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5101419 · Jun 202619922001200920172026
48 results for Margulis spacetimes

We show that Margulis spacetimes without parabolic holonomy are topologically tame. A Margulis spacetime is the quotient of the 33-dimensional Minkowski space by a free proper isometric action of the free group of rank 2\geq 2. We will use our particular point of view that the Margulis spacetime is a manifold-with-bo…

2012-04-24abs ↗pdf ↗

Researchers extend parametrization of Margulis spacetimes using strip deformations.

problem Parametrize Margulis spacetimes with decorated horoballs.
method Use strip deformations to parametrize complete finite-area hyperbolic surfaces with spikes decorated with horoballs.
result Generalized parametrization of Margulis spacetimes with photons.

The study shows that certain spacetimes are isospectrally rigid.

problem Isospectrality of Margulis-Smilga spacetimes for specific Lie groups.
method Analysis of polynomials and rational expressions related to Margulis invariants of semisimple Lie groups.
result Zariski dense finitely generated subgroups of spacetimes are isospectrally rigid.

A Margulis spacetime is a complete affine 3-manifold M with nonsolvable fundamental group. Associated to every Margulis spacetime is a noncompact complete hyperbolic surface S. We show that every Margulis spacetime is orientable, even though S may be nonorientable. We classify Margulis spacetimes when S is homeomorphic…

2011-07-14abs ↗pdf ↗

Let M be a Margulis spacetime whose associated complete hyperbolic surface S has compact convex core. Generalizing the correspondence between closed geodesics on M and closed geodesics on S, we establish an orbit equivalence between recurrent spacelike geodesics on M and recurrent geodesics on S. In contrast, no timeli…

2011-02-02abs ↗pdf ↗

A Margulis spacetime is a complete flat Lorentzian 3-manifold M with free fundamental group. Associated to M is a noncompact complete hyperbolic surface S homotopy-equivalent to M. The purpose of this paper is to classify Margulis spacetimes when S is homeomorphic to a one-holed torus. We show that every such M decompo…

2015-01-19abs ↗pdf ↗

We study strip deformations of convex cocompact hyperbolic surfaces, defined by inserting hyperbolic strips along a collection of disjoint geodesic arcs properly embedded in the surface. We prove that any deformation of the surface that uniformly lengthens all closed geodesics can be realized as a strip deformation, in…

2014-07-21abs ↗pdf ↗

This paper defines the pressure metric on the Moduli space of Margulis spacetimes without cusps and shows that it is positive definite on the constant entropy sections. It also demonstrates an identity regarding the variation of the cross-ratios.

2015-05-04abs ↗pdf ↗

In this article, we provide a necessary and sufficient criterion for proper actions on Hn,n1\mathbb{H}^{n,n-1} in terms of certain special Anosov representations in SO(n,n)\mathsf{SO}(n,n). Moreover, we show that affine Anosov representations of any word hyperbolic group in SO(n,n1)R2n1\mathsf{SO}(n,n-1)\ltimes\mathbb{R}^{2n-1} are infi…

2018-12-10abs ↗pdf ↗

We will discuss fundamental domains for actions of discrete groups on the 3-dimensional Einstein Universe. These will be bounded by crooked surfaces, which are conformal compactifications of surfaces that arise in the construction of Margulis spacetimes. We will show that there exist pairwise disjoint crooked surfaces …

2013-07-24abs ↗pdf ↗

A Margulis spacetime is a complete flat affine Lorentzian 3-manifold with free fundamental group. Associated to MM is a noncompact complete hyperbolic surface ΣΣ. We study double extensions of π1(M)π1(Σ)π_1 (M) \cong π_1 (Σ) when ΣΣ is homeomorphic to a projective plane minus two discs. We classify proper actions of this do…

2015-11-17abs ↗pdf ↗

Crooked planes were defined by Drumm to bound fundamental polyhedra in Minkowski space for Margulis spacetimes. They were extended by Frances to closed polyhedral surfaces in the conformal compactification of Minkowski space (Einstein space) which we call crooked surfaces. The conformal model of anti-de Sitter space is…

2013-02-20abs ↗pdf ↗

In this paper we describe the stable and unstable leaves for the geodesic flow on the space of non-wandering spacelike geodesics of a Margulis Space Time and prove contraction properties of the leaves under the flow. We also show that monodromy of Margulis Space Times are "Anosov representations in non semi-simple Lie …

2014-12-28abs ↗pdf ↗

For every closed hyperbolic Haken 3-manifold and, more generally, for any hyperbolic 3-manifold M which is homeomorphic to the interior of a Haken manifold, the number 0.286 is a Margulis number. If M has non-zero first Betti number, or if M is closed and contains a semi-fiber, then 0.292 is a Margulis number for M.

