
Low-temperature latent heat storage (LHS) systems are suitable for incorporating paraffin as the storage material. However, they face difficulty in actual implementation due to low thermal conductivity (TC). The present study used volcanic ash as an environmentally friendly and cost-effective material to increase the TC of paraffin. Three composites of paraffin/ash were prepared with ash proportions of 10 wt%, 30 wt% and 50 wt%. Characterizations were done to evaluate the average TC and properties. Thermal performance evaluation was conducted by analyzing the static charge/discharge cycle. The average TC for paraffin was 0.214 W/m·K. Adding volcanic ash improved the TC to 19.598 W/m·K. It made the charge/discharge performance of the composite better than that of pure paraffin. The charge rate for the composite ranged from 3.83 ℃/min to 5.12 ℃/min. The highest discharge rate was obtained at 4.21 ℃/min for the composite paraffin50/ash50. The freezing temperature for the composite is influenced by the ash proportion, which can be taken as a suitable approach to adjust the freezing point of paraffin-based thermal energy storage (TES). The detailed results for the characterization and thermal performance evaluation are described thoroughly within the article. The overall result indicates that volcanic ash is applicable for improving the TC and charge/discharge rate of paraffin-based TES.
Citation: Budhi Muliawan Suyitno, Dwi Rahmalina, Reza Abdu Rahman. Increasing the charge/discharge rate for phase-change materials by forming hybrid composite paraffin/ash for an effective thermal energy storage system[J]. AIMS Materials Science, 2023, 10(1): 70-85. doi: 10.3934/matersci.2023005
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Low-temperature latent heat storage (LHS) systems are suitable for incorporating paraffin as the storage material. However, they face difficulty in actual implementation due to low thermal conductivity (TC). The present study used volcanic ash as an environmentally friendly and cost-effective material to increase the TC of paraffin. Three composites of paraffin/ash were prepared with ash proportions of 10 wt%, 30 wt% and 50 wt%. Characterizations were done to evaluate the average TC and properties. Thermal performance evaluation was conducted by analyzing the static charge/discharge cycle. The average TC for paraffin was 0.214 W/m·K. Adding volcanic ash improved the TC to 19.598 W/m·K. It made the charge/discharge performance of the composite better than that of pure paraffin. The charge rate for the composite ranged from 3.83 ℃/min to 5.12 ℃/min. The highest discharge rate was obtained at 4.21 ℃/min for the composite paraffin50/ash50. The freezing temperature for the composite is influenced by the ash proportion, which can be taken as a suitable approach to adjust the freezing point of paraffin-based thermal energy storage (TES). The detailed results for the characterization and thermal performance evaluation are described thoroughly within the article. The overall result indicates that volcanic ash is applicable for improving the TC and charge/discharge rate of paraffin-based TES.
Fractional calculus have recently become a fascinating field of study due to its vast applications in various aspects of modern life. It has been observed that many physical phenomena can be modeled successfully by means of fractional order differential equations, where the integer-order differential equations fails in modeling certain issues [1]. Compared to integer order derivatives some properties of the non-integer order derivatives are very tedious to deal with. Thus, it becomes of great importance to establish more results for fractional calculus. Recently lots of researchers have proposed new and efficient analytical and numerical schemes to approximate the solutions of numerous fractional order problems. In this connection one can find efficient work done by researchers such as the analysis of fractional Drinfeld-Sokolov-Wilson model with exponential memory [2], a homotopy perturbation sumudu transform method (HPSTM) for solving fractional equal width (EW) equation [3]. The ternary-fractional differential transform method, that extends its applicability to encompass initial value problems in the fractal 3D space [1]. The local fractional homotopy perturbation Sumudu transform scheme and the local fractional reduced differential transform method for a fractal vehicular traffic flow problem [4]. The authors in [5] have proposed a numerical algorithm based on homotopic technique to examine the fractional vibration equation in Atangana-Baleanu sense. The authors in [6] have presented the efficiency of the Atangana-Baleanu (AB) derivative over Caputo-Fabrizio (CF) to some nonlinear partial differential equations. The authors in [7] have done a comparative analysis of exothermic reactions model having constant heat source in the porous media via Caputo, Caputo Fabrizio and Atangana-Baleanu theories. In [8] a hybrid numerical scheme based on the homotopy analysis transform method (HATM) to examine the fractional model of nonlinear wave-like equations having variable coefficients is presented. The Klein-Gordon is one of the most important mathematical model which finds its applications in numerous phenomenon in science and engineering. It has been applied to non linear optics, quantum field theory, Plasma physics, fluid dynamics, chemical kinetics and solid state physics [9,10,11]. In literature a lot of work has been done on solving the Klein-Gordon equation analytically some of them are the tanh and the sine-cosine methods [12], the differential transform method [13], Modified Kudryashov method [14,15], ansatz method [16], Exp(−ϕ(ϵ))-expansion method [17], and the variational iteration method [18]. The residual power series method for linear time fractional Klein-Gordon equation [19], homotopy analysis method [20,21], local fractional series expansion method [10], homotopy perturbation method [22], and the fractional Riccati expansion method [23]. In [24] a hybrid method based on local fractional Sumudu transform method and homotopy perturbation technique is employed to find the non differentiable solution of Klein-Gordon equation on Cantor sets. Since Most of the problems cannot be solved analytically so one must use numerical methods. Despite the fact that, numerical approximation of these equations are rare, in literature some excellent work is available, such as Mohebi et al utilized the Compact finite difference method [25] and the implicit RBF meshless method [26] for the approximation of linear time fractional Klein-Gordon equations. M. M. Khader [27] applied an efficient method based on the generalized laguerre polynomials for approximating the linear time fractional Klein-Gordon equations. In [28] the authors used the wavelet method for approximating a class of fractional Klein-Gordon equations. The authors in [29] proposed a numerical algorithm based on the applications of the operational matrices of the Legendre scaling functions for the approximation of fractional Klein-Gordon equation. The authors in [30] applied a high order compact finite difference scheme to two dimensional fractional Klein-Gordon equations. Dehghan et al [31] used radial basis functions to approximate the solution of non linear Klein-Gordon equations. However in these time stepping schemes the computations may be very expansive because each new iteration is dependent on the previous time step. An alternative way is to use the Laplace transform coupled with these numerical methods. In literature one can find numerous research work on the coupling of other numerical methods and Laplace transform. The Laplace transform was first coupled with the boundary integral method by Rizzo and Shippey [32]. Moridis and Reddell coupled Laplace transform with finite difference, boundary element and finite element methods [33,34,35]. In [36] the authors coupled the Galerkin method with Laplace transform. Moridis and Kansa [37] coupled multiquadric method and Laplace transform for the approximation of PDEs. In [38] the author studied RBF method coupled with Laplace transform on unit sphere. Similarly the coupling of Laplace transform with other numerical methods such as spectral method, finite difference method, boundary particle method, RBF method, and the finite element method can be found in [39,40,41,42,43,44] and the references therein. In this work we apply the idea of [45,46], the Laplace transform is coupled with local RBF method to approximate linear time-fractional Klein-Gordon equation. The Laplace transform is used to avoid the stability restrictions, which are commonly encountered in time-stepping procedure. The local radial basis function method is used to resolve the issue of ill-conditioning of the differentiation matrices and the sensitivity of shape parameter in global radial basis functions method. The main idea of the local radial basis function method is the collocation on overlapping sub-domains of the whole domain. The overlapping sub-domains remarkably reduce the size of collocation matrix by solving many small size matrices. Each small matrix has the same size as the number of nodes in the domain of influence of each node. In order to validate our method we consider linear time-fractional Klein-Gordon equation of the form [25]
βα−1∂αχ(x,t)∂tα+η∂χ(x,t)∂t+κχ(x,t)=Lχ(x,t)+βα−1f(x,t),0≤x≤L,1<α≤2,0≤t≤1,η≥0,κ≥0, | (1.1) |
with initial and boundary conditions given in (1.2) and (1.3),
χ(x,0)=f1(x),∂χ(x,t)∂t|t=0=f2(x),x∈Ω, | (1.2) |
Bχ(x,t)=h(t),x∈∂Ω. | (1.3) |
Here L and B are the governing and boundary differential operators, and ∂α∂tα is the Caputo fractional derivative of order α defined by [47]:
∂α∂tαχ(t)=1Γ(p−α)∫t0(t−s)m−α−1dmdsmχ(s)ds,m−1≤α≤m,m∈N. | (1.4) |
Let the Laplace transform of χ(t) be denoted and defined by
ˆχ(s)=L{χ(t)}=∫∞0e−stχ(t)dt, | (1.5) |
and the Laplace transform of the Caputo derivative is defined by
L{∂α∂tαχ(t)}=sαˆχ(s)−m−1∑i=0sα−i−1χ(i)(0). | (1.6) |
Here we construct a local RBF method coupled with Laplace transform for the approximation of the solution of the linear time-fractional Klein-Gordon equations. In order to avoid the time stepping procedure the Laplace transform is used to eliminate the time variable. Then the local RBF method is utilized to approximate the time independent linear PDE.
Applying the Laplace transform to Eqs (1.1) and (1.3), we get
βα−1(sαˆχ(x,s)−sα−1χ(x,0)−sα−2χt(x,0))+η(sˆχ(x,s)−χ(x,0))+κˆχ(x,s)=Lˆχ(x,s)+βα−1ˆf(x,s), | (2.1) |
thus we have the following linear system
(βα−1sαI+ηsI+κI−L)ˆχ(x,s)=ˆg(x,s),x∈Ω, | (2.2) |
Bˆχ(x,s)=h(s),x∈∂Ω, | (2.3) |
where
ˆg(x,s)=βα−1sα−1χ(x,0)+βα−1sα−2χt(x,0)+ηχ(x,0)+βα−1ˆfχ(x,s). |
In the following section the local RBF method is used to approximate the differential operator L and B in order to solve the problem (2.2)–(2.3) in Laplace space.
In local RBF method the approximation of the function ˆχ(x), for a given set of data points {ˆχ(xi):i=1,...,N}, where {xi:i=1,...,N}⊂Ω⊂Rd,d≥1 takes the form
ˆχ(xi)=∑xj∈Ωiλjϕ(‖xi−xj‖), | (2.4) |
where λi={λij:j=1,...,n} is the vector of expansion coefficients, ϕ(r),r≥0 is radial kernel and the distance between the centers xi and xj is r=‖xi−xj‖, and Ωi is a sub domain of Ω containing xi, and around xi it contains n neighboring centers. So we have N number of n×n linear systems given by
^χχi=Φiλi,i=1,2,3,...,N, | (2.5) |
the elements of the interpolation matrix Φi are bikj=ϕ(‖xk−xj‖),wherexk,xj∈Ωi, each n×n system is then solved for the unknowns λi={λij:j=1,...,n}. Next the operator Lˆχ(x), is approximated by
Lˆχ(xi)=∑xj∈ΩiλijLϕ(‖xi−xj‖), | (2.6) |
the above Eq (2.6) can be expressed as
Lˆχ(xi)=λi⋅νi, | (2.7) |
where νi is of order 1×n and λi of order n×1, the entries of νi are shown in the following equation
νi=Lϕ(‖xi−xj‖),xj∈Ωi, | (2.8) |
using Eq (2.5), the coefficients λi can be eliminated as,
λi=(Φi)−1ˆχi, | (2.9) |
using the values of λi from (2.9) in (2.7) we get,
Lˆχ(xi)=νi(Φi)−1ˆχi=wiˆχi | (2.10) |
where,
wi=νi(Φi)−1, | (2.11) |
Hence the linear differential L is approximated using the local RBF method for each center xi as
Lˆχ≡Dˆχ. | (2.12) |
The matrix D is sparse differentiation matrix which approximates the linear differential operator L. The matrix D has order N×N which contains n non-zero and N−n zero entries, where n is the number of centers in the sub domain Ωi. The same procedure can be applied to the boundary operator B.
In literature a large number of radial kernels are available. In this article we have selected the multi-quadrics ϕ(r)=√1+(rc)2 for our numerical approximation. The accuracy of the numerical solution greatly depends on the parameter c. The researchers always search for that value of c which gives an optimal solution. In this regard a large amount of work has been done such as [48,49,50] and references therein. Here we utilize the uncertainty principle [51] for optimal shape parameter c.
Algorithm:
● The interval 1012<Cond<1016 is selected for the condition number (Cond) of the system matrices of the given problem.
