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Imperfect Dark Energy from Kinetic Gravity Braiding

We introduce a large class of scalar-tensor models with interactions containing the second derivatives of the scalar field but not leading to additional degrees of freedom. These models exhibit peculiar features, such as an essential mixing of scalar and tensor kinetic terms, which we have named kin...

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Detalles Bibliográficos
Autores principales: Deffayet, Cedric, Pujolas, Oriol, Sawicki, Ignacy, Vikman, Alexander
Lenguaje:eng
Publicado: 2010
Materias:
Acceso en línea:https://dx.doi.org/10.1088/1475-7516/2010/10/026
http://cds.cern.ch/record/1282649