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Modeling Multicellular Systems Using Subcellular Elements

  • Received: 01 April 2005 Accepted: 29 June 2018 Published: 01 August 2005
  • MSC : 92C10, 92C15, 82C31.

  • We introduce a model for describing the dynamics of large numbers of interacting cells. The fundamental dynamical variables in the model are subcellular elements, which interact with each other through phenomenological intra- and intercellular potentials. Advantages of the model include i) adaptive cell-shape dynamics, ii) flexible accommodation of additional intracellular biology, and iii) the absence of an underlying grid. We present here a detailed description of the model, and use successive mean-field approximations to connect it to more coarse-grained approaches, such as discrete cell-based algorithms and coupled partial differential equations. We also discuss efficient algorithms for encoding the model, and give an example of a simulation of an epithelial sheet. Given the biological flexibility of the model, we propose that it can be used effectively for modeling a range of multicellular processes, such as tumor dynamics and embryogenesis.

    Citation: T. J. Newman. Modeling Multicellular Systems Using Subcellular Elements[J]. Mathematical Biosciences and Engineering, 2005, 2(3): 613-624. doi: 10.3934/mbe.2005.2.613

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  • We introduce a model for describing the dynamics of large numbers of interacting cells. The fundamental dynamical variables in the model are subcellular elements, which interact with each other through phenomenological intra- and intercellular potentials. Advantages of the model include i) adaptive cell-shape dynamics, ii) flexible accommodation of additional intracellular biology, and iii) the absence of an underlying grid. We present here a detailed description of the model, and use successive mean-field approximations to connect it to more coarse-grained approaches, such as discrete cell-based algorithms and coupled partial differential equations. We also discuss efficient algorithms for encoding the model, and give an example of a simulation of an epithelial sheet. Given the biological flexibility of the model, we propose that it can be used effectively for modeling a range of multicellular processes, such as tumor dynamics and embryogenesis.


    An important tool for describing the natural process is a system of fractional differential equations [1,2]. An ordinary system of fractional differential equations (FDEs) is described by

    C0Dαt(q(t))=p(t,q(t)),  t[0,a] (1.1)

    where aR, q:[0,a]Rν is a ν-dimensional vector function and p:[0,a]×RνRν. Here, C0Dαt is the Caputo fractional derivative of order α>0.

    FDEs of the form (1.1) are used in an extensive amount of published papers for describing diverse evolutionary processes. Pollution model for lake [3], dynamical models of happiness [4] and Irving-Mullineux oscillaton [5] are among them.

    A system of type (1.1) has at least n=α (ceil of α) degree of freedom due to the presence of n the integer-order derivative. To have a unique solution more information of the system's states is required. In most applied problems this information on the boundary is known. These problems are referred to as boundary value problems. Initial value problems, terminal value problems (TVPs) and Sturm-Liouville problems are among boundary value problems. For initial value problems, the states of the system in the beginning time of the model are known. These states may include derivatives or more complex operators of the modeled process in the initial time. For initial value problems, the states of the system in the beginning time/point of the model are known. These states may include derivatives or more complex operators of the modeled process in the initial time. For terminal value problems, the system's states are known at the end terminal. However, for Sturm-Liouville problems states of the system are known in both initial and end boundaries. These systems have completely different dynamics and behaviors [6].

    Adding boundaries information is not the only way to reduce the degree of freedom. For example, the information in the intermediate point/time can be used [7] for such a reduction. Such problems are known as intermediate value problems.

    Recently, TVPs for fractional systems of the order less than one (0<α<1) have received some extensive attention and interest [8,9,10,11,12,13,14]. These problems can be described by

    Dαq(t)=p(t,q(t)),  t[0,a],q(a)=qa. (1.2)

    where Dα is fractional derivative and qa is a given ν-dimensional vector. At the first glance, these systems seem to be well-posed with regular source functions [15,16]. Surprisingly, Cong and Tuan [17] revealed some counterexamples. The papers [14,18] pointed out that the well-posedness depends on the terminal value a. For larger a we may not obtain a unique solution.

    Surprisingly, TVPs for fractional differential equations of higher-order derivatives α1 are not well-studied. An order α(1,2] problem on an infinite interval have been studied in [19]. These problems have the form

    C0Dαtq(t)=p(t,q(t),q(t)), t[0,M],q()=q,q()=0. (1.3)

    where q()R is a given number and C0Dαt stands for Caputo derivative.

    This paper's important aim is to study the existence results and regularity of the higher-order terminal value problem for systems of FDEs. The other important aim of this paper is to introduce an analyzed high-order numerical method for solving such problems. Thus, the piecewise polynomial collocation method (PPCM) as a numerical solver is introduced and analyzed in detail.

    The PPCMs have some superior advantages in solving differential or integral equations. For example, if we use polynomials collocation methods (known as spectral methods) we may encounter Runge-phenomena. The piecewise characteristic of the PPCMs avoids such probable divergence. In comparison with Runge-Kutta methods, the coefficient and parameters of the given methods are obtained constructively. It is remarkable to mention that for ordinary differential equations PPCMs, for some piecewise polynomial spaces are equivalent to Runge-Kutta methods. Conclusively, having more parameters (collocation parameters, degree of polynomial space, step size, meshing method) for controlling error, complexity and order of convergence makes the PPCMs competitively superior category of methods.

    This paper is organized as follows: In Sections 2 and 3 we obtain the existence and uniqueness of a mild solution for higher-order FDEs. The regularity for the linear case is studied in Section 4. A numerical method is introduced in Section 5 and analysand in Section 6. Supportive numerical experiments are given in Section 7.

    Consider the system (1.1) with terminal values

    q(a)=q(0)a,Dq(a)=q(1)a,D(n1)q(a)=q(n1)a (2.1)

    where n1<α<n and nN. The ν-dimensional vector function q=[q1,,qν] is an unknown vector and q(i)aRν (i=0,,n1) are known vectors.

    Further, we impose the Lipschitz condition on components of the function p:[0,a]×RνRν. Thus, we suppose

    |pi(t,q1)pi(t,q2)|Liq1q1,q1,q2Rν

    where Li (i=0,,ν) are constants and are not depend on t. Let z=q(n1), (z=q(n)). Taking repeatedly integrals and using terminal values, we obtain

    q(t)=n2i=0(ta)ii!(q(i)aa0(ax)n2i(n2i)!z(x)dx)+t0(tx)n2(n2)!z(x)dx. (2.2)

    By definition of Caputo derivative, we have

    C0Dαtq(t)=C0Dαn+1tDn1q(t)=C0Dαn+1tz.

    Acting Riemann-Liouville integral 0Jαn+1t on both sides of Eq (1.1), we obtain

    z(t)z(0)=0Jαn+1tf(t,q(t)). (2.3)

    Finally, putting t=a and using terminal conditions, we obtain

    z(t)=1Γ(αn+1)(a0p(x,q(x))(ax)nαdxt0p(x,q(x))(tx)nαdx)+q(n1)a. (2.4)

    Remark 1. The solution of the coupled system of (2.2) and (2.4) can be regarded as a mild solution of the system (2.1).

