Two-fluid model shows black holes persist through cosmological bounce and modify background fluid properties under fixed geometry.
A critical review of classical bouncing cosmologies , volume=
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Exact non-perturbative calculation shows circuit complexity stays finite at the bounce and its post-bounce growth correlates with cosmological particle production via a chirping term.
For genuine 3D collapsing Bianchi I initial conditions in mLQC-I, quantum effects damp shear exponentially after the bounce, yielding an isotropic attractor independent of matter content under the weak energy condition.
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Genericness of quantum damping of cosmological shear in modified loop quantum cosmology
For genuine 3D collapsing Bianchi I initial conditions in mLQC-I, quantum effects damp shear exponentially after the bounce, yielding an isotropic attractor independent of matter content under the weak energy condition.