A nonlocal gravity model with a function f(□−1R), where □ is
the d'Alembert operator, is considered. The algorithm, allowing to reconstruct
f(□−1R), corresponding to the given Hubble parameter and the state
parameter of the matter, is proposed. Using this algorithm, we find the
functions f(□−1R), corresponding to de Sitter solutions.Comment: 5 pages, v2: refs. added, to appear in the proceedings of the
International Workshop "Supersymmetries and Quantum Symmetries" (SQS'2011),
Dubna, Russia, July 18-23, 2011, http://theor.jinr.ru/sqs/2011