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Virial Theorem

For a bound stationary state of

H=p22m+V(r),H = \frac{\mathbf p^2}{2m}+V(\mathbf r),

the quantum virial theorem gives

2⟨T⟩=⟨r⋅∇V(r)⟩,2\langle T\rangle = \left\langle \mathbf r\cdot\nabla V(\mathbf r) \right\rangle,

where T=p2/(2m)T=\mathbf p^2/(2m).

In one dimension this becomes

2⟨T⟩=⟨xV′(x)⟩.2\langle T\rangle = \langle xV'(x)\rangle.

If the potential is homogeneous of degree kk,

V(λr)=λkV(r),V(\lambda\mathbf r)=\lambda^kV(\mathbf r),

then Euler’s theorem gives

r⋅∇V=kV,\mathbf r\cdot\nabla V=kV,

and therefore

2⟨T⟩=k⟨V⟩.2\langle T\rangle = k\langle V\rangle.

For the harmonic oscillator, k=2k=2, so ⟨T⟩=⟨V⟩\langle T\rangle=\langle V\rangle. For a Coulomb potential, k=−1k=-1, so 2⟨T⟩=−⟨V⟩2\langle T\rangle=-\langle V\rangle.

  • The state is stationary and bound, or a suitable time average exists.
  • The expectation values are finite.
  • Boundary terms vanish under integration by parts or the equivalent commutator argument is well-defined.
  • Singular potentials require domain care.

Use the dilation generator

G=12(r⋅p+p⋅r).G = \frac12 \left( \mathbf r\cdot\mathbf p+\mathbf p\cdot\mathbf r \right).

For a stationary state, ⟨G⟩\langle G\rangle is time independent, so the expectation of its commutator with HH vanishes. The commutator produces the kinetic term and the scale derivative of the potential.

  • Applying the stationary bound-state form to scattering states.
  • Forgetting boundary terms in finite boxes or singular potentials.
  • Assuming ⟨T⟩=⟨V⟩\langle T\rangle=\langle V\rangle for every potential.
  • Using the Coulomb relation with the wrong sign.
  • Treating the virial theorem as enough to determine the full spectrum.

For a Coulomb potential V(r)=−α/rV(r)=-\alpha/r, what are ⟨T⟩\langle T\rangle and ⟨V⟩\langle V\rangle in terms of the total energy EE?

Solution

The potential is homogeneous of degree k=−1k=-1, so 2⟨T⟩=−⟨V⟩2\langle T\rangle=-\langle V\rangle. Since E=⟨T⟩+⟨V⟩E=\langle T\rangle+\langle V\rangle, we get E=−⟨T⟩E=-\langle T\rangle and therefore

⟨T⟩=−E,⟨V⟩=2E.\langle T\rangle=-E, \qquad \langle V\rangle=2E.

For bound Coulomb states, E<0E<0, so ⟨T⟩>0\langle T\rangle>0 and ⟨V⟩<0\langle V\rangle<0.

  • R. Clausius, “On a mechanical theorem applicable to heat,” Philosophical Magazine 40, 122-127, 1870.
  • R. Shankar, Principles of Quantum Mechanics, 2nd ed., Springer, 1994.
  • D. J. Griffiths and D. F. Schroeter, Introduction to Quantum Mechanics, 3rd ed., Cambridge University Press, 2018.
  • A. Messiah, Quantum Mechanics, Dover, 1999.