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Research article

The principal transmission condition

  • Received: 05 May 2021 Accepted: 02 August 2021 Published: 16 August 2021
  • The paper treats pseudodifferential operators P=Op(p(ξ)) with homogeneous complex symbol p(ξ) of order 2a>0, generalizing the fractional Laplacian (Δ)a but lacking its symmetries, and taken to act on the halfspace Rn+. The operators are seen to satisfy a principal μ-transmission condition relative to Rn+, but generally not the full μ-transmission condition satisfied by (Δ)a and related operators (with μ=a). However, P acts well on the so-called μ-transmission spaces over Rn+ (defined in earlier works), and when P moreover is strongly elliptic, these spaces are the solution spaces for the homogeneous Dirichlet problem for P, leading to regularity results with a factor xμn (in a limited range of Sobolev spaces). The information is then shown to be sufficient to establish an integration by parts formula over Rn+ for P acting on such functions. The formulation in Sobolev spaces, and the results on strongly elliptic operators going beyond certain operators with real kernels, are new. Furthermore, large solutions with nonzero Dirichlet traces are described, and a halfways Green's formula is established, as new results for these operators. Since the principal μ-transmission condition has weaker requirements than the full μ-transmission condition assumed in earlier papers, new arguments were needed, relying on work of Vishik and Eskin instead of the Boutet de Monvel theory. The results cover the case of nonsymmetric operators with real kernel that were only partially treated in a preceding paper.

    Citation: Gerd Grubb. The principal transmission condition[J]. Mathematics in Engineering, 2022, 4(4): 1-33. doi: 10.3934/mine.2022026

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  • The paper treats pseudodifferential operators P=Op(p(ξ)) with homogeneous complex symbol p(ξ) of order 2a>0, generalizing the fractional Laplacian (Δ)a but lacking its symmetries, and taken to act on the halfspace Rn+. The operators are seen to satisfy a principal μ-transmission condition relative to Rn+, but generally not the full μ-transmission condition satisfied by (Δ)a and related operators (with μ=a). However, P acts well on the so-called μ-transmission spaces over Rn+ (defined in earlier works), and when P moreover is strongly elliptic, these spaces are the solution spaces for the homogeneous Dirichlet problem for P, leading to regularity results with a factor xμn (in a limited range of Sobolev spaces). The information is then shown to be sufficient to establish an integration by parts formula over Rn+ for P acting on such functions. The formulation in Sobolev spaces, and the results on strongly elliptic operators going beyond certain operators with real kernels, are new. Furthermore, large solutions with nonzero Dirichlet traces are described, and a halfways Green's formula is established, as new results for these operators. Since the principal μ-transmission condition has weaker requirements than the full μ-transmission condition assumed in earlier papers, new arguments were needed, relying on work of Vishik and Eskin instead of the Boutet de Monvel theory. The results cover the case of nonsymmetric operators with real kernel that were only partially treated in a preceding paper.



    In this paper, we propose shifted-Legendre orthogonal function method for high-dimensional heat conduction equation [1]:

    {ut=k(2ux2+2uy2+2uz2),t[0,1],x[0,a],y[0,b],z[0,c],u(0,x,y,z)=ϕ(x,y,z),u(t,0,y,z)=u(t,a,y,z)=0,u(t,x,0,z)=u(t,x,b,z)=0,u(t,x,y,0)=u(t,x,y,c)=0. (1.1)

    Where u(t,x,y,z) is the temperature field, ϕ(x,y,z) is a known function, k is the thermal diffusion efficiency, and a,b,c are constants that determine the size of the space.

    Heat conduction system is a very common and important system in engineering problems, such as the heat transfer process of objects, the cooling system of electronic components and so on [1,2,3,4]. Generally, heat conduction is a complicated process, so we can't get the analytical solution of heat conduction equation. Therefore, many scholars proposed various numerical algorithms for heat conduction equation [5,6,7,8]. Reproducing kernel method is also an effective numerical algorithm for solving boundary value problems including heat conduction equation [9,10,11,12,13,14]. Galerkin schemes and Green's function are also used to construct numerical algorithms for solving one-dimensional and two-dimensional heat conduction equations [15,16,17,18,19]. Alternating direction implicit (ADI) method can be very effective in solving high-dimensional heat conduction equations [20,21]. In addition, the novel local knot method and localized space time method are also used to solve convection-diffusion problems [22,23,24,25]. These methods play an important reference role in constructing new algorithms in this paper.

