Time-slab identities for a fixed spatial test #
For a Leray–Hopf solution whose momentum identity holds with a pressure, the
pairing of the specified time slices with a fixed smooth compactly supported
spatial field evolves by the integrated flux. This is the pairing formula used
for the cross-testing identity in lem:pv-serrin-uniqueness.
The momentum flux density of (u, Du, p) against a fixed spatial field
ψ: convection, diffusion and pressure terms.
Equations
- One or more equations did not get rendered due to their size.
Instances For
The pairing density of a velocity with a fixed spatial field.
Equations
- ESS.serrinPairing u ψ z = ∑ i : Fin 3, u z i * ψ z.1 i
Instances For
A spatial derivative vanishes outside the topological support.
Outside the support of the spatial field, the flux density vanishes.
The separated test ψ(x) η(t) in the momentum identity with pressure.
The velocity of a finite-energy weak solution is square integrable on the space-time slab.
The weak gradient of a finite-energy weak solution is square integrable on the slab.
The velocity tensor of a finite-energy weak solution is integrable on the slab.
A slab field in L^q with q ≥ 1 is integrable on a compact spatial set times the time
interval.
The pairing of the specified time slices of a finite-energy weak solution with a fixed smooth compactly supported spatial field is the initial pairing plus the time integral of the momentum flux, at every time of the closed interval.