Open Access

Convergence of the point integral method for Laplace–Beltrami equation on point cloud

Research in the Mathematical Sciences20174:22

Received: 13 October 2016

Accepted: 12 May 2017

Published: 6 November 2017


The Laplace–Beltrami operator, a fundamental object associated with Riemannian manifolds, encodes all intrinsic geometry of manifolds and has many desirable properties. Recently, we proposed the point integral method (PIM), a novel numerical method for discretizing the Laplace–Beltrami operator on point clouds (Li et al. in Commun Comput Phys 22(1):228–258, 2017). In this paper, we analyze the convergence of PIM for Poisson equation with Neumann boundary condition on submanifolds that are isometrically embedded in Euclidean spaces.


Laplace–Beltrami operatorNeumann boundaryPoint cloudPoint integral methodConvergence analysis

Mathematics Subject Classification


1 Background

The partial differential equations on manifolds arise in a wide variety of applications. In many problems, including material science [10, 20], fluid flow [22, 25], biology and biophysics [2, 3, 21, 37], people need to study the physical process, for instance diffusion and convection, in curved surfaces which introduce different kinds of PDEs in surfaces. It has been several decades to develop numerical methods for solving PDEs in surfaces. Many methods have been developed, such as surface finite element method [19], level set method [9, 48], grid-based particle method [31, 32] and closest point method [35, 43].

Recently, manifold model attracts more and more attentions in data analysis and image processing [4, 11, 13, 23, 26, 29, 30, 36, 4042, 47]. In the manifold model, data or images are represented as a point cloud, which is defined as a collection of points that are embedded in a high-dimensional Euclidean space. One fundamental assumption in the manifold model is that the point cloud samples a smooth manifold. Thus, the information of the manifold is very useful to understand the data or images. PDEs on the manifold, particularly the Laplace–Beltrami equation, encode several intrinsic information of the manifold, thus helping reveal the underlying structures in the data or images. To get the information encoded in PDEs, we need to solve them in the unstructured point cloud. Given that the point cloud is embedded in a high-dimensional space, the traditional methods for PDEs on 2D surfaces do not work.

In the past few years, efforts have been devoted to develop alternative numerical methods to discretize differential operators on point cloud. Liang and Zhao [34] proposed to discretize differential operators on point cloud via local least square approximations of the manifold. Their method achieves high-order accuracy and flexibility because no mesh is required. In principle, their method can be applied to manifolds with arbitrary dimensions and co-dimensions with or without boundaries. However, if the dimension of the manifold is high, then this method may be unstable because a high-order polynomial is used to fit the data. Lai et al. [28] later proposed the local mesh method to approximate differential operators on point cloud. The principle of the proposed method involves the use of K nearest neighbors to construct local mesh around each points, which is easier to construct than global mesh. Based on the local mesh, discretizing differential operators and computing integrals is then facilitated. When the dimension of the manifold is high, even the construction of local mesh is difficult. Although lacking proof, moving least square or local mesh-based methods achieve high-order accuracy. In principle, the accuracy of the moving least square is arbitrarily high. The accuracy of the local mesh method is second order because the local mesh approximation to the manifold has at most second-order accuracy.

In [33], we proposed the point integral method (PIM), a novel numerical method, for solving the Poisson equation on point cloud. The main idea of the point integral method is to approximate the Poisson equation via the following integral equation:
$$\begin{aligned} -\int _{\mathcal {M}}{\varDelta }_{\mathcal {M}}u(\mathbf {y})\bar{R}_t(\mathbf {x}, \mathbf {y})\mathrm{d}\mu _\mathbf {y}\approx & {} \frac{1}{t}\int _{{\mathcal {M}}} R_t(\mathbf {x}, \mathbf {y})(u(\mathbf {x}) - u(\mathbf {y}))\mathrm {d}\mu _\mathbf {y}\nonumber \\&-2\int _{\partial {\mathcal {M}}}\bar{R}_t(\mathbf {x}, \mathbf {y})\frac{\partial u}{\partial \mathbf {n}}(\mathbf {y})\mathrm {d}\tau _\mathbf {y}, \end{aligned}$$
where \(\mathbf {n}\) is the out normal of \(\partial {\mathcal {M}}\), \({\mathcal {M}}\) is a smooth k-dimensional manifold embedded in \(\mathbb {R}^d\), \(\partial {\mathcal {M}}\) is the boundary of \({\mathcal {M}}\). \(R_t(\mathbf {x},\mathbf {y})\) and \(\bar{R}_t(\mathbf {x},\mathbf {y})\) are kernel functions given as follows
$$\begin{aligned} R_t(\mathbf {x}, \mathbf {y}) = C_tR\left( \frac{|\mathbf {x}-\mathbf {y}|^2}{4t}\right) ,\quad \bar{R}_t(\mathbf {x}, \mathbf {y}) = C_t\bar{R}\left( \frac{|\mathbf {x}-\mathbf {y}|^2}{4t}\right) , \end{aligned}$$
where \(C_t = \frac{1}{(4\pi t)^{k/2}}\) is the normalizing factor. \(R\in C^2(\mathbb {R}^+) \) be a positive function that is integrable over \([0,+\infty )\),
$$\begin{aligned} \bar{R}(r)=\int _r^{+\infty }R(s)\mathrm {d}s. \end{aligned}$$
\({\varDelta }_\mathcal {M}=\text{ div }(\nabla )\) is the Laplace–Beltrami operator (LBO) on \(\mathcal {M}\). Let \({\varPhi }: {\varOmega }\subset \mathbb {R}^k\rightarrow \mathcal {M}\subset \mathbb {R}^d\) be a local parametrization of \(\mathcal {M}\) and \(\theta \in {\varOmega }\). For any differentiable function \(f:\mathcal {M}\rightarrow \mathbb {R}\), define the gradient on the manifold
$$\begin{aligned} \nabla f({\varPhi }(\theta ))&=\sum _{i,j=1}^m g^{ij}(\theta )\frac{\partial {\varPhi }}{\partial \theta _i}(\theta )\frac{\partial f({\varPhi }(\theta ))}{\partial \theta _j}(\theta ), \end{aligned}$$
and for vector field \(F:{\mathcal {M}}\rightarrow T_\mathbf {x}{\mathcal {M}}\) on \({\mathcal {M}}\), where \(T_\mathbf {x}{\mathcal {M}}\) is the tangent space of \({\mathcal {M}}\) at \(\mathbf {x}\in {\mathcal {M}}\), the divergence is defined as
$$\begin{aligned} \text{ div }(F)&= \frac{1}{\sqrt{\det G}}\sum _{k=1}^d\sum _{i,j=1}^m\frac{\partial }{\partial \theta _i}\left( \sqrt{\det G}g^{ij}F^k({\varPhi }(\theta ))\frac{\partial {\varPhi }^k}{\partial \theta _j}\right) , \end{aligned}$$
where \((g^{ij})_{i,j=1,\ldots ,k}=G^{-1}\), \(\det G\) is the determinant of matrix G and \(G(\theta )=(g_{ij})_{i,j=1,\ldots ,k}\) is the first fundamental form which is defined by
$$\begin{aligned} g_{ij}(\theta )=\sum _{k=1}^d\frac{\partial {\varPhi }_k}{\partial \theta _i}(\theta )\frac{\partial {\varPhi }_k}{\partial \theta _j}(\theta ),\quad i,j=1,\ldots ,m. \end{aligned}$$
and \((F^1(\mathbf {x}),\ldots ,F^d(\mathbf {x}))^t\) is the representation of F in the embedding coordinates.

