Non-local cosmological models
arXiv:1806.09616 · doi:10.1088/1361-6382/ab4eb6
Abstract
Nonlocal cosmological models are studied extensively in recent times because of their interesting cosmological consequences. In this paper, we have analyzed background cosmology on a class of non-local models which are motivated by the perturbative nature of gravity at infrared scale. We show that inflationary solutions are possible in all constructed non-local models. However, exit from inflation to RD era is not possible in most of the models.
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- de Sitter Swampland Conjecture in String Field Inflation
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- Spherically symmetric static solutions, newtonian potential and degrees of freedom of a Nonlocal action
- Modified Gravity Corrections in Fundamental Orbital Frequencies in Kerr Spacetime