    Since we use vector functions, we need a norm combined with vector norm and function norm. This combinations brings us to face complexity in calculating induced norm. In this respect, the max norm defined by

    q=max

    seems to be more easier. We establish well-posedness of the inverse problems (1.1) and (2.1). We define the operators \mathcal{P} and \mathcal{Q}:(\mathcal{C}[0, a])^{2\nu} \rightarrow (\mathcal{C}[0, a])^\nu by the right hand sides of systems (2.2) and (2.4), i. e.,

    \begin{equation} \begin{split} \mathcal{P}([\bf{q},\bf{z}])(t) = &\sum\limits_{i = 0}^{n-2}\frac{(t-a)^i}{i!}\left(\bf{q}^{(i)}_{a}-\int_0^a\frac{(a-x)^{n-2-i}}{(n-2-i)!}\bf{z}(x)dx\right)\\ &+\int_0^t \frac{(t-x)^{n-2}}{(n-2)!}\bf{z}(x)dx \end{split} \end{equation} (3.1)

    and

    \begin{equation} \begin{split} \mathcal{Q}([\bf{q},\bf{z}])(t) = &\bf{q}^{(n-1)}_a-\frac{1}{\Gamma(\alpha-n+1)}\int_0^a \frac{\bf{p}(x,\bf{q}(x))}{(a-x)^{n-\alpha}}dx \\ &+\frac{1}{\Gamma(\alpha-n+1)}\int_0^t \frac{\bf{p}(x,\bf{q}(x))}{(t-x)^{n-\alpha}}dx. \end{split} \end{equation} (3.2)

    Let \mathcal{P}_i and \mathcal{Q}_i:(\mathcal{C}[0, a])^{2\nu} \rightarrow \mathcal{C}[0, a] be the i th component of the operator \mathcal{P} and \mathcal{Q}, respectively. Setting \bf{w} = [\bf{q}, \bf{z}] and defining the operator \mathcal{T}:\mathbb{R}^{2\times \nu}\rightarrow \mathbb{R}^{2\times \nu} by

    \mathcal{T}\bf{w} = [\mathcal{P}\bf{w},\mathcal{Q}\bf{w}],

    the Eqs (2.2) and (2.4) can be compactly written as

    \begin{equation} \bf{w} = \mathcal{T}\bf{w}. \end{equation} (3.3)

    It is straightforward to show that for \bf{w}_1 and \bf{w}_2\in (\mathcal{C}[0, a])^{2\nu}. We can write

    \begin{equation} \begin{split} |\mathcal{P}_i(\bf{w}_1)(t)-\mathcal{P}_i(\bf{w}_2)(t)| &\leq \frac{2t^{n-1}}{(n-1)!} \|\bf{w_1}-\bf{w}_2\|_{\infty}. \end{split} \end{equation} (3.4)

    and

    \begin{equation} \begin{split} |\mathcal{Q}_i(\bf{w}_1)(t)-\mathcal{Q}_i(\bf{w_2})(t)| &\leq \frac{2L_Ma^{\alpha-n+1}}{\Gamma(\alpha-n+2)}\|\bf{w_1}-\bf{w}_2\|_{\infty}.\\ \end{split} \end{equation} (3.5)

    where L_M = \max_{i = 1, \ldots, \nu} L_i. Now, the Eqs (3.4) and (3.5) give

    \begin{equation} \|\mathcal{T}\bf{w}_1-\mathcal{T}\bf{w}_2\|_{\infty}\leq \max\{ \frac{2a^{n-1}}{(n-1)!} , \frac{2L_Ma^{\alpha-n+1}}{\Gamma(\alpha-n+2)} \}\|\bf{w_1}-\bf{w}_2\|_{\infty}. \end{equation} (3.6)

    Conclusively, we can estate the following theorem.

    Theorem 3.1. Let each component of the continuous function \bf{p}:[0, a]\times \mathbb{R}^{\nu}\rightarrow \mathbb{R}^{\nu} ( \nu\in \mathbb{N} ) satisfy the Lipschitz condition with the Lipschitz constant L_i and let

    L_M = \max\limits_{i = 1,\cdots,\nu}\{L_i\}.

    Then, the problem (1.1) with terminal conditions (2.1) has a unique mild solution on (\mathcal{C}[0, a])^{2\nu} if

    \begin{equation} \lambda: = \max\{ \frac{2a^{n-1}}{(n-1)!} , \frac{2L_Ma^{\alpha-n+1}}{\Gamma(\alpha-n+2)} \} < 1 \end{equation} (3.7)

    Proof. Suppose \bf{w}\in (\mathcal{C}[0, a])^{2\nu}. Since all integral operators involving in the definition of \mathcal{T} transform a continuous functions into a continuous functions, therefore, \mathcal{T}(\bf{w})\in (\mathcal{C}[0, a])^{2\nu}. The operator \mathcal{T} is contractor by (3.6) and the space (\mathcal{C}[0, a])^{2\nu} is a Banach space by the norm \|.\|_{\infty}. Thus, by contraction mapping theorem \bf{w} = \mathcal{T}(\bf{w}) has a unique solution which completes the proof.

    The next corollary is an important result of Theorem 3.1 which shows the regularity of the solution on more smooth spaces.

    Corollary 1. Suppose the hypotheses of Theorem 3.1 are satisfied. Then, the mild solution \bf{q} obtained from solving systems (2.2) and (2.4) satisfies the system (1.1) with terminal conditions (2.1). Moreover,

    \bf{q}\in (\mathcal{C}^{n-1}[0,a])^{\nu}.

    Proof. Taking derivative from Eq (2.2) and using Theorem 3.1 results \bf{q}^{(n-1)} = \bf{z}\in (\mathcal{C}[0, a])^{\nu}. Thus, \bf{q}\in (\mathcal{C}^{n-1}[0, a])^{\nu}. Similarly, putting t = a in Eq (2.2) and its derivatives, proves that \bf{q} satisfies terminal conditions. Replacing \bf{z} = \bf{q}^{(n-1)} in (2.2) we obtain

    \begin{equation} \begin{split} \bf{q}^{(n-1)} = &\bf{q}^{(n-1)}_a-\frac{1}{\Gamma(\alpha-n+1)}\int_0^a \frac{\bf{p}(x,\bf{q}(x))}{(a-x)^{n-\alpha}}dx\\ &+ {_a \mathcal{J}_t^{\alpha-n+1}} \bf{p}(x,\bf{q}(x)) \end{split} \end{equation} (3.8)

    where {_a \mathcal{J}_t^{\alpha-n+1}} is the Riemann-Liouville fractional integral. Noting that \alpha-n+1 > 0 , we can take a fractional derivative of order \alpha-n+1 from (3.8) to obtain

    \begin{equation} \begin{split} {^C_0D_t^{\alpha-n+1}}\bf{q}^{(n-1)} = {^C_0D_t^{\alpha-n+1}}{_a \mathcal{J}_t^{\alpha-n+1}} \bf{p}(x,\bf{q}(x)) = \bf{p}(x,\bf{q}(x)) \end{split} \end{equation} (3.9)

    which shows that the component \bf{q} of the mild solutions satisfies (1.1).

