Virial Theorem (Statistical Mechanics)
Also known as: Clausius virial theorem · Gravitational virial theorem
In a bound system, twice the kinetic energy always equals the negative of the potential energy — energy is partitioned by the power law of the force.
N-body gravitational cluster simulation. Real-time running averages of kinetic and potential energy shown; virial ratio ⟨T⟩/|⟨V⟩| converges to 0.5 as system virialises.
Equivalent forms
The theorem is purely mechanical — no statistics needed — yet its ensemble average gives the equation of state of real gases via the virial expansion.
Unit systems
- SI:
- J for energies
- astrophysics:
- M☉, pc, km/s; M ∼
- plasma:
- thermal pressure = magnetic pressure in MHD equilibrium
Where it holds
Clausius introduced the virial in 1870 to study equations of state for real gases. Poincaré applied it to stellar dynamics; it became the cornerstone of gravitational astrophysics and plasma confinement.
Why don't clusters of galaxies fly apart?
The virial theorem relates the time-averaged kinetic energy of a bound system to the time-averaged potential energy. It is how astronomers estimate the mass of galaxy clusters — by measuring the velocity dispersion of member galaxies and invoking ⟨T⟩ = −(1/2)⟨V⟩.