Dynamical model for black hole to white hole transitions
arXiv:2505.15096 · doi:10.1103/8m7g-zz3k
Abstract
We present an asymptotically flat spherically symmetric non-singular metric that describes gravitational collapse and matter bounce with transient black hole and white hole regions. The metric provides a dynamical counterpart to proposed static non-singular black holes, and a phenomenological model for possible black hole to white hole transitions in quantum gravity.
10 pages, 4 figures
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