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[Mentors' note: split off from this thread]
Do all black holes have the same density?
Do all black holes have the same density?
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Black holes do not have the same density; in fact, their density decreases as mass increases. The relationship between mass and the Schwarzschild radius indicates that doubling the mass results in an eight-fold increase in volume, thereby reducing density. The density of a black hole is not a fundamental quantity, as it is derived from mass divided by volume, and the volume of a singularity is undefined. Therefore, the concept of density is not particularly useful when discussing black holes, as mass is concentrated at a singularity rather than evenly distributed.
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George Jones said:As mass increases, the density of matter necessary to form a black hole decreases. If fact, if enough stars are used, they don't even have to touch for a black hole to form. In other words the stars have to be close together, but there still can be space between them. Below, I calculate a quantity that I'll call density, but, in reality, the quantity is only suggestive of density.
Setting this "density" to the average density of the sun, about 1400 kg/m^3, gives a black hole mass of about 100 million solar masses. So, if more than 100 million or so (within an order of magnitude) sunlike stars congregate in the centre of a galaxy, they don't have to touch (initially) to form a black hole.
The following calculation is only suggestive, and it is in no way rigorous. Because of the curvature and nature of spacetime, it probably doesn't make sense to calculate the spatial volume inside the event horizon of a black hole.
Density is mass over volume, i.e.,
\rho = \frac{M}{V},
and the volume of a spherical object of radius R is given by 4\pi R^3/3, so the density of a uniform sphere is
\rho = \frac{3M}{4\pi R^3}.
A spherical black hole has event horizon (boundary) located at
R = \frac{2GM}{c^2},
where G is Newton's gravitational constant and c is the speed of light.
Subsituting this equation into the density equation for a spherical black hole gives
\rho = \frac{3c^6}{32\pi G^3} \frac{1}{M^2}.
The first bit is just a constant number, while the second bit shows that the "density" of a spherical black rapidly decreases as mass increases.
Inverting this equation gives
M = \frac{c^3}{4}\sqrt{\frac{3}{2\pi G^3}}\sqrt{\frac{1}{\rho}},
and using the Sun's density for \rho gives the result I mentioned at the top.