Abstract
Angular and energy distributions are reported for 4He in correlation with 1,2,3H and 4He in the reaction 337 MeV 40Ar+natAg. Comparisons are made to a statistical model that includes emitter. Energy spectra important barrier reductions compared to those for cold nuclei, ≈25%, 12%, 8% and 0 for 1H, 4He, 2H and 3H respectively. Emitter deformation alone cannot give an explanation. A transitory nuclear stratosphere is suggested with proton emission favored from its fringes of lowest density.
| Original language | English |
|---|---|
| Pages (from-to) | 253-256 |
| Number of pages | 4 |
| Journal | Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics |
| Volume | 191 |
| Issue number | 3 |
| DOIs | |
| State | Published - Jun 11 1987 |
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