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Article

On Unconditionally Stable New Modified Fractional Group Iterative Scheme for the Solution of 2D Time-Fractional Telegraph Model

1
Department of Mathematics, Virtual University of Pakistan, Lahore 54000, Pakistan
2
Department of Mathematics and General Sciences, Prince Sultan University, Riyadh 11586, Saudi Arabia
3
Department of Medical Research, China Medical University, Taichung 40402, Taiwan
4
Mathematics and Natural Sciences, Prince Mohammad Bin Fahd University, Al Khobar 31952, Saudi Arabia
5
School of Mathematical Sciences, Universiti Sains Malaysia, Gelugor 11800, Malaysia
6
Department of Mathematics, University of Sargodha, Sargodha 40100, Pakistan
*
Authors to whom correspondence should be addressed.
Symmetry 2021, 13(11), 2078; https://doi.org/10.3390/sym13112078
Submission received: 29 September 2021 / Revised: 20 October 2021 / Accepted: 21 October 2021 / Published: 3 November 2021
(This article belongs to the Special Issue Recent Advances in Number Theory and Their Applications)

Abstract

:
In this study, a new modified group iterative scheme for solving the two-dimensional (2D) fractional hyperbolic telegraph differential equation with Dirichlet boundary conditions is obtained from the 2h-spaced standard and rotated Crank–Nicolson FD approximations. The findings of new four-point modified explicit group relaxation method demonstrates the rapid rate of convergence of proposed method as compared to the existing schemes. Numerical tests are performed to test the capability of the group iterative scheme in comparison with the point iterative scheme counterparts. The stability of the derived modified group method is proven by the matrix norm algorithm. The obtained results are tabulated and concluded that exact solutions are exactly symmetric with approximate solutions.

1. Introduction

Partial differential equations have a wide range of applications in applied sciences, including wave propagation, electric signal propagation, and atomic physics [1,2,3,4,5]. In recent years, several numerical techniques for multidimensional hyperbolic partial differential equations have been developed [6,7,8,9,10,11]. For example, Gao and Chi [12] solved one-space-dimensional linear hyperbolic model based on unconditionally stable difference schemes. Youssef [13] studied the class of fractional functional integro-differential equations of the Caputo–Katugampola type. Many techniques have been used to solve fractional partial differential equations using the Caputo and the Caputo–Fabrizio type operators [14,15,16]. Lai and Liu [17] solved the second order fractional partial differential equation using the Galerkin finite element method and Riesz fractional derivative. Akram et al. [18,19] proposed unconditionally stable methods for the fractional hyperbolic models via B-spline approaches. Several years before this, the unconditionally stable alternating dimension implicit schemes for 2D and three-dimensional hyperbolic equations were derived by Mohanty and Jain [20,21]. Later, Mohanty [22] also proposed new difference approach for the solution of telegraphic equation. Meanwhile, Dehghan and Mehebbi [23,24] suggested numerical approaches for 2D linear hyperbolic equations by applying collocation finite difference (FD) approximations. The other derived numerical schemes for hyperbolic partial differential equations can be seen in [25,26].
Most of the researchers discretized their presented issues using various types of discretization techniques such as the FD approach [27], the finite element scheme [28], and the boundary element approach [29], among others. A sparse system of linear equations is obtained in the following form:
A υ = b .
Iterative approaches are ideal for solving this sparse system of linear equations in this case. These iterative methods utilized all of the grid points in the solution domain Ω h , ( h is grid spacing in both x and y direction) including the boundary points to achieve the convergence. Due to the involvement of all the grid knots in the suggested domain Ω h , these methods are forced to utilize a lot of algebraic operations in the iterative loop that resulted in large computational complexities and consume more execution time per iteration for their evaluation.
A number of studies on iterative schemes have been presented to improve the convergence rate in solving Equation (1). One of them is the establishment of the group iterative algorithms capable of reducing iterative process convergence times. We divide the entire domain into groups of knots, and values on each group are explicitly assessed using properly stated FD formulas that reduce the overall amount of arithmetic operations. Evans [30] used the Explicit Group (EG) iterative method to solve the Poisson problem by creating a 4-point block iterative scheme. Evans and Yousif [31,32], Evans and Sahimi [33], Evans and Hasan [11] and Kew and Ali [10] have extensively researched a range of EG iterative techniques for various forms of partial differential equations based on this idea. In addition, another type of group iterative method based on the half-sweep technique called Explicit Decoupled Group (EDG) approach is presented by Abdullah [34] for solving Poisson differential equation. Later, Yousif and Evans [35] and Ibrahim and Abdullah [36] initiated half-sweep approach via EDG iterative scheme for the numerical solution of the elliptic partial differential and diffusion equations, respectively. Later, many authors utilized this approach for several other types of differential equations.
The use of modified groups quarter-sweep technique have been widely shown to provide faster rate of convergence. This approach can be constructed by implementation of FD approximation with 2h grid spacing in the discretized region. The quarter-sweep approach’s basic concept is based on time reduction techniques that use nearly the quarter grid points of the solution region and these points are treat as iterative points that involved in the iterative process. Just by using the quarter grid points of the suggested domain, iterative process reduces the computational complexity of the algorithm and hence ultimately decreases the execution of time per iteration. The remaining grid points that are not included in the iterative process are referred to as direct points, and they can be evaluated directly using the point iterative approach. On the basis of this concept, Othman and Abdullah [37] discovered Modified Explicit Group (MEG) iterative approach for the numerical solution of 2D Poisson differential equation by utilizing the quarter grids stencil of the solution domain and results were found much better and faster than the results obtained from EDG iterative method derived from utilizing the half grids stencil for the same 2D Poission equation [34].
Many authors applied this technique on several types of partial differential equations with promising results [9,38]. Because of the technique’s success with integer derivative PDEs, researchers are now attempting to adapt it to fractional differential equations. Balasim and Ali [39,40,41] recently published preliminary work on parabolic partial differential equations of fractional order. The main purpose of this research is to investigate the capability of this technique for solving the 2D fractional telegraph equation on a family of four points with 2h grid spacing.
Consider the second-order time-fractional hyperbolic telegraph equation [6],
2 α Υ t 2 α + 2 μ ( x , y , t ) α Υ t α + η 2 ( x , y , t ) Υ = a ( x , y , t ) 2 Υ x 2 + b ( x , y , t ) 2 Υ y 2 + f ( x , y , t ) ,
where 1 / 2 < α < 1 , μ ( x , y , t ) > 0 , η ( x , y , t ) > 0 . Also , a ( x , y , t ) > 0 , b ( x , y , t ) are positive real constants and f ( x , y , t ) is the forcing term. If η ( x , y , t ) = 0 , then Equation (2), reduces to the fractional damped wave equation.
Initial and boundary conditions are as follows:
Υ ( x , y , 0 ) = ψ 1 ( x , y ) , Υ t ( x , y , 0 ) = ψ 2 ( x , y ) ,
Υ ( 0 , y , t ) = g 1 ( y , t ) , Υ ( L , y , t ) = g 2 ( y , t ) ,
Υ ( x , 0 , t ) = g 3 ( x , t ) , Υ ( x , L , t ) = g 4 ( x , t ) ,
where Ω Δ = { ( x , y , t ) / 0 < x , y < L , 0 t T } .
Discretize the spatial domain as t k = k τ , k = 0 , 1 , 2 , N , x i = i Δ x , i = 0 , 1 , 2 , M x and y i = j Δ y , j = 0 , 1 , 2 , M y where τ = T N , Δ x = L M x and Δ y = L M y and N, M x and M y are the positive integers. The grid points of the discretized solution domain are given by ( x i , y j , t k ) = ( i Δ x , j Δ y , k τ ) . The exact solution of the fractional differential Equation (2) is Υ i , j , k , while the approximate solution is υ i , j , k and consider the following,
f ( x i , y j , t k ) = f i , j k , a ( x i , y j , t k ) = a i , j k , b ( x i , y j , t k ) = b i , j k ,
η ( x i , y j , t k ) = η i , j k , μ ( x i , y j , t k ) = μ i , j k .
The Caputo’s time fractional derivative is defined as follows:
α υ ( x , y , t ) t α = 1 Γ ( m α ) 0 t υ m ( x , y , ξ ) ξ m d ξ ( t ξ ) α + 1 m , m 1 < α < m .
The following two equations of Caputo’s fractional derivatives of order 2 α and α can be derived from Equation (3) by using the first and second time differential operators.
2 α υ ( x i , y j , t k + 1 / 2 ) t 2 α = 1 Γ ( 3 2 α ) τ 2 α s = 1 k ω s * [ υ i , j k s + 2 2 υ i , j k s + 1 + υ i , j k s ] + O ( τ 3 2 α )
where ω s * = s 2 ( 1 α ) ( s 1 ) 2 ( 1 α ) , s = 1 , 2 k and
α υ ( x i , y j , t k + 1 / 2 ) t α = 1 Γ ( 2 α ) τ α s = 1 k ω s [ υ i , j k s + 2 υ i , j k s + 1 ] + O ( τ 2 α )
where ω s = s 1 α ( s 1 ) 1 α , s = 1 , 2 k .
The structure of this paper is as follows: The derivation of MFEG iterative scheme based on 2h-spaced standard Crank–Nicolson FD approximation is explained in Section 2. Section 3 discusses the MFEG iterative scheme’s stability and convergence. Numerical Experimental and Results are discussed in Section 4. The Conclusions are provided in the last Section 5.

