Investigation of alloying effects on XRF parameters of 3d transition metals in Permendur49, Kovar and Ti50Co50 alloys


Alim B., Ugurlu M., Han I., DEMİR L.

JOURNAL OF RADIATION RESEARCH AND APPLIED SCIENCES, cilt.11, sa.2, ss.144-149, 2018 (SCI-Expanded) identifier

  • Yayın Türü: Makale / Tam Makale
  • Cilt numarası: 11 Sayı: 2
  • Basım Tarihi: 2018
  • Doi Numarası: 10.1016/j.jrras.2017.12.003
  • Dergi Adı: JOURNAL OF RADIATION RESEARCH AND APPLIED SCIENCES
  • Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED)
  • Sayfa Sayıları: ss.144-149
  • Anahtar Kelimeler: Permendur49, Kovar, Ti50Co50, X-ray fluorescence parameters, Fluorescence yields, Fluorescence cross-section, Vacancy transfer probabilities, VACANCY TRANSFER PROBABILITIES, SUBSHELL FLUORESCENCE YIELDS, PRODUCTION CROSS-SECTIONS, ALPHA INTENSITY RATIOS, K-SHELL, RAY-FLUORESCENCE, CHARGE-TRANSFER, ELEMENTS, NI, DELOCALIZATION
  • Atatürk Üniversitesi Adresli: Evet

Özet

The alloying effects on X-ray fluorescence (XRF) parameters such as K shell fluorescence cross-sections (sigma(K alpha), sigma(K beta) and sigma(K)), K shell average fluorescence yields (omega(K)) and K to L shell vacancy transfer probabilities (eta(KL)) of V, Ti, Fe, Co and Ni 3d transition metals in Permendur49 (Fe49Co49V2), Kovar (Fe54Ni29Co17) and Ti50Co50 alloys have been carried out by X-ray fluorescence studies. K X-ray intensity ratios of these 3d transition metals in both pure form and present alloys have been measured following excitation by 22.69 keV X-rays from a 10 mCi Cd-109 radioactive point source. The characteristic K-X-ray spectra from samples were detected by a high-resolution Si(Li) solid-state detector. The investigated fluorescence parameters of present 3d transition elements in alloys indicate significant differences with respect to the pure metals. Consequently, the observed change of the investigated fluorescence parameters can be attributed to the delocalization and charge transfer phenomena between the 3d elements in alloys. (c) 2017 The Egyptian Society of Radiation Sciences and Applications. Production and hosting by Elsevier B.V.