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Resolving the Resonance Conflict in the 18Ne(ɑ,p) Reaction Rate

Abstract Details

2019, Master of Science (MS), Ohio University, Physics and Astronomy (Arts and Sciences).
One of the key reactions for the breakout from hot-CNO cycle into the rp-process in explosive hydrogen burning is 18Ne(alpha,p). At the ~0.4 GK break-out temperature for Type-I X-ray burst conditions, capture through a 1- state in 22Mg at 9.08 MeV is thought to dominate the reaction rate. However, since the most recent reaction rate evaluation, it has been suggested that another 1- state is located at 8.99 MeV. The existence of such a state could drastically change the 18Ne(alpha,p) reaction rate, possibly altering the shape of the X-ray bursts light curve and, consequently, conditions of the underlying neutron star inferred from model-observation comparisons. We set out to confirm or refute the existence of the 8.99 MeV state using neutron time-of-flight spectroscopy at the Edwards Accelerator Laboratory at Ohio University. The results from our recent measurement of 20Ne(3He,n)22Mg will be incorporated into X-ray bursts model calculations in the future.
Zach Meisel (Advisor)
59 p.

Recommended Citations

Citations

  • Sultana, C. I. (2019). Resolving the Resonance Conflict in the 18Ne(ɑ,p) Reaction Rate [Master's thesis, Ohio University]. OhioLINK Electronic Theses and Dissertations Center. http://rave.ohiolink.edu/etdc/view?acc_num=ohiou1566229309544122

    APA Style (7th edition)

  • Sultana, Chowdhury Irin. Resolving the Resonance Conflict in the 18Ne(ɑ,p) Reaction Rate . 2019. Ohio University, Master's thesis. OhioLINK Electronic Theses and Dissertations Center, http://rave.ohiolink.edu/etdc/view?acc_num=ohiou1566229309544122.

    MLA Style (8th edition)

  • Sultana, Chowdhury Irin. "Resolving the Resonance Conflict in the 18Ne(ɑ,p) Reaction Rate ." Master's thesis, Ohio University, 2019. http://rave.ohiolink.edu/etdc/view?acc_num=ohiou1566229309544122

    Chicago Manual of Style (17th edition)