2. Modified Fractional Explicit Group (MFEG) Iterative Scheme

The h -spaced point and group iterative schemes for 2D fractional telegraph equation have been derived by Ali and Ali in [6]. The following standard 2h-spaced iterative scheme can be obtain by utilizing standard 2h-spaced Crank–Nicolson scheme for space-derivatives and Caputo fractional derivatives from Equations (4) and (5) for time-derivatives in Equation (2), we have the following expression,
υ i , j k + 1 = 1 ( p 1 + p 2 + r 1 / 4 + r 2 / 4 + q ) [ r 1 8 ( υ i 2 , j k + 1 + υ i + 2 , j k + 1 ) + r 2 8 ( υ i , j 2 k + 1 + υ i , j + 2 k + 1 )
+ r 1 8 ( υ i 2 , j k + υ i + 2 , j k ) + r 2 8 ( υ i , j 2 k + υ i , j + 2 k ) + ( p 1 ( 1 ω 2 ) p 2 + q ( 2 ω 2 * ) r 1 / 4 r 2 / 4 ) υ i , j k
+ ( p 1 ω k + 2 q ω k * ) υ i , j 1 q υ i , j k 1 + p 1 s = 2 k 1 ( ω s ω s 1 ) υ i , j k s + 1 + q s = 2 k 1 ( 2 ω s * ω s 1 * ) υ i , j k s + 1
q s = 2 k 1 ω s * υ i , j k s + m 0 f i , j k + 1 / 2 ]
with initial and boundary conditions,
υ i , j 0 = ψ 1 ( x i , y j ) , υ t i , j 0 = ψ 2 ( x i , y j )
υ 0 , j k = g 1 ( y j , t ) , υ L , j k = g 2 ( y j , t )
υ i , 0 k = g 3 ( x i , t ) , υ i , L k = g 4 ( x i , t )
for all i = 2 , 4 M x 2 , j = 2 , 4 M y 2 and k = 0 , 1 , 2 , 3 N where,
m 0 = τ 2 α Γ ( 3 2 α ) Γ ( 2 α ) , q = Γ ( 2 α )
p 1 = 2 τ α Γ ( 3 2 α ) μ i , j k , p 2 = m 0 2 1 ( η i , j k ) 2
r 1 = a i , j k m 0 ( Δ x ) 2 , r 2 = b i , j k m 0 ( Δ y ) 2 .
The suggested domain is discretized as, υ t ( x i , y j , 0 ) = υ 1 ( x i , y j ) υ 1 ( x i , y j ) 2 τ . From the initial condition, we have υ t ( x i , y j , 0 ) = ψ 2 ( x i , y j ) which implies υ i , j 1 = υ i , j 1 2 τ ψ 2 ( x i , y j ) .
For k = 0 ,
υ i , j 1 = 1 ( p 1 + p 2 + r 1 / 4 + r 2 / 4 + 2 q ) [ r 1 8 ( υ i 2 , j 1 + υ i + 2 , j 1 ) + r 2 8 ( υ i , j 2 1 + υ i , j + 2 1 ) + r 1 8 ( υ i 2 , j 0 + υ i + 2 , j 0 )
+ r 2 8 ( υ i , j 2 0 + υ i , j + 2 0 ) + ( p 1 ( 1 ω 2 ) p 2 + q ( 2 ω 2 * ) r 1 / 4 r 2 / 4 ) υ i , j 0 + 2 q τ ψ 2 ( x i , y j ) + m 0 f i , j 1 / 2 ]
for all i = 2 , 4 M x 2 , j = 2 , 4 M y 2 and k = 0 , 1 , 2 , 3 N .
When Equation (6) is applied to a group of four points, the result is a 4 × 4 system of equations, as shown below.
D a 1 a 2 a 3 a 1 D a 3 a 2 a 2 a 3 D a 1 a 3 a 2 a 1 D υ i , j k + 1 υ i + 2 , j k + 1 υ i + 2 , j + 2 k + 1 υ i , j + 2 k + 1 = r h s i , j r h s i + 2 , j r h s i + 2 , j + 2 r h s i , j + 2
where D = p 1 + p 2 + r 1 / 4 + r 2 / 4 + q , a 1 = r 1 / 8 , a 2 = 0 , a 3 = r 2 / 8 ,
r h s i , j = r 1 8 ( υ i 2 , j k + 1 ) + r 2 8 ( υ i , j 2 k + 1 ) + r 1 8 ( υ i 2 , j k + υ i + 2 , j k ) + r 2 8 ( υ i , j 2 k + υ i , j + 2 k )
+ ( p 1 ( 1 ω 2 ) p 2 + q ( 2 ω 2 * ) r 1 / 4 r 2 / 4 ) υ i , j k + ( p 1 ω k + 2 q ω k * ) υ i , j 1 q υ i , j k 1
+ p 1 s = 2 k 1 ( ω s ω s 1 ) υ i , j k s + 1 + q s = 2 k 1 ( 2 ω s * ω s 1 * ) υ i , j k s + 1 q s = 2 k 1 ω s * υ i , j k s + m 0 f i , j k ,
r h s i + 2 , j = r 1 8 ( υ i + 4 , j k + 1 ) + r 2 8 ( υ i + 2 , j 2 k + 1 ) + r 1 8 ( υ i , j k + υ i + 4 , j k ) + r 2 8 ( υ i + 2 , j 2 k + υ i + 2 , j + 2 k )
+ ( p 1 ( 1 ω 2 ) p 2 + q ( 2 ω 2 * ) r 1 / 4 r 2 / 4 ) υ i + 2 , j k + ( p 1 ω k + 2 q ω k * ) υ i + 2 , j 1 q υ i + 2 , j k 1
+ p 1 s = 2 k 1 ( ω s ω s 1 ) υ i + 2 , j k s + 1 + q s = 2 k 1 ( 2 ω s * ω s 1 * ) υ i + 2 , j k s + 1 q s = 2 k 1 ω s * υ i + 2 , j k s + m 0 f i + 2 , j k ,
r h s i + 2 , j + 2 = r 1 8 ( υ i + 4 , j + 2 k + 1 ) + r 2 8 ( υ i + 2 , j + 4 k + 1 ) + r 1 8 ( υ i , j + 2 k + υ i + 4 , j + 2 k ) + r 2 8 ( υ i + 2 , j k + υ i + 2 , j + 4 k )
+ ( p 1 ( 1 ω 2 ) p 2 + q ( 2 ω 2 * ) r 1 / 4 r 2 / 4 ) υ i + 2 , j + 2 k + ( p 1 ω k + 2 q ω k * ) υ i + 2 , j + 2 1 q υ i + 2 , j + 2 k 1
+ p 1 s = 2 k 1 ( ω s ω s 1 ) υ i + 2 , j + 2 k s + 1 + q s = 2 k 1 ( 2 ω s * ω s 1 * ) υ i + 2 , j + 2 k s + 1 q s = 2 k 1 ω s * υ i + 2 , j + 2 k s + m 0 f i + 2 , j + 2 k ,
r h s i , j + 2 = r 1 8 ( υ i 2 , j + 2 k + 1 ) + r 2 8 ( υ i , j + 4 k + 1 ) + r 1 8 ( υ i 2 , j + 2 k + υ i + 2 , j + 2 k ) + r 2 8 ( υ i , j k + υ i , j + 4 k )
+ ( p 1 ( 1 ω 2 ) p 2 + q ( 2 ω 2 * ) r 1 / 4 r 2 / 4 ) υ i , j + 2 k + ( p 1 ω k + 2 q ω k * ) υ i , j + 2 1 q υ i , j + 2 k 1
+ p 1 s = 2 k 1 ( ω s ω s 1 ) υ i , j + 2 k s + 1 + q s = 2 k 1 ( 2 ω s * ω s 1 * ) υ i , j + 2 k s + 1 q s = 2 k 1 ω s * υ i , j + 2 k s + m 0 f i , j + 2 k .
Re-write the matrix Equation (7) as:
υ i , j k + 1 υ i + 2 , j k + 1 υ i + 2 , j + 2 k + 1 υ i , j + 2 k + 1 = 1 B 1 ω 1 ω 2 ω 3 ω 4 ω 2 ω 1 ω 4 ω 3 ω 3 ω 4 ω 1 ω 2 ω 4 ω 3 ω 2 ω 1 r h s i , j r h s i + 2 , j r h s i + 2 , j + 2 r h s i , j + 2
where,
B 1 = ( p 1 + p 2 + r 1 / 4 + r 2 / 4 + q ) 4 ( 1 / 32 ) ( p 1 + p 2 + r 1 / 4 + r 2 / 4 + q ) 2 ( r 1 2 + r 2 2 ) + 1 / ( 64 ) 2 ( r 1 2 r 2 2 ) 2 ,
ω 1 = ( p 1 + p 2 + r 1 / 4 + r 2 / 4 + q ) { ( p 1 + p 2 + r 1 / 4 + r 2 / 4 + q ) 2 ( r 1 2 ) / 64 ( r 2 2 ) / 64 } ,
ω 2 = ( r 1 ) / 8 { ( p 1 + p 2 + r 1 / 4 + r 1 / 4 + q ) 2 ( r 1 2 ) / 64 ( r 2 2 ) / 64 } ,
ω 3 = 1 / 32 ( p 1 + p 2 + r 1 / 4 + r 2 / 4 + q ) ( r 1 ) ( r 2 ) ,
ω 4 = ( r 2 ) / 8 { ( p 1 + p 2 + r 1 / 4 + r 2 / 4 + q ) 2 + ( r 1 ) 2 / 64 ( r 2 ) 2 / 64 } .
For the evaluation of Equation (8), we divide the solution domain into groups of four-points with 2h grid spacing as described in [9]. The iterations are generated on group of four-points on some initial guess and continue until predefined tolerance factor ε is achieved. This group is examined explicitly as a single point in the iterative process. The values at the remaining grid points (ungrouped points) can be obtained using the traditional t e x t i t h -spaced FD approximation equation once convergence has occurred.
Equation (7) can be written in the following form,
A υ 1 = B υ 0 + m 0 f 1 / 2 k = 0 A υ k + 1 = B υ k + C υ k 1 + D k υ 1 + s = 2 k 1 C s 1 υ k s + 1 + s = 2 k 1 C s 1 * υ k s + 1 + s = 2 k 1 D s * υ k s + m 0 f k + 1 / 2 k > 0 υ 0 = ϕ
Here are matrices A, B, C, C s , C s * , D k , D s * and vectors υ , f and ϕ are defined in Appendix A.
Lemma 1.
The coefficients ω s and ω s * defined in Equations (4) and (5) for all s = 1 , 2 , k satisfies the following properties [7],
(1). ω s > 0 and ω 1 = 1 , s = 1 , 2 , k
(2). ω s 1 > ω s , s = 1 , 2 , k
(3). ω s 1 ω k 1 , s = 1 , 2 , k
(4). s = 1 k 1 ( ω k s ω k s + 1 ) + ω k = ω 1 , s = 1 , 2 , k
(5). s = 2 k 1 ( ω s ω s 1 ) + ω 1 = ω k 1 , s = 1 , 2 , k
(6). s = 2 k 1 ( 2 ω s * ω s 1 * ) + ω 1 = s = 2 k 1 ( ω s * + ω k 1 * ) , s = 1 , 2 , k .