    The regularity of the solution is important for analyzing numerical methods, especially finite difference methods and methods based on projection [20]. The regularity speaks about the order of differentiability of solutions. Usually, the regularity is investigated in the space \mathcal{C}^m[a, b], (see Corollary 1). But, some good functions such as \sqrt{t}\in \mathcal{C}[a, b] do not belong to \mathcal{C}^m[a, b]. The space \mathcal{C}^m(a, b]\cap \mathcal{C}[a, b] contains such functions. This space is not Banach or complete. Therefore, we need to introduce another Banach space such that

    \mathcal{C}^m[a,b]\subset X\subset \mathcal{C}^m(a,b]\cap \mathcal{C}[a,b].

    In this paper, we study regularity on the following weighted space {\mathcal{C}}^{m, \alpha}(0, a] introduced in [13].

    Definition 4.1. [13] Let 0\leq \alpha < 1 and m\in \mathbb{N}. Then q\in {\mathcal{C}}^{m, \alpha}(0, a] if there exist functions q_i\in {\mathcal{C}}[0, a] for i = 0, \cdots, m+1 such that q = t^{\alpha} q_0+q_1 and

    D^{i}q(t) = t^{\alpha-i}q_{i+1}(t),\ \ i = 1,\cdots,m.

    Theorem 4.2. The space {\mathcal{C}}^{m, \alpha}(0, a] with the norm

    \begin{equation} \|q\|_{\alpha,m}: = \|q\|_{\infty}+\sum\limits_{i = 1}^{m}\|q_{i+1}\|_{\infty} \end{equation} (4.1)

    is a Banach space.

    Proof. Let {q_{n}}\in {\mathcal{C}}^{m, \alpha}(0, a], n\in\mathcal{N} be a Cauchy sequence with norm \|.\|_{\alpha, m}. Thus, by the definition of {\mathcal{C}}^{m, \alpha}(0, a] there exists functions q_{n, i} in \mathcal{C}[0, a] for i = 0, \cdots, m+1 such that q_{n}(t) = t^{\alpha} q_{n, 0}(t)+q_{n, 1}(t) and

    D^{i}q_{n}(t) = t^{\alpha-i}q_{n,i+1}(t),\ i = 1,\cdots,m, \ t\in(0,a].

    From the definition of the norm \|.\|_{\alpha, m}, the sequences q_{n, i} for a fixed i are Cauchy sequence in the Banach space \mathcal{C}[0, a] and thus have a unique limit say q_{i}. Let q defined by q(t) = t^{\alpha} q_0(t)+q_1(t) on [0, a]. Following items show that q\in {\mathcal{C}}^{m, \alpha}(0, a].

    \lim_{n\rightarrow \infty} q_n(t) = \lim_{n\rightarrow \infty} t^{\alpha} q_{n, 0}(t)+q_{n, 1}(t) = t^{\alpha} q_0(t)+q_1(t) = q for all t\in [a, b];

    q\in \mathcal{C}[0, a], since q_0\in \mathcal{C}[0, a] and q_1\in \mathcal{C}[0, a];

    \lim_{n\rightarrow \infty} D^{i}q_n(t) = \lim_{n\rightarrow \infty} t^{\alpha-i}q_{n, i+1}(t) = t^{\alpha-i}q_{i+1}(t). For each t\in(a, b] we can find \epsilon > 0 such that D_{\epsilon} = [t-\epsilon, t]\subset (a, b]. It is trivial that D^{i}q_n(t) converges uniformly to t^{\alpha-i}q_{i+1}(t) on D_{\epsilon} . According to Theorem 7.17 of [21] D^{i}q(t) = \lim_{n\rightarrow \infty} D^{i}q_n(t) on D_{\epsilon}. Thus D^{i}q(t) = t^{\alpha-i}q_{i+1}(t) for all t\in D_\epsilon and hence for all t\in (a, b].

    Let \nu\in \mathbb{N}. For a \nu dimensional vector functions, \bf{p} = [f_1, \ldots, f_{\nu}] in ({\mathcal{C}}^{m, \alpha}(0, a]\subset ({\mathcal{C}}^{m}(0, a])^{r}, we use the max norm defined by

    \|\bf{p}\| = \max\limits_{i = 1,\ldots,\nu}\|f_i\|_{\alpha,m}.

    The system (1.1) with

    \begin{equation} \bf{p}(t,\bf{q}(t)) = A(t)\bf{q}(t)+\bf{b}(t), \ \ t\in [0,a], \end{equation} (4.2)

    is a system of linear FDEs. Here A is a given \nu\times \nu dimensional matrix function and \bf{b}\in (\mathcal{C}[0, a])^\nu is a given source function. To study linear systems we introduce the operators \mathcal{W}_1 and \mathcal{W}_2:(\mathcal{C}[0, a])^{2\nu} \rightarrow (\mathcal{C}[0, a])^\nu by

    \begin{equation} \begin{split} \mathcal{W}_1([\bf{q},\bf{z}])(t) = &-\sum\limits_{i = 0}^{n-2}\frac{(t-a)^i}{i!}\left(\int_0^a\frac{(a-x)^{n-2-i}}{(n-2-i)!}\bf{z}(x)dx\right)\\ &+\int_0^t \frac{(t-x)^{n-2}}{(n-2)!}\bf{z}(x)dx, \end{split} \end{equation} (4.3)

    and

    \begin{equation} \begin{split} \mathcal{W}_2([\bf{q},\bf{z}])(t) = &-\frac{1}{\Gamma(\alpha-n+1)}\int_0^a \frac{A(x)\bf{q}(x)}{(a-x)^{n-\alpha}}dx \\ &+\frac{1}{\Gamma(\alpha-n+1)}\int_0^t \frac{A(x)\bf{q}(x)}{(t-x)^{n-\alpha}}dx. \end{split} \end{equation} (4.4)

    Let us also define the vector valued functions \mathcal{G}_2 and \mathcal{G}_1:[0, a] \rightarrow \mathbb{R}^\nu by

    \begin{equation} \begin{split} \mathcal{G}_1(t) = &\sum\limits_{i = 0}^{n-2}\frac{(t-a)^i}{i!}\left(\bf{q}^{(i)}_{a}\right), \end{split} \end{equation} (4.5)

    and

    \begin{equation} \begin{split} \mathcal{G}_2(t) = &\bf{q}^{(n-1)}_a-\frac{1}{\Gamma(\alpha-n+1)}\int_0^a \frac{\bf{b}(x)}{(a-x)^{n-\alpha}}dx \\ &+\frac{1}{\Gamma(\alpha-n+1)}\int_0^t \frac{\bf{b}(x)}{(t-x)^{n-\alpha}}dx. \end{split} \end{equation} (4.6)

    Let \bf{T} = [\mathcal{W}_1, \mathcal{W}_2]^T and \mathcal{G} = [\mathcal{G}_1, \mathcal{G}_2]^T . Then, the Eqs (2.2) and (2.4) can be written as an inhomogeneous system

    \begin{equation} \bf{w}-\bf{T}(\bf{w}) = \mathcal{G} \end{equation} (4.7)

    where \bf{w} = [\bf{q}, \bf{z}]^T.

    Theorem 4.3. Let a\in\mathbb{R} and \alpha > 0. Assume each component of A and b are in {\mathcal{C}}^{m, \alpha}(0, a]) and the hypotheses of Theorem 3.1 are satisfied for related \bf{p}:[0, a]\times \mathbb{R}^{\nu}\rightarrow \mathbb{R}^{\nu} ( \nu\in \mathbb{N} ).Then, the problem (1.1) with terminal conditions (2.1) has a unique mild solution on ({\mathcal{C}}^{m, \alpha}(0, a])^{2\nu}.

