Astrophysical S-factor for alpha-Capture of (113)In in the p-Process Energy Range

C. Yalcin, R. T. Gueray, N. Oezkan, S. Kutlu, Gy. Gyuerky, J. Farkas, G. G. Kiss, Zs. Fueloep, T. Rauscher, E. Somorjai

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

The cross sections of (113)In(alpha, gamma)(117)Sb and (113)In(alpha,n)(116)Sb reactions have been measured using the activation method. The experiments were carried out at the ATOMKI cyclotron accelerator in the center of mass energy range from 8.7 to 13.7 MeV. Astrophysical S-factors have been calculated, and preliminary results are compared With statistical model predictions.

Original languageEnglish
Title of host publicationCapture Gamma-Ray Spectroscopy and Related Topics
EditorsA. Blazhev, J. Jolie, N. Warr, A. Zilges
PublisherAmerican Institute of Physics (AIP)
Pages631-632
Number of pages2
ISBN (Print)978-0-7354-0623-0
Publication statusPublished - 2009
Event13th International Symposium on Capture Gamma-Ray Spectroscopy and Related Topics - Cologne, Germany
Duration: 25 Aug 200829 Aug 2008

Publication series

NameAIP Conf Procs
Volume1090
ISSN (Print)0094-243X

Conference

Conference13th International Symposium on Capture Gamma-Ray Spectroscopy and Related Topics
Country/TerritoryGermany
CityCologne
Period25/08/0829/08/08

Keywords

  • p-process
  • (113)In
  • nucleosynthesis
  • reaction cross section

Fingerprint

Dive into the research topics of 'Astrophysical S-factor for alpha-Capture of (113)In in the p-Process Energy Range'. Together they form a unique fingerprint.

Cite this