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Numerical Heat Transfer, Part B: Fundamentals
An International Journal of Computation and Methodology
Volume 70, 2016 - Issue 6
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Original Articles

A control volume finite element method with spines for solutions of fractional heat conduction equations

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Pages 503-516 | Received 24 Mar 2016, Accepted 13 Jul 2016, Published online: 26 Oct 2016
 

ABSTRACT

The focus of this paper is the numerical solution of space-fractional heat conduction equations. Typical numerical treatments for fractional diffusion equations (FDEs) are constructed to function on structured grids and cannot be readily applied to problems in arbitrarily shaped domains. Presented is an unstructured control volume finite element method for the solution of FDEs in non-Cartesian domains. This method approximates the fractional derivative flux at given integration points with a weighted sum of gradients along orthogonal spines. Accuracy and utility of the approach are demonstrated by solution of one- and two-sided FDEs in rectangular and cylindrical domains.

Nomenclature

α=

fractional order or locality

β=

bias weighting

Γ=

gamma function

δ=

maximum side length of control volume

Δt=

time step

Δx, Δy=

space step

ν=

diffusivity

g=

Grünwald weight

G=

Gaussian weight

L=

length of spine

NS=

number of steps along spine

q=

flux

qα=

fractional flux

Q=

flow across control volume face

S=

shape functions

T=

local temperature

V=

control volume area

W=

flux weight

x, y=

space coordinate

=

fractional derivative from left and right

Subscript=
x, y=

coordinate axis

Superscript=
RL=

Riemann–Liouville derivative

Nomenclature

α=

fractional order or locality

β=

bias weighting

Γ=

gamma function

δ=

maximum side length of control volume

Δt=

time step

Δx, Δy=

space step

ν=

diffusivity

g=

Grünwald weight

G=

Gaussian weight

L=

length of spine

NS=

number of steps along spine

q=

flux

qα=

fractional flux

Q=

flow across control volume face

S=

shape functions

T=

local temperature

V=

control volume area

W=

flux weight

x, y=

space coordinate

=

fractional derivative from left and right

Subscript=
x, y=

coordinate axis

Superscript=
RL=

Riemann–Liouville derivative

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