The 26Al(p, γ)27Si reaction at low stellar temperature

Details The 26Al(p, γ)27Si reaction at low stellar temperature The 26Al(p, γ)27Si reaction at low stellar temperature

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993nupha.556..123c&link_type=abstract

Nuclear Physics A, Volume 556, Issue 1, p. 123-135.

Physics

Nuclear Physics

26

Scientific paper

Shell-model calculations have been used to predict the locations of states in 27Si which are analogous to well-studied states in 27Al. From this, we have determined the resonance properties of the known states in 27Si near the 26Al + p threshold. The resulting thermonuclear reaction rate is uncertain by about a factor of ten at low temperatures, but it appears that the 26Al(p, γ)27Si reaction is too slow to destroy a significant amount of 26Al at these temperatures.

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