Using the integral approximation, we transfer the LBO to an integral operator. The integral operator is easily discretized on point clouds with proper quadrature rule, because differential operators are nonexistent inside. This is the essential component of PIM. Similar integral approximation is also used in nonlocal diffusion and peridynamic models [1, 1517, 49].

PIM is also related with graph Laplacian, a discrete object that is associated with a graph and reveals many properties of graphs [12]. As observed in [5, 24, 27, 44], the graph Laplacian with the Gaussian weights well approximates the LBO when the vertices of the graph are assumed to be a sample of the underlying manifold. When no boundary is present, Belkin and Niyogi [6] showed that the spectra of the graph Laplacian with Gaussian weights converge to that of \({\varDelta }_{\mathcal {M}}\). Dealing with the boundary remains an unresolved issue. In fact, near the boundary, graph Laplacian is dominated by the first-order derivative and thus fails to be a true Laplacian [7, 27]. Recently, Singer and Wu [45] showed the spectral convergence of the graph Laplacian in the presence of the Neumann boundary. the convergence analysis in both [6] and [45] is based on the connection between the graph Laplacian and the heat operator. Therefore, Gaussian weights are essential.

The main contribution of this paper is that, for Poisson equation with Neumann boundary condition, we prove that the numerical solution computed by the PIM converges to the exact solution in \(H^1\) norm as the density of the sample points tends to infinity. Unlike the methods used in graph Laplacian, we do not relate the integral operator to heat kernel. Instead, we use a strategy that is standard in numerical analysis to prove convergence.

It is well known that the convergence is an easy consequence of consistency and stability. We imply that PIM is stable by proving that PIM preserves the coercivity of the original Laplace–Beltrami operator. Together with the truncation error estimate, we get the convergence of PIM.

The rest of this paper is organized as follows. In Sect. 2, we describe the point integral method for Poisson equation with Neumann boundary condition. The convergence result is stated in Sect. 3. The structure of the proof is shown in Sect. 4. The main body of the proof is presented in Sects. 56 and 7. Finally, the conclusions and discussion of future work are provided in Sec. 8.

2 Point integral method

In this paper, we consider Poisson equation on a smooth, compact k-dimensional submanifold \(\mathcal {M}\) in \(\mathbb {R}^d,\; d\ge k\) with the Neumann boundary
$$\begin{aligned} \left\{ \begin{array}{ll} -{\varDelta }_\mathcal {M} u(\mathbf {x})=f(\mathbf {x}),&{}\quad \mathbf {x}\in \mathcal {M}, \\ \frac{\partial u}{\partial \mathbf {n}}(\mathbf {x})=b(\mathbf {x}),&{}\quad \mathbf {x}\in \partial \mathcal {M}. \end{array} \right. \end{aligned}$$
The manifold \({\mathcal {M}}\) is sampled with a set of sample points P and a subset \(S\subset P\) sampling the boundary of \({\mathcal {M}}\). The points are listed in a fixed order \(P=(\mathbf{p }_1, \ldots , \mathbf{p }_n)\) where \(\mathbf{p }_i \in \mathbb {R}^d, 1\le i\le n\) and without loss of generality, let \(S=(\mathbf{p }_1, \ldots , \mathbf{p }_m)\subset P\) with \(m<n\).
In addition, assuming that we are given two vectors, \(\mathbf {V}= (V_1, \ldots , V_n)^t\), where \(V_i\) is an volume weight of \(\mathbf{p }_i\) in \({\mathcal {M}}\), and \(\mathbf {A}= (A_1, \ldots , A_m)^t\), where \(A_i\) is an area weight of \(\mathbf{p }_i\) in \(\partial {\mathcal {M}}\), thus, for any \(f\in C^1({\mathcal {M}})\) and \(g\in C^1({\mathcal {M}})\),
$$\begin{aligned} \sum _{i=1}^n f(\mathbf{p }_i) V_i\approx \int _{\mathcal {M}}f(\mathbf {x}) \mathrm{d}\mu _\mathbf {x},\quad \sum _{i=1}^m g(\mathbf{p }_i) A_i\approx \int _{\partial {\mathcal {M}}} g(\mathbf {x}) \mathrm{d}\tau _\mathbf {x}. \end{aligned}$$
Here \(\mathrm{d}\mu _\mathbf {x}\) and \(\mathrm{d}\tau _\mathbf {x}\) are the volume form of \({\mathcal {M}}\) and \(\partial {\mathcal {M}}\), respectively.
Using the integral approximation (1), the Poisson equation is approximated with an integral equation,
$$\begin{aligned} \frac{1}{t}\int _{{\mathcal {M}}} R_t(\mathbf {x}, \mathbf {y})(u(\mathbf {x}) - u(\mathbf {y}))\mathrm {d}\mu _\mathbf {y}-2\int _{\partial {\mathcal {M}}}\bar{R}_t(\mathbf {x}, \mathbf {y})b(\mathbf {y})\mathrm {d}\tau _\mathbf {y}=\int _{\mathcal {M}}f(\mathbf {y})\bar{R}_t(\mathbf {x}, \mathbf {y})\mathrm{d}\mu _\mathbf {y}. \end{aligned}$$
No differential operators exist in the integral equation. Therefore, it is easy to discretize on the point cloud with the weight vectors, \(\mathbf {V}\) and \(\mathbf {A}\),
$$\begin{aligned} \frac{1}{t}\sum _{j=1}^nR_t(\mathbf{p }_i,\mathbf{p }_j)(u_i-u_j)V_j-2\sum _{j=1}^m\bar{R}_t(\mathbf{p }_i,\mathbf{p }_j)b(\mathbf{p }_j)A_j=\sum _{j=1}^n\bar{R}_t(\mathbf{p }_i,\mathbf{p }_j)f(\mathbf{p }_j)V_j. \end{aligned}$$
The solution \(\mathbf{u } = (u_1, \ldots , u_n)^t\) to the above linear system provides an approximation of the solution to problem (6).