    Proof. Since \bf{T} is a combination of weakly singular integral operators, it is a compact linear operator on (\mathcal{C}[0, a])^{2\nu} and ({\mathcal{C}}^{m, \alpha}(0, a])^{2\nu} . Also, it is clear that

    \bf{T}({\mathcal{C}}^{m,\alpha}(0,a])^{2\nu})\subset ( {\mathcal{C}}^{m,\alpha}(0,a])^{2\nu}.

    System (25) has a unique solution on (\mathcal{C}[0, a])^{2\nu} by Theorem 3.1. Therefore, the homogeneous system \bf{w}-\bf{T}(\bf{w}) = 0 has the trivial null space in (\mathcal{C}[0, a])^{2\nu} and thus ({\mathcal{C}}^{m, \alpha}(0, a])^{2\nu}. Conclusively, alternative Fredholm theorem asserts that the system (4.7) has a unique solution on ({\mathcal{C}}^{m, \alpha}(0, a])^{2\nu}.

    Remark 2. Regularity of the nonlinear case needs further investigations.

    Example 1. Consider the system (1.1) with a = 0.5, \alpha = 2.5 and \bf{p} defined by (4.2)

    A = \left(\begin{array}{cc} 0 & 0.5 \\ 0.5 & 0 \end{array}\right),\ \ \ \bf{b}(t) = \left(\begin{array}{cc} 1 \\ t \end{array}\right).

    Obviously, L_1 = 0.5, L_2 = 0.5. and thus L_M = 0.5. Therefore,

    \max\{ \frac{2a^{n-1}}{(n-1)!} , \frac{2L_Ma^{\alpha-n+1}}{\Gamma(\alpha-n+2)} \} = 0.7979 < 1

    and Condition (3.7) holds. By Theorem 3.1 the terminal value problem (1.1) with arbitrary terminal value (2.1) has a unique solution on \mathcal{C}[0, a] . Since all components of A and \bf{b} belong to {\mathcal{C}}^{m, \alpha}(0, a], ( m\in\mathbb{N} ) the mild solution belongs to ({\mathcal{C}}^{m, \alpha}(0, a])^4, by Theorem 4.3. Furthermore, we obtain the regularity of the solution of the system (1.1) on the closed interval [0, a] by Corollary 1 and we have

    \bf{q} = (\mathcal{C}^{2}[0,a])^2.

    Considering the memory, one of the best methods for solving the coupled systems (2.2)–(2.4) is to use collocation methods on piecewise polynomial spaces. To implement such methods we partition the solution interval [0, a] into sub-intervals \sigma_i = [t_{i}, t_{i+1}], i = 0, \ldots, N-1, with length h_i: = t_{i+1}-t_i where 0 = t_0 < \ldots < t_{N} = a are nodes of a chosen mesh (uniform or graded mesh) and N\in \mathbb{N}. A graded mesh with exponent r\geq1 is described by

    t_i = a\left(\frac{i}{N}\right)^r,\ \ \ i = 0,\ldots,N.

    Let 0 < c_1 < \ldots < c_m\leq 1 ( m\in\mathbb{N} ) be collocation parameters, t_{n, i} = t_n+c_ih_n ( n = 0, \ldots, N-1 ) be collocation points and let \hat{\bf{q}}_N(t) and \hat{\bf{z}}_N(t) be approximate solutions. The restriction of approximate functions to the \sigma_k is fully determined by Lagrange polynomials interpolation formula

    \begin{equation} \hat{\bf{q}}_N(t){\big|}_{\sigma_k} = \hat{\bf{q}}_N(t_k+hs) = \sum\limits_{j = 1}^m Q_{n,j}L_j(s),\; s\in(0,1] \end{equation} (5.1)

    and

    \begin{equation} \hat{\bf{z}}_N(t){\big|}_{\sigma_k} = \hat{\bf{z}}_N(t_k+hs) = \sum\limits_{j = 1}^m Z_{n,j}L_j(s),\; s\in(0,1] \end{equation} (5.2)

    where Q_{k, j} = \hat{\bf{q}}_N(t_{n, j}), Z_{k, j} = \hat{\bf{z}}_N(t_{k, j}), t_{k, j} = t_k+hc_j and L_j ( j = 1, \ldots, m ) are Lagrange polynomials of degree m-1. The integrals in the operators \mathcal{P} and \mathcal{Q} of systems (3.1) and (3.2) can be discretized as:

    \begin{equation} \begin{split} \int_0^a\frac{(a-x)^{n-2-i}}{(n-2-i)!}\hat{\bf{z}}_N(x)dx = \sum\limits_{l = 0}^{N-1}\sum\limits_{j = 1}^{m}h_l\gamma_{n,i,l,j}Z_{l,j} \end{split} \end{equation} (5.3)

    where

    \gamma_{n,i,l,j} = \int_{0}^{1}\frac{(a-t_l-sh_l)^{n-2-i}}{(n-2-i)!}L_j(s)ds.

    For t\in [t_k, t_{k+1}] ( k = 0, \ldots, N-1 ) we have

    \begin{equation} \begin{split} \int_0^t \frac{(t-x)^{n-2}}{(n-2)!}\hat{\bf{z}}_N(x)dx = \sum\limits_{l = 0}^{k-1}h_l\sum\limits_{j = 1}^{m}\eta_{n,l,j}(v)Z_{l,j}+h_k\sum\limits_{j = 1}^{m}\bar{\eta}_{n,k,j}(v)Z_{k,j}\\ \end{split} \end{equation} (5.4)

    where

    v = \frac{t-t_k}{h_k}\in [0,1],
    \eta_{n,k,l,j}(v) = \int_{0}^{1}\frac{(t_k-t_l+vh_k-sh_l)^{n-2}}{(n-2)!}L_j(s)ds

    and

    \bar{\eta}_{n,k,j}(v) = \int_{0}^{v}\frac{((v-s)h_k)^{n-2}}{(n-2)!}L_j(s)ds.

    Similarly, we discretize integrals of the operator \mathcal{Q}. We have

    \begin{equation} \begin{split} \int_0^a \frac{\bf{p}(x,\hat{\bf{q}}_N(x))}{(a-x)^{n-\alpha}}dx = \sum\limits_{l = 0}^{N-1}h_l\int_{0}^{1} \frac{\bf{p}(t_l+sh_l,\hat{\bf{q}}_N(t_l+sh_l))}{(a-t_l-sh_l)^{n-\alpha}}ds. \end{split} \end{equation} (5.5)

