New- vs. chaotic- inflations
Journal Article
·
· Journal of Cosmology and Astroparticle Physics
- Departament de Física Teòrica and IFIC, Universitat de València-CSIC, E-46100, Burjassot (Spain)
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 O(10{sup −4}–10{sup −3})
- OSTI ID:
- 22524983
- Journal Information:
- Journal of Cosmology and Astroparticle Physics, Vol. 2016, Issue 02; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 1475-7516
- Country of Publication:
- United States
- Language:
- English
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