Planchon's space-time conjecture for the Schrödinger equation

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Let n≥1n\geq 1, let f∈S(Rn)f\in\mathcal{S}(\mathbb{R}^n), and let eitΔfe^{it\Delta}f denote the solution of the free Schrödinger equation. For 2≤r,p<∞2\leq r,p<\infty satisfying

n+1p+1r≤n2,\frac{n+1}{p}+\frac{1}{r}\leq\frac{n}{2},

Planchon's space-time conjecture. One has

∥eitΔf∥LxpLtr(Rn+1)≤C∥f∥H˙s(Rn),s=n2−np−2r.\|e^{it\Delta}f\|_{L_x^pL_t^r(\mathbb{R}^{n+1})}\leq C\|f\|_{\dot{H}^{s}(\mathbb{R}^n)},\qquad s=\frac{n}{2}-\frac{n}{p}-\frac{2}{r}.

This is the space-time counterpart of the classical Strichartz estimate, with the order of the mixed norms reversed. The paper establishes the sharp global estimate when n=2n=2 and improves known critical-case results for n≥3n\geq3, but the conjecture is not stated as resolved in general.

References

Primary source

Junfeng Li, Changxing Miao and Ankang Yu, “The space-time estimates for the Schrödinger equation”, arXiv:2402.13539 (2024).

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