3 Main results

The main contribution of this paper is the establishment of the convergence results for the point integral method for solving problem (6). To simplify the notation and make the proof concise, in the analysis, we consider the homogeneous Neumann boundary conditions, i.e.,
$$\begin{aligned} \left\{ \begin{array}{ll} -{\varDelta }_\mathcal {M} u(\mathbf {x})=f(\mathbf {x}),&{}\quad \mathbf {x}\in \mathcal {M}, \\ \frac{\partial u}{\partial \mathbf {n}}(\mathbf {x})=0,&{}\quad \mathbf {x}\in \partial \mathcal {M}. \end{array} \right. \end{aligned}$$
The analysis can be easily generalized to nonhomogeneous boundary conditions.
The corresponding numerical scheme is
$$\begin{aligned} \frac{1}{t}\sum _{j=1}^n R_t(\mathbf{p }_i,\mathbf{p }_j)(u_i - u_j)V_j = \sum _{j=1}^n \bar{R}_t(\mathbf{p }_i,\mathbf{p }_j) f_jV_j, \end{aligned}$$
where \(f_j=f(\mathbf{p }_j)\).

Before proving the convergence of the point integral method, we need to clarify the meaning of the convergence between the point cloud \((P,\mathbf {V})\) and the manifold \({\mathcal {M}}\). In this paper, we consider the convergence in the sense that \(h(P,\mathbf {V},{\mathcal {M}})\rightarrow 0\) where \(h(P,\mathbf {V},{\mathcal {M}})\) is the integral accuracy index defined as following,

Definition 1

(Integral accuracy index) For the point cloud \((P,\mathbf {V})\) that samples the manifold \({\mathcal {M}}\), the integral accuracy index \(h(P,\mathbf {V},{\mathcal {M}})\) is defined as
$$\begin{aligned} h(P,\mathbf {V},{\mathcal {M}})=\sup _{f\in C^1({\mathcal {M}})}\frac{\left| \int _{\mathcal {M}}f(\mathbf {y}) \mathrm {d}\mu _\mathbf {y}- \sum \nolimits _{i=1}^n f(\mathbf{p }_i)V_i\right| }{|\text {supp}(f)|\Vert f\Vert _{C^1({\mathcal {M}})}}, \end{aligned}$$
where \(\Vert f\Vert _{C^1({\mathcal {M}})} = \Vert f\Vert _\infty +\Vert \nabla f\Vert _\infty \) and \(|\text {supp}(f)|\) is the volume of the support of f.

Using the definition of integrable index, the point cloud \((P,\mathbf {V})\) converges to the manifold \({\mathcal {M}}\) if \(h(P,\mathbf {V},{\mathcal {M}})\rightarrow 0\). In the convergence analysis, we assume that \(h(P,\mathbf {V},{\mathcal {M}})\) is small enough.

Remark 1

In some sense, \(h(P,\mathbf {V},{\mathcal {M}})\) is a measure of the point cloud density.
  1. 1.

    If the volume weight \(\mathbf {V}\) comes from a mesh, one can obtain the integral accuracy index \(h(P,\mathbf {V},{\mathcal {M}})=O(\rho )\) where \(\rho \) is the size of the elements in the mesh and the angle between the normal space of an element and the normal space of \({\mathcal {M}}\) at the vertices of the element is of order \(\rho ^{1/2}\) [46].

  2. 2.

    If the point cloud is sampled from some distribution, from central limit theorem, \(h(P,\mathbf {V},{\mathcal {M}})\sim O(1/\sqrt{n})\) where n is the number of point in P.


Remark 2

To consider the nonhomogeneous Neumann boundary condition or Dirichlet boundary condition, we also have to also assume that \(h(S,\mathbf {A},\partial {\mathcal {M}})\rightarrow 0\), where S is the point set that samples the boundary \(\partial {\mathcal {M}}\) and \(\mathbf {A}\) is the corresponding volume weight on the boundary \(\partial {\mathcal {M}}\).

To obtain the convergence, we also need some assumptions on the regularity of the submanifold \({\mathcal {M}}\) and the integral kernel function R.

Assumption 1

  1. 1.

    Smoothness of the manifold: \({\mathcal {M}}, \partial {\mathcal {M}}\) are both compact and \(C^\infty \) smooth k-dimensional submanifolds isometrically embedded in a Euclidean space \(\mathbb {R}^d\).

  2. 2.
    Assumptions on the kernel function R(r):
    1. (a)

      Smoothness: \(\frac{\mathrm {d}^2 }{\mathrm {d}r^2}R(r)\) is bounded, i.e., there exists a constant C such that \(\left| \frac{\mathrm {d}^2 }{\mathrm {d}r^2}R(r)\right| \le C, \quad \forall r\ge 0\);

    2. (b)

      Nonnegativity: \(R(r)\ge 0\) for any \(r\ge 0\);

    3. (c)

      Compact support: \(R(r) = 0\) for \(\forall r >1\);

    4. (d)

      Nondegeneracy: \(\exists \delta _0>0\) so that \(R(r)\ge \delta _0\) for \(0\le r\le \frac{1}{2}\).


Remark 3

The assumption on the kernel function is very mild. Almost all the smoothed delta functions in the literatures satisfy these condition. One frequently used choice is given by \(\cos \) function:
$$\begin{aligned} R(r)=\left\{ \begin{array}{ll} \frac{1}{2}\left( 1+\cos \pi r\right) , &{}\quad 0\le r\le 1,\\ 0,&{}\quad r>1. \end{array}\right. \end{aligned}$$
The compact support assumption can be relaxed to exponentially decay, like Gaussian kernel. In the nondegeneracy assumption, 1 / 2 may be replaced by a positive number \(\theta _0\) with \(0<\theta _0<1\). Similar assumptions on the kernel function is also used in analysis the nonlocal diffusion problem [18].

Remark 4

For simplicity, R is assumed to be compactly supported. After some mild modifications of the proof, the same convergence results also hold for any kernel function that decays exponentially, like the Gaussian kernel \(G_t(\mathbf {x}, \mathbf {y}) = C_t\exp \left( -\frac{|\mathbf {x}-\mathbf {y}|^2}{4t}\right) \). In fact, for any \(s\ge 1\) and any \(\epsilon >0\), the \(H^s\) mass of the Gaussian kernel over the domain \({\varOmega }=\{ \mathbf {y}\in {\mathcal {M}}| |\mathbf {x}-\mathbf {y}|^2\ge t^{1+\epsilon }\}\) decays faster than any polynomial in t as t goes to 0, i.e., \(\lim _{t\rightarrow 0} \frac{\Vert G_t(\mathbf {x}, \mathbf {y})\Vert _{H^s({\varOmega })}}{t^\alpha } = 0\) for any \(\alpha \). In this way, we can bound any influence of the integral outside a compact support.

All the analysis in this paper is conducted under the assumptions in Assumption 1 and \(h(P,\mathbf {V},{\mathcal {M}})\), t are small enough. One upper bound of t, \(T_0\), is given by \(15\sqrt{2T_0}=\delta \) with \(\delta =\rho \sigma /20\), \(\rho =0.1\) and \(\sigma \) is the minimum of the reaches defined in Proposition 1. In the theorems and the proof, we omit the statement of the assumptions without introducing any confusion.

