Derrick's scaling argument tests a static field configuration by rescaling space. A soliton can be stationary only if energy terms with opposite scaling powers balance at the original scale.
For smooth fields into with nonnegative differentiable potential and finite energy, Derrick scaling in two spatial dimensions forces the potential integral to vanish. Thus the field takes values where and , so its static field equation makes every component harmonic. Each first derivative is an entire harmonic function in L2 space; the mean-value inequality on arbitrarily large balls forces it to vanish. Hence the field is constant. The scale identity alone does not exclude a pure-gradient model; this additional argument uses the flat unconstrained target. Curved-target harmonic maps, for example the O3 nonlinear sigma model, can instead have finite-energy nonconstant solutions.
Under Derrick scaling, an energy term containing spatial derivatives and homogeneous of degree in those derivatives scales as in spatial dimensions.
For a smooth gauge field on with finite positive magnetic energy, dilate its connection one-form by . Its gauge curvature scales as , so the energy scales as . A static stationary configuration must have zero derivative at , forcing and hence . This Derrick scaling argument assumes the dilation preserves the boundary conditions and that boundary terms vanish. It does not exclude four-dimensional Yang-Mills instantons, whose Euclidean action is scale invariant.
In three space dimensions, rescale to and to . The gauge curvature then scales with two derivatives, and the adjoint covariant derivative of the Higgs field with one. Magnetic, Higgs-gradient and potential energies give the displayed formula. Stationarity requires , which permits nonzero energies. In the Bogomolny-Prasad-Sommerfield monopole limit , the Bogomolny equations give .
Stationarity of a static solution under Derrick scaling requires . This necessary relation among the separately scaling energy terms is the Derrick virial identity.
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Derrick's theorem is a result in the field of mathematical physics, particularly in the study of field theories and solitons. It concerns the stability of soliton solutions to certain field equations, specifically addressing the stability under small perturbations of the solutions. The theorem states that if a field configuration (such as a soliton) is localized and satisfies certain energy conditions, then it is stable against small perturbations if and only if its energy does not decrease under rescaling of the spatial variables.