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arXiv · 2606.24215

Nonlinear Stability of Kerr-Sen Black Holes in Merging Binaries

Andrew Carroll·Eric W. Hirschmann·Hyun Lim·David Neilsen·David F. Van Komen·Sebastian Vander Ploeg Fallon
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Abstract

We investigate the stability of Kerr-Sen black holes, which arise in Einstein-Maxwell-dilaton-axion theory. Within a numerical relativity framework, we perform head-on binary black hole simulations with approximate initial data across a portion of the parameter space. We find that for nontrivial electric charge, a dilaton field persists through merger and that in the presence of spin, the remnant will also retain an axion field. The persistence of these fields for long times after merger strongly suggests the stability of these black holes within this alternative gravity theory. We further test whether initially unscalarized black holes will acquire hair in the presence of a scalar background. We find that black holes immersed in such a background retain scalar hair. Furthermore, we find that even initially unscalarized Kerr-Newman black holes will scalarize and remain scalarized throughout the evolution.

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Andrew Carroll, Eric W. Hirschmann, Hyun Lim, David Neilsen, David F. Van Komen, Sebastian Vander Ploeg Fallon. 2026-06-23. Nonlinear Stability of Kerr-Sen Black Holes in Merging Binaries. https://arxiv.org/abs/2606.24215

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