The C 12 (α, 3) O 16 reaction and its implications for stellar helium burning

R. J. Deboer, J. Görres, M. Wiescher, R. E. Azuma, A. Best, C. R. Brune, C. E. Fields, S. Jones, M. Pignatari, D. Sayre, K. Smith, Francis Timmes, E. Uberseder

Research output: Contribution to journalArticle

43 Citations (Scopus)

Abstract

The creation of carbon and oxygen in our Universe is one of the forefront questions in nuclear astrophysics. The determination of the abundance of these elements is key to our understanding of both the formation of life on Earth and to the life cycles of stars. While nearly all models of different nucleosynthesis environments are affected by the production of carbon and oxygen, a key ingredient, the precise determination of the reaction rate of C12(α, 3)O16, has long remained elusive. This is owed to the reaction's inaccessibility, both experimentally and theoretically. Nuclear theory has struggled to calculate this reaction rate because the cross section is produced through different underlying nuclear mechanisms. Isospin selection rules suppress the E1 component of the ground state cross section, creating a unique situation where the E1 and E2 contributions are of nearly equal amplitudes. Experimentally there have also been great challenges. Measurements have been pushed to the limits of state-of-the-art techniques, often developed for just these measurements. The data have been plagued by uncharacterized uncertainties, often the result of the novel measurement techniques that have made the different results challenging to reconcile. However, the situation has markedly improved in recent years, and the desired level of uncertainty ‰10% may be in sight. In this review the current understanding of this critical reaction is summarized. The emphasis is placed primarily on the experimental work and interpretation of the reaction data, but discussions of the theory and astrophysics are also pursued. The main goal is to summarize and clarify the current understanding of the reaction and then point the way forward to an improved determination of the reaction rate.

Original languageEnglish (US)
Article number035007
JournalReviews of Modern Physics
Volume89
Issue number3
DOIs
StatePublished - Sep 7 2017

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helium
reaction kinetics
nuclear astrophysics
carbon
cross sections
visual perception
oxygen
nuclear fusion
ingredients
astrophysics
universe
stars
cycles
ground state

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Cite this

Deboer, R. J., Görres, J., Wiescher, M., Azuma, R. E., Best, A., Brune, C. R., ... Uberseder, E. (2017). The C 12 (α, 3) O 16 reaction and its implications for stellar helium burning. Reviews of Modern Physics, 89(3), [035007]. https://doi.org/10.1103/RevModPhys.89.035007

The C 12 (α, 3) O 16 reaction and its implications for stellar helium burning. / Deboer, R. J.; Görres, J.; Wiescher, M.; Azuma, R. E.; Best, A.; Brune, C. R.; Fields, C. E.; Jones, S.; Pignatari, M.; Sayre, D.; Smith, K.; Timmes, Francis; Uberseder, E.

In: Reviews of Modern Physics, Vol. 89, No. 3, 035007, 07.09.2017.

Research output: Contribution to journalArticle

Deboer, RJ, Görres, J, Wiescher, M, Azuma, RE, Best, A, Brune, CR, Fields, CE, Jones, S, Pignatari, M, Sayre, D, Smith, K, Timmes, F & Uberseder, E 2017, 'The C 12 (α, 3) O 16 reaction and its implications for stellar helium burning', Reviews of Modern Physics, vol. 89, no. 3, 035007. https://doi.org/10.1103/RevModPhys.89.035007
Deboer RJ, Görres J, Wiescher M, Azuma RE, Best A, Brune CR et al. The C 12 (α, 3) O 16 reaction and its implications for stellar helium burning. Reviews of Modern Physics. 2017 Sep 7;89(3). 035007. https://doi.org/10.1103/RevModPhys.89.035007
Deboer, R. J. ; Görres, J. ; Wiescher, M. ; Azuma, R. E. ; Best, A. ; Brune, C. R. ; Fields, C. E. ; Jones, S. ; Pignatari, M. ; Sayre, D. ; Smith, K. ; Timmes, Francis ; Uberseder, E. / The C 12 (α, 3) O 16 reaction and its implications for stellar helium burning. In: Reviews of Modern Physics. 2017 ; Vol. 89, No. 3.
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