Differential rotation alone sustains regular, asymptotically flat, horizonless axisymmetric spacetimes with stable circular orbits, finite tidal forces, and linear stability against axisymmetric perturbations.
Thirring, ¨Uber die Wirkung rotierender ferner Massen in der Einsteinschen Gravitationstheorie, Phys
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Helicity-supported stationary spacetimes: A class of finite-energy, horizonless, axisymmetric solutions
Differential rotation alone sustains regular, asymptotically flat, horizonless axisymmetric spacetimes with stable circular orbits, finite tidal forces, and linear stability against axisymmetric perturbations.