● Using SVD, the interpolation matrix is decomposed as R,P,Q=svd(Φi). The order of Φi is n×n (n is the number of centers in each Ωi), and the n singular values of the matrix Φi lies on the diagonal of the matrix P (P is a diagonal matrix), and the condition number of Φi is Cond=‖Φi‖‖(Φi)−1‖=max(P)min(P).
● The c is searched until the condition 1012<Cond<1016 is satisfied, the algorithm is given as
Step 1: set Cond=1
Step 2: select 1012<Cond<1016
Step 3: whileCond>CondmaxandCond<Condmin
Step 4: R,P,Q=svd(Φi)
Step 5: Cond=max(P)min(P)
Step 6: ifCond<Condmin,c=c−δc
Step 7: ifCond>Condmax,c=c+δc
c(optimal)=c.
Optimal value of the parameter c is obtained, when the above condition is satisfied, and then we can compute the inverse using (Φi)−1=(RPQT)−1=QP−1RT [52]. Hence wi in (2.11) can be computed.
Following the discretization by local RBF method of the linear differential and boundary operators L and B respectively, the system (2.2)–(2.3) is solved for each point s. Finally the solution of the problem (1.1)–(1.3) is obtained using the inverse of Laplace transform
χ(x,t)=12πi∫σ+i∞σ−i∞estˆχ(x,s)ds. | (2.13) |
In applying the Laplace transform method the calculation of inverse Laplace transform is the main difficulty. In many cases it is difficult to find the inverse Laplace transform analytically so numerical methods must be used. A large number of methods for the numerical inversion of Laplace transform have been developed. In this work we use the idea of [39,42] in which the integration is performed over a parabolic or hyperbolic path Γ, so the integral in equation (2.13) can be written as
χ(x,t)=12πi∫Γestˆχ(x,s)ds,σ>σ0, | (2.14) |
where Γ is a path of integration joining σ−i∞ to σ+i∞ and
s=s(ω), | (2.15) |
using (2.15) in (2.14), we find the following expression
χ(x,t)=12πi∫∞−∞es(ω)tˆχ(x,s(ω))sˊ | (2.16) |
Finally the trapezoidal rule with uniform step size k is used to approximate (2.16), as
\begin{equation} \chi_{k}({\bf{x}},t) = \frac{k}{2 \pi i}\sum\limits^{M}_{j = -M} e^{s_{j}t}\hat{\chi}({\bf{x}},s_{j})\acute{s}_{j}, \; \; s_{j} = s(\omega_{j}), \omega_{j} = jk. \end{equation} | (2.17) |
The approximate solution of the proposed scheme is defined by Eq (2.17). The accuracy of (2.17) greatly depends on the path of the integration \Gamma . There are various contours available in the literature. Recently the hyperbolic [41] and parabolic [42] contours are used to approximate the integer and fractional order PDEs. In our computations the hyperbolic path due to [41] is used.
\begin{equation} s(\omega) = \eta+\gamma\left(1-sin(\delta-\iota \omega)\right), \; \mbox{for} \; \omega \in\mathcal{R},\; \; \; \; (\Gamma) \end{equation} | (3.1) |
where \eta \geq 0 , \gamma > 0 , \frac{1}{2}\pi < \beta < \pi , and 0 < \delta < \beta - \frac{1}{2}\pi . In fact, when we choose Im \; \omega = \lambda , the Eq (3.1) is reduced to the left branch of the hyperbola
\begin{equation} \left(\frac{x-\gamma-\eta}{\gamma \sin(\delta+\lambda)}\right)^{2}-\left(\frac{y}{\gamma \cos(\delta+\lambda)}\right)^{2} = 1, \end{equation} | (3.2) |
transforming the strip Z_{r} = \{\omega: Im \; \omega \leq r, r > 0\} into the hyperbola \Omega_{r} = \{s: \omega \in Z_{r}\}\supset \Gamma. Suppose \Sigma_{\phi} = \{s \neq 0 :|arg s|\leq\phi \} \cup 0, \; 0 < \phi < \frac{(1-\alpha)\phi}{2}, and let \Sigma^{\eta}_{\beta} = \eta+\Sigma_{\beta}, \Gamma\subset \Omega_{r}\subset \Sigma^{\eta}_{\beta}. The following theorem gives the error estimate of the scheme for the contour \Gamma .
Theorem 3.1 ([41], Theorem 2.1) let the solution of (1.1) be \chi({\bf{x}}, t) , with \hat{f}({\bf{x}}, t) analyitc in \Sigma^{\eta}_{\beta}. Let \Gamma\subset \Omega_{r}\subset \Sigma^{\eta}_{\beta}, and b > 0 be defined by b = cosh^{-1}(\frac{1}{\theta \tau \sin(\delta)}) , where \tau = \frac{t_0}{T} , 0 < \theta < 1 , 0 < t_0 < T , and let \gamma = \frac{\theta \overline{r}M}{bT}. Then for the approximate solution defined by (2.17), with k = \frac{b}{M}\leq \frac{\overline{r}}{log 2}, \; |\chi({\bf{x}}, t)-\chi_{k}({\bf{x}}, t)|\leq \left(\|\chi_{0}\|+\|\hat{f}({\bf{x}}, t)\|_{\Sigma^{\eta}_{\beta}}\right)CQe^{\eta \tau}g(\rho_{r}M)e^{-\mu M}, for \mu = \frac{\overline{r}(1-\theta)}{b} , \rho_r = \frac{\theta \overline{r} \tau \sin(\delta-r)}{b} , g(x) = \mbox{max}(1, log(\frac{1}{x})) , \overline{r} = 2\pi r , r > 0 , C = C_{\delta, r, \beta} , and t_0\leq t \leq T. Thus the corresponding error estimate is of the order
\text{Error Estimate} = |\chi({\bf{x}},t)-\chi_{k}({\bf{x}},t)| = O(g(\rho_{r}M)e^{-\mu M}). |
In order to investigate the systems (2.2)–(2.3) stability, we represent the system in discrete form as
\begin{equation} Y{\bf{\hat{ \pmb{\mathsf{ χ}}}}} = {\bf{b}}, \end{equation} | (4.1) |
where Y is the sparse differentiation matrix of order N \times N obtained using local RBF method. For the system (4.1) the constant of stability is given by
\begin{equation} C = \sup\limits_{\hat{\chi}\neq0} \frac{\|\hat{\chi}\|}{\|Y\hat{\chi}\|}, \end{equation} | (4.2) |
where C is finite using any discrete norm \|.\| on R^{N} . From (4.2) we may write
\begin{equation} \|Y\|^{-1} \leq \frac{\|\hat{\chi}\|}{\|Y\hat{\chi}\| }\leq C, \end{equation} | (4.3) |
Similarly for the pseudoinverse Y^{†} of Y , we can write
\begin{equation} \|Y^{†}\| = \sup\limits_{v \neq 0} \frac{\|Y^{†} v\|}{\|v\|}. \end{equation} | (4.4) |
Thus we have
\begin{equation} \|Y^{†}\| \geq \sup\limits_{v = Y\hat{\chi}\neq 0}\frac{\|Y^{†}Y\hat{\chi}\| }{\|Y\hat{\chi}\| } = \sup\limits_{\hat{\chi} \neq 0} \frac{\|\hat{\chi}\| }{\|Y\hat{\chi}\| } = C. \end{equation} | (4.5) |
We can see that Eqs (4.3) and (4.5) confirms the bounds for the stability constant C . Calculating the pseudoinverse for approximating the system (4.1) numerically may be very expansive computationally, but it ensures the stability. The MATLAB's function condest can be used to estimate \|Y^{-1}\|_{\infty} in case of square systems, thus we have
\begin{equation} C = \frac{condest(Y')}{\|Y\|_{\infty}} \end{equation} | (4.6) |
This work well with less number of computations for our sparse differentiation matrix Y . Figures 1 and 2 show the bounds for the constant C of our system (2.2)–(2.3) for Problem 3. Selecting N = 50 , M = 80 , n = 15 , and \alpha = 0.8 at t = 1 , we have 1 \leq C \leq 1.1620. It is observed that the stability constant is bounded by very small numbers, which guarantees the stability of the proposed local RBF scheme.