3. Stability and Convergence of the MFEG Iterative Scheme

3.1. Stability Analysis

Suppose that υ i , j k is the approximate solution and Υ i , j k is the exact solution of Equation (7) for all ( i = 2 , 6 M x 2 ), ( j = 2 , 6 M y 2 ) and ( k = 0 , 1 , 2 , N ), then the error ε i , j k = | Υ i , j k u i , j k | will satisfy the matrix Equation (7) at all time levels for all ( i = 2 , 6 M x 2 ), ( j = 2 , 6 M y 2 ) and ( k = 0 , 1 , 2 , N ). Equation (7) will take the following form,
D a 1 a 2 a 3 a 1 D a 3 a 2 a 2 a 3 D a 1 a 3 a 2 a 1 D ε i , j k + 1 ε i + 2 , j k + 1 ε i + 2 , j + 2 k + 1 ε i , j + 2 k + 1 = r h s i , j r h s i + 2 , j r h s i + 2 , j + 2 r h s i , j + 2 .
The above Equation (10) can be written as,
A E 1 = B E 0 k = 0 A E k + 1 = B E k + C E k 1 + D k E 1 + s = 2 k 1 C s 1 E k s + 1 + s = 2 k 1 C s 1 * E k s + 1 + s = 2 k 1 D s * E k s k > 0
where,
E k + 1 = E 2 k + 1 E 6 k + 1 E M x 6 k + 1 E M x 2 k + 1 , E i k + 1 = θ i , 2 k + 1 θ i , 6 k + 1 θ i , M y 6 k + 1 θ i , M y 2 k + 1 , θ i , j k + 1 = ε i , j k + 1 ε i + 2 , j k + 1 ε i + 2 , j + 2 k + 1 ε i , j + 2 k + 1
i = 2 , 6 , M x 2 , j = 2 , 6 , M y 2 .
Theorem 1.
For k = 0 , 1 , 2 , N we have E k + 1 E 0 .
Proof. 
Consider the Equation (11) for k = 0 ,
E 1 A 1 B E 0
E 1 A 1 B B m i n 2 < i < M x 2 { | a i , i | i j , j = 2 M y 2 | a i , j | } E 0
= | p 1 ( 1 ω 2 ) p 2 + q ( 2 ω 2 * ) r 1 / 4 r 2 / 4 | + { | r 1 / 8 | + | r 1 / 8 | + | r 2 / 8 | + | r 2 / 8 | } | p 1 + p 2 + 2 q + r 1 / 4 + r 2 / 4 | { | r 1 / 8 | + | r 1 / 8 | + | r 2 / 8 | + | r 2 / 8 | } E 0
E 1 | p 1 ( 1 ω 2 ) p 2 + q ( 2 ω 2 * ) | | p 1 + p 2 + 2 q | E 0 .
Since 0 < ω 2 , ω 2 * < 1 so the numerator’s p 1 and q coefficients are less than the denominator’s p 1 and q coefficients. Therefore,
E 1 E 0 .
Assume that E s E 0 for all s = 1 , 2 , k , we prove for k + 1 . Again consider Equation (11) for k > 0 ,
E k + 1 A 1 B E k + A 1 C E k 1 + A 1 D k E 1 + s = 2 k 1 A 1 C s 1 E k s + 1
+ s = 2 k 1 A 1 C s 1 * E k s + 1 + s = 2 k 1 A 1 D s * E k s
= [ | p 1 ( 1 ω 2 ) p 2 + q ( 2 ω 2 * ) | + | q | + | p 1 ω k + 2 q ω k * | + | s = 2 k 1 p 1 ( ω s ω s 1 ) |
+ | s = 2 k 1 q ( 2 ω s * ω s 1 * ) | + | s = 2 k 1 q ( ω s * ) | ] . [ 1 | p 1 + p 2 + q | ] E 0 .
The following expression is obtained by adding the coefficients of p 1 and q:
E k + 1 | p 1 { ( 1 ω 2 ) + s = 2 k 1 ( ω s ω s 1 ) + ω k } p 2
+ q { 1 ω 2 * + 2 ω k * + s = 2 k 1 ( 2 ω s * ω s 1 * ) s = 2 k 1 ω s * } | [ 1 | p 1 + p 2 + q | ] E 0 .
Using (5) and (6) in Lemma 1, we have
E k + 1     | p 1 { ( ω k 1 + ω k ) ω 2 } p 2 + q { ( ω k 1 * + 2 ω k * ) ω 2 * } | [ 1 | p 1 + p 2 + q | ] E 0 .
As τ 0 ( i.e the number of time levels increases), p 1 , p 2 0 , therefore
E k + 1     | q { ( ω k 1 * + 2 ω k * ) ω 2 * | | q | ] E 0 .
Using (2) in Lemma 1, we have
1 = ω 0 * > ω 1 * > ω 2 * > > ω k 1 * > ω k * .
As k , both the terms ω k 1 * and ω k * both approaches to zero.
Since 0 < ω 2 * < 1 , thus
E k + 1 E 0 .
 □