    By interpolating \bf{p}(t_l+sh_l, \bf{q}(t_l+sh_l)) on c_i we obtain

    \bf{p}(t_l+sh_l,\hat{\bf{q}}_N(t_l+sh_l))\approx\sum\limits_{j = 1}^m \bf{p}(t_{l,j},Q_{l,j})L_j(s)

    and thus

    \begin{equation} \begin{split} \int_0^a \frac{\bf{p}(x,\hat{\bf{q}}_N(x))}{(a-x)^{n-\alpha}}dx \approx\sum\limits_{l = 0}^{N-1}h_l \sum\limits_{j = 1}^m \bf{p}(t_{l,j},Q_{l,j}) \varrho_{n,l,j}\\ \end{split} \end{equation} (5.6)

    where

    \varrho_{n,l,j} = \int_{0}^{1} \frac{L_j(s)}{(a-t_l-sh_l)^{n-\alpha}}ds

    and finally

    \begin{equation} \begin{split} \int_0^t \frac{\bf{p}(x,\hat{\bf{q}}_N(x))}{(t-x)^{n-\alpha}}dx\approx&\sum\limits_{l = 0}^{k-1} h_l \sum\limits_{j = 1}^m \bf{p}(t_{l,j},Q_{l,j})\zeta_{n,l,j}\\ & +h_k \sum\limits_{j = 1}^m \bf{p}(t_{k,j},Q_{k,j}) \bar{\zeta}_{n,k,j}(v) \end{split} \end{equation} (5.7)

    where

    \zeta_{n,l,j}(v) = \int_{0}^{1} \frac{L_j(s)}{(t-t_l-sh_l)^{n-\alpha}}ds,
    \bar{\zeta}_{n,k,j}(v) = \int_{0}^{v} \frac{L_j(s)}{((v-s)h_k)^{n-\alpha}}ds.

    The discretized mappings \mathcal{P}_N and \mathcal{Q}_N:(\mathcal{C}[0, a])^{2\nu} \rightarrow (PC[0, a])^\nu ( PC stands for piecewise continuous space) related to systems (3.1) and (3.2) can be defined by

    \begin{equation} \begin{split} \mathcal{P}_N([\hat{\bf{q}}_N(t),\hat{\bf{z}}_N])(t) = &\sum\limits_{i = 0}^{n-2}\frac{(t-a)^i}{i!}\left(\bf{q}^{(i)}_{a}-\sum\limits_{l = 0}^{N-1}h_l\sum\limits_{j = 1}^{m}\gamma_{n,i,l,j}Z_{l,j}\right)\\ &+\sum\limits_{l = 0}^{k-1}h_l\sum\limits_{j = 1}^{m}\eta_{n,l,j}(v)Z_{l,j}+h_k\sum\limits_{j = 1}^{m}\bar{\eta}_{n,k,j}(v)Z_{k,j} \end{split} \end{equation} (5.8)

    and

    \begin{equation} \begin{split} \mathcal{Q}_N&([\hat{\bf{q}}_N,\hat{\bf{z}}_N])(t) = \bf{q}^{(n-1)}_a-\frac{1}{\Gamma(\alpha-n+1)}\sum\limits_{l = 0}^{N-1}h_l \sum\limits_{j = 1}^m \bf{p}(t_{l,j},Q_{l,j}) \varrho_{n,l,j} \\ &+\sum\limits_{l = 0}^{k-1} h_l \sum\limits_{j = 1}^m \frac{\bf{p}(t_{l,j},Q_{l,j})\zeta_{n,l,j} (v)}{\Gamma(\alpha-n+1)}+h_k \sum\limits_{j = 1}^m \frac{\bf{p}(t_{k,j},Q_{k,j}) \bar{\zeta}_{n,k,j}(v)}{\Gamma(\alpha-n+1)}. \end{split} \end{equation} (5.9)

    on \sigma_k. Setting \mathcal{T}_N = [\mathcal{P}_N, \mathcal{Q}_N], unknowns vectors Q_{l, j} and Z_{l, j} can be obtained by solving the nonlinear system

    \begin{equation} \mathcal{T}_N ([\hat{\bf{q}}_N(t_{k,o}),\hat{\bf{z}}_N(t_{o,p})]) = [\hat{\bf{q}}_N(t_{k,o}),\hat{\bf{z}}_N(t_{k,o})] \end{equation} (5.10)

    for k = 0, \ldots, N-1 and o = 1, \ldots, m. Taking into account that

    [Q_{k,o},Z_{k,o}] = [\hat{\bf{q}}_N(t_{k,o}),\hat{\bf{z}}_N(t_{k,o})],

    the dense solution can be evaluated in all points of the desired interval by Eqs (5.1) and (5.2). We note that the six parameters \gamma_{n, i, l, j}, \eta_{n, l, j}, \bar{\eta}_{n, k, j}, \varrho_{n, l, j}, \zeta_{n, l, j} and \bar{\zeta}_{n, k, j} fully determines the method for each m . The equations of these six parameters for m = 1 and m = 2 are provided in Tables 1 and 2, respectively.

    Table 1.  The coefficient of the collocation method of order m = 1..
    parameter j=1, i=0, \ldots, n-2, l=0, \ldots, k-1, k=0, \ldots, N-1
    L_j(s) 1
    \gamma_{n, i, l, j} \left((a-t_l)^{n-1-i}-(a-t_l-h_l)^{n-1-i}\right)/\left(h_l(n-1-i)!\right)
    \eta_{n, k, l, j}(v) \left((t_k-t_l+vh_k)^{n-1}-(t_k-t_l+vh_k-h_l)^{n-1}\right)/\left(h_l(n-1)!\right)
    \bar{\eta}_{n, k, j}(v) \left(vh_k\right)^{n-1}/\left(h_k(n-1)!\right)
    \varrho_{n, l, j} \left((a-t_l)^{\alpha-n+1}-(a-t_l-h_l)^{\alpha-n+1})\right)/\left(h_l(\alpha-n+1)\right)
    \zeta_{n, l, j}(v) \left((t_k+vh_k-t_l)^{\alpha-n+1}-(t_k+vh_k-t_l-h_l)^{\alpha-n+1})\right)/\left(h_l(\alpha-n+1)\right)
    \bar{\zeta}_{n, k, j}(v) \left(vh_k\right)^{\alpha-n+1}/\left(h_k(\alpha-n+1)\right)

     | Show Table
    DownLoad: CSV
    Table 2.  The coefficient of the collocation method of order m = 2. Here, we used \varpi_k = t_k+vh_k-t_l and \Theta = a-t_l for simplifying the presentation of formulas.
    parameter j=1, 2 i=0, \ldots, n-2, l=0, \ldots, k-1, k=0, \ldots, N-1
    L_j(s) \frac{(s-c_{3-j})(-1)^{j}}{c_2-c_1}
    \gamma_{n, i, l, j} \frac{(-1)^{j+1}}{(n-2-i)!h_l^2(c_2-c_1)}\left((\Theta-c_{3-j}h_l)\frac{(\Theta-h_l)^{n-1-i}-\Theta^{n-1-i}}{n-1-i}-\frac{(\Theta-h_l)^{n-i}-\Theta^{n-i}}{n-i}\right)
    \eta_{n, k, l, j}(v) \frac{(-1)^{j+1}}{(n-2)!h_l^2(c_2-c_1)}\left((\varpi_k-c_{3-j}h_l)\frac{(\varpi_k-h_l)^{n-1}-\varpi_k^{n-1}}{n-1}-\frac{(\varpi_k-h_l)^{n}-\varpi_k^{n}}{n}\right)
    \bar{\eta}_{n, k, j}(v) \frac{(-1)^{j}}{(n-2)!h_k^2(c_2-c_1)}\left((vh_k-c_{3-j}h_k)\frac{(vh_k)^{n-1}}{n-1}-\frac{(vh_k)^{n}}{n}\right)
    \varrho_{n, l, j} \frac{(-1)^{j+1}}{(c_2-c_1)h_l^2}\left((\Theta-h_lc_{3-j})\frac{(\Theta-h_l)^{\alpha-n+1}-\Theta^{\alpha-n+1}}{\alpha-n+1}-\frac{(\Theta-h_l)^{\alpha-n+2}-\Theta^{\alpha-n+2}}{\alpha-n+2}\right)
    \zeta_{n, l, j}(v) \frac{(-1)^{j+1}}{(c_2-c_1)h_l^2}\left((\varpi_k-c_{3-j}h_l)\frac{(\varpi_k-h_l)^{\alpha-n+1}-\varpi_k^{\alpha-n+1}}{\alpha-n+1}-\frac{(\varpi_k-h_l)^{\alpha-n+2}-(\varpi_k)^{\alpha-n+2}}{\alpha-n+2}\right)
    \bar{\zeta}_{n, k, j}(v) \frac{(-1)^{j}}{(c_2-c_1)h_k^2}\left((vh_k-c_{3-j}h_k)\frac{(vh_k)^{\alpha-n+1}}{\alpha-n+1}-\frac{(vh_k)^{\alpha-n+2}}{\alpha-n+2}\right)