    Legendre orthogonal function system is an important function sequence in the field of numerical analysis. Because its general term is polynomial, Legendre orthogonal function system has many advantages in the calculation process. Scholars use Legendre orthogonal function system to construct numerical algorithm of differential equations [26,27,28].

    Based on the orthogonality of Legendre polynomials, we delicately construct a numerical algorithm that can be extended to high-dimensional heat conduction equation. The proposed algorithm has α-Order convergence, and our algorithm can achieve higher accuracy compared with other algorithms.

    The content of the paper is arranged like this: The properties of shifted Legendre polynomials, homogenization and spatial correlation are introduced in Section 2. In Section 3, we theoretically deduce the numerical algorithm methods of high-dimensional heat conduction equations. The convergence of the algorithm is proved in Section 4. Finally, three numerical examples and a brief summary are given at the end of this paper.

    In this section, the concept of shifted-Legendre polynomials and the space to solve Eq (1.1) are introduced. These knowledge will pave the way for describing the algorithm in this paper.

    The traditional Legendre polynomial is the orthogonal function system on [1,1]. Since the variables t,x,y,z to be analyzed for Eq (1.1) defined in different intervals, it is necessary to transform the Legendre polynomial on [c1,c2], c1,c2R, and the shifted-Legendre polynomials after translation transformation and expansion transformation by Eq (2.1).

    p0(x)=1,p1(x)=2(xc1)c2c11,pi+1(x)=2i+1i+1[2(xc1)c2c11]pi(x)ii+1pi1(x),i=1,2,. (2.1)

    Obviously, {pi(x)}i=0 is a system of orthogonal functions on L2[c1,c2], and

    c2c1pi(x)pj(x)dx={c2c12i+1,i=j,0,ij.

    Let Li(x)=2i+1c2c1pi(x). Based on the knowledge of ref. [29], we begin to discuss the algorithm in this paper.

    Lemma 2.1. [29] {Li(x)}i=0 is a orthonormal basis in L2[c1,c2].

    Considering that the problem studied in this paper has a nonhomogeneous boundary value condition, the problem (1.1) can be homogenized by making a transformation as follows.

    v(t,x,y,z)=u(t,x,y,z)ϕ(x,y,z).

    Here, homogenization is necessary because we can easily construct functional spaces that meet the homogenization boundary value conditions. This makes us only need to pay attention to the operator equation itself in the next research, without considering the interference caused by boundary value conditions.

    In this paper, in order to avoid the disadvantages of too many symbols, the homogeneous heat conduction system is still represented by u, the thermal diffusion efficiency k=1, and the homogeneous system of heat conduction equation is simplified as follows:

    {2ux2+2uy2+2uz2ut=f(x,y,z),t[0,1],x[0,a],y[0,b],z[0,c],u(0,x,y,z)=0,u(t,0,y,z)=u(t,a,y,z)=0,u(t,x,0,z)=u(t,x,b,z)=0,u(t,x,y,0)=u(t,x,y,c)=0. (2.2)

    The solution space of Eq (2.2) is a high-dimensional space, which can be generated by some one-dimensional spaces. Therefore, this section first defines the following one-dimensional space.

    Remember AC represents the space of absolutely continuous functions.

    Definition 2.1. W1[0,1]={u(t)|uAC,u(0)=0,uL2[0,1]}, and

    u,vW1=10uvdt,u,vW1.

    Let c1=0,c2=1, so {Ti(t)}i=0 is the orthonormal basis in L2[0,1], where Ti(t)=Li(t), note Tn(t)=ni=0citi. And {JTn(t)}n=0 is the orthonormal basis of W1[0,1], where

    JTn(t)=ni=0citi+1i+1.

