Abstract
Estimates of the mean free path of relativistic He6 in nuclear emulsion strongly suggest that it is much shorter than the He3 or He4 mean free path. A discussion is given of the important implications of this difference for the interpretation of recent data on secondary helium fragments produced in interactions of relativistic primary beams.
Original language | English (US) |
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Pages (from-to) | 679-681 |
Number of pages | 3 |
Journal | Physical Review C |
Volume | 31 |
Issue number | 2 |
DOIs | |
State | Published - 1985 |