Keywords:
Publications of R. Spartá sorted by first author
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.
B
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] |
C
$^{19}\mathrm{F}$ 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] |
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] |
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] |
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] |
K
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] |
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] |
L
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] |
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] |
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] |
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] |
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] |
N
Strong Resonances at High Excitation Energy in $^{17}\mathrm{O}+$ Alpha Resonance Scattering, , , , , , , , , , , , , and , in: LXIX Nucleus 2019: Fundamental Problems of Nuclear Physics, Nuclei at Borders of Nucleon Stability, High Technologies, Physics of Atomic Nuclei 83, Dubna, Russia, pages 520--522, Pleiades Publishing Ltd, 2020 | pub id: 1161 [DOI] [URL] |
P
Trojan Horse measurement of the $^{18}\mathrm{F}(p,\alpha)^{15}\mathrm{O}$ astrophysical ${S}({E})$-factor, , , , , , , , , , , , , and , The European Physical Journal A 52, 1--9 (2016) | pub id: 176 [DOI] [URL] |
Big bang nucleosynthesis revisited via Trojan Horse method measurements, , , , , , , , * and , The Astrophysical Journal 786, 112 (2014) | pub id: 167 [DOI] [URL] |
Trojan Horse cross section measurements and their impact on primordial nucleosynthesis, , , , , , , and , in: XL Symposium on Nuclear Physics 2017, Journal of Physics: Conference Series 940, Cocoyoc, Morelos, México, pages 012017, {IOP} Publishing, 2018 | pub id: 839 [DOI] [URL] |
Updated evidence of the Trojan horse particle invariance for the $^{2}\mathrm{H}(d,p)^{3}\mathrm{H}$ reaction, , , , *, , , , , and , Phys. Rev. C 87, 025805 (2013) | pub id: 252 [DOI] [URL] |
Trojan Horse particle invariance in fusion reactions, , , , *, , , , and , in: VI International Conference FUSION14, EPJ Web of Conferences 86, EDP Sciences, New Delhi, India, pages 00034, 2015 | pub id: 165 [DOI] [URL] |
S
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] |
T
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] |