Logo CIMPA

Geometry and Dynamics

External organizer

External organizer
Vincent PECASTAING
Affiliation external organizer
Laboratoire J.A. Dieudonné, UMR CNRS 7351 Université Côte d’Azur
Country external organizer
France
Email external organizer
vincent.pecastaing@univ-cotedazur.fr

Local Organizer

Local organizer
Rezki CHEMLAL
Affiliation local organizer
National Higher School of Mathematics
Country local organizer
Algeria
Email local organizer
rezki.chemlal@nhsm.edu.dz

The general theme of this school lies at the intersection of geometry and dynamics, focusing on the interactions between Riemannian and Lorentzian geometries on the one hand, and dynamical systems on the other. For instance, a Lorentzian, Riemannian, or more generally semi-Riemannian metric naturally gives rise to dynamical objects such as:
• the action of its isometry and conformal groups,
• the geodesic flow (a differential equation on the tangent bundle), and
• the Ricci flow (an evolution PDE on the space of all metrics).
In recent years, the field has witnessed several important advances.  We mention only three representative examples:
1. Conformal groups of compact Lorentz manifolds. Lichnerowicz’s conjecture asserts that if the conformal group of a compact Lorentz manifold is essential (i.e. strictly larger than the isometry group, even after conformal rescaling), then the metric must be conformally flat. K. Melnick and V. Pecastaing proved this conjecture in the analytic, simply connected case (J. AMS, 2022).
2. Completeness of compact Lorentz manifolds. The geodesic vector field defines a differential equation on the tangent bundle. Compactness, combined with suitable geometric hypotheses, may imply geodesic completeness—that is, solutions of the ODE exist for all time. This was recently established by L. Mehidi and A. Zeghib (J. Diff. Geom., to appear) for Brinkmann spacetimes, a class of polarized Lorentzian structures that generalize, among others, the physically significant gravitational wave spacetimes.
3. Chaos in cosmology. F. BĂ©guin and T. Dutilleul provided a (partial) proof of chaotic dynamics in Bianchi cosmology (Comm. Math. Phys., 2023, 190 pages). Bianchi dynamics is a kind of geometric flow, similar to Ricci flow, in a homogeneous setting. 
The aim of the proposed courses is to equip participants with the foundational knowledge needed to understand these and related results. We believe the program offers both unity and diversity, through the following contributions:
• Suhr’s course: Introduction to Lorentz geometry.
• Mehidi’s and Sanchez’s course: Study of certain Lorentzian spaces (e.g. Plane waves) with a focus on completeness.
• Monclair’s course: Investigation of special globally hyperbolic Lorentzian manifolds modelled on anti-de Sitter space, and the hyperbolic dynamics of their fundamental groups on boundary spaces.
• Béguin’s course: Analysis of globally hyperbolic spacetimes admitting a free isometric spacelike action of a 3-dimensional group. In this case, the Einstein equations reduce to a polynomial ODE on a 5-dimensional space; the course emphasizes its qualitative analysis and the proof of chaotic behavior.
• War’s course: Rigidity properties of the geodesic flow on Riemannian surfaces. Here Lorentzian geometry is implicit, since Anosov geodesic flows preserve a Lorentz metric (albeit with limited regularity).
• Melnick’s course: Cartan connections as powerful tools for the study of conformal groups and, in particular, for addressing Lichnerowicz’s conjecture.
• Pecastaing’s course: Introduction to tools that will be particularly useful in connection with Melnick’s and Monclair’s lectures.
The courses are designed to be accessible to both Master’s and Doctoral students, and can be adapted, if necessary, to match the average level of the participants. While we emphasize some recent advances related to the theme of this school, the core topics — such as conformal transformations, completeness problems, and the Einstein equation — are fundamental to geometry and dynamical systems. 

Our instructors, who are not only experts but also contributors to these recent developments, will present these themes through the broader (and long) history of the field.

Tentative scientific activities (the definitive programme is/will be on the webpage of the event)

Speaker : Stefan SUHR (Ruhr-University Bochum,Germany)

This mini-course will give an introduction to Lorentzian geometry with a view towards new developments. After discussing basic notions, such as geodesics, curvature, conjugate points, I will review the Einstein equations and the classical singularity theorems. Towards the end of the course, new developments towards low regularity spacetimes will be discussed.

