# Counting orbits of certain infinitely generated non-sharp discontinuous   groups for the anti-de Sitter space

**Authors:** Kazuki Kannaka

arXiv: 1907.09303 · 2023-12-04

## TL;DR

This paper constructs new examples of infinitely generated discontinuous groups acting on 3D anti-de Sitter space, analyzes their orbit counting functions, and demonstrates the existence of groups with arbitrarily large orbit counts and non-sharp properties.

## Contribution

It introduces a family of non-sharp discontinuous groups for AdS3, provides bounds on orbit counting functions, and shows existence of groups with infinitely many Laplacian eigenvalues and arbitrarily large orbit counts.

## Key findings

- Constructed a family of non-sharp discontinuous groups for AdS3.
- Derived bounds for orbit counting functions as radius grows.
- Proved existence of groups with infinitely many Laplacian eigenvalues.

## Abstract

Inspired by an example of Gueritaud-Kassel [Geom. Topol. 2017], we construct a family of infinitely generated discontinuous groups $\Gamma$ for the 3-dimensional anti-de Sitter space $\mathrm{AdS}^{3}$. These groups are not necessarily sharp (a kind of "strong" properly discontinuous condition introduced by Kassel and Kobayashi [Adv. Math. 2016]), and we give its criterion. Moreover, we find upper and lower bounds of the counting $N_{\Gamma}(R)$ of a $\Gamma$-orbit contained in a pseudo-ball $B(R)$ as the radius $R$ tends to infinity. We then find a non-sharp discontinuous group $\Gamma$ for which there exist infinitely many $L^2$-eigenvalues of the Laplacian on the noncompact anti-de Sitter manifold $\Gamma\backslash\mathrm{AdS}^{3}$, by applying the method established by Kassel-Kobayashi. We also prove that for any increasing function $f$, there exists a discontinuous group $\Gamma$ for $\mathrm{AdS}^{3}$ such that the counting $N_{\Gamma}(R)$ of a $\Gamma$-orbit is larger than $f(R)$ for sufficiently large $R$.

## Full text

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## Figures

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## References

12 references — full list in the complete paper: https://tomesphere.com/paper/1907.09303/full.md

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Source: https://tomesphere.com/paper/1907.09303