Covid19: Because of the current health crisis, we have decided to postpone the programme to an ulterior date.
New dates of the programme: January 31  March 11, 2022
Online conference: February 22  February 26, 2021.
Here, for more information.
Purpose of the thematic program:
The main aim of the program is to drive progress by connecting researchers working on different matter models and by advertising open problems that can serve as an entry point for researchers from other areas. In particular, we want to bring together people who work on {different types of }relativistic matter with {each other and with }those who work on nonrelativistic matter. We believe large benefits are to be gained from increased interactions that would hopefully lead to exchanges of ideas and techniques that could be used to spur progress on outstanding problems in both areas.
Key dates of the program:
Spring School: dates to be announced.
Workshop: dates to be announced.
See below for the program of the spring school and a preliminary list of speakers in the workshop.
Please note that attendance is limited at all times to 50 participants. Hence, the attendance to the spring school and the workshop are limited to 50 persons.
The program is supported by the Faculty of Physics of the University of Vienna and Chalmers University of Technology.
Preliminary list of speakers for the workshop
 L. Andersson (AEI)
 M. Dafermos (Cambridge)
 M. Hadžić (University College London) t.b.c.
 P. Hintz (MIT)
 M. Kunze (Unviersity of Cologne)
 J. Jang (University of Southern California)
 P. LeFloch (Sorbonne Université)
 H. Lindblad (John Hopkins University)
 J. Luk (Stanford)
 G. Rein (Universiy of Bayreuth)
 H. Ringström (KTH) t.b.c.
 J. Smulevici (Sorbonne Université)
 J. Speck (Vanderbuilt)
 R. Strain (University of Pennsylvania) t.b.c.
 J. Szeftel (Sorbonne Université)
 M. Taylor (Imperial College London)
 A. Vasy (Stanford University)
 Q. Wang (Oxford)
 S. Wu (University of Michigan)
Lectures of the spring school
 Robert Beig (Vienna), Elasticity as a relativistic matter model
 Markus Kunze (Cologne), A BirmanSchwinger principle in galactic dynamics
 Gerhard Rein (Bayreuth), Selfgravitating matter distributions and the Vlasov equation
 Jared Speck (Vanderbilt), Recent advances in the mathematical theory of relativistic and nonrelativistic compressible Euler flow
Course summaries
 Elasticity as a relativistic matter model
Robert Beig (Uni. Vienna)
The geometrical field theory of elasticity is a branch of continuum mechanics which describes the dynamics of solid materials. Perfect fluids can be viewed as a limiting case of elastic materials. A specific perfect fluid is defined in the simplest case by a function of one variable, the equation of state, whereas an elastic material needs a function of at least two variables. Despite this complication it is conceivable that already in the absence of gravity elasticity is better behaved under time evolution than perfect fluids since elastic materials might not generically develop shocks as fluids are believed to do. We describe the Einstein elastic system and what little is known about it.  A BirmanSchwinger principle in galactic dynamics
Markus Kunze (Cologne)
In this series of lectures I am going to review various aspects of the Antonov stability estimate, a basic tool for proving nonlinear stability in galactic dynamics. In particular, for the VlasovPoisson system we are going to characterize the cases where the best constant in this estimate is attained, and we are going to discuss what this could mean for the overall dynamics.  Selfgravitating matter distributions and the Vlasov equation
Gerhard Rein (Bayreuth)
In astrophysics systems like globular clusters or galaxies are often modeled as a selfgravitating collisionless gas, i.e., as an ensemble of particles (stars), described by a density function on phase space, which interact only by the gravitational field which the particles create collectively. In the Newtonian setup this results in the VlasovPoisson system, in the general relativistic setup this results in the EinsteinVlasov system.
These systems have some remarkable properties. Both systems have a plethora of steady state solutions. For the VlasovPoisson system there exists a welldeveloped existence theory for the corresponding initial value problem, in particular, sufficiently regular data launch singularityfree, global solutions. Hence any break down of solutions of the EinsteinVlasov system must be due to a genuinely relativistic effect and not just due to the matter model. Finally, given a plethora of steady states and some understanding of the time dependent case one can ask about the dynamical stability or instability of these steady states.
In my lectures I will discuss some (and probably not all) of these issues.  Recent advances in the mathematical theory of relativistic and nonrelativistic compressible Euler flow
Jared Speck (Vanderbilt)
The last 15 years have witnessed dramatic advances in the rigorous mathematical theory of solutions to the relativistic Euler equations and their nonrelativistic analog, the compressible Euler equations. Examples of progress include i) Christodoulou’s groundbreaking 2007 monograph on shock formation for relativistic Euler solutions in irrotational and isentropic regions; ii) my work with J. Luk that extends Christodoulou’s result to the compressible Euler equations for an open set of initial data with vorticity; iii) Christodoulou’s recent resolution of the restricted shock development problem (which is essentially a local wellposedness result for irrotational and isentropic weak solutions with a shock singularity); and iv) some recent results on the existence of solutions with rough sound waves. The proofs of these results fundamentally rely on geometric formulations of the equations that exhibit remarkable structural features. The presence of these structures allows one to import insights and techniques from Lorentzian geometry, mathematical general relativity, and the theory of geometric wave equations into the study of compressible fluid mechanics, in total providing the scaffolding for the analysis in the proofs. In this course, I will survey these results and the ideas behind their proofs, and provide some indications about the trajectory of the field.

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