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Seminar on
Mathematical General Relativity
Organizers:
Philippe G. LeFloch (Paris)
Jérémie Szeftel (Paris)
Ghani Zeghib (Lyon)
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ANR Project
“Mathematical General Relativity. Analysis and geometry of spacetimes with low regularity”
February 12, 2014
Laboratoire Jacques-Louis Lions, Université Pierre et Marie Curie, Paris
Lecture room 1525-103
14h Florian Beyer (Dunedin) Graceful exit from inflation for minimally coupled Bianchi A scalar field models
Abstract. We consider the dynamics of Bianchi A scalar field models which undergo inflation. The main question is under which conditions does inflation come to an end and is succeeded by a decelerated epoch. This so-called ‘graceful exit’ from inflation is an important ingredient in the standard model of cosmology, but is, at this stage, only understood for restricted classes of solutions. We present new results obtained by a combination of analytical and numerical techniques.
15h30 Cécile Huneau (ENS, Paris) Vacuum constraint equations for asymptotically flat space-times with a translational Killing field
Abstract. In the presence of a space-like translational Killing field, vacuum Einstein equations in 3+1 dimensions reduces to 2+1 Einstein equations with a scalar field. Minkowski space-time is a trivial solution of vacuum Einstein equation with a translational Killing field. A natural question is therefore the nonlinear stability of Minkowski solution in this setting. A first step in addressing this problem is the study of the constraint equations. The main difficulty in that case is due to the delicate inversion of the Laplacian. In particular, we have to work in the non constant mean curvature setting, which enforces us to consider the intricate coupling of the Einstein constraint equations.
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Conference on
Nonlinear Wave Equations at IHP
Organizers:
Sergiu Klainerman (Princeton)
Philippe G. LeFloch (Paris)
Jérémie Szeftel (Paris)
Fondations des Sciences Mathématiques de Paris
ANR Project
“Mathematical General Relativity. Analysis and geometry of spacetimes with low regularity”
May 21 to May 24, 2013
Institut Henri Poincaré, Paris
Schedule available here
Further informations available here
Poster of the conference here
INVITED SPEAKERS
Lars Andersson (Potsdam)
Stefanos Aretakis (Princeton)
Nicolas Burq (Paris-Sud)
Pieter Blue (Edinburgh)
Mihalis Dafermos (Princeton)
Jean Marc Delort (Paris-Nord)
Gustav Holzegel (London)
Alexandru Ionescu (Princeton)
Joachim Krieger (EPFL)
Jonathan Luk (UPenn)
Franck Merle (Cergy & IHES)
Sung-Jin Oh (Princeton)
Fabrice Planchon (Nice)
Pierre Raphael (Nice)
Igor Rodnianski (MIT)
Chung-Tse Arick Shao (Toronto)
Jacques Smulevici (Paris-Sud)
Jacob Sterbenz (San Diego)
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Seminar on
Mathematical General Relativity
Organizers:
Philippe G. LeFloch (Paris)
Ghani Zeghib (Lyon)
ANR Project
“Mathematical General Relativity. Analysis and geometry of spacetimes with low regularity”
February 20, 2013
Laboratoire Jacques-Louis Lions, Université Pierre et Marie Curie, Paris
Lecture room 1525-103
14h Florian Beyer (Dunedin) Asymptotics and conformal structures of solutions to Einstein’s field equations
Abstract. Roger Penrose’s idea that the essential information about the asymptotics of solutions of the Einstein’s field equations is contained in the conformal structure and the associated conformal boundary has led to astonishing successes. In his original work, he provided several examples which made the importance of his idea evident. However, the question whether general solutions of Einstein’s field equations are compatible with this proposal remained unanswered. Motived by this, Helmut Friedrich has initiated a research programme to tackle this problem based on his so-called conformal field equations. In this talk I report on the status of this work and some of Friedrich’s results, but also on joint work with collaborators at the University of Otago.