3.2. Convergence

Let Υ ( x i , y j , t k + 1 / 2 ) be the analytical solution of Equation (6) and suppose we represent the truncation error by R k + 1 / 2 at the point ( x i , y j , t k + 1 / 2 ) such that
R k + 1 / 2 c ( τ 3 2 α + ( Δ x ) 2 + ( Δ y ) 2 )
where c is constant. Define η i , j k = | Υ ( x i , y j , t k + 1 / 2 ) υ i , j k + 1 / 2 | for all i = 2 , 6 , M x 2 , j = 2 , 6 , M y 2 , k = 0 , 1 , 2 , N and e k + 1 = ( e 2 k + 1 , e 6 k + 1 , e M x 2 k + 1 ) T using e 0 = 0 where,
e i k + 1 = ϑ i , 2 k + 1 ϑ i , 6 k + 1 ϑ i , M y 6 k + 1 ϑ i , M y 2 k + 1 , ϑ i , j k + 1 = η i , j k + 1 η i + 2 , j k + 1 η i + 2 , j + 2 k + 1 η i , j + 2 k + 1
for all i = 2 , 6 , M x 2 , j = 2 , 6 , M y 2 .
Therefore, Equation (11) can be written as,
for k = 0 ,
A e 1 = R 1 / 2
for k > 0 ,
A e k + 1 = B e k + C e k 1 + D k e 1 + s = 2 k 1 C s 1 e k s + 1 + s = 2 k 1 C s 1 * e k s + 1 + s = 2 k 1 D s * e k s + R k + 1 / 2 .
Theorem 2.
The scheme defined in Equation (7) is convergent, hence the following estimate is correct.
e k + 1 z ( α ) ( τ 3 2 α + ( Δ x ) 2 + ( Δ y ) 2 )
where e k = max 2 i M x 2 , 2 j M y 2 , 0 k N | e i , j k | .
Proof. 
We use mathematical induction to prove the theorem by setting
ω 0 * 2 + ω 0 2 = 1 . Assume Equation (13) for the case when k = 0 ,
e 1 = A 1 R 1 / 2
e 1 A 1 R 1 / 2 c Γ ( 2 α ) ( ω 0 * 2 + ω 0 2 ) ( τ 3 2 α + ( Δ x ) 2 + ( Δ y ) 2 )
where z ( α ) = c Γ ( 2 α ) .
We will prove this result using mathematical induction. Now assume that e s z ( α ) R s + 1 / 2 is true for all s = 1 , 2 , k and we prove it for k + 1 .
Assume Equation (14) for the case when k > 0 ,
e k + 1 A 1 B e k + A 1 C e k 1 + A 1 D k e 1 + s = 2 k 1 A 1 C s 1 e k s + 1
+ s = 2 k 1 A 1 C s 1 * e k s + 1 + s = 2 k 1 A 1 D s * e k s + A 1 c R k + 1 / 2
= [ ω k * m o + ω k m o + A 1 B + A 1 C + A 1 D k + s = 2 k 1 A 1 C s 1
+ s = 2 k 1 A 1 C s 1 * + s = 2 k 1 A 1 D s * ] c R k + 1 / 2
= [ | ω k * m o + ω k m o + p 1 { ( ω k 1 + ω k ) ω 2 } p 2 + q { ( ω k 1 * + 2 ω k * ) ω 2 * } | p 1 + p 2 + q | ] c R k + 1 / 2 .
By collecting the coefficients of p 1 and q and (2) of Lemma (1), we have ω 0 > ω 1 > ω 2 > ω 3 > ω k 1 > ω k . When the number of time levels k is increased, the terms ω k , ω k 1 , ω k * , ω k 1 * approaches to zero. As a results,
e k + 1 [ | p 1 ω 2 p 2 + q ω 2 * | | p 1 + p 2 + q | ] c | R k + 1 / 2 .
Since coefficients of p 1 and q in the denominator are larger than the coefficients of p 1 and q in the numerator, therefore
e k + 1 c | R k + 1 / 2 = [ m o ω k * + ω k ] R k + 1 / 2
or
e k + 1 [ m o 1 k 2 α ( ( ω k * ) 1 k 2 α ) + 1 k α ( ω k 1 k α ) ] R k + 1 / 2 .
Since
lim k ( ω k * ) 1 k 2 α = lim k k 2 α ( k ) 2 2 α ( k 1 ) 2 2 α = 1 2 2 α
and
lim k ω k 1 k α = lim k k α ( k ) 1 α ( k 1 ) 1 α = 1 1 α .
Therefore,
e k + 1 [ m o 1 k 2 α ( 2 2 α ) + 1 k α ( 1 α ) ] R k + 1 / 2
or
e k + 1 [ m o k 2 α ( 2 2 α ) k α ( 1 α ) k 2 α ( 2 2 α ) + k α ( 1 α ) ] R k + 1 / 2 .
Multiply and divide the denominator by k 2 α , we have the following inequality,
e k + 1 [ m o k α ( 2 2 α ) ( 1 α ) ( 2 2 α ) + ( 1 α ) k α ] R k + 1 / 2 .
Since k , therefore term ( 1 α ) k α will be zero, hence
e k + 1 ( k τ 2 ) α Γ ( 2 α ) Γ ( 3 2 α ) ( 1 α ) R k + 1 / 2 .
As ( k τ 2 ) α T , therefore
e k + 1 z ( α ) ( τ 3 2 α + ( Δ x ) 2 + ( Δ y ) 2 )
where z ( α ) = Γ ( 2 α ) Γ ( 3 2 α ) ( 1 α ) .
This completes the proof.  □

4. Numerical Problems and Results

Two numerical problems are performed to test the viability of the proposed schemes in solving 2D hyperbolic telegraph differential Equation (2). The numerical tests are run on a PC with a Core 2 Duo 2.8 GHz processor and 2GB of RAM Windows XP SP3 with Cygwin C in Mathematica 11 software. We assume that the step sizes in both x and y directions are the same, i.e., h = Δ x = Δ y in both numerical experiments. Throughout our numerical calculations, we employed the Gauss Seidel method with a relaxation factor of ω e equal to 1. The l i n f t y norm was utilized for the convergence criterion, with a tolerance factor of ε = 10 5 . Various mesh sizes of 20, 30, 40 and 50 were considered for different time steps of 1/20, 1/30, 1/40 and 1/50 in Example 1 and mesh sizes of 25, 35, 45 and 55 were considered for different time steps of 1/25, 1/35, 1/45 and 1/55 in Example 2. The numerical results in Table 1 and Table 2 are obtained using the FSP, FEG, and MFEG iterative methods in terms of elapsed time (in seconds), number of iterations, average absolute error, and maximum absolute error. The fractional standard point (FSP) and fractional explicit group (FEG) iterative schemes are derived in [6] for 2D fractional telegraph equation. Graphs of execution time and iteration count are illustrated in Figure 1 and Figure 2 at various values of α for Example 1 and Example 2.