     | Show Table
    DownLoad: CSV

    For simplifying our analysis we recall some notations. Let S_{m-1}^{-1}(I_h) be the space of piecewise polynomials of degree less than m, ( m\in \mathbb{N} ) on the mesh partitioning I_h = \{t_i:\; i = 0, \cdots, N\}. The projection operator \Pi_{m-1, N}:({\mathcal{C}}[0, a])^{2\nu}\rightarrow \left(S_{m-1}^{-1}(I_h)\right)^{2\nu} is uniquely determined by interpolation on collocation points such that

    \Pi_{m-1,N} (\bf{q}(t_{n,i})) = \bf{q}(t_{n,i}),\; n = 0,\ldots,N-1,\; i = 1,\ldots,m,\; \forall\; \bf{q} \in \left({\mathcal{C}}[0,a]\right)^{2\nu}.

    Since \hat{\bf{w}}_N(t): = [\hat{\bf{q}}_N(t), \hat{\bf{z}}_N(t)]\in \left(S_{m-1}^{-1}(I_h)\right)^{2\nu} we have

    \Pi_N (\hat{\bf{w}}_N(t)) = \hat{\bf{w}}_N(t).

    Thus, Eq (5.10) can be written as

    \begin{equation} \Pi_{m-1,N} \mathcal{T}_N (\hat{\bf{w}}_N(t)) = \hat{\bf{w}}_N(t), \ \ \hat{\bf{w}}_N(t) \in \left(S_{m-1}^{-1}(I_h)\right)^{2\nu}. \end{equation} (6.1)

    A useful theorem regarding \Pi_{m-1, N} that simplifies existence and convergence analysis is the following theorem.

    Theorem 6.1. Let m, N\in\mathbb{N}. Then, \Pi_{m-1, N} is a bounded linear operator. Let

    \Lambda = \|\Pi_{m-1,N}\|

    be induced norm of \Pi_{m-1, N} and

    \begin{equation} \Lambda_1 = \max\limits_{t\in[0,1]}\sum\limits_{i = 1}^m|L_i(s)|. \end{equation} (6.2)

    Then, \Lambda\leq \Lambda_1 and

    \|\Pi_{m-1,N}\bf{q} \|_{\infty}\leq \Lambda\|\bf{q}\|_{\infty}.

    Proof. In each sub-interval \sigma_n of [0, a] by Lagrange interpolation formula, we have

    \Pi_{m-1,N}\bf{q}(t_n+sh_n) = \sum\limits_{i = 1}^mL_i(s)\bf{q}_{n,i},\ s\in [0,1].

    The rest of the proof is straightforward by taking the max norm.

    One of the most fundamental questions is whether the system (6.1) has a unique solution? The answer is affirmative. For \hat{\bf{w}}_N(t) in \left(S_{m-1}^{-1}(I_h)\right)^{2\nu} the operators \mathcal{P}_N of (5.8) and \mathcal{P} of (3.1) are equivalent and we have

    \begin{equation} \mathcal{P}_N(\hat{\bf{w}}_N(t)) = \mathcal{P}(\hat{\bf{w}}_N(t)). \end{equation} (6.3)

    Thus, the inequality (3.4) holds for \mathcal{P}_N and

    \begin{equation} \begin{split} |(\mathcal{P}_N)_i \bf{w}_1-(\mathcal{P}_N)_i \bf{w}_2| &\leq \frac{2t^{n-1}}{(n-1)!} \|\bf{w}_1-\bf{w}_2\|_{\infty} \end{split} \end{equation} (6.4)

    for all \bf{w}_1, \bf{w}_2\in\left(S_{m-1}^{-1}(I_h)\right)^{2\nu}. However, \mathcal{Q}_N is different from \mathcal{Q} in this space and we need further computing. Actually, \mathcal{Q}_N can be described by

    \begin{equation} \begin{split} \mathcal{Q}_N(\bf{w})(t) = &\bf{q}^{(n-1)}_a-\frac{1}{\Gamma(\alpha-n+1)}\int_0^a \frac{\Pi_{m-1,N}\bf{p}(s,\bf{q}(s))}{(a-s)^{n-\alpha}}ds \\ &+\frac{1}{\Gamma(\alpha-n+1)}\int_0^t \frac{\Pi_{m-1,N}\bf{p}(s,\bf{q}(s))}{(t-s)^{n-\alpha}}ds. \end{split} \end{equation} (6.5)

    where \bf{q} is the first \nu element of \bf{w}. More precisely

    \begin{equation} \begin{split} \|&\mathcal{Q}_N(\bf{w}_1)-\mathcal{Q}_N(\bf{w}_2)\|_{\infty} = \\ &\frac{1}{\Gamma(\alpha-n+1)}\int_0^a \frac{1}{(a-s)^{n-\alpha}}ds \|\Pi_{m-1,N}\bf{p}(.,\bf{q}_1)-\Pi_{m-1,N}\bf{p}(.,\bf{q}_2)\|_{\infty} \\ &+\frac{1}{\Gamma(\alpha-n+1)}\int_0^t \frac{1}{(t-s)^{n-\alpha}}ds \|\Pi_{m-1,N}\bf{p}(.,\bf{q}_1)-\Pi_{m-1,N}\bf{p}(.,\bf{q}_2)\|_{\infty}\\ \leq & \frac{2a^{\alpha-n+1}}{\Gamma(\alpha-n+2)}\|\Pi_{m-1,N}\|_{\infty} \|\bf{p}(.,\bf{q}_1)-\bf{p}(.,\bf{q}_2)\|_{\infty}\\ \leq & \frac{2a^{\alpha-n+1}\Lambda L_M}{\Gamma(\alpha-n+2)}\|\bf{q}_1-\bf{q}_2\|_{\infty}. \end{split} \end{equation} (6.6)

    Therefore,

    \begin{equation} \begin{split} \|\Pi_{m-1,N}& \mathcal{T}_N (\bf{w}_1)-\Pi_{m-1,N} \mathcal{T}_N (\bf{w}_2)\|_{\infty} \leq \Lambda \| \mathcal{T}_N (\bf{w}_1)-\mathcal{T}_N (\bf{w}_2)\|_{\infty}\\ &\leq \Lambda \max\left\{\frac{2a^{\alpha-n+1}\Lambda L_M}{\Gamma(\alpha-n+2)},\frac{2a^{n-1}}{(n-1)!}\right\}\|\bf{w}_1-\bf{w}_2\|_{\infty}. \end{split} \end{equation} (6.7)

    Theorem 6.2. Let

    \begin{equation} \lambda_\Lambda: = \max\left\{\frac{2a^{\alpha-n+1}\Lambda^2 L_M}{\Gamma(\alpha-n+2)},\frac{2a^{n-1}\Lambda}{(n-1)!}\right\}\leq 1. \end{equation} (6.8)

    Then, the numerical solution of system (1.1) obtained by (6.1) exists and is unique.

