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Earlier this week, I was reading this paper by Brown [of Brown and Bethe fame].
http://arxiv.org/abs/nucl-th/0504029
Title: Relation of Strangeness Nuggets to Strangeness Condensation and the Maximum Mass of Neutron Stars
Authors: Gerald E. Brown, Chang-Hwan Lee, Mannque Rho
It expands upon the equation of state that Smolin cites as a pillar of his CNS principle, and looks pretty solid. But reading between the lines, I see a more insidious result [for CNS], our universe favors the formation of neutron stars. I was daydreaming about this and the thought occurred to me - when/why do stellar cores collapse? And this thought popped to mind: when the mass density of the iron core exceeds the Chandrasekhar limit.
Somehow that made sense. It explains things like why neutron star masses cluster right around the Chandrasekhar limit.
http://arxiv.org/abs/nucl-th/0504029
Title: Relation of Strangeness Nuggets to Strangeness Condensation and the Maximum Mass of Neutron Stars
Authors: Gerald E. Brown, Chang-Hwan Lee, Mannque Rho
It expands upon the equation of state that Smolin cites as a pillar of his CNS principle, and looks pretty solid. But reading between the lines, I see a more insidious result [for CNS], our universe favors the formation of neutron stars. I was daydreaming about this and the thought occurred to me - when/why do stellar cores collapse? And this thought popped to mind: when the mass density of the iron core exceeds the Chandrasekhar limit.
Somehow that made sense. It explains things like why neutron star masses cluster right around the Chandrasekhar limit.