Let Tn be the rational torus, let Pλ,δ denote its spectral projection operator for spectral parameter λ and window width δ, and let ∥Pλ,δ∥2→p be its operator norm. Define
pc=n−12(n+1),p∗=n−22n,
and
e(p)=n−1n+1(p1−2(n−1)n−3p1−pc1),
with
μ1(p)=2n−1(21−p1),μ2(p)=2n−1−pn.
The Germain–Myerson conjecture. If δ>λ−1+κ for some fixed κ∈(0,1], then there is a constant C=C(n,p,κ,L∗) such that
∥Pλ,δ∥2→p≤⎩⎨⎧C(n,p,κ,L∗)(λδ)2n−1(21−p1)=C(λδ)μ1(p),C(n,p,κ,L∗)(λδ)2n−1(21−p1)=C(λδ)μ1(p),C(n,p,κ,L∗)λ2n−1−pnδ1/2=Cλμ2(p)δ1/2,p≤pc,pc≤p≤p∗ and δ≤λe(p),p∗≤p and δ≥λe(p).
These bounds refine the universal spectral projection estimates for shrinking spectral windows on the torus, down to widths just above the smallest reasonable scale for rational tori. The conjecture was originally stated by Germain and Myerson and was partially proved in the cited work; the full range of estimates remains unresolved.
References
Primary source
Daniel Pezzi, “Sharp Spectral Projection Estimates for the Torus at p_c=2(n+1)n-1”, arXiv:2405.02746 (2024).