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Title: {sup 30}S Beam Development and X-ray Bursts

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.3362583· OSTI ID:21371070
; ; ; ; ; ; ;  [1]; ; ;  [2]; ;  [3]; ;  [4];  [1]
  1. Center for Nuclear Study (CNS), University of Tokyo, Wako, Saitama, 351-0198 (Japan)
  2. Department of Physics and Astronomy, McMaster University, Hamilton, Ontario, L8S-4M1 (Canada)
  3. RIKEN, Institute of Physical and Chemical Research, Wako, Saitama, 351-0198 (Japan)
  4. Department of Physics, Ewha Womans University, Seoul 120-750 (Korea, Republic of)

Over the past three years, we have worked on developing a well-characterized {sup 30}S radioactive beam to be used in a future experiment aiming to directly measure to extrapolate the {sup 30}S(alpha,p) stellar reaction rate within the Gamow window of Type I X-ray bursts. The importance of the {sup 30}S(alpha,p) reaction to X-ray bursts is discussed. Given the astrophysical motivation, the successful results of and challenges involved in the production of a low-energy {sup 30}S beam are detailed. Finally, an overview of our future plans regarding this on-going project are presented.

OSTI ID:
21371070
Journal Information:
AIP Conference Proceedings, Vol. 1213, Issue 1; Conference: 5. European summer school on experimental nuclear astrophysics, Santa Tecla, Sicily (Italy), 20-27 Sep 2009; Other Information: DOI: 10.1063/1.3362583; (c) 2010 American Institute of Physics; ISSN 0094-243X
Country of Publication:
United States
Language:
English