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Article

Fractional Heat Conduction in an Infinite Medium with a Spherical Inclusion

by
Yuriy Povstenko
1,2
1
Institute of Mathematics and Computer Science, Jan Długosz University in Częstochowa, Armii Krajowej 13/15, Częstochowa 42-200, Poland
2
Department of Computer Science, European University of Informatics and Economics (EWSIE) Białostocka 22, Warsaw 03-741, Poland 
Entropy 2013, 15(10), 4122-4133; https://doi.org/10.3390/e15104122
Submission received: 27 August 2013 / Revised: 22 September 2013 / Accepted: 22 September 2013 / Published: 27 September 2013
(This article belongs to the Special Issue Dynamical Systems)

1. Introduction

The standard heat conduction (diffusion) equation for temperature T
is obtained from the balance equation for energy
where ρ is the mass density, C is the specific heat capacity, q is the heat flux vector, and the classical Fourier law which states the linear dependence between the heat flux vector q and the temperature gradient
with k being the thermal conductivity. In the heat conduction Equation (1) is the heat diffusivity coefficient.
To describe heat conduction in media with complex internal structure, the standard parabolic Equation (1) is no longer accurate enough. In nonclassical theories, the Fourier law Equation (3) and the parabolic heat conduction Equation (1) are replaced by more general equations (see [1,2,3,4,5,6]). The time-nonlocal dependence between the heat flux vector q and the temperature gradient [7,8]
results in the heat conduction with memory [7,8]
Several particular cases of choice of the memory kernel were analyzed in [9,10,11,12]. The time-nonlocal dependence between the heat flux vector q and the temperature gradient with the long-tail power kernel [9,10,11,12]
where is the gamma function, can be interpreted in terms of fractional calculus:
where and are the Riemann–Liouville fractional integral and derivative of the order respectively [13,14,15,16]:
The balance Equation (2) and the constitutive Equations (8) and (9) yield the time-fractional equation
with the Caputo fractional derivative
The details of obtaining the time-fractional heat conduction Equation (12) from the balance Equation (2) and the constitutive Equations (8) and (9) can be found in [17].
Equations with fractional derivatives, in particular the time-fractional heat conduction equation (diffusion-wave equation), describe many important physical phenomena in different media (see [9,18,19,20,21,22,23,24,25,26,27,28,29,30,31,32], among many others). Fractional calculus plays a significant part in studies of entropy [33,34,35,36,37,38]. It should be noted that entropy is also used in analysis of anomalous diffusion processes and fractional diffusion equation [39,40,41,42,43,44,45].
Different kinds of boundary conditions for Equation (12) in a bounded domain were analyzed in [46,47]. It should be emphasized that due to the generalized constitutive equations for the heat flux (8) and (9) the boundary conditions for the time-fractional heat conduction equation have their traits in comparison with those for the standard heat conduction equation. The Dirichlet boundary condition specifies the temperature over the surface of a body
For time-fractional heat conduction Equation (12) two types of Neumann boundary condition can be considered: the mathematical condition with the prescribed boundary value of the normal derivative of temperature
and the physical condition with the prescribed boundary value of the heat flux
Here n is the outer unit normal the boundary surface. Similarly, the mathematical Robin boundary condition is a specification of a linear combination of the values of temperature and the values of its normal derivative at the boundary of the domain
with some nonzero constants c1 and c2, while the physical Robin boundary condition specifies a linear combination of the values of temperature and the values of the heat flux at the boundary of the domain. For example, the Newton condition of convective heat exchange between a body and the environment with the temperature TE
where h is the convective heat transfer coefficient, leads to
If the surfaces of two solids are in perfect thermal contact, the temperatures on the contact surface and the heat fluxes through the contact surface are the same for both solids, and the boundary conditions of the fourth kind are obtained:
where subscripts 1 and 2 refer to the first and second solid, respectively, and n is the common unit normal at the contact surface. In fractional calculus, where integrals and derivatives of arbitrary (not only integer) order are considered, there is no sharp boundary between integration and differentiation. For this reason, some authors [15,25] do not use a separate notation for the fractional integral The fractional integral of the order is denoted as . In the equation of perfect thermal contact (23) and , are understood in this sense.
Starting from the pioneering papers [48,49,50,51,52], considerable interest has been shown in solutions to time-fractional heat conduction equation. In the literature, there are only a few papers in which the fractional heat conduction equation (fractional diffusion-wave equation) is studied in composite medium [47,53,54]. In the present paper, the problem of fractional heat conduction in a composite medium consisting of a spherical inclusion and a matrix being in perfect thermal contact at is considered. The heat conduction in each region is described by the time-fractional heat conduction equation with the Caputo derivative of fractional order and , respectively.

