Relative production rates of 6He, 9Be, 12C in astrophysical environments

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Published 30 June 2010 Europhysics Letters Association
, , Citation R. de Diego et al 2010 EPL 90 52001 DOI 10.1209/0295-5075/90/52001

0295-5075/90/5/52001

Abstract

We assume an environment of neutrons and α-particles of given density and temperature where nuclear syntheses into 6He, 9Be and 12C are possible. We investigate the resulting relative abundance as a function of density and temperature. When the relative abundance of α-particles Yα is between 0.4 and 0.9, or larger than 0.9, the largest production is 9Be or 12C, respectively. When Yα<0.4 6He is mostly frequently produced for temperatures above about 2 GK whereas the 9Be production dominates at smaller temperatures.

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