Cosmology of modified gravity with a non-local f(R) [CL]

http://arxiv.org/abs/1509.04254


We consider a modification of GR with a special type of a non-local f(R). The structure of the non-local operators is motivated by the string field theory and p-adic string theory. We pay special account to the stability of the de Sitter solution in our model and formulate the conditions on the model parameters to have a stable configuration. Relevance of unstable configurations for the description of the de Sitter phase during inflation is discussed. Special physically interesting values of parameters are studied in details.

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I. Dimitrijevic, B. Dragovich, J. Grujic, et. al.
Tue, 15 Sep 15
68/83

Comments: 18 pages