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Distributional systems and entropy flux pairs

Definition

Let d,m∈N, let I⊆R be an open time interval, let Ω⊆Rd be open, and let O⊆Rm be open and convex. Put Q=I×Ω. A first-order conservation system on O consists of fluxes Fj∈C1(O;Rm), 1≤j≤d, and the equation ∂tU+∑j=1d∂xjFj(U)=0. A state field U:Q→O is locally bounded if it is measurable and essentially bounded on every compact subset of Q. For an open set Q, g∈Lloc1(Q) means g is measurable and ∫K∣g∣<∞ for every compact K⊆Q. Require also U,F1(U),…,Fd(U)∈Lloc1(Q;Rm). These fields then define regular distributions componentwise. The conservation system holds in distributions on Q when, for every real-valued φ∈Cc∞(Q;Rm), ∫Q(U⋅∂tφ+∑j=1dFj(U)⋅∂xjφ) dx dt=0. This is the test-function meaning of the displayed derivative equation, using the distributional derivative convention in the supplied mathematics. The pairing is bilinear, without complex conjugation.

For an initial-value problem on (0,T)×Ω, T>0, let U0:Ω→O be measurable and locally integrable. Require integrability of the state and fluxes up to the initial boundary: ∫0τ ⁣ ⁣∫K(∣U∣+∑j=1d∣Fj(U)∣) dx dt<∞(0<τ<T, K⊆Ω compact). This condition uses only positive-time values and does not assert a strong trace at t=0. A test function up to the initial boundary is the restriction of a smooth function defined on a neighborhood of [0,T)×Ω, with compact support in [0,T)×Ω; its value at t=0 need not vanish. The initial-value weak identity is ∫0T ⁣ ⁣∫Ω(U⋅∂tφ+∑j=1dFj(U)⋅∂xjφ) dx dt+∫ΩU0(x)⋅φ(0,x) dx=0 for every such real vector test function. The stated integrability up to the initial boundary makes every term finite, including for tests nonzero at t=0; a weak solution with initial data U0 must satisfy these integrability conditions and this identity for all such tests.

A convex entropy-flux pair for the system is a function η∈C2(O;R) that is convex on the convex state domain O and functions qj∈C1(O;R) satisfying Dqj(V)=Dη(V) DFj(V)(V∈O, 1≤j≤d), where convexity means η((1−θ)V+θW)≤(1−θ)η(V)+θη(W) for V,W∈O and θ∈[0,1], and Dη,Dqj are row derivatives while DFj is the Jacobian matrix. For a state field U, require η(U),q1(U),…,qd(U)∈Lloc1 before using their distributions. The entropy inequality on Q means ∂tη(U)+∑j=1d∂xjqj(U)≤0, with the sign convention that this holds exactly when ∫Q(η(U) ∂tψ+∑j=1dqj(U) ∂xjψ) dx dt≥0 for every nonnegative ψ∈Cc∞(Q). With initial data on (0,T)×Ω, require also ∫0τ ⁣ ⁣∫K(∣η(U)∣+∑j=1d∣qj(U)∣) dx dt<∞(0<τ<T, K⊆Ω compact) and η(U0)∈Lloc1(Ω). Use every nonnegative scalar test up to the initial boundary defined above and add ∫Ωη(U0)ψ(0,x) dx to the entropy integral. These conditions make all terms finite even when the test is nonzero at t=0. A weak solution satisfying this inequality is entropy-admissible relative to that pair.

Remarks

For a state field U∈C1(Q;O) satisfying the conservation system pointwise on Q, the compatibility identity and the classical chain rule give ∂tη(U)+∑j∂xjqj(U)=Dη(U)(∂tU+∑jDFj(U)∂xjU)=0. For a merely weak solution this calculation is unavailable; the entropy inequality is an additional condition and does not follow from the weak conservation equation alone.

As a mathematical example of the notation, the one-dimensional spatial reduction of the compressible Euler model in three spatial dimensions uses U=(ρ,ρv,E) and F(U)=(ρv,ρv2+p,v(E+p)), with E=ρe+12ρv2. Here ρ>0 is mass density in kg m−3, v is axial velocity in m s−1, e is specific internal energy in J kg−1, E is total energy density in J m−3, and p=P(ρ,e) is pressure in pascals, with P a separately specified constitutive map. The components of U have units kg m−3, kg m−2 s−1, and J m−3; those of F are the corresponding quantities multiplied by velocity. This is only a mathematical model form, not an adopted physical postulate. An entropy inequality does not establish general compressible-system existence or uniqueness.

Remarks references

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