This section is devoted to the numerical experiments. The proposed method is tested here for 1-D time fractional order Klein-Gordon equations. The multi-quadrics radial kernels \phi (r) = (1+(r c)^2)^{1/2} are used in all our numerical experiments. The Uncertainty principle [51] is used to optimize the shape parameter c . The accuracy of the method is measured using L_{\infty} error defined by
L_{\infty} = \|\chi({\bf{x}},t)-\chi_{k}({\bf{x}},t)\|_{\infty} = \max\limits_{1 \leq j \leq N}(|\chi({\bf{x}},t)-\chi_{k}({\bf{x}},t)|) |
is used. Here \chi_{k} and \chi are the numerical and exact solutions respectively.
If we use \beta = 1 , \kappa = 1 , and \eta = 0, Eq (1.1) takes the form
\begin{equation} \frac{\partial^{\alpha}\chi(x,t)}{\partial t^{\alpha}}+\chi(x,t)- \frac{\partial^{2}\chi(x,t)}{\partial x^{2}} = f(x,t), \end{equation} | (5.1) |
where \; 1\leq \alpha \leq2, \; t\geq 0, \; 0\leq x\leq1, with zero boundary and initial conditions. The domain [0, 1] is selected for the problem with exact solution
\chi(x,t) = t^{2}(e-e^{x})\sin(x), |
and non homogeneous term
\begin{eqnarray*} f(x,t)& = &\frac{2t^{2-\alpha}}{(2-\alpha)\Gamma(2-\alpha)}(e-e^{x})\sin(x)+t^{2}(2e-e^{x})\sin(x)\\&&+2t^{2}e^{x}\cos(x). \end{eqnarray*} |
The MATLAB's command \omega = -M:k:M is used to generate the quadrature points along the path of integration \Gamma . The parameters used in our computations are \alpha = 1.75, \eta = 2, \tau = \frac{t0}{T}, r = 0.1387, \theta = 0.1, \delta = 0.1541, t_0 = 0.5 \; \mbox{and}\; T = 5. Using Eq (3.1) the remaining optimal parameters can be found for the hyperbolic path \Gamma . In our computations n = 6 in the sub domain \Omega_{i} and N = 40 in the global domain \Omega are selected. The error estimates and L_{\infty} errors are shown in Tables 1 and 2. The efficiency of the method can be seen in the results. The actual error and error estimates are shown in Figure 3 and the absolute errors for different values of \alpha are shown in Figure 4. The numerical and the exact solutions are shown in Figures 5 and 6 respectively.
N=60 , n=5 \alpha=1.25 |
M | L_{\infty} Error (\Gamma) | Error Estimate (\Gamma) | CPU time(s) |
10 | 7.65 \times 10^{-4} | 4.4187 | 0.145896 | |
15 | 2.30 \times 10^{-3} | 2.6363 | 0.158580 | |
20 | 1.30 \times 10^{-3} | 1.5582 | 0.169243 | |
30 | 1.38 \times 10^{-4} | 0.5373 | 0.218606 | |
40 | 6.57 \times 10^{-6} | 0.1836 | 0.384568 | |
50 | 1.25 \times 10^{-5} | 0.0625 | 0.682311 | |
60 | 9.58 \times 10^{-6} | 0.0212 | 1.143210 | |
70 | 9.70 \times 10^{-6} | 0.0072 | 2.792846 | |
80 | 9.66 \times 10^{-6} | 0.0024 | 5.805704 | |
[25] 1.34 \times 10^{-6} |
N=60 , n=5 \alpha=1.75 |
M | L_{\infty} Error (\Gamma) | Error Estimate (\Gamma) | CPU time(s) |
10 | 7.65 \times 10^{-4} | 4.4187 | 0.151320 | |
15 | 2.30 \times 10^{-3} | 2.6363 | 0.190760 | |
20 | 1.30 \times 10^{-3} | 1.5582 | 0.173974 | |
30 | 1.38 \times 10^{-4} | 0.5373 | 0.275586 | |
40 | 6.35 \times 10^{-6} | 0.1836 | 0.483761 | |
50 | 1.19 \times 10^{-5} | 0.0625 | 0.732991 | |
60 | 8.99 \times 10^{-6} | 0.0212 | 1.269992 | |
70 | 9.11 \times 10^{-6} | 0.0072 | 3.328360 | |
80 | 9.07 \times 10^{-6} | 0.0024 | 5.789626 | |
[25] 4.45 \times 10^{-5} |
If we use \beta = 1 , \kappa = 1 , and \eta = 1, Eq (1.1) takes the form
\begin{equation} \frac{\partial^{\alpha}\chi(x,t)}{\partial t^{\alpha}}+\frac{\partial \chi(x,t)}{\partial t}+\chi(x,t) = \frac{\partial^{2}\chi(x,t)}{\partial x^{2}}+f(x,t), \end{equation} | (5.2) |
where \; 1\leq \alpha \leq2, \; t\geq 0, \; 0\leq x\leq1, with zero initial and boundary conditions, the exact solution of the problem is
\chi(x,t) = t^{2}x\sin(x-1), |
and non homogeneous term is
\begin{eqnarray*} &&f(x,t) = \frac{2t^{2-\alpha}}{(2-\alpha)\Gamma(2-\alpha)}x\sin(x-1)+2tx\sin(x-1)\\&&+t^{2}x\sin(x-1)-t^{2}(2\cos(x-1)-x\sin(x-1)). \end{eqnarray*} |
