phinds said:
Again very helpful. So IF a neutron star managed somehow to get enough additional mass it WOULD collapse further into a black hole. This really answers my underlying question which I now realize I should have posted in this fashion: is it JUST the amount of mass that creates a black hole or is it some sort of process that could not occur in inert rock.
Well, sort of. Basically, once matter is dense enough compared to its surroundings, it necessarily forms a black hole. In principle, there is nothing that prevents any amount of matter, no matter how small, from achieving this density and becoming a black hole. So
in principle it is possible to make a black hole out of a golf ball.
However, in practice, the only way we know to achieve the densities required is through gravitational collapse of a very massive body. And there it is a combination of the total mass and the amount of pressure it is capable of sustaining. For example, you can make a star a couple hundred times the mass of our sun, and it will still not form a black hole as long as the core remains hot enough to support that outward pressure.
Once the core cools, it can't support the pressure any more, and it collapses to densities sufficient to produce either a neutron star or a black hole.
phinds said:
I do understand that the collapse of a star to a neutron star is NOT just a gravitational collapse because energy is released, but since a mass that is not a black hole (a neutron star) CAN be made to further collapse into a black hole, it IS, from the standpoint of my question, the mass that counts.
Well, actually, it is primarily gravitational collapse. The energy release is comes from gravitational potential energy. If the Earth were to be collapsed to be as dense as a neutron star, for example, it would go from having a radius of about 6,400,000 meters to a radius of about 60 meters. But with the same mass, that results in a
tremendous drop in gravitational potential energy, which, in turn, ends up meaning a tremendous release of energy.
In practice, when a massive star goes supernova, the core collapses into a neutron star while the outer layers of the star are blown away by the tremendous energy released from the gravitational collapse. The final neutron star is much less massive than the star it collapses from.
For a black hole, the difference is even greater: an Earth-mass black hole would have a radius of only a few centimeters (about the size of a golf ball).