Effective Chern-Simons actions of particles coupled to 3D gravity

Point particles in 3D gravity are known to behave as topological defects, while gravitational field can be expressed as the Chern–Simons theory of the appropriate local isometry group of spacetime. In the case of the Poincaré group, integrating out the gravitational degrees of freedom it is possible to obtain the effective action for particle dynamics. We review the known results, both for single and multiple particles, and attempt to extend this approach to the (anti-)de Sitter group, using the factorizations of isometry groups into the double product of the Lorentz group and group. On the other hand, for the de Sitter group one can also perform a contraction to the semidirect product of and the translation group. The corresponding effective action curiously describes a Carrollian particle with the momentum space. We derive this contraction in a more rigorous manner and further explore its properties, including a generalization to the multiparticle case