    Definition 2.2. W2[0,a]={u(x)|uAC,u(0)=u(a)=0,uL2[0,a]}, and

    u,vW2=a0uvdx,u,vW2.

    Similarly, {Pn(x)}n=0 is the orthonormal basis in L2[0,a], and denote Pn(x)=nj=0djxj, where djR.

    Let

    JPn(x)=nj=0djxj+2aj+1x(j+1)(j+2),

    obviously, {JPn(x)}n=0 is the orthonormal basis of W2[0,a].

    We start with solving one-dimensional heat conduction equation, and then extend the algorithm to high-dimensional heat conduction equations.

    {2ux2ut=f(x),t[0,1],x[0,a],u(0,x)=0,u(t,0)=u(t,a)=0. (3.1)

    Let D=[0,1]×[0,a], CC represents the space of completely continuous functions, and Nn represents a set of natural numbers not exceeding n.

    Definition 3.1. W(D)={u(t,x)|uxCC,(t,x)D,u(0,x)=0,u(t,0)=u(t,a)=0,3utx2L2(D)}, and

    u,vW(D)=D3utx23vtx2dσ.

    Theorem 3.1. W(D) is an inner product space.

    Proof. u(t,x)W(D), if u,uW(D)=0, means

    D[3u(t,x)tx2]2dσ=0,

    and it implies

    3u(t,x)tx2=t(2u(t,x)x2)=0.

    Combined with the conditions of W(D), we can get u=0.

    Obviously, W(D) satisfies other conditions of inner product space.

    Theorem 3.2. uW(D),v1(t)v2(x)W(D), then

    u(t,x),v1(t)v2(x)W(D)=u(t,x),v1(t)W1,v2(x)W2.
    Proof.u(t,x),v1(t)v2(x)W(D)=D3u(t,x)tx23[v1(t)v2(x)]tx2dσ=D2x2[u(t,x)t]v1(t)t2v2(x)x2dσ=a02x2u(t,x),v1(t)W12v2(x)x2dx=u(t,x),v1(t)W1,v2(x)W2.

    Corollary 3.1. u1(t)u2(x)W(D),v1(t)v2(x)W(D), then

    u1(t)u2(x),v1(t)v2(x)W(D)=u1(t),v1(t)W1u2(x),v2(x)W2.

    Let

    ρij(t,x)=JTi(t)JPj(x),i,jN.

    Theorem 3.3. {ρij(t,x)}i,j=0is an orthonormal basis inW(D).

    Proof. ρij(t,x),ρlm(t,x)W(D),i,j,l,mN,

    ρij(t,x),ρlm(t,x)W(D)=JTi(t)JPj(x),JTl(t)JPm(x)W(D)=JTi(t),JTl(t)W1JPj(x),JPm(x)W2.

    So

    ρij(t,x),ρlm(t,x)W(D)={1,i=l,j=m,0,others.

    In addition, uW(D), if u,ρijW(D)=0, means

    u(t,x),JTi(t)JPj(x)W(D)=u(t,x),JTi(t)W1,JPj(x)W2=0.

    Note that {JPj(x)}j=0 is the complete system of W2, so u(t,x),JTi(t)W1=0.

    Similarly, we can get u(t,x)=0.

    Let L:W(D)L2(D),

    Lu=2ux2ut.

    So, Eq (3.1) can be simplified as

    Lu=f. (3.2)

    Definition 3.2. ε>0, if uW(D) and

    ||Luf||2L(D)<ε, (3.3)

    then u is called the εbest approximate solution for Lu=f.

    Theorem 3.4. Any ε>0, there is NN, when n>N, then

    un(t,x)=ni=0nj=0ηijρij(t,x) (3.4)

    is the εbest approximate solution for Lu=f, where ηij satisfies

    ||ni=0nj=0ηijLρijf||2L2(D)=mindij||ni=0nj=0dijLρijf||2L2(D),dijR,i,jNn.