This mini-course aims to be an introduction to homogeneous spaces, their differential geometry and their curved versions called Cartan geometries. We will start with basic properties of Lie groups and briefly discuss Maurer-Cartan’s equation. We will see Cartan’s criterion of semi-simplicity and the natural pseudo-Riemannian structure attached to semi-simple Lie groups. We will then discuss homogeneous spaces, with a special emphasis on locally symmetric Riemannian manifolds. Many examples of homogeneous spaces carry natural geometric structures. We will finally discuss Cartan geometries, which are curved version of these geometric structures, in the same sense that a Riemannian manifold is a curved version of Euclidean space.

Speaker : Lilia MEHIDI (CNRS & Université de Bretagne Sud,France),Miguel SANCHEZ (UNIVERSIDAD DE GRANADA,Spain)

Plane waves are special Lorentzian manifolds which can be considered as perturbations of the flat Minkowski space. Together with their different variants, they play a central role in General Relativity. The aim of the lectures is the study of the geometry of these spaces by computing their isometry groups, conformal transformations, curvatures, and their geodesics. If time allows, we will also introduce the subject of compact Lorentzian manifolds modeled on homogeneous plane waves. As deformations of special affine structures, classical questions in affine geometry related to the Auslander conjecture and Bieberbach rigidity can be naturally addressed within this framework

Speaker : Khadim WAR (IMPA,Senegal)

The aim of this lecture series is to study some properties of the geodesic on surface without conjugate points of genius at least two. In the first lecture we give an introduction of the geodesic flow and discuss the geometric properties of the surface that are needed to study ergodic properties; this includes the action of the fundamental group on the universal cover, the Gromov boundary and Morse Lemma. In the second lecture we will introduce the Poincare series and define the measure of maximal entropy via Patterson-Sullivan construction. In the third lecture, we will show that the measure of maximal entropy is unique and we will use the cross ratio function to prove the geodesic flow is mixing with respect to the constructed measure. In the last lecture, we will count the number of closed geodesic known as prime geodesic theorem and we will also count the number of geodesic loops known as sector Theorem.

Speaker : Karin MELNICK (University of Luxembourg,Luxembourg)

This mini-course aims to be an introduction to homogeneous spaces, their differential geometry and their curved versions called Cartan geometries. We will start with basic properties of Lie groups and briefly discuss Maurer-Cartan’s equation. We will see Cartan’s criterion of semi-simplicity and the natural pseudo-Riemannian structure attached to semi-simple Lie groups. We will then discuss homogeneous spaces, with a special emphasis on locally symmetric Riemannian manifolds. Many examples of homogeneous spaces carry natural geometric structures. We will finally discuss Cartan geometries, which are curved version of these geometric structures, in the same sense that a Riemannian manifold is a curved version of Euclidean space.

Speaker : Daniel MONCLAIR (Paris Saclay,France)

Anti-de Sitter geometry consists in the study of Lorentzian manifolds of constant negative sectional curvature. In a foundational preprint, Mess related three dimensional anti-de Sitter geometry and Teichmüller Theory. The work of Barbot extended this relation between anti-de Sitter and hyperbolic geometries in a broader context, including higher dimensions. After laying the foundations of the theory, focusing on geometric similarities between anti-de Sitter and hyperbolic manifolds, we will discuss dynamical similarities through the study of the spacelike geodesic flow. The main themes will be its uniform hyperbolicity (a result of Delarue-M.-Sanders that can be seen as an interpretation of earlier work of Barbot-Mérigot), its relation to Patterson-Sullivan theory and a Lorentzian version of Hausdorff dimension (Glorieux-M.) as well as spectral theory (Delarue-Guillarmou-M.).

Speaker : François BÉGUIN (Université Sorbonne Paris-Nord,France)

The aim of this mini-course will be to explain how certain classes of spacetimes can be studied using techniques from classical finite-dimensional dynamical systems theory. The spacetimes concerned are those that admit a large symmetry group. We will begin by reviewing the classical case of spatially homogeneous and isotropic spacetimes, whose study reduces to that of a differential equation in one dimension. We will then address the case of spatially homogeneous spacetimes, which is far from being completely elucidated and raises interesting questions. We will emphasize the role played in this context by classical concepts and results in dynamics: Lyapunov functions, the stable manifold theorem, uniformly and non-uniformly hyperbolic sets, Pesin theory, ergodic theorems, small divisors, continued fractions, etc...

Info address
National Higher School of Mathematics | Abdelhafid Boussouf technological et scientific hub
Pays
Algeria
Dates
-
Deadline
Language of the school
English

How to participate

For registration and application to a CIMPA financial support, read carefully the instructions given here. If you already know what to do, you can also directly go to the application website, create an account (if necessary) and apply to the school of your choice. Be aware that you will be redirected to an external website.