Zobrazeno 1 - 10
of 73
pro vyhledávání: '"M B, Bennett"'
Autor:
C. Fry, H. Sims, B. A. Brown, H. Zhang, O. Hall, C. J. Prokop, Michael Febbraro, Praveen Shidling, P. Thompson, W.-J. Ong, D. Pérez-Loureiro, Kelly Chipps, D. W. Bardayan, M. R. Hall, B. E. Glassman, Sean Liddick, Jacob Allen, Patrick O'Malley, M. Friedman, M. B. Bennett, S. B. Schwartz, Christopher Wrede, Steven D. Pain
Publikováno v:
Physics Letters B. 778:397-402
Certain astrophysical environments such as thermonuclear outbursts on accreting neutron stars (Type-I X-ray bursts) are hot enough to allow for breakout from the Hot CNO hydrogen burning cycles to the rapid proton capture (rp) process. An important b
Autor:
H. Zhang, Jacob Allen, Praveen Shidling, L. J. Sun, D. W. Bardayan, Michael Febbraro, P. Thompson, M. B. Bennett, Kelly Chipps, C. Fry, M. R. Hall, B. E. Glassman, Christopher Wrede, H. Sims, S. B. Schwartz, O. Hall, Steven D. Pain, M. Friedman, W.-J. Ong, Patrick O'Malley, Sean Liddick, D. Pérez-Loureiro
Publikováno v:
Physical Review C. 99
Background: The $^{15}\mathrm{O}(\ensuremath{\alpha},\ensuremath{\gamma})^{19}\mathrm{Ne}$ bottleneck reaction in Type I x-ray bursts is the most important thermonuclear reaction rate to constrain experimentally, to improve the accuracy of burst ligh
Autor:
D. W. Bardayan, S. Suchyta, B. E. Glassman, E. Aboud, E. McNeice, D. Pérez-Loureiro, Hendrik Schatz, C. Fry, Xianchen Xu, M. Walters, C. J. Prokop, Z. Meisel, C. Langer, M. Friedman, A. Chen, Christopher Wrede, W.-J. Ong, P. Thompson, Steven D. Pain, B. A. Brown, M. B. Bennett, S. B. Schwartz, Patrick O'Malley, Sean Liddick, Kelly Chipps
Publikováno v:
Physical Review C. 98
Background: $^{32}\mathrm{Cl}$ is a neutron-deficient isotope with a $\ensuremath{\beta}$-decay half-life of 298 ms and a spin and parity of ${J}^{\ensuremath{\pi}}={1}^{+}$. Previous measurements of $^{32}\mathrm{Cl} \ensuremath{\beta}$-delayed $\en
Autor:
C. Fry, D. Pérez-Loureiro, P. Thompson, Kelly Chipps, N. Larson, C. J. Prokop, Sean Liddick, W.-J. Ong, M. B. Bennett, C. Langer, D. W. Bardayan, S. B. Schwartz, S. Suchyta, Z. Meisel, B. E. Glassman, Christopher Wrede, Hendrik Schatz, Patrick O'Malley, E. McNeice, Steven D. Pain, M. Walters, B. A. Brown, A. Chen, Xianchen Xu
Publikováno v:
Physical Review C. 97
Autor:
D. W. Bardayan, E. McNeice, C. Fry, C. J. Prokop, D. Pérez-Loureiro, A. Spyrou, Christopher Wrede, M. Santia, M. B. Bennett, Z. Meisel, J. Pereira, Steven D. Pain, F. Naqvi, S. B. Schwartz, A. Bowe, Kelly Chipps, Jordi José, M. Walters, N. Larson, J. Quaglia, Sean Liddick, R. Ortez, Fernando Montes, A. Chen, C. Langer, D. Irvine, S. Shanab, Wei Jia Ong, Patrick O'Malley, S. Suchyta, E. Thiagalingam, B. A. Brown, Anna Simon, P. Thompson, S. J. Quinn, N. Cooper, B. E. Glassman, Hendrik Schatz
Publikováno v:
Physics Procedia. 66:532-536
Classical novae are common thermonuclear explosions in the Milky Way galaxy, occurring on the surfaces of white-dwarf stars that are accreting hydrogen-rich material from companion stars. Nucleosynthesis in classical novae depends on radiative proton
Autor:
H. Zhang, Patrick O'Malley, B. E. Glassman, Kelly Chipps, B. A. Brown, Christopher Wrede, O. Hall, Jacob Allen, H. Sims, Steven D. Pain, Michael Febbraro, M. R. Hall, P. Thompson, Sean Liddick, Praveen Shidling, W.-J. Ong, C. Fry, D. W. Bardayan, D. Pérez-Loureiro, M. B. Bennett, S. B. Schwartz
Publikováno v:
Physical Review C. 96
The $^{15}\mathrm{O}(\ensuremath{\alpha},\ensuremath{\gamma})^{19}\mathrm{Ne}$ reaction is expected to trigger the initial path for breakout from the CNO hydrogen-burning cycles to the rapid proton capture $(rp)$ process in type I x-ray bursts on acc
Autor:
B. A. Brown, Sean Liddick, D. Pérez-Loureiro, C. J. Prokop, N. Cooper, J. Sakstrup, Christopher Wrede, M. Santia, M. B. Bennett, A. Spyrou, Steven D. Pain, S. J. Quinn, S. B. Schwartz, Anna Simon, J. Pereira, Kelly Chipps, A. Bowe, F. Naqvi, E. McNeice, R. Ortez, E. Thiagalingam, A. Chen, S. Shanab
Publikováno v:
Physical Review C. 96
We report the independent experimental confirmation of an isomeric state in the proton drip-line nucleus $^{26}$P. The ${\gamma}$-ray energy and half-life determined are 164.4 $\pm$ 0.3 (sys) $\pm$ 0.2 (stat) keV and 104 $\pm$ 14 ns, respectively, wh
Autor:
Alexander T. Chemey, A. Bowe, P.-L. Tai, Anna Simon, Christopher Prokop, N. Larson, A. Spyrou, M. B. Bennett, J. M. VonMoss, Vandana Tripathi, S. L. Tabor, S. Suchyta, S. J. Quinn, Sean Liddick
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 727:59-64
Beta-decay spectroscopy experiments are limited by the detection efficiency of ions and electrons in the experimental setup. While there is a variety of different experimental setups in use for beta-decay spectroscopy, one popular choice is silicon d
Autor:
S. J. Quinn, C. J. Prokop, D. Pérez-Loureiro, Christopher Wrede, M. Santia, A. Spyrou, S. Shanab, R. Ortez, M. B. Bennett, D. Irvine, Steven D. Pain, B. A. Brown, E. Thiagalingam, S. B. Schwartz, Sean Liddick, J. Sakstrup, Fernando Montes, N. Cooper, Anna Simon, J. Quaglia, Kelly Chipps, A. Chen, A. Bowe, J. Pereira, E. McNeice, F. Naqvi
Publikováno v:
Physical Review C. 93
Background: Measurements of $\ensuremath{\beta}$ decay provide important nuclear structure information that can be used to probe isospin asymmetries and inform nuclear astrophysics studies.Purpose: To measure the $\ensuremath{\beta}$-delayed $\ensure
Publikováno v:
Journal of fish biology. 89(5)
Differences in the reproductive biology of both the Australian weasel shark Hemigaleus australiensis and the Australian sharpnose shark Rhizoprionodon taylori were apparent between individuals from the southern-most extent of their range in eastern A