Rotating elastic bodies in Einstein gravity
Lars Andersson (UM, AEI), Robert Beig (Vienna), Bernd Schmidt (AEI)

TL;DR
This paper proves the existence and uniqueness of stationary, axisymmetric solutions in Einstein gravity for small gravitational constants and angular frequencies, describing rotating elastic bodies in a relativistic setting.
Contribution
It establishes a rigorous mathematical result connecting relativistic elasticity with Einstein gravity for rotating bodies, extending previous non-relativistic models.
Findings
Existence of solutions for small gravitational constants and frequencies
Uniqueness of these solutions under given conditions
Solutions describe rigidly rotating elastic bodies in Einstein gravity
Abstract
We prove that, given a stress-free, axially symmetric elastic body, there exists, for sufficiently small values of the gravitational constant and of the angular frequency, a unique stationary axisymmetric solution to the Einstein equations coupled to the equations of relativistic elasticity with the body performing rigid rotations around the symmetry axis at the given angular frequency.
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