Title: New energy for the 133-keV resonance in the 23Na(p,γ) 24Mg reaction and its impact on nucleosynthesis in globular clusters

Journal Article · · Physical Review C
ORCiD logo [1]; ORCiD logo [2]; ORCiD logo [3]; ORCiD logo [3]; ORCiD logo [3]
  1. North Carolina State Univ., Raleigh, NC (United States); Triangles Univ. Nuclear Lab., Durham, NC (United States); Ohio Univ., Athens, OH (United States); North Carolina State University
  2. North Carolina State Univ., Raleigh, NC (United States); Triangles Univ. Nuclear Lab., Durham, NC (United States); European X-ray Free Electron Laser GmbH, Schenefeld (Germany)
  3. North Carolina State Univ., Raleigh, NC (United States); Triangles Univ. Nuclear Lab., Durham, NC (United States)

Globular cluster stars exhibit star-to-star anticorrelations between oxygen and sodium in their atmospheres. An improved description of the sodium-destroying 23Na +p reaction rates is essential to understanding these observations. We present an energy analysis of 24Mg states based on a new measurement of the 23Na(3He, d) 24Mg reaction. A key resonance in 23Na(p, γ) 24Mg is found to be at $$E$$ $$^{c.m.}_{r}$$ = 133(3) keV, 5 keV lower than previously adopted. This finding has a dramatic effect on the 23Na(p, γ) 24Mg reaction rate, increasing it by a factor of 2 for the recommended rate. Furthermore, the nucleosynthesis impact of this change is investigated.

Research Organization:
North Carolina State Univ., Raleigh, NC (United States)
Sponsoring Organization:
USDOE Office of Science (SC), Nuclear Physics (NP)
Grant/Contract Number:
FG02-97ER41042; SC0017799
OSTI ID:
1821590
Journal Information:
Physical Review C, Journal Name: Physical Review C Journal Issue: 3 Vol. 104; ISSN 2469-9985
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English

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