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PreprintCC BY 4.0arXiv

Symmetry and Rigidity Results for the Mean Field Equation and Hawking Mass on 𝕊2

Abstract

In this paper, we establish symmetry results for solutions of the mean field equation α/2 Δu + eu − 1 = 0 on $ \mathbb{S}^2 $ for 1/3≤ α≤ 1, under a geometric condition (ℋ) introduced below. The proofs utilize the Sphere Covering Inequality and incorporate topological arguments on $ \mathbb{S}^2 $. These results are further applied to demonstrate a rigidity property of the Hawking mass for stable constant mean curvature (CMC) spheres, addressing a question posed by Robert Bartnik in 2002. Our results unify and extend previous rigidity results obtained under symmetry or hemispherical balance assumptions, and apply beyond the nearly spherical setting.

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BibTeX
@misc{gui2026symmetry,
  title = {{Symmetry and Rigidity Results for the Mean Field Equation and Hawking Mass on $\mathbbS^2$}},
  author = {Changfeng Gui and Amir Moradifam},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2605.15448},
  eprint = {2605.15448},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2605.15448},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Symmetry and Rigidity Results for the Mean Field Equation and Hawking Mass on 𝕊^2
AU  - Changfeng Gui
AU  - Amir Moradifam
PY  - 2026
DA  - 2026/09/07
PB  - arXiv
DO  - 10.48550/arxiv.2605.15448
UR  - https://arxiv.org/abs/2605.15448
AB  - In this paper, we establish symmetry results for solutions of the mean field equation α/2 Δu + e^u − 1 = 0 on $ \mathbb{S}^2 $ for 1/3≤ α≤ 1, under a geometric condition (ℋ) introduced below. The proofs utilize the Sphere Covering Inequality and incorporate topological arguments on $ \mathbb{S}^2 $. These results are further applied to demonstrate a rigidity property of the Hawking mass for stable constant mean curvature (CMC) spheres, addressing a question posed by Robert Bartnik in 2002. Our results unify and extend previous rigidity results obtained under symmetry or hemispherical balance assumptions, and apply beyond the nearly spherical setting.
ER  -