Virial theorem

In <a href="/facts/Mechanics/A3yHLQA5">mechanics</a>, the virial theorem provides a general equation that relates the average over time of the total <a href="/facts/Kinetic_energy/aJRxUd4p">kinetic energy</a> of a stable system of discrete particles, bound by a <a href="/facts/Conservative_force/xY5QmC4q">conservative force</a> (where the <a href="/facts/Work_(physics)/mbclFPBs">work</a> done is independent of path), with that of the total <a href="/facts/Potential_energy/I03KLbmn">potential energy</a> of the system. Mathematically, the <a href="/facts/Theorem/f2Pe1FMD">theorem</a> states that

 
 
 
 ⟨
 T
 ⟩
 =
 −
 
 
 1
 2
 
 
 
 
 ∑
 
 k
 =
 1
 
 
 N
 
 
 ⟨
 
 
 F
 
 
 k
 
 
 ⋅
 
 
 r
 
 
 k
 
 
 ⟩
 ,
 
 
 {\displaystyle \langle T\rangle =-{\frac {1}{2}}\,\sum _{k=1}^{N}\langle \mathbf {F} _{k}\cdot \mathbf {r} _{k}\rangle ,}

where 
 
 
 
 T
 
 
 {\displaystyle T}
 
 is the total kinetic energy of the 
 
 
 
 N
 
 
 {\displaystyle N}
 
 particles, 
 
 
 
 
 F
 
 k
 
 
 
 
 {\displaystyle F_{k}}
 
 represents the <a href="/facts/Force/LNAUWMwK">force</a> on the 
 
 
 
 k
 
 
 {\displaystyle k}
 
th particle, which is located at position rk, and <a href="/facts/Angle_brackets/yzGM9J8A">angle brackets</a> represent the average over time of the enclosed quantity. The word virial for the right-hand side of the equation derives from vis, the <a href="/facts/Latin/pM3Kge85">Latin</a> word for "force" or "energy", and was given its technical definition by <a href="/facts/Rudolf_Clausius/RMgFgY7I">Rudolf Clausius</a> in 1870.
The significance of the virial theorem is that it allows the average total kinetic energy to be calculated even for very complicated systems that defy an exact solution, such as those considered in <a href="/facts/Statistical_mechanics/6zMsNYYG">statistical mechanics</a>; this average total kinetic energy is related to the <a href="/facts/Temperature/QyGe4gmj">temperature</a> of the system by the <a href="/facts/Equipartition_theorem/EJfmTK6W">equipartition theorem</a>. However, the virial theorem does not depend on the notion of temperature and holds even for systems that are not in <a href="/facts/Thermal_equilibrium/1D7nGm0d">thermal equilibrium</a>. The virial theorem has been generalized in various ways, most notably to a <a href="/facts/Tensor/pNjFo5tV">tensor</a> form.
If the force between any two particles of the system results from a <a href="/facts/Potential_energy/I03KLbmn">potential energy</a> 
 
 
 
 V
 (
 r
 )
 =
 α
 
 r
 
 n
 
 
 
 
 {\displaystyle V(r)=\alpha r^{n}}
 
 that is proportional to some power 
 
 
 
 n
 
 
 {\displaystyle n}
 
 of the <a href="/facts/Mean_inter-particle_distance/BcQwk8bd">interparticle distance</a> 
 
 
 
 r
 
 
 {\displaystyle r}
 
, the virial theorem takes the simple form

 
 
 
 2
 ⟨
 T
 ⟩
 =
 n
 ⟨
 
 V
 
 TOT
 
 
 ⟩
 .
 
 
 {\displaystyle 2\langle T\rangle =n\langle V_{\text{TOT}}\rangle .}

Thus, twice the average total kinetic energy 
 
 
 
 ⟨
 T
 ⟩
 
 
 {\displaystyle \langle T\rangle }
 
 equals 
 
 
 
 n
 
 
 {\displaystyle n}
 
 times the average total potential energy

⟨
 
 V
 
 TOT
 
 
 ⟩
 
 
 {\displaystyle \langle V_{\text{TOT}}\rangle }
 
. Whereas 
 
 
 
 V
 (
 r
 )
 
 
 {\displaystyle V(r)}
 
 represents the potential energy between two particles of distance 
 
 
 
 r
 
 
 {\displaystyle r}
 
, 
 
 
 
 
 V
 
 TOT
 
 
 
 
 {\displaystyle V_{\text{TOT}}}
 
 represents the total potential energy of the system, i.e., the sum of the potential energy 
 
 
 
 V
 (
 r
 )
 
 
 {\displaystyle V(r)}
 
 over all pairs of particles in the system. A common example of such a system is a star held together by its own gravity, where 
 
 
 
 n
 =
 −
 1
 
 
 {\displaystyle n=-1}
 
.

Virial theorem open-in-new

Virial theorem