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A construction of charged naked singularities for the Einstein--Maxwell-charged scalar field equations in 3+1 dimensions

Abstract

We construct a class of global naked singularity solutions for the (3+1)-dimensional spherically symmetric Einstein--Maxwell-charged scalar field equations. The solutions arise from C1,α asymptotically flat one-ended characteristic initial data with 0<α≪1 and develop a curvature singularity that is not enclosed by an event horizon. The resulting spacetimes are genuinely charged, with a nonzero Maxwell field that satisfies a quantitative positive lower bound up to the singularity and admits an explicit asymptotic profile. As part of the construction, we develop a general framework for constructing naked singularity exteriors, namely, the causal future region of the past light cone emanating from the singularity. The framework accommodates a broad range of singular characteristic data and, in particular, allows for singular behavior of the Maxwell field near the singularity.

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BibTeX
@misc{zheng2026construction,
  title = {{A construction of charged naked singularities for the Einstein--Maxwell-charged scalar field equations in 3+1 dimensions}},
  author = {Weihao Zheng},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2609.33168},
  eprint = {2609.33168},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2609.33168},
}
RIS
TY  - UNPB
TI  - A construction of charged naked singularities for the Einstein--Maxwell-charged scalar field equations in 3+1 dimensions
AU  - Weihao Zheng
PY  - 2026
DA  - 2026/09/27
PB  - arXiv
DO  - 10.48550/arxiv.2609.33168
UR  - https://arxiv.org/abs/2609.33168
AB  - We construct a class of global naked singularity solutions for the (3+1)-dimensional spherically symmetric Einstein--Maxwell-charged scalar field equations. The solutions arise from C^1,α asymptotically flat one-ended characteristic initial data with 0<α≪1 and develop a curvature singularity that is not enclosed by an event horizon. The resulting spacetimes are genuinely charged, with a nonzero Maxwell field that satisfies a quantitative positive lower bound up to the singularity and admits an explicit asymptotic profile. As part of the construction, we develop a general framework for constructing naked singularity exteriors, namely, the causal future region of the past light cone emanating from the singularity. The framework accommodates a broad range of singular characteristic data and, in particular, allows for singular behavior of the Maxwell field near the singularity.
ER  -