Volume 90, Number 5, June 2010
|Number of page(s)||5|
|Published online||30 June 2010|
Relative production rates of 6He, 9Be, 12C in astrophysical environments
Instituto de Estructura de la Materia, CSIC - Serrano 123, E-28006 Madrid, Spain, EU
2 Department of Physics and Astronomy, Aarhus University - DK-8000 Aarhus C, Denmark, EU
Corresponding author: firstname.lastname@example.org
Accepted: 28 May 2010
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.
PACS: 25.10.+s – Nuclear reactions involving few-nucleon systems / 25.40.Lw – Radiative capture / 26.30.Hj – r-process
© EPLA, 2010
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