The solution of the point integral method is a vector \(\mathbf{u }\), while the solution of problem (9) is a function defined on \({\mathcal {M}}\). To make these two solutions comparable, for any solution \(\mathbf{u }= (u_1, \ldots , u_n)^t\) to the problem (10), we construct a function on \({\mathcal {M}}\)
$$\begin{aligned} I_{\mathbf{f }}(\mathbf{u }) (\mathbf {x}) = \dfrac{ \sum \nolimits _{j=1}^n R_t(\mathbf {x}, \mathbf{p }_j)u_j V_j - t\sum \nolimits _{j=1}^n \bar{R}_t(\mathbf {x}, \mathbf{p }_j)f_jV_j}{\sum \nolimits _{j=1}^{n} R_t(\mathbf {x}, \mathbf{p }_j)V_j }. \end{aligned}$$
It is easy to verify that \(I_{\mathbf{f }}(\mathbf{u })\) interpolates \(\mathbf{u }\) at the sample points P, i.e., \(I_{\mathbf{f }}(\mathbf{u })(\mathbf{p }_j) = u_j\) for any \(\mathbf{p }_j\in P\). The following theorem guarantees the convergence of the point integral method.

Theorem 1

Let u be the solution to Problem (9) with \(f\in C^1({\mathcal {M}})\) and the vector \(\mathbf{u }\) be the solution to the problem (10). Then, there exists constants C and \(T_0\) only depend on \({\mathcal {M}}\), such that for any \(t\le T_0\)
$$\begin{aligned} \Vert u-I_{\mathbf{f }}(\mathbf{u })\Vert _{H^1({\mathcal {M}})} \le C\left( t^{1/2} + \frac{h(P, \mathbf{V },{\mathcal {M}})}{t^{3/2}}\right) \Vert f\Vert _{C^1({\mathcal {M}})}, \end{aligned}$$
where \(h(P, \mathbf{V },{\mathcal {M}})\) is the integral accuracy index.

4 Structure of the proof

To simplify the notation, we introduce an integral operator,
$$\begin{aligned} L_t u=\frac{1}{t}\int _{{\mathcal {M}}} R_t(\mathbf {x}, \mathbf {y})(u(\mathbf {x}) - u(\mathbf {y}))\mathrm {d}\mu _\mathbf {y}. \end{aligned}$$
Roughly speaking, the proof the convergence includes an estimate of the truncation error \(L_t(u-I_{\mathbf{f }}(\mathbf{u }))\) and the stability of the integral operator \(L_t\). Here \(u(\mathbf {x})\) is the solution of the problem (9) and \(\mathbf{u }\) is the solution of the problem (10).

First, we have following theorem regarding the stability of the operator \(L_t\).

Theorem 2

Let \(u(\mathbf {x})\) solve the integral equation
$$\begin{aligned} L_t u = r(\mathbf {x}), \end{aligned}$$
where \(r\in H^1({\mathcal {M}})\) with \(\int _{\mathcal {M}}r(\mathbf {x})\mathrm {d}\mu _\mathbf {x}=0\). There exist constants \(C>0, T_0>0\) independent on t, such that
$$\begin{aligned} \Vert u\Vert _{H^1({\mathcal {M}})}\le C\left( \Vert r\Vert _{L^2({\mathcal {M}})}+t\Vert \nabla r\Vert _{L^2({\mathcal {M}})}\right) \end{aligned}$$
provided that \(t\le T_0\).
To apply the stability result, we need \(L_2\) estimate of \(L_t(u-I_{\mathbf{f }}(\mathbf{u }))\) and \(\nabla L_t(u-I_{\mathbf{f }}(\mathbf{u }))\). These truncation errors are analyzed in following two theorems by splitting the truncation error \(L_t(u-I_{\mathbf{f }}(\mathbf{u }))\)
$$\begin{aligned} L_t(u-I_{\mathbf{f }}(\mathbf{u }))=L_t(u-u_t))+L_t(u_t-I_{\mathbf{f }}(\mathbf{u })), \end{aligned}$$
where \(u_t\) is the solution of the integral equation
$$\begin{aligned} \frac{1}{t}\int _{{\mathcal {M}}} R_t(\mathbf {x}, \mathbf {y})(u(\mathbf {x}) - u(\mathbf {y}))\mathrm {d}\mu _\mathbf {y}=\int _{\mathcal {M}}f(\mathbf {y})\bar{R}_t(\mathbf {x},\mathbf {y})\mathrm {d}\mu _\mathbf {y}. \end{aligned}$$
For the second term, we have

Theorem 3

Let \(u_t(\mathbf {x})\) be the solution of the problem  (14) and \(\mathbf{u }\) be the solution of the problem (10). If \(f\in C^1({\mathcal {M}})\), then there exists constants \(C, T_0\) depending only on \({\mathcal {M}}\), so that
$$\begin{aligned} \Vert L_{t} \left( I_{\mathbf{f }}\mathbf{u }- u_{t}\right) \Vert _{L^2({\mathcal {M}})}\le & {} \frac{Ch(P,\mathbf {V},{\mathcal {M}})}{t^{3/2}}\Vert f\Vert _{C^1({\mathcal {M}})}, \end{aligned}$$
$$\begin{aligned} \Vert \nabla L_{t} \left( I_{\mathbf{f }}\mathbf{u }- u_{t}\right) \Vert _{L^2({\mathcal {M}})}\le & {} \frac{Ch(P,\mathbf {V},{\mathcal {M}})}{t^{2}}\Vert f\Vert _{C^1({\mathcal {M}})}. \end{aligned}$$
as long as \(t\le T_0\) and \(\frac{h(P,\mathbf {V},{\mathcal {M}})}{\sqrt{t}}\le T_0\), \(h(P,\mathbf {V},{\mathcal {M}})\) is the integral difference index in Definition 1.

In the analysis, we found that the error term \(L_t(u-u_t)\) has boundary layer structure. In the interior region, it is \(O(\sqrt{t})\) and in a layer adjacent to the boundary with width \(O(\sqrt{t})\), the error is O(1).

