Publication Date:
2013-12-05
Description:
Author(s): 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, and E. Thiagalingam Classical novae are expected to contribute to the 1809-keV Galactic γ -ray emission by producing its precursor 26 Al, but the yield depends on the thermonuclear rate of the unmeasured 25 Al( p , γ ) 26 Si reaction. Using the β decay of 26 P to populate the key J π =3 + resonance in this reaction, we report the f... [Phys. Rev. Lett. 111, 232503] Published Wed Dec 04, 2013
Keywords:
Nuclear Physics
Print ISSN:
0031-9007
Electronic ISSN:
1079-7114
Topics:
Physics
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