There is an upper limit to the mass of a neutron-degenerate object, the Tolman-Oppenheimer-Volkoff limit, which is analogous to the Chandrasekhar limit for electron-degenerate objects. The precise limit is unknown, as it depends on the equations of state of nuclear matter, for which a highly accurate model is not yet available...Whether quark-degenerate matter forms at all in these situations depends on the equations of state of both neutron-degenerate matter and quark-degenerate matter, both of which are poorly known.
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Singularity
At densities greater than those supported by any degeneracy, gravity overwhelms all other forces. To the best of our current understanding, the body collapses to form a black hole. In the frame of reference that is co-moving with the collapsing matter, all the matter ends up in an infinitely dense singularity at the center of the event horizon. In the frame of reference of an observer at infinity, the collapse asymptotically approaches the event horizon
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http://en.wikipedia.org/wiki/Neutron_degeneracy_pressure
Our science seems to begin the break down at just beyond neutron degeneracy...and generally quantum mechanics and general relativity fail to show exactly what is present at the big bang and at black hole singularities... equations diverge there, leading to apparent infinities, but I think most physicsts think that's a result of inadequate models rather than a reflection of actual infinities.
Anyway, if a bound is found, likely it will be at the big bang or black hole singularities.