Pressure
Definition and physical interpretation
In thermodynamics, pressure is an intensive variable that characterizes the system’s mechanical tendency to expand or contract against its boundary . For a uniform isotropic fluid in mechanical equilibrium , it coincides with the familiar force-per-area on a surface element, averaged over microscopic fluctuations.
Thermodynamically, pressure is defined as the variable conjugate to volume in the energy balance for a simple compressible system.
Thermodynamic definition via fundamental differentials
For a single-component simple compressible system with state described by , the differential form of the fundamental relation (see internal energy and the first law ) is
Here is defined by the partial derivative
Equivalently, in the entropy representation ,
These definitions make sense at equilibrium ; away from equilibrium, “pressure” may require additional structure (e.g., stress tensors) and may not be a single state variable.
Work and sign conventions
For a quasistatic compression/expansion, the mechanical work contribution is
under the standard pressure–volume work sign convention (consistent with the general work sign convention and the fact that work is path-dependent ). With this choice, expansion () corresponds to work done by the system, so .
Relations to free energies and response functions
Pressure can be expressed as a derivative of thermodynamic potentials obtained by a Legendre transform :
From the Helmholtz free energy ,
From the Gibbs free energy ,
A key linear response quantity controlled by pressure is the isothermal compressibility
which must satisfy for thermodynamic stability .
Finally, pressure is tied to the equation of state (or equivalent forms), which encodes material-specific information beyond the general structure of the laws.