PACS 78.70.BjThe results of the new measurements of the linear absorption coefficient for positrons emitted from 22 Na and 68
Ge\68 Ga sources are presented. As a result, improvements were made to the well-known Gleason et al. (G. I. Gleason et al., Nucleonics 8, 12 (1951) [1]) formula giving the value of the mass absorption coefficient. It was shown that this coefficient depended not only on the maximum energy of emitted positrons but also on the atomic number the implanted absorber and exhibited an oscillatory dependence on atomic number for heavy absorbers.
Introduction Positrons emitted in a β+ decay have energies from almost zero up to a definite maximum. Except for very high energy (greater than several MeV) the main slowing-down interaction is with the electrons of the matter through which the particle passes. In matter, due to its small mass, the positron makes fewer collisions in a given distance, travels a large distance, is deflected easily and so does not travel in straight lines. The combination of the tortuous trajectory and continuous distribution of energy indicates that the positrons do not show a definite range but are absorbed approximately exponentially as a function of the penetration depth. It is common knowledge that the penetration depth profile is characterized by only one physical parameter -the linear absorption coefficient -α + . Such conclusions were established over fifty years ago supported by a transmission experiment, where positrons passed thought thin foils of different thickness. From this experiment Gleason et al. [1] proposed that the linear absorption coefficient depends only on the maximum energy of implanted positrons and density of the matter as follows: