Density of almost squares of horospherical orbits in non-uniform quotients of
Konstantin Andritsch
Source abstract
Let be an irreducible, non-uniform lattice and define the space . Let be the standard horospherical subgroup in . We show that for every and with dense -orbit, the -orbit evaluated at almost squares, , is dense in . The main idea of the proof is to shadow large periodic -orbits and reduce the statement to a density statement within the periodic -orbit, i.e. a statement for the -torus . This then follows from an effective version of Weyl's inequality to deduce the result. The effective shadowing of periodic -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 .
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