| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10722747 | Physics Letters B | 2012 | 5 Pages |
Abstract
We suggest a class of generally covariant ghost-free nonlocal gravity models generating de Sitter or anti-de Sitter background with an arbitrary value of the effective cosmological constant and featuring a mechanism of dark matter simulation. These models interpolate between the general relativistic phase on a flat spacetime background and their strongly coupled infrared (anti-)de Sitter phase with two propagating massless graviton modes.
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Authors
A.O. Barvinsky,