    Proof. According to the Theorem 3.3, if u satisfies Eq (3.2), then u(t,x)=i=0j=0ηijρij(t,x), where ηij is the Fourier coefficient of u.

    Note that L is a bounded operator [30], hence, any ε>0, there is NN, when n>N, then

    ||i=n+1j=n+1ηijρij||2W(D)<ε||L||2.

    So,

    ||ni=0nj=0ηijLρijf||2L2(D)=mindij||ni=0nj=0dijLρijf||2L2(D)||ni=0nj=0ηijLρijf||2L2(D)=||ni=0nj=0ηijLρijLu||2L2(D)=||i=n+1j=n+1ηijLρij||2L2(D)||L||2||i=n+1j=n+1ηijρij||2W(D)< ε.

    For obtain un(t,x), we need to find the coefficients ηij by solving Eq (3.5).

    min{ηij}ni,j=0J=Lunf2L2(D) (3.5)

    In addition,

    J=Lunf2L2(D)=Lunf,LunfL2(D)=Lun,LunL2(D)2Lun,fL2(D)+f,fL2(D)=ni=0nj=0nl=0nm=0ηijηlmLρij,LρlmL2(D)2ni=0nj=0ηijLρij,fL2(D)+f,fL2(D).

    So,

    Jηij=2nl=0nm=0ηlmLρij,LρlmL2(D)2ηijLρij,fL2(D),i,jNn

    and the equations Jηij=0,i,jNn can be simplified to

    Aη=B, (3.6)

    where

    A=(Lρij,LρlmL2(D))N×N,N=(n+1)2,η=(ηij)N×1,B=(Lρij,fL2(D))N×1.

    Theorem 3.5. Aη=B has a unique solution.

    Proof. It can be proved that A is nonsingular. Let η satisfy Aη=0, that is,

    ni=0nj=0Lρij,LρlmL2(D)ηij=0,l,mNn.

    So, we can get the following equations:

    ni=0nj=0ηijLρij,ηlmLρlmL2(D)=0,l,mNn.

    By adding the above (n+1)2 equations, we can get

    ni=0nj=0ηijLρij,nl=0nm=0ηlmLρlmL2(D)=ni=0nj=0ηijLρij2L2(D)=0.

    So,

    ni=0nj=0ηijLρij=0.

    Note that L is reversible. Therefore, ηij=0,i,jNn.

    According to Theorem 3.5, un(t,x) can be obtained by substituting η=A1B into un=ni=0nj=0ηijρij(t,x).

    {2ux2+2uy2ut=f(x,y),t[0,1],x[0,a],y[0,b],u(0,x,y)=0,u(t,0,y)=u(t,a,y)=0,u(t,x,0)=u(t,x,b)=0. (3.7)

    Similar to definition 2.2, we can give the definition of linear space W3[0,b] as follows:

    W3[0,b]={u(y)|uAC,y[0,b],u(0)=u(b)=0,uL2[0,b]}.

    Similarly, let {Qn(y)}n=0 is the orthonormal basis in L2[0,b], and denote Qn(y)=nk=0qkyk.

    Let

    JQn(y)=nk=0qkyk+2bk+1y(k+1)(k+2),

    it is easy to prove that {JQn(y)}n=0 is the orthonormal basis of W3[0,b].

    Let Ω=[0,1]×[0,a]×[0,b]. Now we define a three-dimensional space.

    Definition 3.3 W(Ω)={u(t,x,y)|2uxyCC,(t,x,y)Ω,u(0,x,y)=0, u(t,0,y)=u(t,a,y)=0,u(t,x,0)=u(t,x,b)=0,5utx2y2L2(Ω)}, and

    u,vW(Ω)=Ω5utx2y25vtx2y2dΩ,u,vW(Ω).

    Similarly, we give the following theorem without proof.

    Theorem 3.6. {ρijk(t,x,y)}i,j,k=0is an orthonormal basis ofW(Ω), where

    ρijk(t,x,y)=JTi(t)JPj(x)JQk(y),i,j,kNn.