    Proof. The operator \Pi_{m-1, N} \mathcal{T}_N:\left(S_{m-1}^{-1}(I_h)\right)^{2\nu}\rightarrow \left(S_{m-1}^{-1}(I_h)\right)^{2\nu} is a contractor by (6.7). Thus, by using contraction mapping theorem, \Pi_{m-1, N} \mathcal{T}_N admits a unique fixed-point.

    Remark 3. Obviously, if

    \begin{equation} \max\left\{\frac{2a^{\alpha-n+1}\Lambda_1^2 L_M}{\Gamma(\alpha-n+2)},\frac{2a^{n-1}\Lambda_1}{(n-1)!}\right\}\leq 1 \end{equation} (6.9)

    holds, then Eq (6.8) holds too. For m = 1 we have \Lambda_1 = 1, and Eq (3) matches with Eq (3.7). However, our estimate may not be optimal for higher degrees of approximations. Also, we guess using the convergence properties of \Pi_{m-1, N} when N\rightarrow \infty, we may obtain a convergence result without dependency on \Lambda_1.

    An important question is how to solve the nonlinear Eq (6.1). There are many methods available in literature that we can employ. The Newton iteration method is one of them [14]. The advantage is that it is fast. The disadvantage is that it needs computation of Jacoby as well as a good initial value for an iteration. It increases competition cost for higher dimension (computation of \nu^2 function for each iteration) and complexity of the implementation. However, strict restriction of \lambda_\Lambda and analytic discussion of the previous section is constructive and suggests the use of an iterative method. Since the operator \Pi_{m-1, N} \mathcal{T}_N is a contractor operator, beginning with an arbitrary initial value grantees the convergence of the related iterative method. In our algorithm, we initialize the iteration by

    \hat{\bf{w}}_{N,0} = [\bf{q}_a^{(0)},\bf{q}_a^{(n-1)}]^T.

    Then, we estimate the solution by the recursive formula

    \begin{equation} \hat{\bf{w}}_{N,k} = \Pi_{m-1,N} \mathcal{T}_N (\hat{\bf{w}}_{N,k-1}(t)), \ \ k\in \mathbb{N}. \end{equation} (6.10)

    The computation of iteration (6.10) continues with the smallest \kappa such that

    \|\hat{\bf{w}}_{N,\kappa}-\hat{\bf{w}}_{N,\kappa-1}\| < Tol

    where Tol is a desired user tolerance. We report such \kappa as a number of iteration to achieve the given tolerance.

    Theorem 6.3. Suppose \hat{\bf{w}}_N = [\hat{\bf{w}}_N, \hat{\bf{w}}_N] ( N\in\mathbb{N} ) be a discretized collocation solution of (2.2) and (2.4) described by (6.1). Let the conditions of Theorems 3.1 and 6.2 be fulfilled. Then, the coupled systems (2.2) and (2.4) have a unique solution \bf{w} on (\mathcal{C}[0, a])^{2\nu} and the \hat{\bf{w}}_N converges to the \bf{w}. Furthermore, supposing \bf{w}\in ({\mathcal{C}}^{m, \alpha}(0, a])^{2\nu} implies

    \|\hat{\bf{w}}_N-\bf{w}\|_{\infty} = \left\{\begin{array}{ll} O(N^{-r\beta_{min}}),& 1\leq r < \frac{m}{\beta_{min}},\\ O(N^{-m}),& r\geq \frac{m}{\beta_{min}}. \end{array}\right.

    Proof. Let \bf{w} be the solution of the coupled systems (2.2) and (2.4). Define the residue operator by

    \begin{equation} R(\bf{w})(t): = (\mathcal{T}-\Pi_N \mathcal{T}_N)(\bf{w})(t) \end{equation} (6.11)

    and let \bf{e} = \hat{\bf{w}}_N-\bf{w}. Subtracting Eq (3.3) from (6.1), we obtain

    \begin{equation} \begin{split} \hat{\bf{w}}_N(t)-\bf{w}& = \Pi_N \mathcal{T}_N (\hat{\bf{w}}_N(t))-\mathcal{T}\bf{w}\\ & = \Pi_N \mathcal{T}_N (\hat{\bf{w}}_N(t))-\Pi_N \mathcal{T}_N(\bf{w})(t)-R(\bf{w})(t). \end{split} \end{equation} (6.12)

    Taking maximum norm, we obtain

    \|\bf{e}\|_{\infty}\leq \|\Pi_N \mathcal{T}_N (\hat{\bf{w}}_N(t))-\Pi_N \mathcal{T}_N(\bf{w})(t)\|_{\infty}+\|R(\bf{w})(t)\|_{\infty}.

    Applying Eq (6.8), we obtain

    \|\bf{e}\|_{\infty}\leq \lambda_{\Lambda} \|\hat{\bf{w}}_N(t)-\bf{w}\|_{\infty}+\|R(\bf{w})(t)\|_{\infty}

    and finally

    \begin{equation} \|\bf{e}\|_{\infty}\leq (1-\lambda_\Lambda)^{-1}\|R(\bf{w})(t)\|_{\infty}, \ \ \mbox{if} \; \lambda_\Lambda\neq 1. \end{equation} (6.13)

    This is a good news since we can obtain the asymptotic behavior of \|R(\bf{w})\|_{\infty} for the known \bf{w}. Thanks to Theorem 8 of [20], one can easily prove that

    \|R(\bf{w})\|_{\infty} = O(N^{-m})+O(N^{-r\beta_{min}})

    which completes the proof.

    All numerical experiments is implemented in MATLAB software. The tolerance number for solving related nonlinear equations is Tol = 10^{-14}. This tolerance is close to the floating-point relative accuracy 2.2204e-16 for data type of double-precision (64 bit) in standard machine. The numerical examples show theoretically the obtained order of convergence is sharp and can not be improved more.

