New bounds for GL(3)×GL(2) shifted convolution sums
Abstract
Shifted convolution sums of GL(3)×GL(2) type have been extensively studied in several important settings, while a number of natural cases remain open. In this paper, we first revisit the shifted convolution sums involving λπ(1,n) and the divisor function d(n), improving the recent power saving of 1/42 obtained by Blomer and Li to 1/22. We also treat the corresponding sums involving λπ(1,n) and r(n,𝒬), settling a previously open case and obtaining a power saving of 1/22. Here λπ(1,n) denotes the normalized Fourier coefficients of a Hecke--Maass cusp form π on SL(3,ℤ), and r(n,𝒬) denotes the number of representations of a positive integer n by a positive definite integral binary quadratic form 𝒬. The proof combines two circle methods with a different organization of the major-arc analysis. A key point is that the nonzero Poisson frequencies are kept together in a single coefficient vector, rather than estimated separately, which allows them to be controlled by a finite matrix norm. The zero Poisson frequency is treated separately: its contribution is independent of the reduced residue class, and its arithmetic mean cancels the constant term in the complementary Jutila weight before absolute values are taken. We make this cancellation explicit, including the relevant normalization and local factors. The same mechanism extends to the binary quadratic-form setting, while the remaining Jutila contribution is handled by the available correlation estimates.
Related
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- Selberg sieve weights and sign changes of Kloosterman sums. I. Uniform asymptotics for shifted weights
- Sharp Matrix-Weighted Lower Bounds for Non-Degenerate Convolution Calderón--Zygmund Operators
- Sharp lower bounds for shifted moments of Dedekind zeta functions
- Stability and Error Estimates for Convolution Quadrature under Radial Symbol Bounds
BibTeX
@misc{hu2026bounds,
title = {{New bounds for $\mathrmGL(3)\times\mathrmGL(2)$ shifted convolution sums}},
author = {Guangwei Hu and Guangshi Lü},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2610.20182},
eprint = {2610.20182},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2610.20182},
}
RIS
TY - UNPB
TI - New bounds for GL(3)×GL(2) shifted convolution sums
AU - Guangwei Hu
AU - Guangshi Lü
PY - 2026
DA - 2026/10/14
PB - arXiv
DO - 10.48550/arxiv.2610.20182
UR - https://arxiv.org/abs/2610.20182
AB - Shifted convolution sums of GL(3)×GL(2) type have been extensively studied in several important settings, while a number of natural cases remain open. In this paper, we first revisit the shifted convolution sums involving λ_π(1,n) and the divisor function d(n), improving the recent power saving of 1/42 obtained by Blomer and Li to 1/22. We also treat the corresponding sums involving λ_π(1,n) and r(n,𝒬), settling a previously open case and obtaining a power saving of 1/22. Here λ_π(1,n) denotes the normalized Fourier coefficients of a Hecke--Maass cusp form π on SL(3,ℤ), and r(n,𝒬) denotes the number of representations of a positive integer n by a positive definite integral binary quadratic form 𝒬. The proof combines two circle methods with a different organization of the major-arc analysis. A key point is that the nonzero Poisson frequencies are kept together in a single coefficient vector, rather than estimated separately, which allows them to be controlled by a finite matrix norm. The zero Poisson frequency is treated separately: its contribution is independent of the reduced residue class, and its arithmetic mean cancels the constant term in the complementary Jutila weight before absolute values are taken. We make this cancellation explicit, including the relevant normalization and local factors. The same mechanism extends to the binary quadratic-form setting, while the remaining Jutila contribution is handled by the available correlation estimates.
ER -