Example 1.
Consider the 2D time-fractional telegraph model together where the forcing term is defined by [6],
2 α υ t 2 α + α υ t α + υ = 2 υ x 2 + 2 υ y 2 2 sin ( x ) sin ( y ) ( sin ( t ) cos ( t ) ) .
Initial and boundary conditions are defined as follows:
υ ( x , y , 0 ) = ψ 1 ( x , y ) = sin ( x ) sin ( y ) , υ t ( x , y , 0 ) = ψ 2 ( x , y ) = 0
υ ( 0 , y , t ) = g 1 ( y , t ) = 0 , υ ( 1 , y , t ) = g 2 ( 1 , y , t ) = cos ( t ) sin ( 1 ) sin ( y )
υ ( x , 0 , t ) = g 3 ( x , t ) = 0 , υ ( x , 1 , t ) = g 4 ( x , 1 , t ) = cos ( t ) sin ( x ) sin ( 1 ) .
The exact solution is υ ( x , y , t ) = sin ( x ) sin ( y ) cos ( t ) .
Example 2.
The 2D telegraph equation of fractional order is given by the following expression [6],
2 α υ t 2 α + α υ t α + υ = 2 υ x 2 + 2 υ y 2 sinh ( x ) sinh ( y ) ( 2 α sin ( t ) β 2 cos ( t ) + 3 cos ( t ) )
Let α = 10 and β = 5 , thus we have,
f ( x , y , t ) = sinh ( x ) sinh ( y ) ( 25 cos ( t ) 20 sin ( t ) 3 cos ( t ) ) ,
with the initial and boundary conditions:
υ ( x , y , 0 ) = ψ 1 ( x , y ) = sinh ( x ) sinh ( y ) , υ t ( x , y , 0 ) = ψ 2 ( x , y ) = 0
υ ( 0 , y , t ) = g 1 ( y , t ) = 0 , υ ( 1 , y , t ) = g 2 ( 1 , y , t ) = cos ( t ) sinh ( 1 ) sinh ( y )
υ ( x , 0 , t ) = g 3 ( x , t ) = 0 , υ ( x , 1 , t ) = g 4 ( x , 1 , t ) = cos ( t ) sinh ( x ) sinh ( 1 ) .
The exact solution is υ ( x , y , t ) = cos ( t ) sinh ( x ) sinh ( y ) .
In Table 1 and Table 2, it is can be seen that execution time and iteration count decrease as value of α moves towards 2 by providing more accurate results.
The average absolute error and maximum absolute error are calculated by taking the absolute average and maximum absolute value of the column vector of errors, respectively. The maximum absolute error of the exact solution Υ i , j , k and approximate solution υ i , j , k is defined as follows:
e ( τ , h ) = max 2 i M x 2 , 2 j M y 2 , 0 k N { | Υ i , j k υ i , j k | } .
The temporal convergence order of the proposed method is defined as,
γ 1 o r d e r log 2 e ( 2 τ , h ) e ( τ , h ) ,
and the spatial convergence order of the proposed method is defined as,
γ 2 o r d e r log 2 e ( τ , 2 h ) e ( τ , h )
Table 3 and Table 4 represent the values of maximum absolute error and temporal convergence order of MFEG iterative scheme at various values of α of Example 1 and Example 2. For fixed value of h = π 200 and different values of τ , it is observed that MFEG iterative scheme generates ( 3 2 α ) temporal convergence order as shown in Table 3 and Table 4. Meanwhile, the Table 5 and Table 6 show the values of maximum absolute error and spatial convergence order of MFEG iterative scheme at various values of α of Example 1 and Example 2. For fixed value of τ = 0.001 and different values of h, it shows that MFEG iterative scheme gets second-order spatial accuracy as exposed in Table 5 and Table 6.
The ranges of percentages of MFEG method against FSP and FEG methods in terms of execution time and number of iterations of Example 1 at α = 0.55 and Example 2 at α = 0.90 are summarized in Table 7 and Table 8, respectively.
Table 7 and Table 8 refer to the study of the percentages of MFEG method in term of the execution timings and number of iterations against FSP and FEG methods for solving the 2D fractional telegraph equation. Table 7 shows efficiency of execution of timings of MFEG method in Example 1 is about (26.0–42.0)% and (50.0–55.0)% of FSP and FEG methods while Table 8 indicates the execution of timings of MFEG method in Example 2 is merely about (24.0–37.0)% and (45.0–63.0)% of FSP and FEG method. The efficient percentages of MFEG iterative method for the number of iterations for both examples can also been seen in Table 7 and Table 8.

