Mixmaster Behavior in Inhomogeneous Cosmological Spacetimes
Marsha Weaver, James Isenberg, Beverly K. Berger

TL;DR
This paper provides numerical evidence that inhomogeneous cosmological spacetimes generally exhibit Mixmaster behavior near singularities, supporting the conjecture that such behavior is typical in Einstein's equations.
Contribution
It demonstrates through numerical analysis that inhomogeneous spacetimes tend to evolve towards Mixmaster dynamics near singularities, confirming a longstanding theoretical conjecture.
Findings
Evidence of Mixmaster behavior at generic points in inhomogeneous spacetimes
Supports the conjecture of Belinskii et al. on generic singularity behavior
Numerical results align with theoretical predictions of complex oscillatory dynamics
Abstract
Numerical investigation of a class of inhomogeneous cosmological spacetimes shows evidence that at a generic point in space the evolution toward the initial singularity is asymptotically that of a spatially homogeneous spacetime with Mixmaster behavior. This supports a long-standing conjecture due to Belinskii et al. on the nature of the generic singularity in Einstein's equations.
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