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Accueil du site > Agenda > Colloques et rencontres > Archives > Agenda 2014 > 94e rencontre entre mathématiciens et physiciens théoriciens : Riemann, Einstein et la geométrie
IRMA, 1820 septembre 2014
La 94ème rencontre entre mathématiciens et physiciens théoriciens aura pour thème : Riemann, Einstein, et la géométrie.
The 94th Encounter between Mathematicians and Theoretical Physicists will take place at Institut de Recherche Mathématique Avancée (University of Strasbourg and CNRS) on September 1820, 2014. The theme will be : "Riemann, Einstein and geometry".
Organizers : Athanase Papadopoulos (Strasbourg) and Sumio Yamada (Tokyo)
The invited speakers include :
JeanPierre Bourguignon (Paris)
Mihalis Dafermos (Princeton)
Erwann Delay (Avignon)
Jacques Franchi (Strasbourg)
Hubert Goenner (Göttingen)
Eric Gourgoulhon (Observatoire de Paris)
Oussama Hijazi (Nancy)
Gerhard Huisken (Tübingen)
Emmanuel Humbert (Tours)
Marc Mars (Salamanca)
Andre Neves (Imperial College, London)
JeanPhilippe Nicolas (Brest)
JeanMarc Schlenker (Luxembourg)
Richard Schoen (UC Irvine)
Tetsuya Shiromizu (Kyoto)
The talks will be in English. Some of the talks will be survey talks intended for a general audience.
Graduate students and young mathematicians are welcome. Registration is required (and free of charge) at this link. Hotel booking can be asked for through the registration link.
List of participants (see here)
For practical and other questions please contact the organizers :
Athanase Papadopoulos : athanase.papadopoulos@math.unistra.fr
Sumio Yamada : yamada@math.gakushuin.ac.jp


09h00 
Richard Schoen  UC IrvineThe impact of General Relativity on Riemannian GeometryAbstract. While it is true that the ideas of Riemann were put to use by Einstein in the formulation of the theory of General Relativity, there have also been important applications of ideas originating in General Relativity to Riemannian Geometry. These include much of our understanding of the behavior of scalar curvature. In this survey talk we will describe this interaction for a general audience. 


10h00 
Pause 


10h30 
Marc Mars  SalamancaMarginally outer trapped surfaces : properties, propagation and equilibrium configurationsAbstract. Marginally outer trapped surfaces (MOTS) are expected to be suitable quasilocal replacements of black holes. In this talk I will discuss a number of results where this expectation is analyzed in detail. I will introduce the notion of stability of MOTS and discuss some of its consequences, in particular, for the propagation of MOTS given a 3+1 decomposition of the spacetime. I will also analyze the interplay between MOTS and event horizons in stationary/static situations. 


11h30 
Emmanuel Humbert  ToursMass of a compact manifoldAbstract. General relativity is a geometric theory: it is therefore not surprising that many problems of general relativity can be solved by geometric tools. But it is much more surprising that a famous problem in geometric analysis/PDEs  the Yamabe problem was solved by Schoen using the positive mass theorem, which comes from the general relativity. Schoen's argument lead to the definition of the mass of a compact manifold. In this talk, we will present this object for a nonspecialist audience and will finish by stating our recent results obtained together with Andreas Hermann. 


14h00 
Eric Gourgoulhon  Observatoire de ParisSome aspects of differential geometry in black hole spacetimesAbstract. Black hole solutions of Einstein equations will be reviewed, putting forward their geometrical properties. Both exact solutions and numerical ones will be discussed, as well as the quasilocal approach, based on trapping horizons. Some focus will be put on the (null and timelike) geodesic curves. Free softwares for investigating these spacetimes will also be presented: Gyoto [1] for computing geodesics and SageManifolds [2] for symbolic tensor calculus. [1] http://gyoto.obspm.fr/ ; [2] http://sagemanifolds.obspm.fr/ 


15h00 
Pause 


15h30 
Hubert Goenner  GoettingenAlbert Einstein and mathematicsAbstract. Albert Einstein's relation to mathematics will be reviewed. The mathematical methods applied by him and the question whether he has made a genuine contribution to mathematics will be discussed. Also included is a look at his philosophical and emotional position with regard to mathematics. This talk is intended for a general audience. 


