Single-transition attractor conjecture for Bianchi type VI−1/9_{-1/9}

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Let A\mathcal{A} denote the attractor describing generic behaviour near the initial singularity, and let K∘\mathrm{K}^{\circ}, TR1\mathcal{T}_{R_1}, TR3\mathcal{T}_{R_3}, and TN−\mathcal{T}_{N_-} denote the Kasner subset and the indicated transition subsets. Single-transition attractor conjecture. The attractor is

A=K∘∪TR1∪TR3∪TN−.\mathcal{A}=\mathrm{K}^{\circ}\cup\mathcal{T}_{R_1}\cup\mathcal{T}_{R_3}\cup\mathcal{T}_{N_-}.

This is the stronger conjecture motivated by numerical evidence that multiple transitions become increasingly rare, so that only single transitions contribute asymptotically; the source also notes supporting analytical and cosmological-billiard arguments, but gives no resolution.

References

Primary source

Phillipo Lappicy and Claes Uggla, “Oscillatory spacelike singularities: The Bianchi type VI_-1/9 vacuum models”, arXiv:2410.10375 (2025).

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