The MATLAB's command \omega = -M:k:M is used to generate the quadrature points along the path of integration \Gamma . The parameters used in our computations are \alpha = 1.75, r = 0.1387, \delta = 0.1541, \theta = 0.1, \tau = \frac{t0}{T}, \eta = 2, t_0 = 0.5 \; \mbox{and}\; T = 5. Using Eq (3.1) the remaining optimal parameters can be found for the hyperbolic path \Gamma . In our computations n = 7 centers in the sub domain \Omega_{i} and N = 50 in the global domain \Omega are selected. The error estimates and L_{\infty} errors are shown in Tables 3 and 4. Also the maximum absolute errors for different values of \alpha are shown in Table 5, which shows the efficiency of the proposed method. The numerical and exact solutions of this problem are shown in Figures 7 and 8 respectively and plot of Actual error and Error Estimate corresponding to problem 2 are shown in Figure 9.
M=80 , n=5 \alpha=1.25 |
N | L_{\infty} Error (\Gamma) | Error Estimate (\Gamma) | CPU time(s) |
10 | 5.77 \times 10^{-5} | 0.0024 | 0.561563 | |
20 | 1.27 \times 10^{-5} | 0.0024 | 1.125699 | |
30 | 3.55 \times 10^{-6} | 0.0024 | 1.252799 | |
40 | 2.43 \times 10^{-6} | 0.0024 | 2.716533 | |
50 | 2.87 \times 10^{-6} | 0.0024 | 4.686349 | |
60 | 3.78 \times 10^{-6} | 0.0024 | 6.319554 | |
80 | 8.38 \times 10^{-6} | 0.0024 | 8.773851 | |
90 | 8.20 \times 10^{-7} | 0.0024 | 9.862299 | |
[25] 5.91 \times 10^{-7} |
N=50 , n=7 \alpha=1.75 |
M | L_{\infty} Error (\Gamma) | Error Estimate (\Gamma) | CPU time(s) |
10 | 3.32 \times 10^{-4} | 4.4187 | 0.146540 | |
15 | 9.63 \times 10^{-4} | 2.6363 | 0.160951 | |
20 | 5.71 \times 10^{-4} | 1.5582 | 0.170815 | |
30 | 6.70 \times 10^{-5} | 0.5373 | 0.212776 | |
40 | 7.76 \times 10^{-6} | 0.1836 | 0.361477 | |
50 | 4.25 \times 10^{-6} | 0.0625 | 0.585600 | |
60 | 5.48 \times 10^{-6} | 0.0212 | 1.047157 | |
70 | 5.42 \times 10^{-6} | 0.0072 | 1.872323 | |
80 | 5.44 \times 10^{-6} | 0.0024 | 4.417500 | |
[25] 7.59 \times 10^{-6} |
x | \alpha=1.25 | \alpha=1.5 | \alpha=1.75 | \alpha=1.95 |
0 | 1.463 \times 10^{-6} | 1.463 \times 10^{-6} | 1.463 \times 10^{-6} | 1.463 \times 10^{-6} |
0.1 | 1.353 \times 10^{-6} | 1.340 \times 10^{-6} | 1.326 \times 10^{-6} | 1.315 \times 10^{-6} |
0.2 | 1.155 \times 10^{-6} | 1.131 \times 10^{-6} | 1.104 \times 10^{-6} | 1.079 \times 10^{-6} |
0.3 | 9.710 \times 10^{-7} | 9.400 \times 10^{-7} | 9.010 \times 10^{-7} | 8.630 \times 10^{-7} |
0.4 | 8.170 \times 10^{-7} | 7.820 \times 10^{-7} | 7.360 \times 10^{-7} | 6.850 \times 10^{-7} |
0.5 | 6.760 \times 10^{-7} | 6.410 \times 10^{-7} | 5.910 \times 10^{-7} | 5.320 \times 10^{-7} |
0.6 | 5.180 \times 10^{-7} | 4.860 \times 10^{-7} | 4.370 \times 10^{-7} | 3.740 \times 10^{-7} |
0.7 | 3.510 \times 10^{-7} | 3.240 \times 10^{-7} | 2.830 \times 10^{-7} | 2.220 \times 10^{-7} |
0.8 | 1.620 \times 10^{-7} | 1.430 \times 10^{-7} | 1.130 \times 10^{-7} | 6.200 \times 10^{-8} |
0.9 | 1.300 \times 10^{-8} | 2.300 \times 10^{-8} | 3.900 \times 10^{-8} | 6.800 \times 10^{-8} |
1 | 3.590 \times 10^{-7} | 3.590 \times 10^{-7} | 3.590 \times 10^{-7} | 3.590 \times 10^{-7} |
Here we consider the 1-D linear Klein-Gordon equation of the form [19]
\begin{equation} \frac{\partial^{\alpha}\chi(x,t)}{\partial t^{\alpha}} = \frac{\partial^{2}\chi(x,t)}{\partial x^{2}}+\chi(x,t), \; 0\leq \alpha \leq1,\; t\geq 0, \; x\in R, \end{equation} | (5.3) |
with initial condition \chi(x, 0) = 1+\sin(x) and exact solution \chi(x, t) = \sin(x)+E_{\alpha}(t^{\alpha}) , where E_{\alpha}(t) = \sum^{\infty}_{m = 0}\frac{t^{m}}{\Gamma(\alpha m+1)}. The domain [-4, 4] is selected for the given problem. The quadrature points are generated using the MATLAB's command \omega = -M:k:M along the path of integration \Gamma . The parameters used in our computations are \alpha = 0.8, r = 0.1387, \eta = 2, \tau = \frac{t0}{T}, \theta = 0.1, \delta = 0.1541, t_0 = 0.5 \; \mbox{and}\; T = 5. Using Eq (3.1) the remaining optimal parameters can be found for the hyperbolic path \Gamma . In our computations we select n = 6 centers in the sub domain \Omega_{i} and N = 40 in the global domain \Omega are selected. The error estimates and L_{\infty} errors are shown in Tables 6 and 7. Similar behavior is observed as in the previous examples. The numerical and exact solutions for problem 3 are shown in Figures 10 and 11 and plot of Actual error and Error Estimate corresponding to problem 3 are shown in Figure 12.
