Abstract
We compute finite temperature corrections to the scalar potential in maximally symmetric SU(N, 1) supergravity. In the large N limit, the zero temperature potential is only scaled by the thermal corrections. As an example, we apply the general result to a class of phenomenologically interesting no-scale supergravity models.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 181-184 |
| Number of pages | 4 |
| Journal | Physics Letters B |
| Volume | 152 |
| Issue number | 3-4 |
| DOIs | |
| State | Published - Mar 7 1985 |
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