| 11. | Likewise, degenerate matter still has normal thermal pressure, but at extremely high densities, the degeneracy pressure usually dominates.
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| 12. | If preons exist, preon-degenerate matter might occur at densities greater than that which can be supported by quark-degenerate matter.
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| 13. | Quark-degenerate matter may occur in the cores of neutron stars, depending on the equations of state of neutron-degenerate matter.
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| 14. | If preons exist, preon-degenerate matter might occur at densities greater than that which can be supported by quark-degenerate matter.
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| 15. | Quark-degenerate matter may occur in the cores of neutron stars, depending on the equations of state of neutron-degenerate matter.
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| 16. | The white dwarf consists of degenerate matter, and so is largely unresponsive to heat, while the accreted hydrogen is not.
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| 17. | Hypothetically, there is a spherical crystal of ( neutronium / nihilon / neutron degenerate matter ) with a 1 cm diametre.
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| 18. | The equation of state for degenerate matter is " soft ", meaning that adding more mass will result in a smaller object.
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| 19. | :: Agreed-I think we are talking about degenerate matter here, but I don't see how that can be constructed just from protons alone.
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| 20. | A fluid of neutrons at 0 K will probably be a form of degenerate matter, suggesting an inherent pressure related to their density.
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