    Therefore, we can get un as

    un(t,x,y)=ni=0nj=0nk=0ηijkρijk(t,x,y), (3.8)

    according to the theory in Section 3.1, we can find all ηijk,i,j,kNn.

    {2ux2+2uy2+2uz2ut=f(x,y,z),t[0,1],x[0,a],y[0,b],z[0,c],u(0,x,y,z)=0,u(t,0,y,z)=u(t,a,y,z)=0,u(t,x,0,z)=u(t,x,b,z)=0,u(t,x,y,0)=u(t,x,y,c)=0. (3.9)

    By Lemma 2.1, note that the orthonormal basis of L2[0,c] is {Rn(z)}n=0, and denote Rn(z)=nm=0rmzm, where rm is the coefficient of polynomial Rn(z).

    We can further obtain the orthonormal basis JRn(z)=nm=0rmzm+2cm+1z(m+1)(m+2) of W4[0,c], where

    JRn(z)=nm=0rmzm+2cm+1z(m+1)(m+2),

    and

    W4[0,c]={u(z)|uAC,z[0,c],u(0)=u(c)=0,uL2[0,c]}.

    Let G=[0,1]×[0,a]×[0,b]×[0,c]. Now we define a four-dimensional space.

    Definition 3.4. W(G)={u(t,x,y,z)|3uxyzCC,(t,x,y,z)G,u(0,x,y,z)=0,u(t,0,y,z)=u(t,a,y,z)=0, u(t,x,0,z)=u(t,x,b,z)=0,u(t,x,y,0)=u(t,x,y,c)=0,7utx2y2z2L2(G)}, and

    u,vW(G)=

    where dG = dtdxdydz.

    Similarly, we give the following theorem without proof.

    Theorem 3.7. \{\rho_{ijk}(t, x, y, z)\}_{i, j, k, m = 0}^\infty \mathit{\mbox{is an orthonormal basis of}}\; W(G) , where

    \rho_{ijkm}(t,x,y,z) = JT_i(t)JP_j(x)JQ_k(y)JR_m(z),\; \; i,j,k,m\in \mathbb{N}.

    Therefore, we can get u_n as

    \begin{equation} u_n(t,x,y,z) = \sum\limits_{i = 0}^{n}\sum\limits_{j = 0}^{n}\sum\limits_{k = 0}^{n}\sum\limits_{m = 0}^{n}\eta_{ijkm}\rho_{ijkm}(t,x,y,z), \end{equation} (3.10)

    according to the theory in Section 3.1, we can find all \eta_{ijkm}, \; \; i, j, k, m\in\mathbb{N}_n.

    Suppose u(t, x) = \sum\limits_{i = 0}^{\infty}\sum\limits_{j = 0}^{\infty}\eta_{ij}\rho_{ij}(t, x) is the exact solution of Eq (3.5). Let P_{N_1, N_2}u(t, x) = \sum\limits_{i = 0}^{N_1} \sum\limits_{j = 0}^{N_2} \eta_{ij}T_i(t)P_j(x) is the projection of u in L(D) .

    Theorem 4.1. Suppose \dfrac{\partial^{r+l} u(t, x)}{\partial t^{r}\partial x^{l}}\in L^2(D) , and N_1 > r, N_2 > l , then, the error estimate of P_{N_1, N_2}u(t, x) is

    ||u-P_{N_1,N_2}u||_{L^2(D)}^2 \leq C N^{-\alpha},

    where C is a constant, N = min\{N_1, N_2\}, \alpha = min\{r, l\}.

    Proof. According to the lemma in ref. [29], it follows that

    ||u-u_{N_1}||_{L_t^2[0,1]}^2 = ||u-P_{t,N_1}u||_{L_t^2[0,1]}^2\leq C_1 N_1^{-r}|| \dfrac{\partial^r}{\partial t^r}u(t,x) ||_{L_t^2[0,1]}^2,

    where u_{N_1} = P_{t, N_1}u represents the projection of u on variable t in L^2[0, 1] , and ||\cdot||_{L_t^2[0, 1]} represents the norm of (\cdot) with respect to variable t in L^2[0, 1] .

