PeterDonis
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Ibix said:On a sphere you should see more cubes radially than naive analysis of the circumference would suggest, surely?
Yes, you're right, I misstated the difference between the black hole spacetime (more precisely, a single spacelike slice of constant Schwarzschild coordinate time in a black hole spacetime) and a 3-sphere. Giving the math will make it clearer: the 3-sphere metric, in "Schwarzschild-like" coordinates where ##r## is the areal radius and we have picked any point we like as the origin, is:
$$
ds^2 = \frac{1}{1 - k r^2} dr^2 + r^2 d\Omega^2
$$
where ##k## is a constant related to the "Radius of curvature" of the 3-sphere.
The metric of the Flamm paraboloid, which is the geometry of a constant Schwarzschild time spacelike slice of a black hole spacetime, is:
$$
ds^2 = \frac{1}{1 - \frac{2M}{r}} dr^2 + r^2 d\Omega^2
$$
where ##M## is the mass of the hole.
Both of these metrics have the coefficient of ##dr^2## larger than 1, so you are right that they both allow you to fit more cubes radially than you would expect based on tangential distances. But the dependence on ##r## of how many more cubes you can fit radially is very different.