5. Conclusions

In this study, the unconditionally stable modified group relaxation method is constructed in the numerical solution of 2D hyperbolic telegraph equation. The MFEG method is derived from the standard Crank–Nicolson FD approximation with 2h grid spacing. It is observed that the suggested algorithm has more efficiency as compared to the other existing methods such as fractional standard point and fractional explicit group methods presented in [6]) in terms of number of iterations and elapsed CPU-timings. Amongst the schemes tested, the MFEG method is proven to require the least computational cost in terms of execution of timings. Moreover, it shown that the derived numerical temporal and spatial convergence order support our theoretical derivations. For a better convergence rate, in future, we will apply splitting-type preconditioner in block formulation applied to a class of group relaxation iterative methods for the numerical solution of various types of 2D time-fractional problems.

Author Contributions

Conceptualization, A.A., T.A. (Thabet Abdeljawad), A.I., T.A. (Tayyaba Akram) and M.A.; Formal analysis, A.A., T.A. (Thabet Abdeljawad), A.I., T.A. (Tayyaba Akram) and M.A.; Funding acquisition, T.A. (Thabet Abdeljawad); Investigation, A.A., T.A. (Thabet Abdeljawad), A.I., T.A. (Tayyaba Akram) and M.A.; Methodology, A.A., T.A. (Thabet Abdeljawad), A.I., T.A. (Tayyaba Akram) and M.A.; Software, A.A., T.A. (Thabet Abdeljawad), A.I., T.A. (Tayyaba Akram) and M.A.; Visualization, A.A., T.A. (Thabet Abdeljawad), A.I., T.A. (Tayyaba Akram) and M.A.; Writing—original draft, A.A., T.A.(Thabet Abdeljawad), A.I., T.A. (Tayyaba Akram) and M.A. All authors have read and agreed to the published version of the manuscript.

Funding

The second author will financially support the paper.

Institutional Review Board Statement

Not applicable.

Informed Consent Statement

Not applicable.

Data Availability Statement

All data generated or analyzed during this study are included in this article.

Acknowledgments

The author T. Abdeljawad would like to thank Prince Sultan University for the support through TAS research lab.

Conflicts of Interest

The authors declare that they have no conflict of interest to report regarding the present study.