N=70 , n=10 , \alpha=0.25 |
M | L_{\infty} Error (\Gamma) | Error Estimate (\Gamma) | CPU time(s) |
10 | 7.37 \times 10^{0} | 4.4187 | 0.168655 | |
20 | 4.14 \times 10^{-1} | 1.5582 | 0.216721 | |
30 | 3.13 \times 10^{-1} | 0.5373 | 0.268500 | |
40 | 9.80 \times 10^{-3} | 0.1836 | 0.352215 | |
50 | 1.49 \times 10^{-2} | 0.0625 | 0.480307 | |
60 | 2.60 \times 10^{-3} | 0.0212 | 0.899249 | |
70 | 8.67 \times 10^{-4} | 0.0072 | 2.037757 | |
80 | 8.90 \times 10^{-4} | 0.0024 | 3.956089 | |
90 | 8.12 \times 10^{-4} | 8.18 \times 10^{-4} | 6.517429 |
N=40 , n=6 , \alpha=0.8 |
M | L_{\infty} Error (\Gamma) | Error Estimate (\Gamma) | CPU time(s) |
10 | 2.68 \times 10^{0} | 4.4187 | 0.158384 | |
15 | 4.53 \times 10^{-1} | 2.6363 | 0.162534 | |
20 | 3.36 \times 10^{-1} | 1.5582 | 0.162535 | |
30 | 1.59 \times 10^{-1} | 0.5373 | 0.189903 | |
40 | 2.0 \times 10^{-3} | 0.1836 | 0.245566 | |
50 | 8.70 \times 10^{-3} | 0.0625 | 0.344221 | |
60 | 1.10 \times 10^{-3} | 0.0212 | 0.502084 | |
70 | 6.32 \times 10^{-4} | 0.0072 | 0.923548 | |
80 | 5.70 \times 10^{-4} | 0.0024 | 2.520403 |
In this article, we constructed a local RBF method based on Laplace transform proposed for the approximation of the solution of the linear time fractional Klein-Gordon equations. In time stepping procedure usually the time instability is encountered and for accuracy we need a very small time step size. Global RBF methods are efficient and accurate only for small amount of nodes. They become inefficient and the differentiation matrix becomes ill-conditioned for large amount of nodes. The main advantage of this method is that it avoids the time stepping procedure with the help of Laplace transform, and the local RBF method has been used to resolve the issue of ill-conditioning. The numerical results confirmed the stability and convergence of the method. The comparison of the results with other methods led us to conclude that the proposed local RBF method coupled with Laplace transform is an efficient method for approximation of the solution of the linear time fractional Klein-Gordon equations.
The authors wish to thank the referees for their careful reading of the manuscript and valuable suggestions.This work was supported in part by the National Key Research and Development Program under Grant 2018YFB0904205, in part by the Key Laboratory of Pattern Recognition and Intelligent Information Processing, Institutions of Higher Education of Sichuan Province under Grant MSSB-2020-12.
The authors declare that no competing interests exist.
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N=60 , n=5 \alpha=1.25 |
M | L_{\infty} Error (\Gamma) | Error Estimate (\Gamma) | CPU time(s) |
10 | 7.65 \times 10^{-4} | 4.4187 | 0.145896 | |
15 | 2.30 \times 10^{-3} | 2.6363 | 0.158580 | |
20 | 1.30 \times 10^{-3} | 1.5582 | 0.169243 | |
30 | 1.38 \times 10^{-4} | 0.5373 | 0.218606 | |
40 | 6.57 \times 10^{-6} | 0.1836 | 0.384568 | |
50 | 1.25 \times 10^{-5} | 0.0625 | 0.682311 | |
60 | 9.58 \times 10^{-6} | 0.0212 | 1.143210 | |
70 | 9.70 \times 10^{-6} | 0.0072 | 2.792846 | |
80 | 9.66 \times 10^{-6} | 0.0024 | 5.805704 | |
[25] 1.34 \times 10^{-6} |
N=60 , n=5 \alpha=1.75 |
M | L_{\infty} Error (\Gamma) | Error Estimate (\Gamma) | CPU time(s) |
10 | 7.65 \times 10^{-4} | 4.4187 | 0.151320 | |
15 | 2.30 \times 10^{-3} | 2.6363 | 0.190760 | |
20 | 1.30 \times 10^{-3} | 1.5582 | 0.173974 | |
30 | 1.38 \times 10^{-4} | 0.5373 | 0.275586 | |
40 | 6.35 \times 10^{-6} | 0.1836 | 0.483761 | |
50 | 1.19 \times 10^{-5} | 0.0625 | 0.732991 | |
60 | 8.99 \times 10^{-6} | 0.0212 | 1.269992 | |
70 | 9.11 \times 10^{-6} | 0.0072 | 3.328360 | |
80 | 9.07 \times 10^{-6} | 0.0024 | 5.789626 | |
[25] 4.45 \times 10^{-5} |
M=80 , n=5 \alpha=1.25 |
N | L_{\infty} Error (\Gamma) | Error Estimate (\Gamma) | CPU time(s) |
