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While jet quenching in ultrarelativistic heavy-ion collisions is firmlyestablished as a phenomenon resulting from the interplay between hardperturbative and soft fluid-dynamical Quantum Chromodynamics (or equivalentlythe interaction between hard probes and bulk QCD matter), less is known withcertainty about the reaction of bulk matter to the passage of a jet. On generalgrounds, a jet interacting while passing through a medium represents a sourceof energy and momentum for the bulk matter fluid. If the precise form of such asource term is known, the reaction of the medium can be computed using fluiddynamics. Recent advances in the understanding of hard probes due to the wealthof data from RHIC and LHC allow to constrain the source term better bydetermining the energy flow away from hard modes. The aim of this work is todiscuss what can be learned from such constraints in the context of thein-medium shower evolution code YaJEM-DE and to illustrate the role offluctuations in the energy deposition.

The space-time structure of the energy deposition into the bulk medium due to jet quenching