Keywords:
Publications of S. Romano sorted by recency
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.
Searching for resonance states in $^{22}\mathrm{Ne}(p,\gamma)^{23}\mathrm{Na}$, , , *, , , , , , , , , , , , , , , and , Phys. Rev. C 108, 045802 (2023) | pub id: 1350 [DOI] [URL] |
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] |
A New Reaction Rate of the $^{27}\mathrm{Al}(p/\alpha)^{24}\mathrm{Mg}$ Reaction Based on Indirect Measurements at Astrophysical Energies and Implications for $^{27}\mathrm{Al}$ Yields of Intermediate-mass Stars, , , *, , , , , , , , , , , , , , , , , , , , and , The Astrophysical Journal 941, 96 (2022) | pub id: 1307 [DOI] [URL] |
Exploring the astrophysical energy range of the $^{27}\mathrm{Al}(p,\alpha)^{24}\mathrm{Mg}$ reaction: A new recommended reaction rate, , , *, , , , , , , , , , , , , , , , , , and , Physics Letters B 826, 136917 (2022) | pub id: 1207 [DOI] [URL] |
Experimental study of the $^{30}\mathrm{Si}(^3\mathrm{He},d)^{31}\mathrm{P}$ reaction and thermonuclear reaction rate of $^{30}\mathrm{Si}(p,\gamma)^{31}\mathrm{P}$, , , *, , , , , , , , , , , , and , Phys. Rev. C 105, 015805 (2022) | pub id: 1195 [DOI] [URL] |
$^{19}\mathrm{F}$ spectroscopy and implications for astrophysics, , , , , , , , , , , , , , , , , , and , in: Nuclear Physics in Astrophysics IX, Journal of Physics: Conference Series 1668, Frankfurt, Germany, pages 012023, {IOP} Publishing, 2020 | pub id: 1159 [DOI] [URL] |
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] |
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] |
Observation of $^{15}\mathrm{N}+\alpha$ resonant structures in $^{19}\mathrm{F}$ using the thick target in inverse kinematics scattering method, , , , , , , , , , , , , , , , , , and , Phys. Rev. C 99, 034301 (2019) | pub id: 927 [DOI] [URL] |
Neutron enhancement from laser interaction with a critical fluid, , , *, , , , , , , , , , , , , , and , Physics Letters A 382, 94--98 (2018) | pub id: 785 [DOI] [URL] |
Range of plasma ions in cold cluster gases near the critical point, , , *, , , , , , , , , , , , , , and , Physics Letters A 381, 1682 - 1686 (2017) | pub id: 643 [DOI] [URL] |
Measurement of the $^{10}\mathrm{B}(p,{\alpha}_{0})^{7}\mathrm{Be}$ cross section from 5 keV to 1.5 MeV in a single experiment using the Trojan horse method, , , , , , , , , , , , , , , , , , , , , , , , , , , , , and , Phys. Rev. C 95, 035801 (2017) | pub id: 601 [DOI] [URL] |
Reaction rate of the $^{13}\mathrm{C}(\alpha,n)^{16}\mathrm{O}$ neutron source using the ANC of the $-3~\mathrm{keV}$ resonance measured with the THM, , , , , *, *, , , , , , , , and , in: Nuclear Physics in Astrophysics VI (NPA6), Journal of Physics: Conference Series 665, Lisbon, Portugal, pages 012013, 2016 | pub id: 516 [DOI] [URL] |
Clustering in Non-Self-Conjugate Nuclei, *, , , , , , , , , , , , , , , , and , in: Proceedings of the Yukawa International Seminar 2011 (YKIS2011), Progress of Theoretical Physics Supplement 196, Kyoto, Japan, pages 184-191, 2012 | pub id: 436 [DOI] [URL] |
Measurement of the $-3~\mathrm{keV}$ Resonance in the Reaction $^{13}\mathrm{C}(\alpha,n)^{16}\mathrm{O}$ of Importance in the $s$-Process, , , , , *, *, , , , , , , , and , Phys. Rev. Lett. 109, 232701 (2012) | pub id: 327 [DOI] [URL] |
Experimental study of the $^{18}\mathrm{O}(d,p)^{19}\mathrm{O}$ reaction and the ANC Method, , , , , , *, , , , , , , , , , , , and , in: 11th International Conference on Nucleus-Nucleus Collisions (NN2012), Journal of Physics: Conference Series 420, San Antonio, Texas, pages 012142, 2013 | pub id: 317 [DOI] [URL] |
On the Measurement of the $^{13}\mathrm{C}(\alpha, n)^{16}\mathrm{O}$ ${S}$-factor at Negative Energies and its Influence on the $s$-process, , , , , *, *, , , , , , , , and , The Astrophysical Journal 777, 143 (2013) | pub id: 316 [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] |
New determination of the $^2\mathrm{H}(d,p)^3\mathrm{H}$ and $^2\mathrm{H}(d,n)^3\mathrm{He}$ reaction rates at astrophysical energies, , , , *, , , , , , , , , , , , , , and , The Astrophysical Journal 785, 96 (2014) | pub id: 166 [DOI] [URL] |
Measurement of the $^{13}\mathrm{C}(\alpha, n)^{16}\mathrm{O}$ reaction at astrophysical energies using the Trojan Horse Method. Focus on the $-3~\mathrm{keV}$ sub-threshold resonance, , , , , *, *, , , , , , , , and , in: INPC 2013 – International Nuclear Physics Conference, EPJ Web of Conferences 66, EDP Sciences, Firenze, Italy, pages 07010, 2014 | pub id: 155 [DOI] [URL] |
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] |
Measurement of the 20 and 90~keV Resonances in the $^{18}\mathrm{O}(p,\alpha)^{15}\mathrm{N}$ Reaction via the Trojan Horse Method, , , *, , , , , , , , , , , , , , , , , , , and , Phys. Rev. Lett. 101, 152501 (2008) | pub id: 82 [DOI] [URL] |