Saavedra, E; et al (November 2024, Physical Review C)
3. Impact of ${}^{16}\mathrm{O}(e,e^{\prime }\alpha ){}^{12}\mathrm{C}$ measurements on the ${}^{12}\mathrm{C}(\alpha ,\gamma ){}^{16}\mathrm{O}$ astrophysical reaction rate

   https://doi.org/10.1103/PhysRevC.100.065802  

   Holt, R. J.; Filippone, B. W. (December 2019, Physical Review C)
4. Optical model potentials for deuteron scattering off ${}^{24}\mathrm{Mg},$ ${}^{28}\mathrm{Si},$ ${}^{58}\mathrm{Ni},$ ${}^{90}\mathrm{Zr},$ ${}^{116}\mathrm{Sn},$ and ${}^{208}\mathrm{Pb}$ at $\approx 100 \mathrm{MeV}\text{/}\text{nucleon}$

   https://doi.org/10.1103/PhysRevC.110.044314  

   Patel, D; Cuong, D C; Howard, K B; Garg, U; Khoa, Dao T; Akimune, H; Berg, G_P A; Fujiwara, M; Harakeh, M N; Itoh, M; et al (October 2024, Physical Review C)
5. ${}^{28}\mathrm{Si}(p,t){}^{26}\mathrm{Si}$ data reconsidered for the astrophysical ${}^{25}\mathrm{Al}(p,\gamma ){}^{26}\mathrm{Si}$ rate

   https://doi.org/10.1103/PhysRevC.108.035804  

   Bardayan, D. W. (September 2023, Physical Review C)