Theorem 4

Let \(u(\mathbf {x})\) be the solution of the problem (9) and \(u_t(\mathbf {x})\) be the solution of the corresponding integral equation (14). Let
$$\begin{aligned} I_{bd} =\sum _{j=1}^d \int _{\partial {\mathcal {M}}}n^j(\mathbf {y})(\mathbf {x}-\mathbf {y})\cdot \nabla (\nabla ^ju(\mathbf {y}))\bar{R}_t(\mathbf {x}, \mathbf {y})p(\mathbf {y})\mathrm {d}\tau _\mathbf {y}, \end{aligned}$$
$$\begin{aligned} L_t (u- u_t)=I_{in}+I_{bd}. \end{aligned}$$
where \(\mathbf {n}(\mathbf {y})=(n^1(\mathbf {y}),\ldots ,n^d(\mathbf {y}))\) is the out normal vector of \(\partial {\mathcal {M}}\) at \(\mathbf {y}\), \(\nabla ^j\) is the jth component of gradient \(\nabla \).
If \(u\in H^3({\mathcal {M}})\), then there exists constants \(C, T_0\) depending only on \({\mathcal {M}}\) and \(p(\mathbf {x})\), so that,
$$\begin{aligned} \left\| I_{in}\right\| _{L^2({\mathcal {M}})}\le Ct^{1/2}\Vert u\Vert _{H^3(\mathcal {M})},\quad \left\| \nabla I_{in}\right\| _{L^2({\mathcal {M}})} \le C\Vert u\Vert _{H^3(\mathcal {M})}, \end{aligned}$$
as long as \(t\le T_0\).

To utilize the boundary layer structure, we need a stability result specifically for the boundary term.

Theorem 5

Let \(u(\mathbf {x})\) solve the integral equation
$$\begin{aligned} L_t u = \int _{\partial {\mathcal {M}}}\mathbf {b}(\mathbf {y})\cdot (\mathbf {x}-\mathbf {y})\bar{R}_t(\mathbf {x}, \mathbf {y})\mathrm {d}\tau _\mathbf {y}-\bar{b}, \end{aligned}$$
where \(|{\mathcal {M}}|=\int _{\mathcal {M}}\mathrm {d}\mu _\mathbf {x}\) and
$$\begin{aligned} \bar{b}=\frac{1}{|{\mathcal {M}}|}\int _{\mathcal {M}}\left( \int _{\partial {\mathcal {M}}}\mathbf {b}(\mathbf {y})\cdot (\mathbf {x}-\mathbf {y})\bar{R}_t(\mathbf {x}, \mathbf {y})\mathrm {d}\tau _\mathbf {y}\right) \mathrm {d}\mathbf {x}. \end{aligned}$$
Then, there exist constant \(C>0, T_0>0\) independent on t, such that
$$\begin{aligned} \Vert u\Vert _{H^1({\mathcal {M}})}\le C\sqrt{t}\;\Vert \mathbf {b}\Vert _{H^1({\mathcal {M}})}. \end{aligned}$$
as long as \(t\le T_0\).
Theorem 1 is an easy corollary from Theorems 234 and 5. Theorems 2 and 3 imply that
$$\begin{aligned} \Vert u_t-I_{\mathbf{f }}(\mathbf{u })\Vert _{H^1({\mathcal {M}})}=O\left( \frac{h(P,\mathbf {V},{\mathcal {M}})}{t^{3/2}}\right) \end{aligned}$$
and Theorems 24 and 5 imply
$$\begin{aligned} \Vert u-u_t\Vert _{H^1({\mathcal {M}})}=O\left( t^{1/2}\right) , \end{aligned}$$
which prove Theorem 1.

In the rest of the paper, we prove Theorems 234 and 5, respectively.

5 Error analysis of the integral approximation (Theorem 4)

In this section, we need to introduce a special parametrization of the manifold \({\mathcal {M}}\). This parametrization is based on following proposition. First, we define the reaches of a manifold following the definition in [38]. Consider a compact Riemannian submanifold \({\mathcal {M}}\) of a Euclidean space \(\mathbb {R}^d\). We can define the set
$$\begin{aligned} G({\mathcal {M}})=\{x\in \mathbb {R}^d:&\;\;\text {there exist distinct}\; p,q\in {\mathcal {M}}\\&\;\text {such that}\; d(x,{\mathcal {M}})=|x-p|=|x-q|\} \end{aligned}$$
where \(d(x,{\mathcal {M}})=\inf _{y\in {\mathcal {M}}}|x-y|\). The closure of \(G({\mathcal {M}})\), denoted as \(\bar{G}({\mathcal {M}})\), is called the medial axis of \({\mathcal {M}}\). For any \(p\in {\mathcal {M}}\), the reach at p is defined as the distance of p to the medial axis, i.e.,
$$\begin{aligned} \tau (p,{\mathcal {M}})=\inf _{y\in \bar{G}({\mathcal {M}})} |p-y|. \end{aligned}$$

Proposition 1

Assume both \({\mathcal {M}}\) and \(\partial {\mathcal {M}}\) are compact and \(C^2\) smooth. \(\sigma \) is the minimum of the reaches of \({\mathcal {M}}\) and \(\partial {\mathcal {M}}\), i.e.,
$$\begin{aligned} \sigma =\min \left\{ \inf _{p\in {\mathcal {M}}}\tau (p,{\mathcal {M}}), \inf _{p\in \partial {\mathcal {M}}}\tau (p,\partial {\mathcal {M}})\right\} . \end{aligned}$$
For any point \(\mathbf {x}\in {\mathcal {M}}\), there is a neighborhood \(U\subset {\mathcal {M}}\) of \(\mathbf {x}\), so that there is a parametrization \({\varPhi }: {\varOmega }\subset \mathbb {R}^k \rightarrow U\) satisfying the following conditions. For any \(\rho \le 0.1\),
  1. (i)

    \({\varOmega }\) is convex and contains at least half of the ball \(B_{{\varPhi }^{-1}(\mathbf {x})}(\frac{\rho }{5} \sigma )\), i.e., \(vol({\varOmega }\cap B_{{\varPhi }^{-1}(\mathbf {x})}(\frac{\rho }{5} \sigma )) > \frac{1}{2}(\frac{\rho }{5}\sigma )^k w_k\) where \(w_k\) is the volume of unit ball in \(\mathbb {R}^k\);

  2. (ii)

    \(B_{\mathbf {x}}(\frac{\rho }{10} \sigma ) \cap {\mathcal {M}}\subset U\).

  3. (iii)

    The determinant the Jacobian of \({\varPhi }\) is bounded: \((1-2\rho )^k \le |D{\varPhi }| \le (1+2\rho )^k\) over \({\varOmega }\).

  4. (iv)

    For any points \(\mathbf {y}, \mathbf {z}\in U\), \(1-2\rho \le \frac{|\mathbf {y}-\mathbf {z}|}{\left| {\varPhi }^{-1}(\mathbf {y}) - {\varPhi }^{-1}(\mathbf {z})\right| } \le 1+3\rho \).


This proposition basically says there exists a local parametrization of small distortion if \(({\mathcal {M}}, \partial {\mathcal {M}})\) satisfies certain smoothness, and moreover, the parameter domain is convex and big enough. The proof of this proposition can be found in “Appendix A.” Next, we introduce a special parametrization of the manifold \({\mathcal {M}}\).

