| First name(s): |
V. |
| Last name(s): |
Eremenko |
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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.
| Determination of the asymptotic normalization coefficients for $^{14}\mathrm{C} + n\rightarrow{}^{15}\mathrm{C}$, the $^{14}\mathrm{C}(n,\gamma)^{15}\mathrm{C}$ reaction rate, and evaluation of a new method to determine spectroscopic factors, M. McCleskey, A. M. Mukhamedzhanov, L. Trache, R. E. Tribble, A. Banu, V. Eremenko, V. Z. Goldberg, Y.-W. Lui, E. McCleskey, B. T. Roeder, A. Spiridon, F. Carstoiu, V. Burjan, Z. Hons and I. J. Thompson, Phys. Rev. C 89, 044605 (2014)
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pub id: 100 [DOI] [URL]
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| Proton decay of excited states in $^{12}\mathrm{N}$ and $^{13}\mathrm{O}$ and the astrophysical $^{11}\mathrm{C}(p,\gamma)^{12}\mathrm{N}$ reaction rate, L. G. Sobotka*, W. W. Buhro, R. J. Charity, J. M. Elson, M. F. Jager, J. Manfredi, M. H. Mahzoon, A. M. Mukhamedzhanov, V. Eremenko, M. McCleskey, R. G. Pizzone, B. T. Roeder, A. Spiridon, E. Simmons, L. Trache, M. Kurokawa and P. Navrátil, Phys. Rev. C 87, 054329 (2013)
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pub id: 312 [DOI] [URL]
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| Publisher's Note: Proton decay of excited states in $^{12}\mathrm{N}$ and $^{13}\mathrm{O}$ and the astrophysical $^{11}\mathrm{C}(p,\gamma)^{12}\mathrm{N}$ reaction rate, L. G. Sobotka*, W. W. Buhro, R. J. Charity, J. M. Elson, M. F. Jager, J. Manfredi, M. H. Mahzoon, A. M. Mukhamedzhanov, V. Eremenko, M. McCleskey, R. G. Pizzone, B. T. Roeder, A. Spiridon, E. Simmons, L. Trache, M. Kurokawa and P. Navrátil, Phys. Rev. C 87, 069902 (2013)
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pub id: 313 [DOI] [URL]
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