Abstract
The dispersion of the collective excitation in the n=4 shells of xenon has been calculated, including all significant partial-wave contributions, by a time-dependent, self-consistent-field method. The calculation reveals details of the physical mechanism that produces the dispersion. The calculated dispersion coefficient is compared with experimental results.
| Original language | English |
|---|---|
| Pages (from-to) | 1981-1984 |
| Number of pages | 4 |
| Journal | Physical Review A |
| Volume | 32 |
| Issue number | 4 |
| DOIs | |
| State | Published - 1985 |