Appendix A

Here,
υ k + 1 = υ 2 k + 1 υ 6 k + 1 υ M x 6 k + 1 υ M x 2 k + 1 , f k + 1 / 2 = f 2 k + 1 / 2 f 6 k + 1 / 2 f M x 6 k + 1 / 2 f M x 2 k + 1 / 2 , ϕ = ϕ 2 ϕ 6 ϕ M x 6 ϕ M x 2
υ i k + 1 = g i , 2 k + 1 g i , 6 k + 1 g i , M y 6 k + 1 g i , M y 2 k + 1 , g i , j k + 1 = υ i , j k + 1 υ i + 2 , j k + 1 υ i + 2 , j + 2 k + 1 υ i , j + 2 k + 1
i = 2 , 6 , M x 2 , j = 2 , 6 , M y 2 .
f i k + 1 / 2 = d i , 2 k + 1 / 2 d i , 6 k + 1 / 2 d i , M y 6 k + 1 / 2 d i , M y 2 k + 1 / 2 , d i , j k + 1 / 2 = f i , j k + 1 / 2 f i + 2 , j k + 1 / 2 f i + 2 , j + 2 k + 1 / 2 f i , j + 2 k + 1 / 2
i = 2 , 6 , M x 2 , j = 2 , 6 , M y 2
ϕ i = ψ i , 2 ψ i , 6 ψ i , M y 6 ψ i , M y 2 , ψ i , j = ϕ i , j ϕ i + 2 , j ϕ i + 2 , j + 2 ϕ i , j + 2
i = 2 , 6 , M x 2 , j = 2 , 6 , M y 2 , and
A = M 1 M 2 M 3 M 1 M 2 0 0 M 3 M 1 M 2 M 3 M 1 , B = N 1 N 2 N 3 N 1 N 2 0 0 N 3 N 1 N 2 N 3 N 1
C = L 1 L 1 0 0 L 1 L 1 , D k = P 1 P 1 0 0 P 1 P 1
C s 1 = Υ 1 Υ 1 0 0 Υ 1 Υ 1 , C s 1 * = V 1 V 1 0 0 V 1 V 1
D s * = Q 1 Q 1 0 0 Q 1 Q 1
M 1 = S 1 S 2 S 3 S 1 S 2 0 0 S 3 S 1 S 2 S 3 S 1 , M 2 = S 4 S 4 0 0 S 4 S 4
M 3 = S 5 S 5 0 0 S 5 S 5 , N 1 = R 1 R 2 R 3 R 1 R 2 0 0 R 3 R 1 R 2 R 3 R 1
N 2 = R 4 R 4 0 0 R 4 R 4 , N 3 = R 5 R 5 0 0 R 5 R 5
L 1 = H 1 H 1 0 0 H 1 H 1 , P 1 = H 2 H 2 0 0 H 2 H 2
Υ 1 = H 3 H 3 0 0 H 3 H 3 , V 1 = H 4 H 4 0 0 H 4 H 4
Q 1 = H 5 H 5 0 0 H 5 H 5 , S 1 = D r 1 / 8 0 r 2 / 8 r 1 / 8 D r 1 / 8 0 0 r 1 / 8 D r 1 / 8 r 2 / 8 0 r 1 / 8 D
where D = p 1 + p 2 + r 1 / 4 + r 2 / 4 + q ,
S 2 = r 1 / 8 0 0 0 0 0 0 0 0 0 0 0 0 0 0 r 1 / 8 , S 3 = 0 0 0 0 0 r 1 / 8 0 0 0 0 r 1 / 8 0 0 0 0 0 , S 4 = r 2 / 8 0 0 0 0 r 2 / 8 0 0 0 0 0 0 0 0 0 0
R 1 = W 1 r 1 / 8 0 r 2 / 8 r 1 / 8 W 1 r 1 / 8 0 0 r 1 / 8 W 1 r 1 / 8 r 2 / 8 0 r 1 / 8 W 1
where W 1 = p 1 ( 1 ω 2 ) p 2 + q ( 2 ω 2 * ) r 1 / 4 r 2 / 4 ,
R 2 = r 1 / 8 0 0 0 0 0 0 0 0 0 0 0 0 0 0 r 1 / 8 , R 3 = 0 0 0 0 0 r 1 / 8 0 0 0 0 r 1 / 8 0 0 0 0 0 , R 4 = r 2 / 8 0 0 0 0 r 2 / 8 0 0 0 0 0 0 0 0 0 0
S 5 = 0 0 0 0 0 0 0 0 0 r 2 / 8 0 0 0 0 r 2 / 8 , R 5 = 0 0 0 0 0 0 0 0 0 0 r 2 / 8 0 0 0 0 r 2 / 8
H 1 = q 0 0 0 0 q 0 0 0 0 q 0 0 0 0 q , H 2 = p 1 ω k + 2 q ω k * 0 0 0 0 p 1 ω k + 2 q ω k * 0 0 0 0 p 1 ω k + 2 q ω k * 0 0 0 0 p 1 ω k + 2 q ω k *
H 3 = p 1 ( ω s ω s 1 ) 0 0 0 0 p 1 ( ω s ω s 1 ) 0 0 0 0 p 1 ( ω s ω s 1 ) 0 0 0 0 p 1 ( ω s ω s 1 )
H 4 = q ( 2 ω s * ω s 1 * ) 0 0 0 0 q ( 2 ω s * ω s 1 * ) 0 0 0 0 q ( 2 ω s * ω s 1 * ) 0 0 0 0 q ( 2 ω s * ω s 1 * )
H 5 = q ω s * 0 0 0 0 q ω s * 0 0 0 0 q ω s * 0 0 0 0 q ω s * .

