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We consider an ancient solution $g(•, t)$ of the Ricci flow on a compact surface that exists for t∈ (−∞, T) and becomes spherical at time $t = T$. We prove that the metric $g(•, t)$ is either a family of contracting spheres, which is a type I ancient solution, or a King–Rosenau solution, which is a type II ancient solution.
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Daskalopoulos et al. (2012) studied this question.
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