Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Karen Ostdiek"'
Autor:
Stephanie Lyons, Patrick O'Malley, U. Garg, J. Hu, Christopher Seymour, Wanpeng Tan, M. Şenyiğit, A. Gyurjinyan, T. Anderson, Y. K. Gupta, M. R. Hall, B. K. Nayak, Q. Liu, B. Vande Kolk, B. Frentz, N. Sensharma, Kouichi Hagino, Wenting Lu, Richard deBoer, Karen Ostdiek, O. Hall, K. B. Howard, Michael S. Smith, Edward Lamere, Ramandeep Gandhi, Michael Skulski, A. Long
Publikováno v:
Physics Letters B, Vol 806, Iss, Pp 135473-(2020)
Quasi-elastic scattering measurements have been performed using 16O and 24Mg projectiles off 90Zr at energies around the Coulomb barrier. Experimental data have been analyzed in the framework of coupled channels (CC) calculations using the code CCFUL
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e7d83fe6b8b3f6c0b4d5d82f4146a950
http://www.sciencedirect.com/science/article/pii/S037026932030277X
http://www.sciencedirect.com/science/article/pii/S037026932030277X
Autor:
Jacob Allen, J. Hu, J. J. Kolata, D. W. Bardayan, Catherine Nicoloff, A. M. Rogers, K. T. Macon, Kelly Chipps, M. R. Hall, B. Frentz, Patrick O'Malley, S. L. Henderson, S. Strauss, J. M. Kelly, Tan Ahn, Mallory Smith, J. C. Blackmon, Maxime Brodeur, Steven D. Pain, Y. K. Gupta, R. O. Torres-Isea, A. Long, J. Riggins, F. D. Becchetti, Karen Ostdiek, O. Hall
Publikováno v:
Physics Procedia. 90:415-420
The 14O(α,p)17F reaction is an important trigger reaction to the α-p process in X-ray bursts. The most stringent experimental constraints on its astrophysical rate come from measurements of the time-inverse reaction, 17F(p,α)14O. Previous studies
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::171e040be0b9437a075b2d46d94ad736
https://doi.org/10.1016/j.phpro.2017.09.043
https://doi.org/10.1016/j.phpro.2017.09.043
Autor:
A. M. Clark, Philippe Collon, Tom Woodruff, Michael Skulski, Greg Chmiel, Marc W. Caffee, Tyler Anderson, Karen Ostdiek, Austin Nelson
Publikováno v:
Physical Review C. 96
Short-lived radionuclides (SLRs) with half-lives less than 100 Myr are known to have existed around the time of the formation of the solar system around 4.5 billion years ago. Understanding the production sources for SLRs is important for improving o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::60e1ca7afc79b1907f6a313fd1cc650b
https://doi.org/10.1103/physrevc.96.015803
https://doi.org/10.1103/physrevc.96.015803
Autor:
Karen Ostdiek, Austin Nelson, John P. Greene, Michael Skulski, Walter Kutschera, A. M. Clark, Philippe Collon, Rugard Dressler, Matthew Bowers, Tyler Anderson, Michael Paul, W. Bauder, Daniel Robertson, Dorothea Schumann, Wenting Lu
Publikováno v:
Physical Review C. 95
The half-life of the neutron-rich nuclide $^{60}\mathrm{Fe}$ has been in dispute in recent years. A measurement in 2009 published a value of $(2.62\ifmmode\pm\else\textpm\fi{}0.04)\ifmmode\times\else\texttimes\fi{}{10}^{6}$ years, almost twice that o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fd0f9521fece13755a8937c951a671f7
https://doi.org/10.1103/physrevc.95.055809
https://doi.org/10.1103/physrevc.95.055809
Autor:
Wenting Lu, Donald Robertson, T. Anderson, Philippe Collon, R. Almus, P. Gastis, G. Perdikakis, W. Bauder, Michael Skulski, Karen Ostdiek
Equilibrium charge state distributions of stable 60Ni, 59Co, and 63Cu beams passing through a 1 μm thick Mo foil were measured at beam energies of 1.84 MeV/u, 2.09 MeV/u, and 2.11 MeV/u respectively. A 1-D position sensitive Parallel Grid Avalanche
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a4ce933f6a17d966aa692a1f4490cf3a
http://arxiv.org/abs/1509.07472
http://arxiv.org/abs/1509.07472
Autor:
Wenting Lu, Daniel Robertson, Matthew Bowers, Mary Beard, Yoav Kashiv, W. Bauder, Philippe Collon, Karen Ostdiek
Publikováno v:
Physical Review C. 88
Short-lived radionuclides (SLRs) with lifetimes τ < 100 Myr are known to have been extant when the Solar System formed over 4.5 billion years ago. Identifying the sources of SLRs is important for understanding the time scales of Solar System formati
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e648c0bfc1b4d950507818818d78e920
https://doi.org/10.1103/physrevc.88.065802
https://doi.org/10.1103/physrevc.88.065802
Autor:
B. E. Schultz, J. M. Kelly, J. Hu, J. Riggins, Jacob Allen, Tan Ahn, Patrick O'Malley, D. W. Bardayan, K. T. Macon, Maxime Brodeur, Catherine Nicoloff, B. Frentz, F. D. Becchetti, Y. K. Gupta, J. Long, R. O. Torres-Isea, O. Hall, S. Strauss, Michael S. Smith, S. L. Henderson, J. J. Kolata, Karen Ostdiek, Steven D. Pain, M. R. Hall, J. C. Blackmon, A. Long
Publikováno v:
Journal of Physics: Conference Series. 730:012004
Many astrophysical events, such as novae and X-ray bursts, are powered by reactions with radioactive nuclei. Studying the properties of these nuclei in the laboratory can therefore further our understanding of these astrophysical explosions. The Twin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::51daf6eccf490b9ae04c327ec9e41381
https://doi.org/10.1088/1742-6596/730/1/012004
https://doi.org/10.1088/1742-6596/730/1/012004