30S(alpha,p) in X-Ray Bursts at CRIB
D. Kahl, A. A. Chen, S. Kubono, D. N. Binh, J. Chen, T. Hashimoto, S., Hayakawa, D. Kaji, A. Kim, Y. Kurihara, N. H. Lee, S. Nishimura, Y. Ohshiro,, K. Setoodeh nia, Y. Wakabayashi, H. Yamaguchi
TL;DR
This paper discusses the development of a well-characterized 30S radioactive beam intended for future experiments to measure the 30S(alpha,p) reaction rate relevant to Type I X-ray bursts.
Contribution
It reports on the progress in producing and characterizing a 30S radioactive beam for astrophysical reaction rate measurements.
Findings
Successful development of a 30S radioactive beam
Characterization of the beam for future experiments
Preparation for direct measurement of stellar reaction rates
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.
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