Keywords:
Publications of E. Somorjai sorted by title
Authors associated with the Cyclotron Institute are , and those associated with Center of Excellence in Nuclear Training And University-based Research (CENTAUR) have a * next to their name.
Measurement of the 10~keV resonance in the $^{10}\mathrm{B}(p,\alpha_0)^{7}\mathrm{Be}$ reaction via the Trojan Horse method, , , , , , , , , , , , , , , , , *, , , , , , , , , , and , Phys. Rev. C 90, 035801 (2014) | pub id: 122 [DOI] [URL] |
THM determination of the 65~keV resonance strength intervening in the $^{17}\mathrm{O}(p,\alpha)^{14}\mathrm{N}$ reaction rate, , , , , , , , , , , , , , *, , , , , , and , in: Exotic Nuclei and Nuclear/Particle Astrophysics (V). from Nuclei to Stars: Carpathian Summer School of Physics 2014, AIP Conference Proceedings 1645, Sinaia, Romania, pages 392-396, 2015 | pub id: 188 [DOI] [URL] |
A
Astrophysical $S$-factor for the $^3\mathrm{He}(\alpha,\gamma)^7\mathrm{Be}$ reaction via the asymptotic normalization coefficient ({ANC}) method, , , , , *, , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , and *, Physics Letters B 807, 135606 (2020) | pub id: 1040 [DOI] [URL] |
D
Determination of the astrophysical factor of the $^3\mathrm{He}(\alpha,\gamma)^7\mathrm{Be}$ down to zero energy using the asymptotic normalization coefficient method, , , , , *, , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , and *, in: 28th International Nuclear Physics Conference (INPC 2022), Journal of Physics: Conference Series 2586, Cape Town South Africa, pages 012093, {IOP} Publishing, 2023 | pub id: 1337 [DOI] [URL] |
I
Indirect determination of the astrophysical $S$ factor for the $^6\mathrm{Li}(p,\gamma)^7\mathrm{Be}$ reaction using the asymptotic normalization coefficient method, , , , , *, , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , and *, Phys. Rev. C 104, 015807 (2021) | pub id: 1142 [DOI] [URL] |