Jet Quenching in Relativistic Heavy-Ion Collisions

In this work jets were simulated on top of either event-by-event 0+1 or 2+1 relativistic hydrodynamic backgrounds using JEWEL+vUSPhydro with two different initial conditions: TRENTo and MC-KLN. The effects of hydrodynamics and initial state on the shape and substructure observables (such as mass, $p_T^D$ and girth) and on jet $v_n$ are presented. No distinguishable impact on shape and substructure observables was seen whereas the comparison between jet $v_n$ calculations and experimental data is significantly improved by the insertion of a realistic hydrodynamic background.