“…At high energies, where p + p ⊥ > p − , the probe is highly localized around x − = 0 and one can simplify the field's spacetime dependence to be A µ (x) ≈ A µ (x + , x). Additionally, the structure describing local parton-medium interactions, Ψ(p − q)γ µ A a µ (q)T a Ψ(p), with q the exchanged momentum with the medium, only receives contributions from the µ = + component [66,[68][69][70], up to power suppressed terms in the jet 1 Though in this work we are interested in the evolution of jets in the quark-gluon plasma, the same formulation also applies to jet evolution in cold nuclear matter. 2 We write the Hamiltonian in the operator form, and its full expression, in terms of field operators, can be found in Ref.…”