The noncommutative fractional Fourier law in bounded and unbounded domains

Abstract

Using the spectral theory on the S-spectrum it is possible to define the fractional powers of a large class of vector operators. This possibility leads to new fractional diffusion and evolution problems that are of particular interest for nonhomogeneous materials where the Fourier law is not simply the negative gradient operator but it is a nonconstant coefficients differential operator of the formwhere, Ω can be either a bounded or an unbounded domain in R 3 whose boundary ∂Ω is considered suitably regular, Ω is the closure of Ω and e ℓ , for ℓ = 1, 2, 3 are the imaginary units of the quaternions H. The operators T ℓ := a ℓ (x)∂x ℓ , for ℓ = 1, 2, 3, are called the components of T and a1, a2, a3 : Ω ⊂ R 3 → R are the coefficients of T .In this paper we study the generation of the fractional powers of T , denoted by Pα(T ) for α ∈ (0, 1), when the operators T ℓ , for ℓ = 1, 2, 3 do not commute among themselves. To define the fractional powers Pα(T ) of T we have to consider the weak formulation of a suitable boundary value problem associated with the pseudo S-resolvent operator of T . In this paper we consider two different boundary conditions. If Ω is unbounded we consider Dirichlet boundary conditions. If Ω is bounded we consider the natural Robin-type boundary conditions associated with the generation of the fractional powers of T represented by the operator 3 ℓ=1 a 2 ℓ (x)n ℓ (x)∂x ℓ + a(x)I, for x ∈ ∂Ω, where I is the identity operator, a : ∂Ω → R is a given function and n = (n1, n2, n3) is the outward unit normal vector to ∂Ω. The Robin-type boundary conditions associated with the generation of the fractional powers of T are, in general, different from the Robin boundary conditions associated to the heat diffusion problem which leads to operators of the type 3 ℓ=1 a ℓ (x)n ℓ (x)∂x ℓ + b(x)I, x ∈ ∂Ω. For this reason we also discuss the conditions on the coefficients a1, a2, a3 : Ω ⊂ R 3 → R of T and on the coefficient b : ∂Ω → R so that the fractional powers of T are compatible with the physical Robin boundary conditions for the heat equations.