On Modified Gravity

We consider some aspects of nonlocal modified gravity, where nonlocality is of the type $R \mathcal{F}(\Box) R$. In particular, using ansatz of the form $\Box R = c R^\gamma,$ we find a few $R(t)$ solutions for the spatially flat FLRW metric. There are singular and nonsingular bounce solutions. For late cosmic time, scalar curvature R(t) is in low regime and scale factor a(t) is decelerated. R (t) = 0 satisfies all equations when k = -1.Comment: added references; made some clarifications; 8 page

Aspects of WZW models at critical level

We consider non-compact WZW models at critical level (equal to the dual Coxeter number) as tensionless limits of gravitational backgrounds in string theory. Special emphasis is placed on the Euclidean black hole coset SL(2,R)_k/U(1) when k=2. In this limit gravity decouples in the form of a Liouville field with infinite background charge and the world-sheet symmetry of the model becomes a truncated version of W_\infty without Virasoro generator. This is regarded as manifestation of Langlands duality for the SL(2,R)_k current algebra that relates small with large values of the level in the two extreme limits. However, the physical interpretation of the SL(2,R)_k/U(1) coset model below the self-dual value k=3 remains elusive including the non-conformal theory at k=2.Comment: 11 pages, contribution to the proceedings of 37th International Symposium Ahrenshoop (Berlin, 2004