Do All Black Holes Have the Same Density?

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Discussion Overview

The discussion centers around the question of whether all black holes have the same density, exploring the concept of density in relation to black holes, including theoretical implications and calculations. Participants examine the definitions and relevance of density in the context of black holes, touching on aspects of general relativity and the nature of singularities.

Discussion Character

  • Debate/contested
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • Some participants suggest that as mass increases, the density necessary to form a black hole decreases, with calculations indicating that a black hole formed from a large number of stars does not require them to be in contact.
  • One participant argues that density is a derived quantity and not useful for black holes, as the volume of a singularity is not defined.
  • Another participant points out that the relationship between mass and the Schwarzschild radius implies that doubling the mass increases the volume significantly, thus reducing density.
  • It is noted that the mass of a black hole is not evenly distributed, being concentrated at a singularity, which complicates the concept of density further.
  • Some calculations are presented to illustrate that the density of a black hole, if defined in terms of a hypothetical sphere around the event horizon, decreases as the black hole's mass increases.
  • A participant mentions a scenario where stars could collapse into a black hole without touching, indicating that the average density just before the event horizon forms could be very low.
  • One participant expresses a misconception about black holes being made of a uniform "black hole matter" with constant average density, which is identified as incorrect.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the concept of density in relation to black holes, with multiple competing views and interpretations of density and its relevance remaining present throughout the discussion.

Contextual Notes

The discussion highlights limitations in defining density for black holes, particularly regarding the nature of singularities and the assumptions involved in calculations related to mass and volume.

EnumaElish
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[Mentors' note: split off from this thread]
Do all black holes have the same density?
 
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I am not sure what you mean by "density". The following may or may not be relevant. It certainly is not rigourous..

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.
 
Density is a derived quantity, not a fundamental one, equal to mass divided by volume. The volume of a singularity is not defined, so neither is the density. It just isn't a useful concept for black holes.
 
Short answer: No, as you can see just by looking at the relationship between the mass and the Schwarzschild radius. Doubling the mass doubles the "radius" so increases the "volume" eight-fold, commensurately reducing the "density".

Longer answer: Those scare-quotes are in the short answer for a reason. The volume of a black hole, and hence its density, aren't especially well defined. The first and most obvious problem is that the mass is not distributed evenly inside the black hole; as far as GR will tell us (and there's no reason to believe this particular prediction) it is concentrated in a point of zero volume at the singularity in the "center" so there's no physical significance to any density you might calculate. Second, the Schwarzschild radius is not the length of a line segment between the central singularity and the event horizon (in fact, there is no such thing) so you can't just plug it into the formula for the volume of a sphere.

Usually when someone speaks of the "density" of a black hole, they mean the ratio of the mass to the volume of a hypothetical sphere whose surface area is equal to the surface area of the event horizon. And if that's what you mean by the density, you can go with the short answer above: the bigger the black hole, the lower the density.
 
But the utility of George's calculation is, for example, suppose some process carried away most of the angular momentum of the stars within our galaxy, so they inevitably start collapsing. Then, the calculation show that stars are inside the event horizon before they are touching (and in some sense, before 'whatever' happens at the center, assuming it is not a singularity). In fact if there were a cloud of dust with the mass of the milky way, that had low angular momentum and was collapsing, its [average] density just before the event horizon formed would be less than that of air.
 
I always thought they're all made of "black hole matter" with constant average density, like some exotic black diamond. Patently false.
 

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