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Bilinear space–time estimate for Schrödinger evolutions (Conjecture B.1)

Establish the bilinear space–time inequality for separated frequency supports: for f1,f2 supported in subsets of B(Ne,1) with dist(supp f1, supp f2) ≥ 2, show that ∥(e^{itΔ}f1)(e^{itΔ}f2)∥_{L_x^p L_t^r(R^{n+1})} ≤ C_{p,r} N^{κ(p,r)} ∥f1∥_{L^2(R^n)} ∥f2∥_{L^2(R^n)} if and only if (n+2)/p + 1/r ≤ (n+1)/2 and 2 ≤ p,r < ∞, where κ(p,r) is the exponent of N appearing in (B.1).

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Background

The authors propose a bilinear space–time conjecture that would imply the global space–time Conjecture 1.2 and is closely linked to Fourier restriction problems. They also provide a necessary condition supporting the proposed sharp range of (p,r). Establishing this bilinear inequality in the full if-and-only-if range would resolve Conjecture 1.2 via their reduction.

References

Conjecture B.1 (Bilinear space-time estimate). Suppose that f , f are supported on 1 subsets of B (Ne ,1)1with dist(suppf ,supp1 ) ≥ b2 2. it∆ it∆ 1 1− 1 2 (B.1) |e f1e f2|2. LxLt (Rn+1) ≤ C p,rN p r f 1 L 2 f2 L2,

holds if and only if n+2 + 1 ≤ n+1 ,2 ≤ p,r < ∞. p r

The space-time estimates for the Schrödinger equation (2402.13539 - Li et al., 21 Feb 2024) in Conjecture B.1, Appendix B