Keywords:
Publications of G. L. Guardo sorted by journal and type
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.
Phys. Rev. C
Assessing the near threshold cross section of the $^{17}\mathrm{O}(n,\alpha)^{14}\mathrm{C}$ reaction by means of the Trojan horse method, , , , , , , , , , , , , , , and , Phys. Rev. C 95, 025807 (2017) | pub id: 602 [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] |
Suppression of the centrifugal barrier effects in the off-energy-shell neutron + $^{17}\mathrm{O}$ interaction, , , , , , , , , , , , , , , , , , , , , *, , , , , , , , and , Phys. Rev. C 87, 012801(R) (2013) | pub id: 248 [DOI] [URL] |
Phys. Rev. Lett.
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] |
Physics Letters A
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] |
The Astrophysical Journal
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] |
Matter and Radiation at Extremes
Radioisotope production using lasers: From basic science to applications, , *, , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , and , Matter and Radiation at Extremes 9, 037203 (2024) | pub id: 1360 [DOI] [URL] |
Phys. Rev. C
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] |
Physics Letters B
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] |
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] |
The Astrophysical Journal
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] |
The European Physical Journal A
The $^3\mathrm{He}+^5\mathrm{He}\rightarrow\alpha+\alpha$ reaction below the Coulomb barrier via the Trojan Horse Method, , , , *, , , , , , , , , , , , , , , , , , , , , , , and , The European Physical Journal A 57, 20 (2021) | pub id: 1091 [DOI] [URL] |
Publications of type Inproceedings
2014
Application of the Trojan Horse Method to study neutron induced reactions: the $^{17}\mathrm{O}(n,\alpha)^{14}\mathrm{C}$ reaction, , , , , , , , , , , , , , , , , , , , , *, , , , , , , , and , in: INPC 2013 – International Nuclear Physics Conference, EPJ Web of Conferences 66, Firenze, Italy, pages 07008, 2014 | pub id: 379 [DOI] |
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] |
2016
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] |
2023
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] |