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Choplin |
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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.
Experimental Determination of $\alpha$ Widths of $^{21}\mathrm{Ne}$ Levels in the Region of Astrophysical Interest: New $^{17}\mathrm{O}+\alpha$ Reaction Rates and Impact on the Weak $s$ Process, F. Hammache, P. Adsley*, L. Lamia, D. S. Harrouz, N. de Séréville, B. Bastin, A. Choplin, T. Faestermann, C. Fougères, R. Hertenberger, R. Hirschi, M. La Cognata, A. Meyer, S. Palmerini, R. G. Pizzone, F. de Oliveira Santos, S. Romano, A. Tumino and H. -F. Wirth, Phys. Rev. Lett. 132, 182701 (2024)
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pub id: 1379 [DOI] [URL]
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Constraints on key $^{17}\mathrm{O}(\alpha,\gamma)^{21}\mathrm{Ne}$ resonances and impact on the weak $s$ process, M. Williams, A. M. Laird, A. Choplin, P. Adsley*, B. Davids, U. Greife, K. Hudson, D. Hutcheon, A. Lennarz and C. Ruiz, Phys. Rev. C 105, 065805 (2022)
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pub id: 1244 [DOI] [URL]
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The impact of $^{17}\mathrm{O}+\alpha$ reaction rate uncertainties on the $s$-process in rotating massive stars, J. Frost-Schenk, P. Adsley*, A. M. Laird, R. Longland, C. Angus, C. Barton, A. Choplin, C. Aa Diget, R. Hirschi, C. Marshall, F. Portillo~Chaves and K. Setoodehnia, Monthly Notices of the Royal Astronomical Society 514, 2650--2657 (2022)
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pub id: 1243 [DOI] [URL]
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A new $^{12}\mathrm{C}+^{12}\mathrm{C}$ nuclear reaction rate: Impact on stellar evolution, E. Monpribat, S. Martinet, S. Courtin, M. Heine, S. Ekström, D. G. Jenkins, A. Choplin, P. Adsley*, D. Curien, M. Moukaddam, J. Nippert, S. Tsiatsiou and G. Meynet, Astronomy & Astrophysics 660, A47 (2022)
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pub id: 1217 [DOI] [URL]
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