English

Discrete parabolic groups in ${\rm PSL}(3, \Bbb{C})$

Dynamical Systems 2022-07-18 v5

Abstract

We study and classify the purely parabolic discrete subgroups of PSL(3,C)PSL(3,\Bbb{C}). This includes all discrete subgroups of the Heisenberg group Heis(3,C){\rm Heis}(3,\Bbb{C}). While for PSL(2,C)PSL(2,\Bbb{C}) every purely parabolic subgroup is Abelian and acts on PC1\Bbb{P}^1_\Bbb{C} with limit set a single point, the case of PSL(3,C)PSL(3,\Bbb{C}) is far more subtle and intriguing. We show that there are five families of purely parabolic discrete groups in PSL(3,C)PSL(3,\Bbb{C}), and some of these actually split into subfamilies. We classify all these by means of their limit set and the control group. We use first the Lie-Kolchin Theorem and Borel's fixed point theorem to show that all purely parabolic discrete groups in PSL(3,C)PSL(3,\Bbb{C}) are virtually triangularizable. Then we prove that purely parabolic groups in PSL(3,C)PSL(3,\Bbb{C}) are virtually solvable and polycyclic, hence finitely presented. We then prove a slight generalization of the Lie-Kolchin Theorem for these groups: they are either virtually unipotent or else Abelian of rank 2 and of a very special type. All the virtually unipotent ones turn out to be conjugate to subgroups of the Heisenberg group Heis(3,C){\rm Heis}(3,\Bbb{C}). We classify these using the obstructor dimension introduced by Bestvina, Kapovich and Kleiner. We find that their Kulkarni limit set is either a projective line, a cone of lines with base a circle or else the whole PC2\Bbb{P}^2_\Bbb{C}. We determine the relation with the Conze-Guivarc'h limit set of the action on the dual projective space PˇC2\check{\Bbb{P}}^2_\Bbb{C} and we show that in all cases the Kulkarni region of discontinuity is the largest open set where the group acts properly discontinuously.

Cite

@article{arxiv.1802.08360,
  title  = {Discrete parabolic groups in ${\rm PSL}(3, \Bbb{C})$},
  author = {Waldemar Barrera and Angel Cano and Juan Pablo Navarrete and Jose Seade},
  journal= {arXiv preprint arXiv:1802.08360},
  year   = {2022}
}

Comments

Mayor changes in the new version

R2 v1 2026-06-23T00:30:56.432Z