Zobrazeno 1 - 10
of 21
pro vyhledávání: '"R. Ortez"'
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:
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:
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
Autor:
Stephen Quinn, C. J. Prokop, Christopher Wrede, M. Santia, Steven D. Pain, N. Cooper, J. Quaglia, Dan Irvine, M. B. Bennett, A. Chen, S. B. Schwartz, Kelly Chipps, Jorge Pereira, Anna Simon, R. Ortez, E. Thiagalingam, S. Shanab, A. Bowe, A. Spyrou, E. McNeice, F. Naqvi, Sean Liddick, Fernando Montes, Jordi José
Publikováno v:
Proceedings of XIII Nuclei in the Cosmos — PoS(NIC XIII).
Autor:
R. Ortez, C. J. Prokop, Sean Liddick, Fernando Montes, E. Thiagalingam, A. Spyrou, D. Irvine, N. Cooper, Christopher Wrede, M. Santia, D. Pérez-Loureiro, M. B. Bennett, Steven D. Pain, J. Pereira, S. J. Quinn, F. Naqvi, S. B. Schwartz, E. McNeice, Kelly Chipps, A. Bowe, J. Sakstrup, J. Quaglia, A. Chen, Anna Simon, S. Shanab
Publikováno v:
Physical Review C. 92
Background: The Doppler broadening of gamma-ray peaks is due to nuclear recoil from beta-delayed nucleon emission can be used to measure the energies of the nucleons. This method has never been tested using beta-delayed proton emission or applied to
Autor:
A. García, A. Chen, T. Faestermann, C. Fry, D. Pérez-Loureiro, H.-F. Wirth, Anuj Parikh, Ralf Hertenberger, Shawn Bishop, R. Ortez, B. A. Brown, Christopher Wrede
Publikováno v:
Physical Review C. 91
Background: The thermonuclear Cl-34g,Cl-m(p,gamma)Ar-35 reaction rates are unknown due to a lack of experimental nuclear physics data. Uncertainties in these rates translate to uncertainties in S-34 production in models of classical novae on oxygen-n
Autor:
Christopher Wrede, M. Santia, A. Spyrou, Christopher Prokop, Kelly Chipps, Steven D. Pain, Sean Liddick, E. McNeice, Fernando Montes, A. Bowe, Anna Simon, J. Quaglia, Jordi José, M. B. Bennett, A. Chen, J. Pereira, N. Cooper, S. Shanab, F. Naqvi, S. B. Schwartz, S. J. Quinn, D. Irvine, R. Ortez, E. Thiagalingam
Publikováno v:
Physical Review Letters. 111
Classical novae are expected to contribute to the 1809-keV Galactic $\ensuremath{\gamma}$-ray emission by producing its precursor $^{26}\mathrm{Al}$, but the yield depends on the thermonuclear rate of the unmeasured $^{25}\mathrm{Al}(p,\ensuremath{\g
Autor:
M B, Bennett, C, Wrede, K A, Chipps, J, José, S N, Liddick, M, Santia, A, Bowe, A A, Chen, N, Cooper, D, Irvine, E, McNeice, F, Montes, F, Naqvi, R, Ortez, S D, Pain, J, Pereira, C, Prokop, J, Quaglia, S J, Quinn, S B, Schwartz, S, Shanab, A, Simon, A, Spyrou, E, Thiagalingam
Publikováno v:
Physical review letters. 111(23)
Classical novae are expected to contribute to the 1809-keV Galactic γ-ray emission by producing its precursor 26Al, but the yield depends on the thermonuclear rate of the unmeasured 25Al(p,γ)26Si reaction. Using the β decay of 26P to populate the
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Akademický článek
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