2010-06-17abs ↗pdf ↗

Given an affine isometry of R3\R^3 with hyperbolic linear part, its Margulis invariant measures signed Lorentzian displacement along an invariant spacelike line. In order for a group generated by hyperbolic isometries to act properly on R3\R^3, the sign of the Margulis invariant must be constant over the group. We show…

2003-11-04abs ↗pdf ↗

Given a discrete subgroup of the isometries of n-dimensional hyperbolic space there is always a region kept precisely invariant under the stabilizer of a parabolic fixed point, called the Margulis region. While in dimensions 2 and 3 this region is a horoball, it has in general a more complicated shape due to the existe…

2012-09-25abs ↗pdf ↗

Let E\mathbf{E} be a flat Lorentzian space of signature (2,1)(2, 1). A Margulis space-time is a noncompact complete flat Lorentzian 33-manifold E/Γ\mathbf{E}/Γ with a free holonomy group ΓΓ of rank g,g2\mathbf{g}, \mathbf{g} \geq 2. We consider the case when ΓΓ contains a parabolic element. We obtain a characterization o…

2017-10-25abs ↗pdf ↗

This paper applies the authors' forthcoming work, "Affine deformations of a three-holed sphere" in Lorentzian geometry to prove a result in hyperbolic geometry. Namely, an infinitesimal deformation of a hyperbolic structure of a three-holed sphere which infinitesimally lengthens the three boundary components infinitesi…

2009-07-03abs ↗pdf ↗

Under certain assumptions on CAT(0) spaces, we show that the geodesic flow is topologically mixing. In particular, the Bowen-Margulis' measure finiteness assumption used in recent work of Ricks is removed. We also construct examples of CAT(0) spaces which do not admit finite Bowen-Margulis measure.

2015-09-18abs ↗pdf ↗

The study calculates volume and entropy asymptotics in nonpositive curvature manifolds.

problem Volume and entropy asymptotics in nonpositive curvature manifolds.
method Volume and entropy calculations using Riemannian volume and geodesic flow.
result Margulis function is continuous and constant if and only if the manifold has constant negative curvature.

Arithmetic spaces simplified to simplicial complexes.

problem Understanding the complexity of arithmetic locally symmetric spaces.
method Homotopy equivalence to a simplicial complex with linearly bounded simplices, using a strengthened Margulis collar lemma.
result Arithmetic locally symmetric spaces are homotopy equivalent to simplicial complexes with linearly bounded simplices.

We study the geometry of the Margulis region associated with an irrational screw translation gg acting on the 4-dimensional real hyperbolic space. This is an invariant domain with the parabolic fixed point of gg on its boundary which plays the role of an invariant horoball for a translation in dimensions 3\leq 3. Th…

2013-04-19abs ↗pdf ↗

Margulis space-times with parabolic holonomy elements are stable under sufficiently small deformations.

problem Stability of Margulis space-times with parabolic holonomy elements
method Combining compactification and partial generalization of earlier work
result Openness result on the number of conjugacy classes of parabolic elements under deformation

We prove a Kazhdan-Margulis-Zassenhaus lemma for Hilbert geometries. More precisely, in every dimension nn there exists a constant εn>0\varepsilon_n > 0 such that, for any properly open convex set ØØ and any point xØx \in Ø, any discrete group generated by a finite number of automorphisms of ØØ, which displace xx at …

2011-06-16abs ↗pdf ↗

If λλ is a positive real number strictly less than log3\log3, there is a positive number VλV_λ such that every orientable hyperbolic 3-manifold of volume greater than VλV_λ admits λλ as a Margulis number. If λ<(log3)/2λ<(\log3)/2, such a VλV_λ can be specified explicitly, and is bounded above by $$λ\bigg(6+\frac{880}{\log3-2λ}…

2010-10-13abs ↗pdf ↗

Quantifies how geodesic planes isolate in hyperbolic 3-manifolds.

problem Understanding isolation properties of geodesic planes in hyperbolic 3-manifolds.
method Quantitative estimates of geodesic planes in frame bundles, using tight areas and densities.
result Polynomial estimates of isolation properties with degree given by modified critical exponents.

We prove a Margulis' Lemma à la Besson Courtois Gallot, for manifolds whose fundamental group is a nontrivial free product A*B, without 2-torsion. Moreover, if A*B is torsion-free we give a lower bound for the homotopy systole in terms of upper bounds on the diameter and the volume entropy. We also provide examples and…

2012-04-07abs ↗pdf ↗

Small deformations of a specific type of Lorentzian space-time preserve its structure.

problem Deformations of Margulis space-times with parabolics.
method Use of previous work on compactification and Carrière's decomposition of the space-time.
result Sufficiently small deformations of the group Γ still act properly on the space-time.

Geodesics in curved spaces spread evenly over time.

problem Equidistribution of geodesics in negatively curved spaces.
method Proving equidistribution of geodesic flow orbits towards measures of maximal entropy and Bowen-Margulis measure.
result Equidistribution of divergent geodesics in negative curvature as their complexity increases.

This paper proves explicit bilipschitz bounds on the change in metric between the thick part of a cusped hyperbolic 3-manifold N and the thick part of any of its long Dehn fillings. Given a bilipschitz constant J > 1 and a thickness constant epsilon > 0, we quantify how long a Dehn filling suffices to guarantee a J-bil…

2019-07-31abs ↗pdf ↗