| 31. | Neutron star relativistic equations of state describe the relation of radius vs . mass for various models.
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| 32. | Another definition of a relativistic star is one with the equation of state of a supermassive size.
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| 33. | In all, there will be equations for each potential, resulting in a total of equations of state.
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| 34. | The classical thermodynamic properties of an ideal gas can be described by two equations of state :.
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| 35. | This equation can be shown to be consistent with the usual equations of state employed by thermodynamics.
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| 36. | Which only depends upon the equilibrium state potentials like temperature and density ( equation of state ).
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| 37. | :: See equation of state # Other equations of state of interest ( stiffened equation of state ).
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| 38. | Any equation expliciting one of these transport coefficient in the conservation variables is called an equation of state.
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| 39. | For a perfect fluid, another equation of state relating density \ rho and pressure p must be added.
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| 40. | :: See equation of state # Other equations of state of interest ( stiffened equation of state ).
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