Recently it has been speculated that a set of diffeomorphisms exist which act non-trivially on the horizon of some black holes such as kerr and Kerr-Newman black hole. cite{Haco:2018ske,Haco:2019ggi}. Using this symmetry in covariant phase space formalism one can obtains conserved charges as surface integrals on the horizon. Kerr-Bolt spacetime is well-known for its asymptotically topology and has been studied widely in recent years. In this work we are going to study Kerr-Bolt black hole and provide a holographically describtion of it in term of warped confromal field theory.
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