Thank you again for your response, Angela. Very clarifying for me.
I hope I can read more about all this stuff in the future, including most of these papers on ancient DNAs.
As for Y marks, high population would be one factor that avoid random extinctions, it seems.
Just for example, imagine if the so-called "barbarians" had the will and the ways to "replace" us. We'd have nowadays much more R-U106 and I1 than we have, and much less R-U152 (which is btw my maternal grandfather's lineage) in North Italy. Or the opposite: Romans in the North before that.
I know, I know... It's a big "if", actually disconnected to these people as we know them.
What I mean is that there's a range of variables/contexts involved in this Y phenomenon. I believe everyone would agree with that.
Fascinating stuff.
Hg O is very old. If we're talking on some specific young subclade, then ok.
E-M81 seems a good example, yes, of a recent clade (TMRCA is young - even younger than R-L151's) being very frequent in a populous area (North Africa). Thanks.
Well, perhaps this high population we have nowadays is one reason why I found the phenomenon that impressive. Possibly it'd become a bit less impressive looking to this configuration when it was just settled, many years ago, way before this huge populational growth from recent times.
Btw, as I suggested in another thread, given the fact that certain clades may suffer special relative expansions everytime and everywhere for some casual reasons (including founder effects, but not only, and including somewhat stable societies), the "tendency" is that these reasons link to the most frequent (ancestor) clades in the group involved, which would imply another tendency of an already frequent hg becoming even more frequent along the time. It'd be just one factor, of course, and that's generally speaking. I called this phenomenon "(Y) inertia", and I also compared it to a "wave", but it may stop anytime and "recede", so to speak, for whatever reasons/correlations (as replacements, but then the logic would apply to the newcomers'). Well, never mind. That's another story, offtopic and certainly too complex to be detailed here; plus, while it's interesting per se, I'm affraid the writer and the readers would also feel bored.
All that said, we were also talking on replacement. Depending on the situation just before this recent expansion of E-M81, for example, the parallel with IEs would be even "stronger".
Out ot curiosity, Maciamo's hypotheses regarding E-M81:
https://www.eupedia.com/europe/Haplogroup_E1b1b_Y-DNA.shtml#M81_origins