The defocusing power-type wave equation has the conserved nonnegative energy
For in three spatial dimensions, conserved positive wave energy controls . The Sobolev inequality gives . Differentiated wave energy estimates and the Gronwall inequality then give , where bounds the corresponding initial Sobolev norms.
Multiplying a defocusing wave equation by and integrating by parts gives a weighted spacetime identity. For a radial solution and radial weight, its coercive terms are
In three dimensions, away from the origin and . Hence as a distribution.
Let be a global sufficiently regular finite-energy solution of on , with , and let be its conserved nonnegative wave energy. Then the Morawetz estimate for the defocusing wave equation is
The constant depends on and the spatial dimension, not the upper endpoint of the time interval. A finite-time version holds on every interval of smooth existence. A global spacetime bound does not itself assert existence of a global solution.[ref]
Use the radial multiplier in the Morawetz identity for the defocusing wave equation. Its action is bounded by using the Hardy inequality in Euclidean space. The radial weight has nonnegative angular terms and ; the remaining nonlinear term has positive coefficient proportional to . Integration in time bounds its spacetime integral by endpoint actions, and monotone convergence gives the infinite-time statement. The estimate limits how long nonlinear wave energy can remain concentrated near a fixed location.
For a radial function in three dimensions, setting removes the radial first derivative because . The defocusing power equation becomes
on the half-line.
In three dimensions set for a radial function satisfying . If the source has support in and , the Duhamel principle bounds its contribution to by for . Its backward characteristic interval meets the source in a set of length at most one, and . Division by gives for compactly supported initial data.
For and a radial weight ,

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