16h30 
Michalis Dafermos  PrincetonTBA 


19h30 
Conference Dinner Restaurant Le Petit Bois VertEverybody is invitedAddress: 2 quai de la Bruche (quartier petite France); a map will be provided. 


09h00 
Andre Neves  Imperial College (London)Minmax theory in GeometryAbstract. The first use of minmax theory in geometry was found by Birkhoff around 100 years ago. In the last years, the theory has made a comeback and has been used to solve some long standing open questions. I will survey some of its applications. This is joint work with Fernando Marques. 


10h00 
Pause 


10h30 
Erwann Delay  AvignonA study of some curvature operators near the euclidean metricAbstract. We first review the prescribed Ricci curvature type problem on a riemannian manifold. In the second part we will focus on the case of Rn. We will then show that some curvature operators of Ricci (or Einstein) type, are locally invertible near the euclidian metric. In the smooth case, we then deduce that the image of some RiemannChristoffel type operators are smooth submanifolds in the neighbourhood of the euclidean metric. 


11h30 
Oussama Hijazi  NancyOn a LiuYau type Inequality for SurfacesAbstract. We report on a recent joint work with S. Raulot and S. Montiel regarding an application of the use of the Dirac operator and its conformal covariance for surfaces in the Minkowski spacetime. 


14h30 
JeanPierre Bourguignon  BruxellesTBA



15h30 
Pause 


16h00 
JeanMarc Schlenker  LuxembourgAntide Sitter geometry and its connections to Teichmüller theoryAbstract. Antide Sitter (AdS) geometry is the constant curvature (1) Lorentzian geometry, it can be considered as the Lorentzian analog of hyperbolic geometry. AdS was introduced as a solution of Einstein's equations with negative cosmological constant. There are deep connections between Teichmüller theory, the study of the space of complex structures on a surface, and 3dimensional hyperbolic geometry. We will describe other deep connections, discovered more recently, between 3dimensional AdS manifolds and Teichmüller theory. This talk is part of the monthly colloquium talk series at IRMA. 


09h00 
Jacques Franchi  StrasbourgFrom Riemannian to relativistic diffusions 


10h00 
Pause 


10h30 
Tetsuya Shiromizu  KyotoPositive mass as a principle ?Abstract. According to recent observations, our universe is in the phase of accelerating expansion. To explain this, cosmologists are seriously thinking of introduction of dark energy models and/or modifications of gravitational theory. I will discuss the role of positive mass in such theories and see that the form of a certain theory compatible with positive mass is strongly limited. Therefore, as imposed in linearized theory, one may be able to adopt the positive mass as a new additional principle to construct the theory for dark energy/modified gravity. For such theories, stability will be automatically guaranteed in kinematical sense. 


11h30 
JeanPierre Nicolas  BrestThe conformal approach to asymptotic analysisAbstract. This talk, based on joint works with Lionel Mason, will be devoted to Roger Penrose's introduction of conformal geometric methods in general relativity in the mid 1960's and how they changed asymptotic analysis in that framework. We shall focus on two closely related aspects: scattering theory and peeling. The conformal compactification was introduced by Penrose in order to provide a natural reformulation of the notion of peeling that was initially due to Sachs. His work was interpreted as claiming that the asymptotic behaviour of test fields in flat spacetime provides a model for generic asymptotically flat situations, which triggered a long controversy. It also inspired Friedlander to propose a reinterpretation of the LaxPhillips scattering in conformal geometric terms and alternative geometric tools for developing scattering theories. The use of conformal geometry for analyzing the asymptotic behaviour of test fields in general relativity provides flexible techniques that allow the treatment of time dependent situations. Penrose's initial formulation can be recast, using geometrical energy estimates, into an analytically robust framework ensuring optimal results. We shall explain the notion of peeling as described by Penrose, its reformulation using energy estimates and how a complete understanding of the peeling of test fields in the Schwarzschild metric can be obtained. Then we shall explain the principles of conformal scattering as developed by Friedlander and their extension to non stationary spacetimes and black hole geometries. 
Dernière mise à jour le 18092014