Zobrazeno 1 - 10
of 53
pro vyhledávání: '"S B Schwartz"'
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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b477bf63609e8b0d6fb344370a3241ad
https://doi.org/10.1016/j.physletb.2018.01.041
https://doi.org/10.1016/j.physletb.2018.01.041
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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8afe1ea47da53ba4327d91d0829015ab
https://doi.org/10.1103/physrevc.99.065801
https://doi.org/10.1103/physrevc.99.065801
Autor:
S. B. Schwartz
Publikováno v:
Luso-Brazilian Review. 53:E59-E61
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c53d3136773962e79bbfe95241dabaef
https://doi.org/10.3368/lbr.53.2.e59
https://doi.org/10.3368/lbr.53.2.e59
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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8f478a44a6215d7030924555fe9906ce
https://doi.org/10.1103/physrevc.98.024309
https://doi.org/10.1103/physrevc.98.024309
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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::337c76539fa7763a18b5de442f68d1f2
https://doi.org/10.1103/physrevc.97.065803
https://doi.org/10.1103/physrevc.97.065803
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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e8ebaf6d5cc6a44359b28e6a58e46fd3
https://doi.org/10.1016/j.phpro.2015.05.070
https://doi.org/10.1016/j.phpro.2015.05.070
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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::1d5e5f1c949134b83b4897fbb8e7a28b
https://doi.org/10.1103/physrevc.96.032801
https://doi.org/10.1103/physrevc.96.032801
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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::add6d59d96c4a811c2f94e6c66e03360
https://doi.org/10.1103/physrevc.96.014306
https://doi.org/10.1103/physrevc.96.014306
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
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8cdffc249e21d4c84ed7b04a5159279f
https://doi.org/10.1103/physrevc.93.064320
https://doi.org/10.1103/physrevc.93.064320
Autor:
D. Pérez-Loureiro, M. B. Bennett, B. A. Brown, Sean Liddick, C. J. Prokop, B. E. Glassman, Patrick O'Malley, S. B. Schwartz, M. Walters, C. Langer, N. Larson, C. Fry, A. Chen, Hendrik Schatz, Kelly Chipps, E. McNeice, P. Thompson, Christopher Wrede, Zach Meisel, Steven D. Pain, D. W. Bardayan, Xianchen Xu, W.-J. Ong, S. Suchyta
Publikováno v:
Physical Review Letters. 116
The thermonuclear ^{30}P(p,γ)^{31}S reaction rate is critical for modeling the final elemental and isotopic abundances of ONe nova nucleosynthesis, which affect the calibration of proposed nova thermometers and the identification of presolar nova gr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e38d1878407ea552cfea424462a136f2
https://doi.org/10.1103/physrevlett.116.102502
https://doi.org/10.1103/physrevlett.116.102502