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Experimental Investigation of the 19Ne(p,γ)20Na Reaction Rate and Implications for Breakout from the Hot CNO Cycle

Journal Article · · Physical Review Letters
 [1];  [2];  [2];  [2];  [2];  [2];  [2];  [3];  [3];  [3];  [3];  [3];  [3];  [3];  [3];  [4];  [4];  [4];  [5]
  1. Florida State University, Tallahassee, FL (United States); Florida State University
  2. Florida State University, Tallahassee, FL (United States)
  3. Louisiana State University, Baton Rouge, LA (United States)
  4. University of North Florida, Jacksonville, FL (United States)
  5. National Centre for Nuclear Research, Otwock (Poland)
The 19Ne(p,γ)20Na reaction is the second step of a reaction chain which breaks out from the hot CNO cycle, following the 15O(α,γ)19Ne reaction at the onset of x-ray burst events. We investigate the spectrum of the lowest proton-unbound states in 20Na in an effort to resolve contradictions in spin-parity assignments and extract reliable information about the thermal reaction rate. Here, the proton-transfer reaction 19Ne(d,n)20Na is measured with a beam of the radioactive isotope 19Ne at an energy around the Coulomb barrier and in inverse kinematics. We observe three proton resonances with the 19Ne ground state, at 0.44, 0.66, and 0.82 MeV c.m. energies, which are assigned 3+, 1+, and (0+), respectively. In addition, we identify two resonances with the first excited state in 19Ne, one at 0.20 MeV and one, tentatively, at 0.54 MeV. These observations allow us for the first time to experimentally quantify the astrophysical reaction rate on an excited nuclear state. Our experiment shows an efficient path for thermal proton capture in 19Ne(p,γ)20Na, which proceeds through ground state and excited-state capture in almost equal parts and eliminates the possibility for this reaction to create a bottleneck in the breakout from the hot CNO cycle.
Research Organization:
Florida State University, Tallahassee, FL (United States)
Sponsoring Organization:
National Science Foundation; USDOE; USDOE Office of Science (SC), Nuclear Physics (NP)
Grant/Contract Number:
FG02-02ER41220; FG02-96ER40978
OSTI ID:
1669891
Alternate ID(s):
OSTI ID: 1330290
OSTI ID: 1536440
Journal Information:
Physical Review Letters, Journal Name: Physical Review Letters Journal Issue: 18 Vol. 117; ISSN 0031-9007
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English

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Nuclear Physics of the Outer Layers of Accreting Neutron Stars text January 2018
Experimental study of intruder components in light neutron-rich nuclei via single-nucleon transfer reaction text January 2021