Publication Date:
2011-04-13
Description:
Author(s): C. E. Beer, A. M. Laird, A. St. J. Murphy, M. A. Bentley, L. Buchman, B. Davids, T. Davinson, C. A. Diget, S. P. Fox, B. R. Fulton, U. Hager, D. Howell, L. Martin, C. Ruiz, G. Ruprecht, P. Salter, C. Vockenhuber, and P. Walden The ^{18} F(p,α)^{15} O reaction rate is crucial for understanding the final abundance of ^{18} F predicted by nova models. The γ-ray emission in the first few hours after a nova outburst is expected to be dominated by 511 keV annihilation photons from the decay of ^{18} F, and so understanding i... [Phys. Rev. C 83, 042801] Published Tue Apr 12, 2011
Keywords:
Nuclear Astrophysics
Print ISSN:
0556-2813
Electronic ISSN:
1089-490X
Topics:
Physics
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