Abstract
We present new cosmological constraints on single-field inflation in light of the Wilkinson Microwave Anisotropy Probe satellite mission five-year results (WMAP5). We find that the cosmic microwave background data are quite consistent with a Harrison-Zel'dovich primordial spectrum with no running and zero tensor amplitude.
| Original language | English |
|---|---|
| Pages (from-to) | 86-90 |
| Number of pages | 5 |
| Journal | Nuclear Physics B - Proceedings Supplements |
| Volume | 194 |
| Issue number | C |
| DOIs | |
| State | Published - Oct 2009 |
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