    By integrating both sides of the above formula with respect to x , we can get

    \begin{equation*} \begin{array}{lll} ||u-u_{N_1}||_{L^2(D)}^2 &\leq & C_1 N_1^{-r} \int_0^a ||\dfrac{\partial^r}{\partial t^r}u||_{L_t^2[0,1]}^2 dx\\ & = & C_1 N_1^{-r}||\dfrac{\partial^r}{\partial t^r}u||_{L^2(D)}^2. \end{array} \end{equation*}

    Moreover,

    \begin{equation*} \begin{array}{lll} u(t,x)-u_{N_1}(t,x) & = & \sum\limits_{i = N_1+1}^{\infty} \langle u, T_i\rangle _{L_t^2[0,1]}T_i(t)\\ & = & \sum\limits_{i = N_1+1}^{\infty} \sum\limits_{j = 0}^{\infty} \langle \langle u, T_i\rangle _{L_t^2[0,1]}, P_j\rangle_{L_x^2[0,a]} P_j(x)T_i(t). \end{array} \end{equation*}

    According to the knowledge in Section 3,

    ||u-u_{N_1}||_{L^2(D)}^2 = \sum\limits_{i = N_1+1}^{\infty} \sum\limits_{j = 0}^{\infty}c_{ij}^2,

    where c_{ij} = \langle \langle u, T_i\rangle _{L_t^2[0, 1]}, P_j\rangle_{L_x^2[0, a]} .

    Therefore,

    \sum\limits_{i = N_1+1}^{\infty} \sum\limits_{j = 0}^{\infty}c_{ij}^2\leq C_1 N_1^{-r}||\dfrac{\partial^r}{\partial t^r}u||_{L^2(D)}^2.

    Similarly,

    \sum\limits_{i = 0}^{\infty} \sum\limits_{j = N_2+1}^{\infty}c_{ij}^2\leq C_2 N_2^{-l}||\dfrac{\partial^l}{\partial x^l}u||_{L^2(D)}^2.

    In conclusion,

    \begin{equation*} \begin{array}{lll} ||u-P_{N_1,N_2}u||_{L^2(D)}^2 & = & ||(\sum\limits_{i = 0}^{\infty} \sum\limits_{j = 0}^{\infty}-\sum\limits_{i = 0}^{N_1} \sum\limits_{j = 0}^{N_2})c_{ij}^2 T_i(t)P_j(x)||_{L^2(D)}^2\\ &\leq & \sum\limits_{i = N_1+1}^{\infty} \sum\limits_{j = 0}^{N_2}c_{ij}^2+\sum\limits_{i = 0}^{\infty} \sum\limits_{j = N2+1}^{\infty}c_{ij}^2\\ &\leq & \sum\limits_{i = N_1+1}^{\infty} \sum\limits_{j = 0}^{\infty}c_{ij}^2+\sum\limits_{i = 0}^{\infty} \sum\limits_{j = N_2+1}^{\infty}c_{ij}^2\\ &\leq & C_1 N_1^{-r}|| \dfrac{\partial^r}{\partial t^r}u||_{L^2(D)}^2 + C_2 N_2^{-l}|| \dfrac{\partial^l}{\partial x^l}u||_{L^2(D)}^2\\ &\leq & C N^{-\alpha}. \end{array} \end{equation*}

    Theorem 4.2. Suppose \dfrac{\partial^{r+l} u(t, x)}{\partial t^{r}\partial x^{l}}\in L^2(D) , u_n(t, x) is the \varepsilon- best approximate solution of Eq (3.2), and n > max\{r, l\} , then,

    ||u-u_n||_{W(D)}^2 \leq C n^{-\alpha}.

    where C is a constant, \alpha = min\{r, l\}.