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Figure 1. Graphs of execution timings of point and group iterative schemes on various mesh sizes for Example 1 and Example 2.
Figure 1. Graphs of execution timings of point and group iterative schemes on various mesh sizes for Example 1 and Example 2.
Symmetry 13 02078 g001
Figure 2. Graphs of number of iterations of point and group iterative schemes on various mesh sizes for Example 1 and Example 2.
Figure 2. Graphs of number of iterations of point and group iterative schemes on various mesh sizes for Example 1 and Example 2.
Symmetry 13 02078 g002
Table 1. Approximate results of FSP, FEG and MFEG methods for various values of α of Example 1.
Table 1. Approximate results of FSP, FEG and MFEG methods for various values of α of Example 1.
α = 0.55 α = 0.75 α = 0.95
h 1 MethodTime(s)Ite.Ave.ErrMax.ErrTime(s)Ite.Ave.ErrMax.ErrTime(s)Ite.Ave.ErrMax.Err
20FSP8.3625677.364 × 10 2 9.432 × 10 2 4.8754486.853 × 10 3 7.562 × 10 3 3.6854328.742 × 10 4 9.347 × 10 4
FEG6.8324425.940 × 10 2 6.380 × 10 2 3.0765297.543 × 10 3 8.804 × 10 3 2.1832204.774 × 10 4 5.559 × 10 4
MFEG3.4972216.632 × 10 2 7.521 × 10 2 2.6423168.053 × 10 3 9.063 × 10 3 1.7632105.942 × 10 4 6.347 × 10 4
30FSP32.783946.376 × 10 2 8.543 × 10 2 17.321735.746 × 10 3 6.654 × 10 3 9.8743447.774 × 10 4 8.454 × 10 4
FEG18.936454.656 × 10 2 5.687 × 10 2 8.8743416.123 × 10 3 7.543 × 10 3 5.7054253.087 × 10 4 4.762 × 10 4
MFEG9.3742255.635 × 10 2 6.073 × 10 2 5.3865227.756 × 10 3 8.664 × 10 3 2.8312124.589 × 10 4 5.784 × 10 4
40FSP74.0961285.384 × 10 2 7.543 × 10 2 37.4931014.543 × 10 3 5.765 × 10 3 19.420626.995 × 10 4 7.788 × 10 4
FEG40.295683.599 × 10 2 4.843 × 10 2 21.784535.755 × 10 3 6.142 × 10 3 11.096352.850 × 10 4 3.424 × 10 4
MFEG21.842374.421 × 10 2 5.602 × 10 2 12.785276.348 × 10 3 7.264 × 10 3 7.7539163.640 × 10 4 4.847 × 10 4
50FSP112.741634.596 × 10 2 6.563 × 10 2 57.7321363.954 × 10 3 4.543 × 10 3 27.842875.543 × 10 4 6.807 × 10 4
FEG59.094792.596 × 10 2 3.803 × 10 2 31.285764.684 × 10 3 5.843 × 10 3 16.832471.984 × 10 4 2.852 × 10 4
MFEG29.543363.947 × 10 2 4.826 × 10 2 15.272325.931 × 10 3 6.631 × 10 3 7.1679212.915 × 10 4 3.642 × 10 4
Table 2. Approximate results of FSP, FEG and MFEG methods for various value of α of Example 2.
Table 2. Approximate results of FSP, FEG and MFEG methods for various value of α of Example 2.
α = 0.60 α = 0.75 α = 0.90
h 1 MethodTime(s)Ite.Ave.ErrMax.ErrTime(s)Ite.Ave.ErrMax.ErrTime(s)Ite.Ave.ErrMax.Err
25FSP7.5321646.652 × 10 2 7.360 × 10 2 4.1273455.789 × 10 3 6.870 × 10 3 3.0523298.376 × 10 4 9.665 × 10 4
FEG6.0432344.634 × 10 2 5.631 × 10 2 2.4328245.784 × 10 3 6.327 × 10 3 1.5532146.346 × 10 4 7.833 × 10 4
MFEG3.0898156.743 × 10 2 7.287 × 10 2 1.6287135.849 × 10 3 6.428 × 10 3 0.993794.332 × 10 4 5.354 × 10 4
35FSP30.843885.850 × 10 2 6.826 × 10 2 16.435704.584 × 10 3 5.876 × 10 3 8.7843427.766 × 10 4 8.425 × 10 4
FEG17.485433.421 × 10 3 4.698 × 10 2 7.6943364.733 × 10 2 5.073 × 10 3 4.4958195.047 × 10 4 6.369 × 10 4
MFEG8.4542235.753 × 10 2 6.241 × 10 2 4.7342194.392 × 10 3 5.673 × 10 3 2.0206103.354 × 10 4 4.734 × 10 4
45FSP72.1721124.562 × 10 2 5.387 × 10 2 35.654973.870 × 10 3 4.685 × 10 3 18.998586.897 × 10 4 7.426 × 10 4
FEG39.632582.522 × 10 2 3.947 × 10 2 20.992473.585 × 10 3 4.205 × 10 3 10.984284.384 × 10 4 5.388 × 10 4
MFEG20.286274.754 × 10 2 5.785 × 10 2 11.985203.731 × 10 3 4.673 × 10 3 6.0362142.983 × 10 4 3.755 × 10 4
55FSP110.841463.782 × 10 2 4.846 × 10 2 55.4501262.589 × 10 3 3.695 × 10 3 26.996835.583 × 10 4 6.480 × 10 4
FEG57.908741.764 × 10 2 2.628 × 10 2 30.643622.699 × 10 3 3.126 × 10 3 15.997383.354 × 10 4 4.349 × 10 4
MFEG27.853393.467 × 10 2 4.437 × 10 3 14.654342.789 × 10 3 3.735 × 10 3 9.9857181.473 × 10 4 2.630 × 10 4
Table 3. The maximum absolute error and temporal convergence order of MFEG iterative scheme at various values of α when h = π 200 subject to Example 1.
Table 3. The maximum absolute error and temporal convergence order of MFEG iterative scheme at various values of α when h = π 200 subject to Example 1.
h / τ α = 0.65 α = 0.85
h τ e ( τ , h ) γ 1 -order e ( τ , h ) γ 1 -order
π 200 1/507.6432 × 10 4 -5.6311  × 10 4 -
1/1006.8721 × 10 4 1.74324.6543 × 10 4 1.9973
1/1508.9074 × 10 5 1.76536.2953 × 10 5 2.0016
1/2007.4285 × 10 5 1.78625.8514 × 10 5 2.0014
Table 4. The maximum absolute error and temporal convergence order of MFEG iterative scheme at various values of α when h = π 200 and subject to Example 2.
Table 4. The maximum absolute error and temporal convergence order of MFEG iterative scheme at various values of α when h = π 200 and subject to Example 2.
h / τ α = 0.70 α = 0.95
h τ e ( τ , h ) γ 1 -order e ( τ , h ) γ 1 -order
π 200 1/1004.6210 × 10 4 -5.6532 × 10 4 -
1/1503.6778 × 10 4 1.80454.7654 × 10 4 2.0001
1/2002.9816 × 10 4 1.82578.3680 × 10 5 2.0008
1/2508.8243 × 10 5 1.84667.6328 × 10 5 2.0006
Table 5. The maximum absolute error and spatial convergence order of MFEG iterative scheme at various values of α when τ = 0.001 subject to Example 1.
Table 5. The maximum absolute error and spatial convergence order of MFEG iterative scheme at various values of α when τ = 0.001 subject to Example 1.
h / τ α = 0.65 α = 0.85
h τ e ( τ , h ) γ 2 -order e ( τ , h ) γ 2 -order
1 1000 π 20 3.6532 × 10 3 -2.5443  × 10 3 -
π 40 2.5321 × 10 3 1.92641.7632 × 10 3 2.0023
π 60 5.7423 × 10 4 1.95538.6432 × 10 4 2.0019
π 80 4.6234 × 10 4 1.98237.7425 × 10 4 2.0014
Table 6. The maximum absolute error and spatial convergence order of MFEG iterative scheme at various values of α when τ = 0.001 subject to Example 2.
Table 6. The maximum absolute error and spatial convergence order of MFEG iterative scheme at various values of α when τ = 0.001 subject to Example 2.
h / τ α = 0.70 α = 0.95
h τ e ( τ , h ) γ 2 -order e ( τ , h ) γ 2 -order
1 1000 π 25 3.6743 × 10 3 -7.6843  × 10 4 -
π 45 2.6743 × 10 3 1.90436.7843 × 10 4 2.0034
π 65 9.9743 × 10 4 1.93458.6743 × 10 5 2.0028
π 85 8.6743 × 10 4 1.95847.5843 × 10 5 2.0015
Table 7. The percentages of MFEG method against FSP and FEG methods at α = 0.55 in Example 1.
Table 7. The percentages of MFEG method against FSP and FEG methods at α = 0.55 in Example 1.
MethodExecution Time (sec.)Number of Iterations (Ite.)
FSP(26.20–41.82)%(22.30–32.60)%
FEG(49.60–54.80)%(45.40–56.30)%
Table 8. The percentages of MFEG method against FSP and FEG methods at α = 0.90 in Example 2.
Table 8. The percentages of MFEG method against FSP and FEG methods at α = 0.90 in Example 2.
MethodExecution Time (sec.)Number of Iterations (Ite.)
FSP(23.74–37.24)%(21.64–31.90)%
FEG(44.62–63.25)%(47.20–65.25)%
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Ali, A.; Abdeljawad, T.; Iqbal, A.; Akram, T.; Abbas, M. On Unconditionally Stable New Modified Fractional Group Iterative Scheme for the Solution of 2D Time-Fractional Telegraph Model. Symmetry 2021, 13, 2078. https://doi.org/10.3390/sym13112078

AMA Style

Ali A, Abdeljawad T, Iqbal A, Akram T, Abbas M. On Unconditionally Stable New Modified Fractional Group Iterative Scheme for the Solution of 2D Time-Fractional Telegraph Model. Symmetry. 2021; 13(11):2078. https://doi.org/10.3390/sym13112078

Chicago/Turabian Style

Ali, Ajmal, Thabet Abdeljawad, Azhar Iqbal, Tayyaba Akram, and Muhammad Abbas. 2021. "On Unconditionally Stable New Modified Fractional Group Iterative Scheme for the Solution of 2D Time-Fractional Telegraph Model" Symmetry 13, no. 11: 2078. https://doi.org/10.3390/sym13112078

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