“…We use the Keldysh real time Non‐Equilibrium Green's Functions , but instead of the standard Keldysh triplet we employ the equivalent choice , where is the “less” particle correlation function (Langreth‐Wilkins (LW) convention ). These Green's functions obey their Dyson equations, whose integro‐differential form is (with , and ; opposite spin denoted by ) for the propagators (only the equation for the retarded is shown), while for we have: The propagators are insensitive to the initial conditions and obey the equal time boundary condition …”