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Strongly stable CMC-one hypersurfaces in every hyperbolic space of dimension at least four
Abstract
For every integer d≥4, we prove strong stability for a subfamily of classical rotational hypersurfaces in ℍd with normalized mean curvature one. The examples are complete, two-sided, properly embedded, and nowhere umbilic, with topology ℝ×𝕊d−2. An explicit positive supersolution yields a quantitative stability inequality for all compactly supported test functions. Consequently, endpoint horospherical rigidity fails in every ambient dimension at least four.
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BibTeX
@misc{wang2026strongly,
title = {{Strongly stable CMC-one hypersurfaces in every hyperbolic space of dimension at least four}},
author = {Zihao Wang},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.22059},
eprint = {2609.22059},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.22059},
}
RIS
TY - UNPB
TI - Strongly stable CMC-one hypersurfaces in every hyperbolic space of dimension at least four
AU - Zihao Wang
PY - 2026
DA - 2026/09/18
PB - arXiv
DO - 10.48550/arxiv.2609.22059
UR - https://arxiv.org/abs/2609.22059
AB - For every integer d≥4, we prove strong stability for a subfamily of classical rotational hypersurfaces in ℍ^d with normalized mean curvature one. The examples are complete, two-sided, properly embedded, and nowhere umbilic, with topology ℝ×𝕊^d−2. An explicit positive supersolution yields a quantitative stability inequality for all compactly supported test functions. Consequently, endpoint horospherical rigidity fails in every ambient dimension at least four.
ER -