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Density of almost squares of horospherical orbits in non-uniform quotients of SL2(R)×SL2(R)\operatorname{SL}_2(\mathbb{R})\times\operatorname{SL}_2(\mathbb{R})

Konstantin Andritsch

Source record

Source: arXiv

Published: Sep 21, 2026

arXiv: 2609.24752

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Source abstract

Let ΓSL2(R)×SL2(R)Γ\subset\operatorname{SL}_2(\mathbb{R})\times\operatorname{SL}_2(\mathbb{R}) be an irreducible, non-uniform lattice and define the space X=SL2(R)×SL2(R)/ΓX = \operatorname{SL}_2(\mathbb{R})\times\operatorname{SL}_2(\mathbb{R})/Γ. Let UU be the standard horospherical subgroup in SL2(R)×SL2(R)\operatorname{SL}_2(\mathbb{R})\times\operatorname{SL}_2(\mathbb{R}). We show that for every δ>0δ>0 and xXx\in X with dense UU-orbit, the UU-orbit evaluated at almost squares, {(u(n2δ,m2δ) : n,mN}x\{(u_{(n^{2-δ},m^{2-δ})}~:~n,m\in\mathbb{N}\}\cdot x, is dense in XX. The main idea of the proof is to shadow large periodic UU-orbits and reduce the statement to a density statement within the periodic UU-orbit, i.e. a statement for the 22-torus T2\mathbb{T}^2. This then follows from an effective version of Weyl's inequality to deduce the result. The effective shadowing of periodic UU-orbits is achieved using tools from homogeneous dynamics, namely quantitative non-divergence of horospherical subgroups, recurrence under the diagonal flow and effective equidistribution of expanding horospherical subgroups. Our approach follows the strategy of the work \cite{KR25} of \citeauthor{KR25} who established density of almost squares of the horocycle flow for non-uniform lattices in SL2(R)\operatorname{SL}_2(\mathbb{R}).

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