Naty1
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"So when gravity is strong enough then matter turns into energy .."
That is speculation. Things start out that way and stars are born from clouds of gas, but then the nuclear processes run their course permitting further compression and greater density.
As stellar masses get more dense due to gravitational energy, things progress in density to electron degeneracy, then neutron, then quark, then apparently collapse to a black hole...by that time no one knows what happens to 'mass'...we believe the singularity is one of time, not space.
Regarding neutron stars:
Tolman–Oppenheimer–Volkoff limit
http://en.wikipedia.org/wiki/Tolman–Oppenheimer–Volkoff_limit
That is speculation. Things start out that way and stars are born from clouds of gas, but then the nuclear processes run their course permitting further compression and greater density.
As stellar masses get more dense due to gravitational energy, things progress in density to electron degeneracy, then neutron, then quark, then apparently collapse to a black hole...by that time no one knows what happens to 'mass'...we believe the singularity is one of time, not space.
Regarding neutron stars:
Modern estimates range from approximately 1.5 to 3.0 solar masses. [before collapse to a black hole] [3] The uncertainty in the value reflects the fact that the equations of state for extremely dense matter are not well known.
In a neutron star less massive than the limit, the weight of the star is balanced by short-range repulsive neutron-neutron interactions mediated by the strong force and also by the quantum degeneracy pressure of neutrons, preventing collapse. If its mass is above the limit, the star will collapse to some denser form. It could form a black hole, or change composition and be supported in some other way (for example, by quark degeneracy pressure if it becomes a quark star). Because the properties of hypothetical more exotic forms of degenerate matter are even more poorly known than those of neutron-degenerate matter, most astrophysicists assume, in the absence of evidence to the contrary, that a neutron star above the limit collapses directly into a black hole.
Tolman–Oppenheimer–Volkoff limit
http://en.wikipedia.org/wiki/Tolman–Oppenheimer–Volkoff_limit
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