Interior evolution of regular Schwarzschild black holes

Abstract

We present an exact, purely geometric account of the interior dynamics of Schwarzschild black holes, formulated without invoking any specific gravitational theory and free of additional charges beyond the total mass $\mathcal{M}$. We show that dynamical evolution generically produces new singularities, absent in the static case, whose resolution imposes highly restrictive conditions on gravitational collapse.

5 pages, 4 figures; added references

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