New measurement of the α asymptotic normalization coefficient of the 1/2+ state in O17 at 6.356 MeV that dominates the C13(α,n)O16 reaction rate at temperatures relevant for the s process

M. L. Avila, G. V. Rogachev, E. Koshchiy, L. T. Baby, J. Belarge, K. W. Kemper, A. N. Kuchera, and D. Santiago-Gonzalez
Phys. Rev. C 91, 048801 – Published 16 April 2015

Abstract

Background: Accurate knowledge of the C13(α,n)O16 reaction cross section is important for the understanding of the s process in asymptotic giant branch stars, since it is considered to be the main source of neutrons. The subthreshold 1/2+ state at excitation energy of 6.356 MeV in O17 has a strong influence on the reaction cross section at energies relevant for astrophysics. Several experiments have been performed to determine the contribution of this state to the C13(α,n)O16 reaction rate. Nevertheless, significant discrepancies between different measurements remain.

Purpose: The aim of this work is to investigate these discrepancies.

Method: An 8 MeV C13 beam (below the Coulomb barrier) was used to study the α-transfer reaction Li6(C13,d)O17.

Results: The squared Coulomb-modified asymptotic normalization coefficient of the 1/2+ state in O17 measured in this work is (C̃α13CO17(1/2+))2=3.6±0.7fm1.

Conclusions: Discrepancy between the results of α-transfer experiments have been resolved. However, some discrepancy with the most recent measurement using the Trojan Horse method remains.

  • Figure
  • Figure
  • Figure
  • Figure
  • Received 22 January 2015

DOI:https://doi.org/10.1103/PhysRevC.91.048801

©2015 American Physical Society

Authors & Affiliations

M. L. Avila1,*, G. V. Rogachev2,†, E. Koshchiy2, L. T. Baby1, J. Belarge1, K. W. Kemper1, A. N. Kuchera1,‡, and D. Santiago-Gonzalez1,§

  • 1Department of Physics, Florida State University, Tallahassee, Florida 32306, USA
  • 2Department of Physics & Astronomy and Cyclotron Institute, Texas A&M University, College Station, Texas 77843, USA

  • *Physics Division, Argonne National Laboratory, Argonne Illinois 60439, USA; mavila@anl.gov
  • rogachev@tamu.edu
  • National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
  • §Department of Physics and Astronomy, Louisiana State University, Baton Rouge, Louisiana 70803, USA.

Article Text (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 91, Iss. 4 — April 2015

Reuse & Permissions
Access Options
CHORUS

Article Available via CHORUS

Download Accepted Manuscript
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review C

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×