Resonances in 19Ne with relevance to the astrophysically important 18F(p,$\alpha$)15O reaction

Autor: Nicolas de Séréville, C. Angulo, Pedja Ujic, O. Kamalou, Alexander Murphy, F. de Oliveira, L. Achouri, P. J. Woods, D. J. Mountford, T. Davinson, Pierre Descouvemont, J. R. Brown, S. T. Pittman, Alison Laird

Publikováno v: PoS-Proceedings of Science
VI European Summer School on Experimental Nuclear Astrophysics
VI European Summer School on Experimental Nuclear Astrophysics, Sep 2011, Acireale, Italy. pp.050
Physical Review C
Physical Review C, American Physical Society, 2012, 85, pp.022801. ⟨10.1103/PhysRevC.85.022801⟩
Physical Review C, 2012, 85, pp.022801. ⟨10.1103/PhysRevC.85.022801⟩

The most intense gamma-ray line observable from novae is likely to be from positron annihilation associated with the decay of 18F. The uncertainty in the destruction rate of this nucleus through the 18F(p,{\alpha})15O reaction presents a limit to int

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c2461ab94ea84d51b0830d3109aa4779
https://hal.in2p3.fr/in2p3-00702716