Derrick's theorem

Derrick's theorem is an argument by physicist G. H. Derrick which shows that stationary localized solutions to a nonlinear wave equation or nonlinear Klein–Gordon equation in spatial dimensions three and higher are unstable.

Derrick's paper,[1] which was considered an obstacle to interpreting soliton-like solutions as particles, contained the following physical argument about non-existence of stable localized stationary solutions to the nonlinear wave equation now known under the name of Derrick's Theorem.

is a differentiable function with

The energy of the time-independent solution

is given by A necessary condition for the solution to be stable is

( x ) = θ ( λ x )

is an arbitrary constant, and write

for a variation corresponding to a uniform stretching of the particle.

Derrick's argument works for

Let be a solution to the equation in the sense of distributions.

satisfies the relation known as Pokhozhaev's identity (sometimes spelled as Pohozaev's identity).

[3] This result is similar to the virial theorem.

We may write the equation

in the Hamiltonian form

, the Hamilton function is given by and

are the variational derivatives of

and satisfies the equation with

denoting a variational derivative of the functional

is a critical point of

), Derrick's argument shows that

( θ ( λ x ) ) < 0

is not a point of the local minimum of the energy functional

Therefore, physically, the solution

A related result, showing non-minimization of the energy of localized stationary states (with the argument also written for

, although the derivation being valid in dimensions

) was obtained by R. H. Hobart in 1963.

[4] A stronger statement, linear (or exponential) instability of localized stationary solutions to the nonlinear wave equation (in any spatial dimension) is proved by P. Karageorgis and W. A. Strauss in 2007.

[5] Derrick describes some possible ways out of this difficulty, including the conjecture that Elementary particles might correspond to stable, localized solutions which are periodic in time, rather than time-independent.

Indeed, it was later shown[6] that a time-periodic solitary wave

may be orbitally stable if the Vakhitov–Kolokolov stability criterion is satisfied.