Constrained Analysis of Topologically Massive Gravity
arXiv:hep-th/9408045 · doi:10.1007/BF01553998
Abstract
We quantize the Einstein gravity in the formalism of weak gravitational fields by using the constrained Hamiltonian method. Special emphasis is given to the 2+1 spacetime dimensional case where a (topological) Chern-Simons term is added to the Lagrangian.
15 pages, IF-UFRJ-21/94