| First name(s): |
D. |
| Last name(s): |
Santiago |
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Authors associated with the Cyclotron Institute are underlined, and those associated with Center of Excellence in Nuclear Training And University-based Research (CENTAUR) have a * next to their name.
| Measurement of the −3 keV Resonance in the Reaction 13C(α,n)16O of Importance in the s-Process, M. La Cognata, C. Spitaleri, O. Trippella, G. G. Kiss, G. V. Rogachev*, A. M. Mukhamedzhanov, M. Avila, G. L. Guardo, E. Koshchiy, A. Kuchera, L. Lamia, S. M. R. Puglia, S. Romano, D. Santiago and R. Spartá, Phys. Rev. Lett. 109, 232701 (2012)
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pub id: 327 [DOI] [URL]
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| On the Measurement of the 13C(α,n)16O S-factor at Negative Energies and its Influence on the s-process, M. La Cognata, C. Spitaleri, O. Trippella, G. G. Kiss, G. V. Rogachev*, A. M. Mukhamedzhanov, M. Avila, G. L. Guardo, E. Koshchiy, A. Kuchera, L. Lamia, S. M. R. Puglia, S. Romano, D. Santiago and R. Spartá, The Astrophysical Journal 777, 143 (2013)
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pub id: 316 [DOI] [URL]
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| Reaction rate of the 13C(α,n)16O neutron source using the ANC of the −3 keV resonance measured with the THM, M. La Cognata, C. Spitaleri, O. Trippella, G. G. Kiss, G. V. Rogachev*, A. M. Mukhamedzhanov, M. Avila, G. L. Guardo, E. Koshchiy, A. Kuchera, L. Lamia, S. M. R. Puglia, S. Romano, D. Santiago and R. Spartá, in: Nuclear Physics in Astrophysics VI (NPA6), Journal of Physics: Conference Series 665, Lisbon, Portugal, pages 012013, 2016
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pub id: 516 [DOI] [URL]
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