PeterDonis
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PAllen said:It is correct that there are likely no non-rotating BH in existence.
Actually, it's quite possible that there aren't even any slightly rotating BH in existence. The usual assumption is that a BH formed by collapse of a single star would have negligible spin, but I'm not sure that's actually true. We don't have data on the spins of other stars AFAIK, but if we compute the spin parameter of the Sun, we find that it's about 0.5--which is certainly not negligible.
Here's the quick computation: the Sun's mass in geometric units is about ##2 \times 10^{30}## kg, or about 1480 meters in geometric units. The Sun's angular momentum in geometric units is ##GL / c^3##, where ##L## is the angular momentum in conventional units, which is about ##4.4 \times 10^{41}##. But the geometric parameter ##a## in the Kerr metric is ##j / m##, where ##j## is the angular momentum in geometric units and ##m## is the mass in geometric units. So if we take the ratio ##L / M## in conventional units (where ##L## is the angular momentum and ##M## is the mass), and then divide by ##c##, we will get ##a##. So we get
$$
a = \frac{4.4 \times 10^{41}}{2 \times 10^{30} \times 3 \times 10^8} \approx 740
$$
So ##a \approx 0.5 m##. If we assume that a typical star that collapses to a BH has a similar ratio of angular momentum to mass, then we would expect a BH formed by stellar collapse to have a significant spin parameter.