Min–Oo conjecture for metrics on the hemisphere

At least 18 years old · documented by

Let gg) be a smooth Riemannian metric on the closed hemisphere S+3\mathbb{S}^3_+ satisfying the following conditions: its scalar curvature obeys Rg≥6{\mathrm R}_g\geq 6; its induced boundary metric is the standard metric, g∣∂S+3=gS2g|_{\partial \mathbb{S}^3_+}=g_{\mathbb{S}^2}; and ∂S+3\partial \mathbb{S}^3_+ is totally geodesic with respect to gg. Min–Oo conjecture. Then (S+3,g)(\mathbb{S}^3_+,g) is isometric to the standard round hemisphere (S+3,gS3)(\mathbb{S}^3_+,g_{\mathbb{S}^3}). The conjecture aimed to characterize the de Sitter solution as the unique zero-mass initial data under a positive cosmological constant. It is refuted in full generality by counterexamples, although positive rigidity results remain available under strengthened hypotheses.

References

Primary source

Virginia Agostiniani, Stefano Borghini and Lorenzo Mazzieri, “Mass-type invariants in the presence of a cosmological constant”, arXiv:2603.01543 (2026).

Additional references

11 papers in this index state this conjecture (2007–2026). The statement above is taken from the most recent of them; the others are arXiv:2410.23406, arXiv:1805.10221, arXiv:1505.04311, arXiv:1103.4805, arXiv:1008.3097, arXiv:1005.2782, arXiv:1004.3088, arXiv:0911.0380, arXiv:0907.5549, arXiv:0711.4595.

Progress summary

Never refreshed

Nothing recorded yet. Refresh searches the literature and the public web for attempts on this problem, and writes the first summary here.

Solutions 0

No solutions have been posted yet.