Cargando…
UV-extending Ghost Inflation
We present a setup that provides a partial UV-completion of the ghost inflation model up to a scale which can be almost as high as the Planck mass. This is achieved by coupling the inflaton to the Lorentz-violating sector described by the Einstein-aether theory or its khronometric version. Compared...
Autores principales: | Ivanov, Mikhail M., Sibiryakov, Sergey |
---|---|
Lenguaje: | eng |
Publicado: |
2014
|
Materias: | |
Acceso en línea: | https://dx.doi.org/10.1088/1475-7516/2014/05/045 http://cds.cern.ch/record/1662802 |
Ejemplares similares
-
Testing Lorentz invariance of dark matter
por: Blas, Diego, et al.
Publicado: (2012) -
Time-Sliced Perturbation Theory for Large Scale Structure I: General Formalism
por: Blas, Diego, et al.
Publicado: (2015) -
Time-Sliced Perturbation Theory II: Baryon Acoustic Oscillations and Infrared Resummation
por: Blas, Diego, et al.
Publicado: (2016) -
Eternal inflation
por: Winitzki, Sergei
Publicado: (2009) -
Reheating after inflation
por: Lozanov, Kaloian
Publicado: (2020)