The separate universe problem: 40 years on
B. J. Carr, Tomohiro Harada

TL;DR
This paper revisits the concept of the separate-universe scale, clarifies its implications for primordial black holes across different equations of state, and refines earlier calculations considering recent criticisms, emphasizing the scale's relation to the horizon size.
Contribution
It provides a refined calculation of the separate-universe scale for various equations of state, addressing previous misconceptions and clarifying the conditions under which black holes or baby universes form.
Findings
For $-1/3 < k < \infty$, the scale is of order the horizon size.
Primordial black holes cannot be much larger than the horizon at formation.
For $-1 < k < -1/3$, large regions produce baby universes instead of black holes.
Abstract
The claim that an overdense (positive curvature) region in the early universe cannot extend beyond some maximum scale and remain part of our universe, first made 40 years ago, has recently been questioned by Kopp et al. Their analysis is elucidating and demonstrates that one cannot constrain the form of primordial density perturbations using this argument. However, the notion of a separate-universe scale still applies and it places an important upper limit on the mass of primordial black holes forming at any epoch. We calculate this scale for equations of state of the form with , refining earlier calculations on account of the Kopp et al. criticisms. For , the scale is always of order the cosmological particle horizon size, with a numerical factor depending on . This confirms the earlier claim that a primordial black hole cannot be…
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