    Proof. According to Theorem 3.4 and Theorem 4.1, the following formula holds.

    \begin{equation*} ||u-u_n||_{W(D)}^2 \leq ||u-P_{N_1,N_2}u||_{L^2(D)}^2\leq C n^{-\alpha}. \end{equation*}

    So, the \varepsilon- approximate solution has \alpha convergence order, and the convergence rate is related to n , where represents the number of bases, and the convergence order can calculate as follows.

    \begin{equation} C.R. = log_{\frac{n_2}{n_1}}\frac{max|e_{n_1}|}{max|e_{n_2}|}. \end{equation} (4.1)

    Where n_i, i = 1, 2 represents the number of orthonormal base elements.

    Here, three examples are compared with other algorithms. N represents the number of orthonormal base elements. For example, N = 10 \times 10 , which means that we use the orthonormal system \{\rho_{ij}\}_{i, j = 0}^{10} of W(D) for approximate calculation, that is, we take the orthonormal system \{JT_i(t)\}_{i = 0}^{10} and \{JP_j(x)\}_{j = 0}^{10} to construct the \varepsilon- best approximate solution.

    Example 5.1. Consider the following one-demensional heat conduction system [7,20]

    \begin{eqnarray*} \left\{ \begin{array}{l} u_t = u_{xx},\; \; (t,x)\in [0,1]\times[0,2\pi],\\ u(0,x) = \sin(x),\\ u(t,0) = u(t,2\pi) = 0. \end{array} \right. \end{eqnarray*}

    The exact solution of Ex. 5.1 is e^{-t}\sin x .

    In Table 1, C.R. is calculated according to Eq (4.2). The errors in Tables 1 and 2 show that the proposed algorithm is very effective. In Figures 1 and 2, the blue surface represents the surface of the real solution, and the yellow surface represents the surface of u_n . With the increase of N , the errors between the two surfaces will be smaller.

    Table 1.  \max |u-u_n| for Ex. 5.1.
    N HOC-ADI Method [20] FVM [7] Present method C.R.
    4 \times 4 6.12E-3 4.92E-2 9.892E-3
    6 \times 6 1.68E-3 2.05E-2 4.319E-4 3.8613
    8 \times 8 7.69E-4 1.27E-2 9.758E-6 6.5873
    10 \times 10 4.40E-4 9.20E-3 1.577E-7 9.2432

     | Show Table
    DownLoad: CSV
    Table 2.  |u-u_n| for Ex. 5.1 ( n = 9 ).
    |u-u_n| t=0.1 t=0.3 t=0.5 t=0.7 t=0.9
    x=\frac{\pi}{5} 1.195E-8 3.269E-8 5.009E-8 6.473E-8 8.127E-8
    x=\frac{3\pi}{5} 2.583E-8 7.130E-8 1.088E-7 1.390E-7 1.577E-7
    x=\frac{7\pi}{5} 2.583E-8 7.130E-8 1.088E-7 1.390E-7 1.577E-7
    x=\frac{9\pi}{5} 1.195E-8 3.269E-8 5.009E-8 6.473E-8 8.127E-8

     | Show Table
    DownLoad: CSV
    Figure 1.  u\; \; \mbox{and}\; \; u_{n} in Example 5.1( n = 9 ).
    Figure 2.  |u(1, x)-u_{n}(1, x)| in Example 5.1( n = 9 ).

    Example 5.2. Consider the following two-demensional heat conduction system [20,21]

    \begin{eqnarray*} \left\{ \begin{array}{l} u_t = u_{xx}+u_{yy},\; \; (t,x,y)\in [0,1]\times[0,1]\times[0,1],\\ u(0,x,y) = \sin(\pi x)\sin(\pi y),\\ u(t,0,y) = u(t,1,y) = u(t,x,0) = u(t,x,1) = 0. \end{array} \right. \end{eqnarray*}

    The exact solution of Ex. 5.2 is u = e^{-2\pi^2 t}\sin(\pi x)\sin(\pi y) .

    Example 5.2 is a two-dimensional heat conduction equation. Table 3 shows the errors comparison with other algorithms. Table 4 lists the errors variation law in the x- axis direction. Figures 3 and 4 show the convergence effect of the scheme more vividly.

