Abstract
The constraints on grand unified models required to obtain an inflationary universe scenario are outlined, especially a new assesment of the reheating that follows inflation. The implications forvarious supersymmetric models are discussed.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 45-48 |
| Number of pages | 4 |
| Journal | Physics Letters B |
| Volume | 131 |
| Issue number | 1-3 |
| DOIs | |
| State | Published - Nov 10 1983 |
| Externally published | Yes |
All Science Journal Classification (ASJC) codes
- Nuclear and High Energy Physics
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