Author/Authors :
R. Bonetti، نويسنده , , C. Carbonini، نويسنده , , A. Guglielmetti، نويسنده , , M. Hussonnois، نويسنده , , D. Trubert، نويسنده , , C. Le Naour، نويسنده ,
Abstract :
By using glass track detectors in 4π geometry we measured the branching ratio of 230U for emission of Ne clusters to be B=(4.8±2.0)×10−14 and an upper limit for 18O emission from 226Th to be B<3.2×10−14. On the basis of theoretical calculations, the most probable neon cluster comes out to be 22Ne.