Let \(\rho =0.1\), \(\sigma \) be the minimum of the reaches of \({\mathcal {M}}\) and \(\partial {\mathcal {M}}\) and \(\delta =\rho \sigma /20\). For any \(\mathbf {x}\in {\mathcal {M}}\), denote
$$\begin{aligned} B_{\mathbf {x}}^\delta =\left\{ \mathbf {y}\in \mathcal {M}: |\mathbf {x}-\mathbf {y}|\le \delta \right\} ,\quad \mathcal {M}_{\mathbf {x}}^t=\left\{ \mathbf {y}\in \mathcal {M}: |\mathbf {x}-\mathbf {y}|^2\le 4t\right\} \end{aligned}$$
and we assume t is small enough such that \(2\sqrt{t}\le \delta \).
Since the manifold \(\mathcal {M}\) is compact, there exists a \(\delta \)-net, \(\mathcal {N}_\delta =\{ \mathbf {q}_i\in \mathcal {M},\;i=1,\ldots ,N\}\), such that
$$\begin{aligned} \mathcal {M}\subset \bigcup _{i=1}^N B_{\mathbf {q}_i}^\delta , \end{aligned}$$
and there exists a partition of \({\mathcal {M}}\), \(\{\mathcal {O}_i, \;i=1,\ldots ,N\}\), such that \(\mathcal {O}_i\cap \mathcal {O}_j=\emptyset ,\; i\ne j\) and
$$\begin{aligned} {\mathcal {M}}=\bigcup _{i=1}^N \mathcal {O}_i,\quad \mathcal {O}_i\subset B_{\mathbf {q}_i}^\delta ,\quad i=1,\ldots ,N. \end{aligned}$$
Using Proposition 1, there exist a parametrization \({\varPhi }_i: {\varOmega }_i\subset \mathbb {R}^k \rightarrow U_i\subset \mathcal {M},\; i=1,\ldots , N\), such that
  1. 1.

    (Convexity) \(B_{\mathbf {q}_i}^{2\delta }\subset U_i\) and \({\varOmega }_i\) is convex;

  2. 2.

    (Smoothness) \({\varPhi }_i\in C^3({\varOmega }_i)\);

  3. 3.
    (Locally small deformation) For any points \(\theta _1, \theta _2\in {\varOmega }_i\),
    $$\begin{aligned} \frac{1}{2}\left| \theta _1-\theta _2\right| \le \left\| {\varPhi }_i(\theta _1)-{\varPhi }_i(\theta _2)\right\| \le 2\left| \theta _1-\theta _2\right| . \end{aligned}$$
Using the partition, \(\{\mathcal {O}_i, \;i=1,\ldots ,N\}\), for any \(\mathbf {y}\in {\mathcal {M}}\), there exists unique \(J(\mathbf {y})\in \{1,\ldots ,N\}\), such that
$$\begin{aligned} \mathbf {y}\in \mathcal {O}_{J(\mathbf {y})}\subset B_{\mathbf {q}_{J(\mathbf {y})}}^\delta . \end{aligned}$$
Moreover, using the condition, \(2\sqrt{t}\le \delta \), we have \(\mathcal {M}_{\mathbf {y}}^t \subset B_{\mathbf {q}_{J(\mathbf {y})}}^{2\delta }\subset U_{J(\mathbf {y})}\). Then, \({\varPhi }_{J(\mathbf {y})}^{-1}(\mathbf {x})\) and \({\varPhi }_{J(\mathbf {y})}^{-1}(\mathbf {y})\) are both well defined for any \(\mathbf {x}\in \mathcal {M}_{\mathbf {y}}^t\).
Now, we define an auxiliary function, \(\eta (\mathbf {x},\mathbf {y})\) for any \(\mathbf {y}\in {\mathcal {M}},\;\mathbf {x}\in \mathcal {M}_{\mathbf {y}}^t\). Let
$$\begin{aligned} \xi (\mathbf {x},\mathbf {y})={\varPhi }_{J(\mathbf {y})}^{-1}(\mathbf {x})-{\varPhi }_{J(\mathbf {y})}^{-1}(\mathbf {y})\in \mathbb {R}^k,\quad \eta (\mathbf {x},\mathbf {y})=\xi (\mathbf {x},\mathbf {y})\cdot \partial {\varPhi }_{J(\mathbf {y})}(\alpha (\mathbf {x},\mathbf {y}))\in \mathbb {R}^d, \end{aligned}$$
where \(\alpha (\mathbf {x},\mathbf {y})={\varPhi }^{-1}_{J(\mathbf {y})}(\mathbf {y})\) and \(\partial \) is the gradient operator in the parameter space, i.e.,
$$\begin{aligned} \partial {\varPhi }_j(\theta )=\left( \frac{\partial {\varPhi }_j}{\partial \theta _1}(\theta ),\frac{\partial {\varPhi }_j}{\partial \theta _2}(\theta ),\ldots ,\frac{\partial {\varPhi }_j}{\partial \theta _k}(\theta )\right) , \quad \theta \in {\varOmega }_j\subset \mathbb {R}^k. \end{aligned}$$
Now, we state the proof of Theorem 4.