    Example 2. Let 1 < \alpha\leq 2 and

    \bf{p}(t,\bf{q}) = \left( \begin{array}{c} 0.1\sin(y_1+y_2)-0.1\sin(t^{2.5}+t^2)+\frac{\Gamma(3.5)}{\Gamma(3.5-\alpha)}t^{2.5-\alpha}\\ 0.1\cos(y_1-y_2)-0.1\sin(t^{2.5}-t^2)+\frac{\Gamma(3)}{\Gamma(3-\alpha)}t^{2-\alpha} \end{array}\right)

    on [0, 0.15]. We note that \bf{p}(t, .)\in (\mathcal{C}[0, 0.25])^{2} but \bf{p}(t, .)\notin (\mathcal{C}^1[0, 0.25])^{2}. Since L_M = 0.1, one can check that the conditions of Theorem 3.1 for a = 0.25 hold and the system (2.1) with boundary condition

    y(a) = [0.0225,0.058095]^T

    and

    Dy(a) = [0.3,0.58095]^T

    has a unique solution on [0, a]. The solution by Corollary 1 belongs to (\mathcal{C}^1[0, a])^2. We apply a numerical method based on collocation parameter c = [0.5, 1]. Thus, the dense solution on each sub-interval \sigma_k ( k = 0, \cdots, N-1 ) of a given partition can be described by

    \begin{equation} \hat{\bf{w}}_N(t_k+hs) = 2(W_{n,1}(1-s)+(s-0.5)W_{n,2}),\; s\in(0,1]. \end{equation} (7.1)

    An estimated norm of the given method can be determined by (6.2) and we have

    \Lambda_1 = \max\limits_{s\in[0,1]}2(|1-s|+|s-.5|) = 2(1.5) = 3.

    Taking into account (6.8), we obtain

    \lambda_{\Lambda_1} = \max\{0.78663,0.9\} = 0.9.

    Consequently, by using Theorem 6.2 the nonlinear Eq (6.1) has a unique solution and the iteration process (6.10) converges to that solution. Theorem 6.3 implies the numerical solution converges to the exact solution by following order ( \mathrm{O} )

    \begin{equation} \mathrm{O} = \left\{\begin{array}{ll} 0.5r, & r\leq 4,\\ 2,& r > 4. \end{array}\right. \end{equation} (7.2)

    In Tables 3 and 4, we provided the maximum error

    E(r,N) = \|\hat{\bf{w}}_N-\bf{w}\|_{\infty},
    Table 3.  Numerical results of the proposed collocation method with c = [0, 1], m = 2 and r = 1, 2 .
    N E(1, N) O_N It E(2, N) O_N It
    2 0.17015 0.49 10 0.12032 1.00 9
    4 0.12032 0.49 10 0.06016 1.00 10
    8 0.08507 0.50 10 0.03008 1.00 10
    16 0.06016 0.50 10 0.01504 0.99 10
    32 0.04254 0.50 10 0.00752 1.00 10
    64 0.03008 0.50 10 0.00376 1.00 10
    128 0.02127 - 10 0.00188 - 10

     | Show Table
    DownLoad: CSV
    Table 4.  Numerical results of the proposed collocation method with c = [0, 1], m = 2 and r = 3, 4 .
    N E(3, N) O_N It E(4, N) O_N It
    2 0.08509 1.50 9 0.12054 1.78 9
    4 0.03008 1.50 10 0.03486 1.95 10
    8 0.01063 1.50 10 0.00896 1.98 10
    16 0.00376 1.50 10 0.00226 2.00 10
    32 0.00133 1.50 10 0.0006 1.99 10
    64 0.00047 1.50 10 0.00014 1.99 10
    128 0.00017 - 10 3.5439e-05 - 10

     | Show Table
    DownLoad: CSV

    estimated order of proposed method ( O_N ) and the number of iteration for required tolerance. As we see O_N = 0.5, 1, 1.5, 2 for r = 1, 2, 3, 4 respectively, which is in agreement with theoretical result (see Eq (7.2)).

    Remark 4. Theorem 1 provides a sharp result when we consider all the components of the state of the system 1 ( \bf{w} = [\bf{q}, \bf{z}] ). However, it can be improved for the desired state of the solution \bf{q}. According to Corollary 1, \bf{q} has better regularity for n\geq 1. Thus, we guess that the order of convergence for \bf{q} component with uniform mesh r = 1, can be greater than or equal to n-1. Thus, for that component, a greater graded mesh exponent is not necessary. The error E_{\bf{q}}(r, N) = \|\hat{\bf{q}}_N-\bf{q}\|_{\infty} and the estimated order of convergence of Example 2 is reported in Table 5. The order 2 is achieved with r = 1.5 .

    Table 5.  Numerical results of the proposed collocation method with c = [0, 1], m = 2 and r = 1, 2 for y component.
    N E_{\bf{q}}(1, N) O_N It E_{\bf{q}}(4, N) O_N It
    2 0.00593 1.46 10 0.00544 1.91 10
    4 0.00214 1.47 10 0.00145 1.96 10
    8 0.00077 1.48 10 0.00037 1.97 10
    16 0.00027 1.48 10 9.501e-05 2.01 10
    32 9.803e-05 1.49 10 2.354e-05 1.94 10
    64 3.484e-05 1.49 10 6.122e-06 2.01 10
    128 1.236e-05 NaN 10 1.522e-06 NaN 10

     | Show Table
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    To show the sharpness of theoretical results, we add numerical experiments for the case m = 1 with c = 0.5 (for other choice of c on [0, 1] we have similar results). The dense solution on each sub-interval \sigma_k can be described by

    \begin{equation} \hat{\bf{w}}_N(t_k+hs) = W_{n,1},\; s\in(0,1]. \end{equation} (7.3)

    In this case \Lambda_1 = 1 and by (6.8)

    \lambda_{\Lambda_1} = \max\{0.087404, 0.3\} = 0.3.

    Consequently, by using Theorem 6.2 the nonlinear Eq (6.1) related to m = 1 has a unique solution and the iteration process (6.10) converges to the exact solution. By Theorem 6.3 we expect

    \begin{equation} \it{Order} = \left\{\begin{array}{ll} 0.5r, & r\leq 2,\\ 1,& r > 2. \end{array}\right. \end{equation} (7.4)

    The sharpness of this result can be seen in Table 6.

    Table 6.  Numerical results of the proposed collocation method with c = 0.5, m = 1 and r = 1, 2 .
    N E(1, N) O_N It E(2, N) O_N It
    2 0.29073 0.50008 8 0.20597 0.99 9
    4 0.20556 0.50024 9 0.10305 0.99 9
    8 0.14533 0.50024 10 0.051533 0.99 10
    16 0.10275 0.50019 10 0.025768 1.00 10
    32 0.072644 0.50015 10 0.012884 1.00 10
    64 0.051362 0.50011 10 0.006442 1.00 10
    128 0.036316 - 10 0.003221 - 10

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    Remark 5. The low order method have the advantage of supporting larger class of terminal value problem with large value of a . The reason is that with m = 1, we have \Lambda_1 = 1 which is three times smaller than \Lambda_1 for the case m = 2.

    TVPs for higher-order (greater than one) fractional differential equations are rarely studied in the literature. In this paper, we tried to have a comprehensive study with a simple analysis to cover all general interests. Many questions in this topic deserve to study with more scrutiny. The regularity of nonlinear cases as well as optimal bound for obtaining well-posed problems are among them. We think the terminal value problem is important in applied since it monitors the past evolution of a dynamical system. Also, it can be regarded as a control problem for having the desired future by finding suitable initial value. We think this topic will catch more interest similar to the initial value problem.

    The authors declare that there are no conflicts of interest.

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