Cargando…
A No-Scale Inflationary Model to Fit Them All
The magnitude of B-mode polarization in the cosmic microwave background as measured by BICEP2 favours models of chaotic inflation with a quadratic $m^2 \phi^2/2$ potential, whereas data from the Planck satellite favour a small value of the tensor-to-scalar perturbation ratio $r$ that is highly consi...
| Autores principales: | , , , |
|---|---|
| Publicado: |
2014
|
| Materias: | |
| Acceso en línea: | https://dx.doi.org/10.1088/1475-7516/2014/08/044 http://cds.cern.ch/record/1697726 |