Astrophysical Reaction Rate of 12 C(α, γ) 16 O

  • Kunz R
  • Fey M
  • Jaeger M
  • et al.
250Citations
Citations of this article
22Readers
Mendeley users who have this article in their library.

Abstract

A new astrophysical reaction rate of 12C(α, γ)16O has been calculated based on our recent determination of the E1- and E2-capture cross sections. The R-matrix method has been applied to describe the SE1- and SE2-factor functions as well as the data of elastic α scattering and the β-delayed α decay of 16N from other experiments. The resulting reaction rate for stellar temperatures of T9=0.04-10 is presented in both tabular form and an analytic expression. A new temperature dependence of the reaction rate was obtained when compared with reported evaluations. The associated uncertainties were reduced considerably in comparison to previous determinations.

Cite

CITATION STYLE

APA

Kunz, R., Fey, M., Jaeger, M., Mayer, A., Hammer, J. W., Staudt, G., … Paradellis, T. (2002). Astrophysical Reaction Rate of 12 C(α, γ) 16 O. The Astrophysical Journal, 567(1), 643–650. https://doi.org/10.1086/338384

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free