The Stability of the Minkowski space for the Einstein-Vlasov system
arXiv:1707.06141 · doi:10.2140/apde.2021.14.425
Abstract
We prove the global stability of the Minkowski space viewed as the trivial solution of the Einstein-Vlasov system. To estimate the Vlasov field, we use the vector field and modified vector field techniques developed in [FJS15; FJS17]. In particular, the initial support in the velocity variable does not need to be compact. To control the effect of the large velocities, we identify and exploit several structural properties of the Vlasov equation to prove that the worst non-linear terms in the Vlasov equation either enjoy a form of the null condition or can be controlled using the wave coordinate gauge. The basic propagation estimates for the Vlasov field are then obtained using only weak interior decay for the metric components. Since some of the error terms are not time-integrable, several hierarchies in the commuted equations are exploited to close the top order estimates. For the Einstein equations, we use wave coordinates and the main new difficulty arises from the commutation of the energy-momentum tensor, which needs to be rewritten using the modified vector fields.
139 pages
References in corpus (5)
- Hidden symmetries and decay for the Vlasov equation on the Kerr spacetime
- A non-variational approach to nonlinear stability in stellar dynamics applied to the King model
- On the asymptotic behavior of solutions to Einstein's vacuum equations in wave coordinates
- A commuting-vector-field approach to some dispersive estimates
- Sharp asymptotics for the solutions of the three-dimensional massless Vlasov-Maxwell system with small data
Cited by in corpus (13)
- The non-isentropic Einstein-Euler system written in a symmetric hyperbolic form
- On the Hoop conjecture and the weak cosmic censorship conjecture for the axisymmetric Einstein-Vlasov system
- Stable cosmologies with collisionless charged matter
- Stability of vacuum for the Landau equation with hard potentials
- Global nonlinear stability of large dispersive solutions to the Einstein equations
- Nonlinear stability of self-gravitating massive fields. A wave-Klein-Gordon model
- Decay estimates for the massless Vlasov equation on Schwarzschild spacetimes
- Spherical accretion of a collisionless kinetic gas into a generic static black hole
- Static solutions to the spherically symmetric Einstein-Vlasov system: a particle-number-Casimir approach
- A Birman-Schwinger Principle in General Relativity: Linearly Stable Shells of Collisionless Matter Surrounding a Black Hole
- Decay and non-decay for the massless Vlasov equation on subextremal and extremal Reissner-Nordström black holes
- -Equilibrium of Gas in Spacetime of Multi-horizon Black Holes
- A general relativistic kinetic theory approach to linear transport in generic hydrodynamic frame