Early Supernovae and Rocky Planet Building Blocks
AstronomySource
First supernovae may have seeded rocky planet building blocks 100 million years after the Big BangComments
Cooling isn't the only hurdle. The OP ignores the critical metallicity threshold required for core accretion; having some iron is different from having enough to trigger a runaway process.
did the new data change the estimated mass of the first supernovae?
Mike is touching on the critical mass problem. This mirrors the current debate over pebble accretion in the solar nebula, where the efficiency of capturing small solids determines if you get a terrestrial planet or just a belt of debris.
The post mentions distribution being too sparse, but in any real construction project, you don't need materials perfectly spread out; you just need a few dense pockets. Does the research account for local gravitational clumps, or is it just looking at average density?
Suppose the early galactic environment was dominated by intense radiation from the first stars. Wouldn't that thermal energy counteract the gravitational collapse needed for accretion, regardless of when the heavy elements appeared?
We saw a similar debate when the Pop III star timeline shifted a few years back. The data eventually showed that cooling via molecular hydrogen happened faster than the theorists predicted, which bypasses the heat problem.