Alloying effect on K shell X-ray fluorescence cross-sections and intensity ratios of Cu and Sn in Cu1Sn1-x alloys using the 59.5 keV gamma rays

Dogan M., Olgar M. A., Cengiz E., Tirasoglu E.

RADIATION PHYSICS AND CHEMISTRY, cilt.126, ss.111-115, 2016 (SCI-Expanded) identifier identifier

  • Yayın Türü: Makale / Tam Makale
  • Cilt numarası: 126
  • Basım Tarihi: 2016
  • Doi Numarası: 10.1016/j.radphyschem.2016.05.019
  • Dergi Adı: RADIATION PHYSICS AND CHEMISTRY
  • Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Sayfa Sayıları: ss.111-115
  • Karadeniz Teknik Üniversitesi Adresli: Evet

Özet

K-beta/K-alpha, intensity ratios and sigma K-alpha,K-beta production cross-sections of Cu and Sn were measured in pure metals and in different alloys which have different compositions (CuxSn1-x x=0.48, 0.41, 0.14 and 0.06). The samples were excited by 59.5 keV gamma-rays from Am-241 annular radioactive source. K X-rays emitted by samples were counted by an Ultra-LEGe detector with a resolution of 150 eV at 5.9 keV. Comparison of the sigma(K beta) production cross-sections and K beta/K alpha X-ray intensity ratio values for Cu and Sn with the theoretical and semi-empirical calculations indicates that they are in the inverse direction with concentration of constituent element in the alloys. The results show that variations in these parameters can be explained with the charge transfer process between the elements which constitute the alloys. (C) 2016 Elsevier Ltd. All rights reserved.