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Optimal constant in the Heisenberg inequality with Riemannian distance in Schwarzschild geometry

Establish the precise optimal constant C(n) in the Heisenberg-type inequality (1/2) ∫_ℰ |ψ|^2 dv_g ≤ (∫_ℰ d^2 |ψ|^2 dv_g)^{1/2} (∫_ℰ |∇_g ψ|^2 dv_g)^{1/2} on the Riemannian manifold (ℰ, g), where ℰ = {x ∈ ℝ^n : |x| > 1} is the exterior of the Schwarzschild black hole, g is the reduced Schwarzschild metric g = (r^{n−2}/(r^{n−2}−1)) dr ⊗ dr + r^2 g_{S^{n−1}}, d is the Riemannian distance to the event horizon given by d(r) = ∫_1^r √(ξ^{n−2}/(ξ^{n−2}−1)) dξ, and ψ ranges over locally absolutely continuous functions satisfying ψ^2(x) |x|^n → 0 as |x| → ∞; in particular, ascertain whether the constant 1/2 is optimal.

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Background

The authors prove a sharp Heisenberg-type inequality on the Schwarzschild exterior using an induced distance s(r), with optimal constant 1/2 and an explicit family of minimizers. Since s(r) ≤ d(r), they derive a corollary Heisenberg inequality with the Riemannian distance d(r) that also has constant 1/2.

Because s(r) ~ d(r)/n for large r, they note that the inequality with d(r) may admit a larger optimal constant. Their current method cannot establish or refute the optimality of 1/2 for the d-based inequality, leaving the exact constant unresolved.

References

Since s=d/n+o(d) as d\rightarrow\infty, it may well be the case that the constant 1/2 is not optimal here. This cannot be proven or disproven with the method we have developed so far, and is again left as an open problem.

Hardy inequalities and uncertainty principles in the presence of a black hole (2403.06562 - Paschalis, 11 Mar 2024) in Remark following the Heisenberg corollary (Comparison with the Riemannian distance), Section “Heisenberg inequality”