Density of almost squares of horospherical orbits in non-uniform quotients of SL2(R)×SL2(R)
Konstantin Andritsch
Abstract
Let Γ⊂SL2(R)×SL2(R) be an irreducible, non-uniform lattice and define the space X = SL2(R)×SL2(R)/Γ. Let U be the standard horospherical subgroup in SL2(R)×SL2(R). We show that for every δ>0 and x∈ X with dense U-orbit, the U-orbit evaluated at almost squares, \(u(n2-δ,m2-δ)~:~n,m∈N\· x, is dense in X. The main idea of the proof is to shadow large periodic U-orbits and reduce the statement to a density statement within the periodic U-orbit, i.e. a statement for the 2-torus T2. This then follows from an effective version of Weyl's inequality to deduce the result. The effective shadowing of periodic U-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 KR25 of KR25 who established density of almost squares of the horocycle flow for non-uniform lattices in SL2(R).
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