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New portal to the O15(α,γ)Ne19 resonance triggering CNO-cycle breakout

Journal Article · · Physical Review C
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  1. Michigan State Univ., East Lansing, MI (United States)
  2. Univ. of Notre Dame, Notre Dame, IN (United States)
  3. Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States); Univ. of Tennessee, Knoxville, TN (United States)
  4. Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States)
  5. Texas A & M Univ., College Station, TX (United States)
  6. Univ. of Surrey, Guildford (United Kingdom)
The 15O(α,γ)19Ne reaction is expected to trigger the initial path for breakout from the CNO hydrogen-burning cycles to the rapid proton capture (rp) process in type I x-ray bursts on accreting neutron stars. The thermonuclear reaction rate has a major impact on models of type I x-ray burst observables and it depends on the small α-particle branching ratio, Γα/Γ, of the 4.03 MeV state in 19Ne. Attempts to measure Γα/Γ by populating the 4.03 MeV state using nuclear reactions have only led to strong upper limits. In the present work, we report the first experimental evidence that the 4.03 MeV 19Ne state is populated in 20Mg β-delayed proton emission. Furthermore this new channel has the potential to provide the necessary sensitivity to detect a finite value of Γα/Γ.
Research Organization:
Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States)
Sponsoring Organization:
USDOE
Grant/Contract Number:
AC05-00OR22725
OSTI ID:
1513412
Alternate ID(s):
OSTI ID: 1395605
Journal Information:
Physical Review C, Journal Name: Physical Review C Journal Issue: 3 Vol. 96; ISSN PRVCAN; ISSN 2469-9985
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English

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Cited By (2)

Nuclear physics of the outer layers of accreting neutron stars journal July 2018
Nuclear Physics of the Outer Layers of Accreting Neutron Stars text January 2018

Figures / Tables (3)


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