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Kirill Pankratov's avatar

This post is such a good summary of the "wallasea problem".

Yet I am not convinced by the Mondal et al work.

First, even by stretching their model parameters to the max, they obtained only a small difference in coalescence times between PNG-Afr and Asi-Afr compared to real data, (compare fig 1 and 4 from their paper).

Second, surely there must be other Eurasian populations that could experience strong bottlenecks and long isolation. Yet the coalescence time between all Eurasians and Afr Yoruba is very consistent, and doesn't exceeds 75 my, that is likely happened after Toba.

I thing the right explanation is the most obvious one -that there was an early HS population in SEA that was mostly but not fully replaced by newcomers after 50 ky but left some genetic trace.

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Scott's avatar

John, is my interpretation of the RCCR method correct here?

Say you have two populations, popA and popB, with an RCCR value of 0.5 (on a scale from 0 to 1) at 50k ybp. Does that essentially mean that 50% of the unique drift that defines popA as popA distinct from popB (and vice versa) had accumulated by 50k ybp?

Looking at "Table 1 Best fitted parameter values of model A," they have the separation of African and OOA populations at 62k ybp, with a 10k year long bottleneck. The estimated effective population size of OOA during that time is only 726 - that seems like a very, very low population size to be able to ride out a 10k year bottleneck without just going extinct.

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