Abstract
We show that "spiralized" models of new-inflation can be experimentally identified mostly by their positive spectral running in direct contrast with most chaotic-inflation models which have negative runnings typically in the range of (10-4-10-3).
| Original language | English |
|---|---|
| Article number | 061 |
| Journal | Journal of Cosmology and Astroparticle Physics |
| Volume | 2016 |
| Issue number | 2 |
| DOIs | |
| State | Published - 2016.02.23 |
Keywords
- cosmology of theories beyond the SM
- inflation
- physics of the early universe
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