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Small field models with gravitational wave signature supported by CMB data.
We study scale dependence of the cosmic microwave background (CMB) power spectrum in a class of small, single-field models of inflation which lead to a high value of the tensor to scalar ratio. The inflaton potentials that we consider are degree 5 polynomials, for which we precisely calculate the po...
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| Main Authors: | , |
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| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Public Library of Science (PLoS)
2018-01-01
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| Colecção: | PLoS ONE |
| Acesso em linha: | http://europepmc.org/articles/PMC5993128?pdf=render |
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