Let \(r(\mathbf {x})=-(L_t u-L_tu_t)\) be the residual, then we have
$$\begin{aligned} r(\mathbf {x})= & {} -\frac{1}{t}\int _{{\mathcal {M}}}R_t(\mathbf {x},\mathbf {y})(u(\mathbf {x})-u(\mathbf {y}))\mathrm {d}\mu _\mathbf {y}\\&+2\int _{\partial {\mathcal {M}}}\bar{R}_t(\mathbf {x},\mathbf {y})g(\mathbf {y})\mathrm {d}\tau _\mathbf {y}-\int _{{\mathcal {M}}}\bar{R}_t(\mathbf {x},\mathbf {y})f(\mathbf {y})\mathrm {d}\mu _\mathbf {y}\\= & {} -\frac{1}{t}\int _{{\mathcal {M}}}R_t(\mathbf {x},\mathbf {y})(u(\mathbf {x})-u(\mathbf {y}))\mathrm {d}\mu _\mathbf {y}+\int _{{\mathcal {M}}}\bar{R}_t(\mathbf {x},\mathbf {y}){\varDelta }_{\mathcal {M}}u(\mathbf {y})\mathrm {d}\mu _\mathbf {y}\\&+\frac{1}{t}\int _{{\mathcal {M}}}(\mathbf {x}-\mathbf {y})\cdot \nabla u(\mathbf {y})R_t(\mathbf {x},\mathbf {y})\mathrm {d}\mathrm {d}\mu _\mathbf {y}\\= & {} -\frac{1}{t}\int _{{\mathcal {M}}}R_t(\mathbf {x},\mathbf {y})(u(\mathbf {x})-u(\mathbf {y})-(\mathbf {x}-\mathbf {y})\cdot \nabla u(\mathbf {y}))\mathrm {d}\mu _\mathbf {y}\\&+\int _{{\mathcal {M}}}\bar{R}_t(\mathbf {x},\mathbf {y}){\varDelta }_{\mathcal {M}}u(\mathbf {y})\mathrm {d}\mu _\mathbf {y}. \end{aligned}$$
Here, we use that fact that
$$\begin{aligned} \int _{{\mathcal {M}}}\bar{R}_t(\mathbf {x},\mathbf {y})f(\mathbf {y})\mathrm {d}\mu _\mathbf {y}=\int _{{\mathcal {M}}}\bar{R}_t(\mathbf {x},\mathbf {y}){\varDelta }_{\mathcal {M}}u(\mathbf {y})\mathrm {d}\mu _\mathbf {y}, \end{aligned}$$
$$\begin{aligned} \int _{\partial {\mathcal {M}}}\bar{R}_t(\mathbf {x},\mathbf {y})g(\mathbf {y})\mathrm {d}\tau _\mathbf {y}= & {} \int _{\partial {\mathcal {M}}}\bar{R}_t(\mathbf {x},\mathbf {y})\frac{\partial u}{\partial \mathbf {n}}(\mathbf {y})\mathrm {d}\tau _\mathbf {y}\\= & {} \int _{{\mathcal {M}}}\bar{R}_t(\mathbf {x},\mathbf {y}){\varDelta }_{\mathcal {M}}u(\mathbf {y})\mathrm {d}\mu _\mathbf {y}+\int _{{\mathcal {M}}}\nabla _\mathbf {y}\bar{R}_t(\mathbf {x},\mathbf {y})\cdot \nabla u(\mathbf {y})\mathrm {d}\mu _\mathbf {y}\\= & {} \int _{{\mathcal {M}}}\bar{R}_t(\mathbf {x},\mathbf {y}){\varDelta }_{\mathcal {M}}u(\mathbf {y})\mathrm {d}\mu _\mathbf {y}\\&+\frac{1}{2t}\int _{{\mathcal {M}}}(\mathbf {x}-\mathbf {y})\cdot \nabla u(\mathbf {y})R_t(\mathbf {x},\mathbf {y})\mathrm {d}\mu _\mathbf {y}, \end{aligned}$$
where the last equality comes from:
$$\begin{aligned}&\int _\mathcal {M}\nabla u(\mathbf {y})\cdot \nabla _\mathbf {y}\bar{R}_t(\mathbf {x},\mathbf {y}) \mathrm {d}\mu _\mathbf {y}\nonumber \\&\quad =\frac{1}{2t}\int _\mathcal {M}\left( \partial _{i'}{\varPhi }^l g^{i'j'}\partial _{j'}u(\mathbf {y})\right) \; \left( \partial _{m'}{\varPhi }^l g^{m'n'}\partial _{n'}{\varPhi }^j (x^j-y^j) R_t(\mathbf {x},\mathbf {y})\right) \mathrm {d}\mu _\mathbf {y}\nonumber \\&\quad =\frac{1}{2t}\int _\mathcal {M}\left( \partial _{n'}{\varPhi }^j g^{j'n'}\partial _{j'}u(\mathbf {y})\right) \; \left( (x^j-y^j) R_t(\mathbf {x},\mathbf {y})\right) \mathrm {d}\mu _\mathbf {y}\nonumber \\&\quad =\frac{1}{2t}\int _\mathcal {M}(x^j-y^j)\nabla ^j u(\mathbf {y}) R_t(\mathbf {x},\mathbf {y}) \mathrm {d}\mu _\mathbf {y}\nonumber \\&\quad =\frac{1}{2t}\int _{{\mathcal {M}}}(\mathbf {x}-\mathbf {y})\cdot \nabla u(\mathbf {y})R_t(\mathbf {x},\mathbf {y})\mathrm {d}\mu _\mathbf {y}. \end{aligned}$$
Here, \({\varPhi }^i,\; i=1,\ldots , d\), is the ith component of the parameterization function \({\varPhi }\) and the parameterization function \({\varPhi }={\varPhi }_{J(\mathbf {y})}\), \(J(\mathbf {y})\) is the index function given in (20). In the rest of the proof, without introducing any confusion, we always drop the subscript of the parameterization function.
First, we split the residual \(r(\mathbf {x})\) to four terms
$$\begin{aligned} r(\mathbf {x}) = r_1(\mathbf {x})+r_2(\mathbf {x})+r_3(\mathbf {x})-r_4(\mathbf {x}), \end{aligned}$$
$$\begin{aligned} r_1(\mathbf {x})= & {} \frac{1}{t}\int _{{\mathcal {M}}}\left( u(\mathbf {x})-u(\mathbf {y})-(\mathbf {x}-\mathbf {y})\cdot \nabla u(\mathbf {y})-\frac{1}{2}\eta ^i\eta ^j(\nabla ^i\nabla ^j u(\mathbf {y}))\right) R_t(\mathbf {x},\mathbf {y}) \mathrm {d}\mu _\mathbf {y}, \\ r_2(\mathbf {x})= & {} \frac{1}{2t}\int _{{\mathcal {M}}}\eta ^i\eta ^j(\nabla ^i\nabla ^j u(\mathbf {y}))R_t(\mathbf {x},\mathbf {y}) \mathrm {d}\mu _\mathbf {y}-\int _{\mathcal {M}}\eta ^i(\nabla ^i\nabla ^j u(\mathbf {y})\nabla ^j\bar{R}_t(\mathbf {x},\mathbf {y}) \mathrm {d}\mu _\mathbf {y}, \\ r_3(\mathbf {x})= & {} \int _{\mathcal {M}}\eta ^i(\nabla ^i\nabla ^j u(\mathbf {y})\nabla ^j\bar{R}_t(\mathbf {x},\mathbf {y}) \mathrm {d}\mu _\mathbf {y}+\int _{\mathcal {M}}\text{ div } \; \left( \eta ^i(\nabla ^i\nabla u(\mathbf {y})\right) \bar{R}_t(\mathbf {x},\mathbf {y}) \mathrm {d}\mu _\mathbf {y}, \\ r_4(\mathbf {x})= & {} \int _{\mathcal {M}}\text{ div } \; \left( \eta ^i(\nabla ^i\nabla u(\mathbf {y})\right) \bar{R}_t(\mathbf {x},\mathbf {y}) \mathrm {d}\mu _\mathbf {y}+ \int _{{\mathcal {M}}}{\varDelta }_{\mathcal {M}}u(\mathbf {y})\bar{R}_t(\mathbf {x},\mathbf {y}) \mathrm {d}\mu _\mathbf {y}. \end{aligned}$$
