Keywords:
Publications of O. Trippella
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.
2023
Determination of the astrophysical factor of the 3He(α,γ)7Be 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] |
2021
Indirect determination of the astrophysical S factor for the 6Li(p,γ)7Be reaction using the asymptotic normalization coefficient method, , , , , *, , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , and , Phys. Rev. C 104, 015807 (2021) | pub id: 1142 [DOI] [URL] |
The 3He+5He→α+α reaction below the Coulomb barrier via the Trojan Horse Method, , , , , , , , , , , , , , , , , , , , , , , , , , , and , The European Physical Journal A 57, 20 (2021) | pub id: 1091 [DOI] [URL] |
2020
Astrophysical S-factor for the 3He(α,γ)7Be reaction via the asymptotic normalization coefficient ({ANC}) method, , , , , *, , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , and , Physics Letters B 807, 135606 (2020) | pub id: 1040 [DOI] [URL] |
Constraining the 22Ne(α,γ)26Mg and 22Ne(α,n)25Mg reaction rates using sub-Coulomb α-transfer reactions, , *, , , *, , , , , , and , Physics Letters B 802, 135267 (2020) | pub id: 976 [DOI] [URL] |
2018
Neutron enhancement from laser interaction with a critical fluid, , , , , , , , , , , , , , , , , and , Physics Letters A 382, 94--98 (2018) | pub id: 785 [DOI] [URL] |
2017
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] |
2016
Reaction rate of the 13C(α,n)16O neutron source using the ANC of the −3 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] |
2015
Updated THM Astrophysical Factor of the 19F(p,α)16O Reaction and Influence of New Direct Data at Astrophysical Energies, , , , , , and , The Astrophysical Journal 805, 128 (2015) | pub id: 186 [DOI] [URL] |
2014
Measurement of the 13C(α,n)16O reaction at astrophysical energies using the Trojan Horse Method. Focus on the −3 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] |
2013
On the Measurement of the 13C(α,n)16O S-factor at Negative Energies and its Influence on the s-process, , , , , *, , , , , , , , , and , The Astrophysical Journal 777, 143 (2013) | pub id: 316 [DOI] [URL] |
2012
Measurement of the −3 keV Resonance in the Reaction 13C(α,n)16O of Importance in the s-Process, , , , , *, , , , , , , , , and , Phys. Rev. Lett. 109, 232701 (2012) | pub id: 327 [DOI] [URL] |