Lee–Rogers–Seeger local space-time conjecture

Let n1n\geq1, let ff be a function on Rn\mathbb{R}^n, and let Bα,pp(Rn)B_{\alpha,p}^p(\mathbb{R}^n) be the non-homogeneous Besov space with norm

fBα,pp=(k02kαpPkfpp)1/p.\|f\|_{B_{\alpha,p}^p}=\left(\sum_{k\geq0}2^{k\alpha p}\|P_kf\|_{p}^p\right)^{1/p}.

For 2p<2\leq p<\infty and 2r2\leq r\leq\infty satisfying

np+1r<n2,2n+1p+1r<n,\frac{n}{p}+\frac{1}{r}<\frac{n}{2},\qquad \frac{2n+1}{p}+\frac{1}{r}<n,

Lee–Rogers–Seeger local space-time conjecture. The estimate

eitΔfLxpLtr(Rn×[0,1])fBα,pp(Rn),α=n(12p)2r,\|e^{it\Delta}f\|_{L_x^pL_t^r(\mathbb{R}^n\times[0,1])}\lesssim\|f\|_{B_{\alpha,p}^p(\mathbb{R}^n)},\qquad \alpha=n\left(1-\frac{2}{p}\right)-\frac{2}{r},

holds. The conjecture was proved for n=1n=1, while the higher-dimensional case remains open; partial results follow from square-function and Fourier-restriction estimates.

Sources & referencesView supporting material

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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