A new identity expresses the null energy condition of the author's kappa-models as a time derivative of the metric function, yielding monotonicity rules for the black hole mass.
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Null energy condition of dynamical black holes in spatially flat FLRW space-times
A new identity expresses the null energy condition of the author's kappa-models as a time derivative of the metric function, yielding monotonicity rules for the black hole mass.