10 | 5.77 \times 10^{-5} | 0.0024 | 0.561563 | |
20 | 1.27 \times 10^{-5} | 0.0024 | 1.125699 | |
30 | 3.55 \times 10^{-6} | 0.0024 | 1.252799 | |
40 | 2.43 \times 10^{-6} | 0.0024 | 2.716533 | |
50 | 2.87 \times 10^{-6} | 0.0024 | 4.686349 | |
60 | 3.78 \times 10^{-6} | 0.0024 | 6.319554 | |
80 | 8.38 \times 10^{-6} | 0.0024 | 8.773851 | |
90 | 8.20 \times 10^{-7} | 0.0024 | 9.862299 | |
[25] 5.91 \times 10^{-7} |
N=50 , n=7 \alpha=1.75 |
M | L_{\infty} Error (\Gamma) | Error Estimate (\Gamma) | CPU time(s) |
10 | 3.32 \times 10^{-4} | 4.4187 | 0.146540 | |
15 | 9.63 \times 10^{-4} | 2.6363 | 0.160951 | |
20 | 5.71 \times 10^{-4} | 1.5582 | 0.170815 | |
30 | 6.70 \times 10^{-5} | 0.5373 | 0.212776 | |
40 | 7.76 \times 10^{-6} | 0.1836 | 0.361477 | |
50 | 4.25 \times 10^{-6} | 0.0625 | 0.585600 | |
60 | 5.48 \times 10^{-6} | 0.0212 | 1.047157 | |
70 | 5.42 \times 10^{-6} | 0.0072 | 1.872323 | |
80 | 5.44 \times 10^{-6} | 0.0024 | 4.417500 | |
[25] 7.59 \times 10^{-6} |
x | \alpha=1.25 | \alpha=1.5 | \alpha=1.75 | \alpha=1.95 |
0 | 1.463 \times 10^{-6} | 1.463 \times 10^{-6} | 1.463 \times 10^{-6} | 1.463 \times 10^{-6} |
0.1 | 1.353 \times 10^{-6} | 1.340 \times 10^{-6} | 1.326 \times 10^{-6} | 1.315 \times 10^{-6} |
0.2 | 1.155 \times 10^{-6} | 1.131 \times 10^{-6} | 1.104 \times 10^{-6} | 1.079 \times 10^{-6} |
0.3 | 9.710 \times 10^{-7} | 9.400 \times 10^{-7} | 9.010 \times 10^{-7} | 8.630 \times 10^{-7} |
0.4 | 8.170 \times 10^{-7} | 7.820 \times 10^{-7} | 7.360 \times 10^{-7} | 6.850 \times 10^{-7} |
0.5 | 6.760 \times 10^{-7} | 6.410 \times 10^{-7} | 5.910 \times 10^{-7} | 5.320 \times 10^{-7} |
0.6 | 5.180 \times 10^{-7} | 4.860 \times 10^{-7} | 4.370 \times 10^{-7} | 3.740 \times 10^{-7} |
0.7 | 3.510 \times 10^{-7} | 3.240 \times 10^{-7} | 2.830 \times 10^{-7} | 2.220 \times 10^{-7} |
0.8 | 1.620 \times 10^{-7} | 1.430 \times 10^{-7} | 1.130 \times 10^{-7} | 6.200 \times 10^{-8} |
0.9 | 1.300 \times 10^{-8} | 2.300 \times 10^{-8} | 3.900 \times 10^{-8} | 6.800 \times 10^{-8} |
1 | 3.590 \times 10^{-7} | 3.590 \times 10^{-7} | 3.590 \times 10^{-7} | 3.590 \times 10^{-7} |
N=70 , n=10 , \alpha=0.25 |
M | L_{\infty} Error (\Gamma) | Error Estimate (\Gamma) | CPU time(s) |
10 | 7.37 \times 10^{0} | 4.4187 | 0.168655 | |
20 | 4.14 \times 10^{-1} | 1.5582 | 0.216721 | |
30 | 3.13 \times 10^{-1} | 0.5373 | 0.268500 | |
40 | 9.80 \times 10^{-3} | 0.1836 | 0.352215 | |
50 | 1.49 \times 10^{-2} | 0.0625 | 0.480307 | |
60 | 2.60 \times 10^{-3} | 0.0212 | 0.899249 | |
70 | 8.67 \times 10^{-4} | 0.0072 | 2.037757 | |
80 | 8.90 \times 10^{-4} | 0.0024 | 3.956089 | |
90 | 8.12 \times 10^{-4} | 8.18 \times 10^{-4} | 6.517429 |
N=40 , n=6 , \alpha=0.8 |
M | L_{\infty} Error (\Gamma) | Error Estimate (\Gamma) | CPU time(s) |
10 | 2.68 \times 10^{0} | 4.4187 | 0.158384 | |
15 | 4.53 \times 10^{-1} | 2.6363 | 0.162534 | |
20 | 3.36 \times 10^{-1} | 1.5582 | 0.162535 | |
30 | 1.59 \times 10^{-1} | 0.5373 | 0.189903 | |
40 | 2.0 \times 10^{-3} | 0.1836 | 0.245566 | |
50 | 8.70 \times 10^{-3} | 0.0625 | 0.344221 | |
60 | 1.10 \times 10^{-3} | 0.0212 | 0.502084 | |
70 | 6.32 \times 10^{-4} | 0.0072 | 0.923548 | |
80 | 5.70 \times 10^{-4} | 0.0024 | 2.520403 |
N=60 , n=5 \alpha=1.25 |
M | L_{\infty} Error (\Gamma) | Error Estimate (\Gamma) | CPU time(s) |
10 | 7.65 \times 10^{-4} | 4.4187 | 0.145896 | |
15 | 2.30 \times 10^{-3} | 2.6363 | 0.158580 | |
20 | 1.30 \times 10^{-3} | 1.5582 | 0.169243 | |
30 | 1.38 \times 10^{-4} | 0.5373 | 0.218606 | |
40 | 6.57 \times 10^{-6} | 0.1836 | 0.384568 | |
50 | 1.25 \times 10^{-5} | 0.0625 | 0.682311 | |
60 | 9.58 \times 10^{-6} | 0.0212 | 1.143210 | |
70 | 9.70 \times 10^{-6} | 0.0072 | 2.792846 | |
80 | 9.66 \times 10^{-6} | 0.0024 | 5.805704 | |
[25] 1.34 \times 10^{-6} |
N=60 , n=5 \alpha=1.75 |
