Particle decay of astrophysically-important 19Ne levels

Author:

Bardayan D W,Chipps K A,Ahn S,Blackmon J C,Greife U,Jones K L,Kontos A,Kozub R L,Linhardt L,Manning B,Matos M,O’Malley P D,Ota S,Pain S D,Peters W A,Pittman S T,Sachs A,Schmitt K T,Smith M S,Thompson P

Abstract

Abstract The 15O(α,γ)19Ne reaction is an important trigger reaction leading to the rapid proton (rp) capture process in X-ray bursts. The primary uncertainty in determining its astrophysical rate is the uncertain α branching ratios of levels near Ex = 4.1 MeV in 19Ne. These states have been populated in a study of the 20Ne(p, d)19Ne reaction, and α branching ratios are reported in this manuscript.

Publisher

IOP Publishing

Subject

General Physics and Astronomy

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