The thermodynamic conditions within the mantle would allow many hydrocarbon molecules to be at equilibrium under high pressure and high temperature.

These thermodynamic conditions are known to be the cause of MHV related erosion.

When the thermodynamic conditions are met, the vapors react with the gas in the vicinity of the substrate to form films.

As the vapors arrive at the surface, they chemically combine under proper thermodynamic conditions to form a metal carbide film.

If subcooling is not generous enough, the refrigerant remains in thermodynamic conditions close to saturation easing flash-gas appearance.

This happens because the piping is designed for a specific refrigerant mixture that allows liquid in the liquid line, given certain thermodynamic conditions.

These are the highest volumetric molecular hydrogen uptakes for a porous material under these thermodynamic conditions.

The onset of thermal decomposition depends on the different thermodynamic conditions such as heating rates.

The stability of hydrocarbons in the thermodynamic conditions of the Earth.

This kind of system usually requires the use of expensive electronic control systems to monitor the fluid thermodynamic conditions.