    Table 3.  The absolute errors \max |u-u_n| for Ex. 5.2 ( t = 1, (x, y)\in [0, 1]\times[0, 1] ).
    N CCD-ADI Method [21] RHOC-ADI Method [20] Present method C.R.
    4 \times 4 \times 4 8.820E-3 3.225E-2 5.986E-3
    8 \times 8 \times 8 6.787E-5 1.969E-3 3.126E-5 2.52704

     | Show Table
    DownLoad: CSV
    Table 4.  The absolute errors |u-u_n| for Ex. 5.2 ( t = 1, n = 7 ).
    |u-u_n| y=0.1 y=0.3 y=0.5 y=0.7 y=0.9
    x=0.1 7.414E-6 1.963E-5 2.421E-5 1.963E-5 7.414E-6
    x=0.3 1.963E-5 5.130E-5 6.347E-5 5.130E-5 1.963E-5
    x=0.5 2.421E-5 6.347E-5 7.839E-5 6.347E-5 2.421E-5
    x=0.7 1.963E-5 5.130E-5 6.347E-5 5.130E-5 1.963E-5
    x=0.9 7.414E-6 1.963E-5 2.421E-5 1.963E-5 7.414E-6

     | Show Table
    DownLoad: CSV
    Figure 3.  u\; \; \mbox{and}\; \; u_{n} in Example 5.2( n = 7 ).
    Figure 4.  u-u_{n} in Example 5.2( n = 7 ).

    Example 5.3. Consider the three-demensional problem as following:

    \begin{eqnarray*} \left\{ \begin{array}{l} (\dfrac{1}{a^2}+\dfrac{1}{b^2}+\dfrac{1}{c^2})u_t = u_{xx}+u_{yy}+u_{zz},\; \; (t,x,y,z)\in [0,1]\times[0,a]\times[0,b]\times[0,c],\\ u(0,x,y) = \sin(\dfrac{\pi x}{a})\sin(\dfrac{\pi y}{b})\sin(\dfrac{\pi z}{c}),\\ u(t,0,y) = u(t,1,y) = u(t,x,0) = u(t,x,1) = 0. \end{array} \right. \end{eqnarray*}

    The exact solution of Ex. 5.3 is u = e^{-\pi^2t}\sin(\dfrac{\pi x}{a})\sin(\dfrac{\pi y}{b})\sin(\dfrac{\pi z}{c}) .

    Example 5.3 is a three-dimensional heat conduction equation, this kind of heat conduction system is also the most common case in the industrial field. Table 5 lists the approximation degree between the \varepsilon- best approximate solution and the real solution when the boundary time t = 1 .

    Table 5.  The absolute errors |u-u_n| for Ex. 5.3 ( t = 1, z = 0.1, n = 2 ).
    |u-u_n| y=0.2 y=0.6 y=1.0 y=1.4 y=1.8
    x=0.1 1.130E-3 2.873E-3 3.451E-3 2.873E-3 1.130E-3
    x=0.3 2.893E-3 7.350E-3 8.820E-3 7.350E-3 2.893E-3
    x=0.5 3.482E-3 8.838E-3 1.059E-2 8.838E-3 3.482E-3
    x=0.7 2.893E-3 7.350E-3 8.820E-3 7.735E-3 2.893E-3
    x=0.9 1.130E-3 2.873E-3 3.451E-3 2.873E-3 1.130E-3

     | Show Table
    DownLoad: CSV

    The Shifted-Legendre orthonormal scheme is applied to high-dimensional heat conduction equations. The algorithm proposed in this paper has some advantages. On the one hand, the algorithm is evolved from the algorithm for solving one-dimensional heat conduction equation, which is easy to be understood and expanded. On the other hand, the standard orthogonal basis proposed in this paper is a polynomial structure, which has the characteristics of convergence order.

    This work has been supported by three research projects (2019KTSCX217, 2020WQNCX097, ZH22017003200026PWC).

    The authors declare no conflict of interest.



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