15h30 Julien Cortier (IHES, Bures-sur-Yvette) On the mass of asymptotically hyperbolic manifolds
Abstract. By analogy with the ADM mass of asymptotically Euclidean manifolds, a set of global charges can be defined for asymptotically hyperbolic manifolds. We will review their various definitions and , in particular, focus on the notion of “mass aspect” tensor, which gives rise to the energy-momentum vector and arises in the hyperbolic formulation of the positive mass theorem. We will compute these quantities for examples such that the Schwarzschild-anti de Sitter metrics, and we will present a family of counter-examples with “non-positive” mass when completeness is not assumed.
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Seminar on
Mathematical General Relativity
Organizers:
S. Klainerman (Princeton)
P.G. LeFloch (Paris)
A. Zeghib (Lyon)
Fondations des Sciences Mathématiques de Paris
ANR Project
“Mathematical General Relativity. Analysis and geometry of spacetimes with low regularity”
Thursday January 17, 2013
Laboratoire J-L Lions
Université Pierre et Marie Curie, Paris
Lecture room (see below)
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11h (Room 15-25- 104) Sergiu Klainerman (Princeton) On the formation of trapped surfaces
Abstract. I will talk about a new result obtained in collaboration with J. Luk and I. Rodnianski in which we relax significantly Christodoulou’s main condition for the formation of trapped surfaces in vacuum.
14h (Room 15-25-326) Chung-Tse Arick Shao (Toronto) Null cones to infinity, curvature flux, and Bondi mass
Abstract. In general relativity, the Bondi mass in an asymptotically flat spacetime represents, roughly, the mass remaining in the system after some has radiated away. In this talk, we make sense of and control the Bondi mass for a single null cone in an Einstein-vacuum spacetime under minimal assumptions. In terms of regularity, we assume only small weighted curvature flux along the null cone and small data on an initial sphere of the cone. Furthermore, we make no global assumptions on the spacetime, as all our conditions deal only with the single null cone under consideration. This work is joint with S. Alexakis.
15h30 (Room 15-25-326) Gustav Holzegel (Princeton) Existence of dynamical vacuum black holes
Abstract. This is joint work with Mihalis Dafermos and Igor Rodnianski. We prove the existence of a large class of non-stationary vacuum black holes whose exterior geometry asymptotes in time to a fixed Schwarzschild or Kerr metric. The spacetimes are constructed by solving a backwards scattering problem for the vacuum Einstein equations with characteristic data prescribed on the horizon and at null infinity. The data admits the full functional degrees of freedom to specify data for the Einstein equations. An essential feature of the construction is that the solutions converge to stationarity exponentially fast with their decay rate intimately related to the surface gravity of the horizon and hence to the strength of the celebrated redshift effect which, in our backwards construction, is seen as a blueshift.
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Seminar on
Mathematical General Relativity
Organizers:
Philippe G. LeFloch (Paris)
Ghani Zeghib (Lyon)
ANR Project
“Mathematical General Relativity. Analysis and geometry of spacetimes with low regularity”
Friday December 21, 2012
Laboratoire Jacques-Louis Lions, Université Pierre et Marie Curie, Paris
Lecture room 1525-3-21
Speaker
11h15 – José A. Font (Valencia) Simulations of neutron star mergers and black hole-torus systems
Abstract. Merging binary neutron stars are among the strongest sources of gravitational waves and have features compatible with the events producing short–hard gamma-ray bursts. Numerical relativity has reached a stage where a complete description of the inspiral, merger and post-merger phases of the late evolution of binary neutron star systems is possible. This talk presents an overview of numerical relativity simulations of binary neutron star mergers and the evolution of the resulting black hole–torus systems. Such numerical work is based upon a basic theoretical framework which comprises the Einstein’s equations for the gravitational field and the hydrodynamics equations for the evolution of the matter fields. The most well-established formulations for both systems of equations are briefly discussed, along with the numerical methods best suited for their numerical solution, specifically high-order finite-differencing for the case of the gravitational field equations and high-resolution shock-capturing schemes for the case of the relativistic Euler equations. A number of recent results are reviewed, namely the outcome of the merger depending on the initial total mass and equation of state of the binary, as well as the post-merger evolution phase once a black hole–torus system is produced. Such system has been shown to be subject to non-axisymmetric instabilities leading to the emission of large amplitude gravitational waves.

