Inner-horizon blueshift coordinate ($V_{-}\propto -e^{-{\kappa }_{-}v}$)

Near a nondegenerate outgoing inner Cauchy horizon, a regular null coordinate behaves as $V_{-}\propto -e^{-{\kappa }_{-}v}$, where ${\kappa }_{-}>0$ is the magnitude of the inner-horizon surface gravity. Transforming stress components gives $T_{V_{-}{V}_{-}}\propto e^{2{\kappa }_{-}v}{T}_{vv}$. Even a small power-law tail can therefore cause an unbounded locally measured flux, motivating mass inflation.