preprint draft Sven Joscha Henheik author 31d731d7-d235-11ea-ad11-b50331c8d7fb0000-0003-1106-327X Bipul Poudyal author Roderich Tumulka author LaEr department Random matrices beyond Wigner-Dyson-Mehta project Particle creation terms in quantum Hamiltonians are usually ultraviolet divergent and thus mathematically ill defined. A rather novel way of solving this problem is based on imposing so-called interior-boundary conditions on the wave function. Previous papers showed that this approach works in the non-relativistic regime, but particle creation is mostly relevant in the relativistic case after all. In flat relativistic space-time (that is, neglecting gravity), the approach was previously found to work only for certain somewhat artificial cases. Here, as a way of taking gravity into account, we consider curved space-time, specifically the super-critical Reissner-Nordstr\"om space-time, which features a naked timelike singularity. We find that the interior-boundary approach works fully in this setting; in particular, we prove rigorously the existence of well-defined, self-adjoint Hamiltonians with particle creation at the singularity, based on interior-boundary conditions. We also non-rigorously analyze the asymptotic behavior of the Bohmian trajectories and construct the corresponding Bohm-Bell process of particle creation, motion, and annihilation. The upshot is that in quantum physics, a naked space-time singularity need not lead to a breakdown of physical laws, but on the contrary allows for boundary conditions governing what comes out of the singularity and thereby removing the ultraviolet divergence. 2025 eng 2409.0067710.48550/arXiv.2409.00677 https://research-explorer.ista.ac.at/record/19540 S.J. Henheik, B. Poudyal, R. Tumulka, ArXiv (n.d.). Henheik SJ, Poudyal B, Tumulka R. How a space-time singularity helps remove the ultraviolet divergence problem. <i>arXiv</i>. doi:<a href="https://doi.org/10.48550/arXiv.2409.00677">10.48550/arXiv.2409.00677</a> Henheik, Sven Joscha, Bipul Poudyal, and Roderich Tumulka. “How a Space-Time Singularity Helps Remove the Ultraviolet Divergence Problem.” <i>ArXiv</i>, n.d. <a href="https://doi.org/10.48550/arXiv.2409.00677">https://doi.org/10.48550/arXiv.2409.00677</a>. Henheik SJ, Poudyal B, Tumulka R. How a space-time singularity helps remove the ultraviolet divergence problem. arXiv, <a href="https://doi.org/10.48550/arXiv.2409.00677">10.48550/arXiv.2409.00677</a>. Henheik, Sven Joscha, et al. “How a Space-Time Singularity Helps Remove the Ultraviolet Divergence Problem.” <i>ArXiv</i>, doi:<a href="https://doi.org/10.48550/arXiv.2409.00677">10.48550/arXiv.2409.00677</a>. Henheik, S. J., Poudyal, B., &#38; Tumulka, R. (n.d.). How a space-time singularity helps remove the ultraviolet divergence problem. <i>arXiv</i>. <a href="https://doi.org/10.48550/arXiv.2409.00677">https://doi.org/10.48550/arXiv.2409.00677</a> S. J. Henheik, B. Poudyal, and R. Tumulka, “How a space-time singularity helps remove the ultraviolet divergence problem,” <i>arXiv</i>. . 195522025-04-11T12:07:25Z2026-04-07T12:37:11Z