2. Statement of the Problem

Consider the time-fractional heat conduction equations in a spherical inclusion
and in a matrix
under the initial conditions
and the boundary condition of perfect thermal contact
The boundedness condition at the origin and the zero condition at infinity are also assumed:
The limitations on α and β in Equations (26–29) express the fact that if or , then the additional condition on the first time derivative should be also imposed.
In what follows we restrict ourselves to the particular case when a sphere is at initial uniform temperature T0 and the matrix is at initial zero temperature
The Laplace transform with respect to time t applied to Equations (24) and (25) leads to two ordinary differential equations
having the solutions
It follows from conditions at the origin and at infinity Equation (32) that
The integration constants B1 and B2 are obtained from the perfect thermal contact boundary conditions Equations (30) and (31)
Hence, the solution is written as
Now we will investigate the approximate solution of the considered problem for small values of time. In the case of classical heat conduction this method was described in [55,56]. Based on Tauberian theorems for the Laplace transform (see, for example [57]), for small values of time t (the large values of the transform variable S) we can neglect the exponential term in comparison with 1,
thus obtaining
In the following particular cases , ; the denominator in Equations (47) and (48) can be treated as a cubic equation and the decomposition into the sum of partial fractions can be obtained similar to that used in [58].
Now we will consider another particular case when
To invert the Laplace transform the following formula will be used [14,15,16]
where is the generalized Mittag-Leffler function in two parameters
Additionally [51,52,59,60,61]
Here is the Wright function [1,51,52,62]
whereas is the Mainardi function [15,51,52]
From Equations (47) and (48) we get:
where
It should be emphasized that the solution is expressed in terms of the Mainardi function and the Wright function . The limitation in Equations (51–53) means that in Equations (56) and (57).

4. Conclusions

We have obtained the approximate solution to the time-fractional heat conduction equations in a composite body consisting of a matrix and spherical inclusion with different thermophysical properties. The conditions of perfect thermal contact have been assumed: the temperatures at the boundary surface are equal and the heat fluxes through the contact surface are the same. The Laplace integral transform allows us to obtain the ordinary differential equations for temperatures. Inversion of the Laplace transform has been carried out analytically for small values of time.

Acknowledgments

The author thanks the anonymous reviewers for their helpful suggestions.

Conflicts of Interest

The author declares no conflict of interest.

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Povstenko, Y. Fractional Heat Conduction in an Infinite Medium with a Spherical Inclusion. Entropy 2013, 15, 4122-4133. https://doi.org/10.3390/e15104122

AMA Style

Povstenko Y. Fractional Heat Conduction in an Infinite Medium with a Spherical Inclusion. Entropy. 2013; 15(10):4122-4133. https://doi.org/10.3390/e15104122

Chicago/Turabian Style

Povstenko, Yuriy. 2013. "Fractional Heat Conduction in an Infinite Medium with a Spherical Inclusion" Entropy 15, no. 10: 4122-4133. https://doi.org/10.3390/e15104122

APA Style

Povstenko, Y. (2013). Fractional Heat Conduction in an Infinite Medium with a Spherical Inclusion. Entropy, 15(10), 4122-4133. https://doi.org/10.3390/e15104122

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