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30S(alpha,p) in X-Ray Bursts at CRIB

arXiv:1010.4958 · doi:10.1063/1.3485188

Abstract

Over the past three years, we have worked on developing a well-characterized 30S radioactive beam to be used in a future experiment aiming to directly measure the 30S(alpha,p) stellar reaction rate within the Gamow window of Type I X-ray bursts.

3 pages, 1 figure, Origin of Matter and Evolution of the Galaxies (OMEG10), March 2010, Osaka, Japan