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gr-qc2026
How much chaos can be generated by gravitational collapse before reaching the Planck scale?
David Brizuela, Sara F. Uria, Edward Wilson-Ewing
According to the Belinski-Khalatnikov-Lifshitz (BKL) conjecture the dynamics of general relativity near singularities is highly chaotic. However, since general relativity breaks do…
gr-qc2026
Tunnelling across a trapped region and out of a black hole
Edward Wilson-Ewing
The quantum field theory for a massless scalar field on a two-dimensional non-singular black hole spacetime with an outer and an inner horizon predicts that there is a non-vanishin…