M | L_{\infty} Error (\Gamma) | Error Estimate (\Gamma) | CPU time(s) |
10 | 7.65 \times 10^{-4} | 4.4187 | 0.151320 | |
15 | 2.30 \times 10^{-3} | 2.6363 | 0.190760 | |
20 | 1.30 \times 10^{-3} | 1.5582 | 0.173974 | |
30 | 1.38 \times 10^{-4} | 0.5373 | 0.275586 | |
40 | 6.35 \times 10^{-6} | 0.1836 | 0.483761 | |
50 | 1.19 \times 10^{-5} | 0.0625 | 0.732991 | |
60 | 8.99 \times 10^{-6} | 0.0212 | 1.269992 | |
70 | 9.11 \times 10^{-6} | 0.0072 | 3.328360 | |
80 | 9.07 \times 10^{-6} | 0.0024 | 5.789626 | |
[25] 4.45 \times 10^{-5} |
M=80 , n=5 \alpha=1.25 |
N | L_{\infty} Error (\Gamma) | Error Estimate (\Gamma) | CPU time(s) |
10 | 5.77 \times 10^{-5} | 0.0024 | 0.561563 | |
20 | 1.27 \times 10^{-5} | 0.0024 | 1.125699 | |
30 | 3.55 \times 10^{-6} | 0.0024 | 1.252799 | |
40 | 2.43 \times 10^{-6} | 0.0024 | 2.716533 | |
50 | 2.87 \times 10^{-6} | 0.0024 | 4.686349 | |
60 | 3.78 \times 10^{-6} | 0.0024 | 6.319554 | |
80 | 8.38 \times 10^{-6} | 0.0024 | 8.773851 | |
90 | 8.20 \times 10^{-7} | 0.0024 | 9.862299 | |
[25] 5.91 \times 10^{-7} |
N=50 , n=7 \alpha=1.75 |
M | L_{\infty} Error (\Gamma) | Error Estimate (\Gamma) | CPU time(s) |
10 | 3.32 \times 10^{-4} | 4.4187 | 0.146540 | |
15 | 9.63 \times 10^{-4} | 2.6363 | 0.160951 | |
20 | 5.71 \times 10^{-4} | 1.5582 | 0.170815 | |
30 | 6.70 \times 10^{-5} | 0.5373 | 0.212776 | |
40 | 7.76 \times 10^{-6} | 0.1836 | 0.361477 | |
50 | 4.25 \times 10^{-6} | 0.0625 | 0.585600 | |
60 | 5.48 \times 10^{-6} | 0.0212 | 1.047157 | |
70 | 5.42 \times 10^{-6} | 0.0072 | 1.872323 | |
80 | 5.44 \times 10^{-6} | 0.0024 | 4.417500 | |
[25] 7.59 \times 10^{-6} |
x | \alpha=1.25 | \alpha=1.5 | \alpha=1.75 | \alpha=1.95 |
0 | 1.463 \times 10^{-6} | 1.463 \times 10^{-6} | 1.463 \times 10^{-6} | 1.463 \times 10^{-6} |
0.1 | 1.353 \times 10^{-6} | 1.340 \times 10^{-6} | 1.326 \times 10^{-6} | 1.315 \times 10^{-6} |
0.2 | 1.155 \times 10^{-6} | 1.131 \times 10^{-6} | 1.104 \times 10^{-6} | 1.079 \times 10^{-6} |
0.3 | 9.710 \times 10^{-7} | 9.400 \times 10^{-7} | 9.010 \times 10^{-7} | 8.630 \times 10^{-7} |
0.4 | 8.170 \times 10^{-7} | 7.820 \times 10^{-7} | 7.360 \times 10^{-7} | 6.850 \times 10^{-7} |
0.5 | 6.760 \times 10^{-7} | 6.410 \times 10^{-7} | 5.910 \times 10^{-7} | 5.320 \times 10^{-7} |
0.6 | 5.180 \times 10^{-7} | 4.860 \times 10^{-7} | 4.370 \times 10^{-7} | 3.740 \times 10^{-7} |
0.7 | 3.510 \times 10^{-7} | 3.240 \times 10^{-7} | 2.830 \times 10^{-7} | 2.220 \times 10^{-7} |
0.8 | 1.620 \times 10^{-7} | 1.430 \times 10^{-7} | 1.130 \times 10^{-7} | 6.200 \times 10^{-8} |
0.9 | 1.300 \times 10^{-8} | 2.300 \times 10^{-8} | 3.900 \times 10^{-8} | 6.800 \times 10^{-8} |
1 | 3.590 \times 10^{-7} | 3.590 \times 10^{-7} | 3.590 \times 10^{-7} | 3.590 \times 10^{-7} |
N=70 , n=10 , \alpha=0.25 |
M | L_{\infty} Error (\Gamma) | Error Estimate (\Gamma) | CPU time(s) |
10 | 7.37 \times 10^{0} | 4.4187 | 0.168655 | |
20 | 4.14 \times 10^{-1} | 1.5582 | 0.216721 | |
30 | 3.13 \times 10^{-1} | 0.5373 | 0.268500 | |
40 | 9.80 \times 10^{-3} | 0.1836 | 0.352215 | |
50 | 1.49 \times 10^{-2} | 0.0625 | 0.480307 | |
60 | 2.60 \times 10^{-3} | 0.0212 | 0.899249 | |
70 | 8.67 \times 10^{-4} | 0.0072 | 2.037757 | |
80 | 8.90 \times 10^{-4} | 0.0024 | 3.956089 | |
90 | 8.12 \times 10^{-4} | 8.18 \times 10^{-4} | 6.517429 |
N=40 , n=6 , \alpha=0.8 |
M | L_{\infty} Error (\Gamma) | Error Estimate (\Gamma) | CPU time(s) |
10 | 2.68 \times 10^{0} | 4.4187 | 0.158384 | |
15 | 4.53 \times 10^{-1} | 2.6363 | 0.162534 | |
20 | 3.36 \times 10^{-1} | 1.5582 | 0.162535 | |
30 | 1.59 \times 10^{-1} | 0.5373 | 0.189903 | |
40 | 2.0 \times 10^{-3} | 0.1836 | 0.245566 | |
50 | 8.70 \times 10^{-3} | 0.0625 | 0.344221 | |
60 | 1.10 \times 10^{-3} | 0.0212 | 0.502084 | |
70 | 6.32 \times 10^{-4} | 0.0072 | 0.923548 | |
80 | 5.70 \times 10^{-4} | 0.0024 | 2.520403 |