Linked from

The 83 pages that link to Equation of state, each with the reason it gives.

• High-pressure mineral physicsRelated: It converts measurements into density profiles for planetary interiors.

• Maxwell relationsRelated: Equations of state supply measurable derivatives used after applying a Maxwell relation.

• Millisecond pulsarRelated: Pulsar mass and radius measurements constrain the equation of state of neutron-star matter.

• Neutron degeneracy pressureRelated: Neutron-star structure depends on how pressure changes with density.

• High-pressure chemistryRelated: It quantifies compression and helps compare measured behavior across conditions.

• Stellar coreRelated: It links core temperature and density to the pressure that supports the star.

• Tolman–Oppenheimer–Volkoff limitRelated: The neutron-star equation of state determines how much mass pressure can support.

• Color superconductivityRelated: The phase's pressure and energy density would contribute to the dense-matter equation of state.

• Johannes Diderik van der WaalsNarrower topic: His model became a landmark example of a molecularly informed equation of state.

• Degenerate matterRelated: It translates quantum statistics and interactions into predictions of stellar structure.

• Equilibrium thermodynamicsRelated: Equilibrium properties are linked by equations of state, such as the ideal gas law.

• Fundamental thermodynamic relationRelated: Derivatives of the fundamental relation can supply pressure and temperature equations of state.

• Implicit functionRelated: Thermodynamic relations often define one state variable only implicitly from the others.

• Mineral physicsRelated: Equations of state translate mineral measurements into density profiles for planetary interiors.

• Quark starRelated: A quark-matter equation of state predicts a star's mass, radius, and stability.

• Astrophysical fluid dynamicsRelated: It closes fluid equations by specifying how astrophysical matter responds to compression and heating.

• Amagat's lawNarrower topic: Amagat’s law is a volume-composition rule whose accuracy depends on the gas equation of state.

• Giant planetRelated: Interior models depend on how hydrogen, helium, and other materials behave under immense pressure.

• Hydrodynamic modelRelated: Compressible-flow models need it to close the equations and relate pressure to fluid state.

• Intensive and extensive propertiesRelated: Equations of state connect intensive variables with extensive measures of system size.

• Percy Williams BridgmanRelated: Bridgman measured how pressure changes the volumes of many substances.

• Virial expansionNarrower topic: The virial expansion is one particular representation of a gas equation of state.

• Birch's lawRelated: It supplies density estimates needed alongside seismic velocity in deep-Earth models.

• Classical fluidRelated: It closes fluid models by relating pressure to density and temperature.

• Atmospheric physicsRelated: It links atmospheric temperature and pressure changes to air density.

• Buchdahl's theoremRelated: Realistic equations of state determine whether stellar models approach the theorem’s limit.

• Crocco's theoremRelated: It helps express entropy and pressure gradients in forms used with Crocco's relation.

• Exotic starRelated: It determines whether a proposed exotic interior can support a star against gravity.

• High-energy-density plasmaRelated: It determines how the plasma responds when compressed or heated.

• Internal pressureNarrower topic: Internal pressure is obtained from how a system’s mechanical pressure varies with temperature and volume.

• Iron planetRelated: Interior models use iron and silicate equations of state to translate measurements into likely structure.

• Theorem of Corresponding StatesNarrower topic: Corresponding states compares the equations of state of different substances.

• Thermodynamic equationsBroader topic: It gives explicit constraints among a system's state variables.