where \(\nabla ^i,\; i=1,\ldots ,d\), is the ith component of the gradient \(\nabla \), \(\eta ^i, \; i=1,\ldots ,d\) is the ith component of \(\eta (\mathbf {x},\mathbf {y})\) defined in (21). To simplify the notation, we drop the variable \((\mathbf {x},\mathbf {y})\) in the function \(\eta (\mathbf {x},\mathbf {y})\).
Next, we will prove the theorem by estimating above four terms one by one. First, we consider \(r_1\). Let
$$\begin{aligned} d(\mathbf {x},\mathbf {y})=u(\mathbf {x})-u(\mathbf {y})-(\mathbf {x}-\mathbf {y})\cdot \nabla u(\mathbf {y})-\frac{1}{2}\eta ^i\eta ^j(\nabla ^i\nabla ^j u(\mathbf {y})). \end{aligned}$$
we have
$$\begin{aligned} \int _{\mathcal {M}}|r_1(\mathbf {x})|^2\mathrm {d}\mu _\mathbf {x}= & {} \int _{\mathcal {M}}\left| \int _{\mathcal {M}}R_t(\mathbf {x},\mathbf {y})\mathrm{d}(\mathbf {x},\mathbf {y}) \mathrm {d}\mu _\mathbf {y}\right| ^2\mathrm {d}\mu _\mathbf {x}\\\le & {} (\max _\mathbf {y})^2 \int _{\mathcal {M}}\left( \int _{\mathcal {M}}R_t(\mathbf {x},\mathbf {y})\mathrm {d}\mu _\mathbf {y}\right) \left( \int _{\mathcal {M}}R_t(\mathbf {x},\mathbf {y})|\mathrm{d}(\mathbf {x},\mathbf {y})|^2\mathrm {d}\mu _\mathbf {y}\right) \mathrm {d}\mu _\mathbf {x}\\\le & {} C\int _{\mathcal {M}}\int _{\mathcal {M}}R_t(\mathbf {x},\mathbf {y})|\mathrm{d}(\mathbf {x},\mathbf {y})|^2\mathrm {d}\mu _\mathbf {y}\mathrm {d}\mu _\mathbf {x}\end{aligned}$$
$$\begin{aligned} \int _{\mathcal {M}}\int _{\mathcal {M}}R_t(\mathbf {x},\mathbf {y})|\mathrm{d}(\mathbf {x},\mathbf {y})|^2\mathrm {d}\mu _\mathbf {y}\mathrm {d}\mu _\mathbf {x}= & {} \sum _{i=1}^N \int _{\mathcal {M}}\int _{\mathcal {O}_i}R_t(\mathbf {x},\mathbf {y})|\mathrm{d}(\mathbf {x},\mathbf {y})|^2\mathrm {d}\mu _\mathbf {y}\mathrm {d}\mu _\mathbf {x}\\= & {} \sum _{i=1}^N \int _{\mathcal {O}_i}\left( \int _{{\mathcal {M}}_{\mathbf {y}}^t}R_t(\mathbf {x},\mathbf {y})|\mathrm{d}(\mathbf {x},\mathbf {y})|^2\mathrm {d}\mu _\mathbf {x}\right) \mathrm {d}\mu _\mathbf {y}. \end{aligned}$$
Using Newton–Leibniz formula, we get
$$\begin{aligned} \mathrm{d}(\mathbf {x},\mathbf {y})= & {} u(\mathbf {x})-u(\mathbf {y})-(\mathbf {x}-\mathbf {y})\cdot \nabla u(\mathbf {y})-\frac{1}{2}\eta ^i\eta ^j(\nabla ^i\nabla ^j u(\mathbf {y})) \\= & {} \xi ^{i}\xi ^{i'}\int _0^1\int _0^1\int _0^1s_1\frac{\mathrm{d}}{\mathrm{d}s_3} \left( \partial _{i}{\varPhi }^j(\alpha +s_3 s_1\xi )\partial _{i'}{\varPhi }^{j'}(\alpha +s_3s_2 s_1\xi )\right. \\&\left. \times \nabla ^{j'}\nabla ^ju({\varPhi }(\alpha +s_3s_2s_1 \xi ))\right) \mathrm {d}s_3\mathrm {d}s_2\mathrm {d}s_1 \\= & {} \xi ^{i}\xi ^{i'}\xi ^{i''}\int _0^1\int _0^1\int _0^1s_1^2s_2\partial _{i}{\varPhi }^j(\alpha +s_3 s_1\xi )\partial _{i''}\partial _{i'}{\varPhi }^{j'} \\&\times (\alpha +s_3s_2 s_1\xi )\nabla ^{j'}\nabla ^ju({\varPhi }(\alpha +s_3s_2s_1 \xi )) \mathrm {d}s_3\mathrm {d}s_2\mathrm {d}s_1 \\&+\xi ^{i}\xi ^{i'}\xi ^{i''}\int _0^1\int _0^1\int _0^1s_1^2\partial _{i''}\partial _{i}{\varPhi }^j \\&\times (\alpha +s_3 s_1\xi )\partial _{i'}{\varPhi }^{j'}(\alpha +s_3s_2 s_1\xi )\nabla ^{j'}\nabla ^ju({\varPhi }(\alpha +s_3s_2s_1 \xi )) \mathrm {d}s_3\mathrm {d}s_2\mathrm {d}s_1 \\&+\xi ^{i}\xi ^{i'}\xi ^{i''}\int _0^1\int _0^1\int _0^1s_1^2s_2\partial _{i}{\varPhi }^j \\&\times (\alpha +s_3s_2 s_1\xi )\partial _{i'}{\varPhi }^{j'}(\alpha +s_3s_2 s_1\xi )\partial _{i''}{\varPhi }^{j''}(\alpha +s_3s_2 s_1\xi ) \\&\times \nabla ^{j''}\nabla ^{j'}\nabla ^ju({\varPhi }(\alpha +s_3s_2s_1 \xi ))\mathrm {d}s_3\mathrm {d}s_2\mathrm {d}s_1 \end{aligned}$$
Here, \(\alpha =\alpha (\mathbf {x},\mathbf {y})={\varPhi }_{J(\mathbf {y})}^{-1}(\mathbf {y})\), \(\xi =\xi (\mathbf {x},\mathbf {y})={\varPhi }_{J(\mathbf {y})}^{-1}(\mathbf {x})-{\varPhi }_{J(\mathbf {y})}^{-1}(\mathbf {y})\). In above derivation, we need the convexity property of the parameterization function to make sure all the integrals are well defined.
Using above equality and the smoothness of the parameterization functions, it is easy to show that
$$\begin{aligned}&\int _{\mathcal {O}_i}\left( \int _{{\mathcal {M}}_{\mathbf {y}}^t}R_t(\mathbf {x},\mathbf {y})|\mathrm{d}(\mathbf {x},\mathbf {y})|^2\mathrm {d}\mu _\mathbf {x}\right) \mathrm {d}\mu _\mathbf {y}\\&\quad \le Ct^3 \int _0^1\int _0^1\int _0^1\int _{\mathcal {O}_i}\int _{{\mathcal {M}}_{\mathbf {y}}^t}R_t(\mathbf {x},\mathbf {y})\left| D^{2,3}u({\varPhi }_{J(\mathbf {y})}(\alpha +s_3s_2s_1 \xi ))\right| ^2\mathrm {d}\mu _\mathbf {x}\mathrm {d}\mu _\mathbf {y}\mathrm {d}s_3\mathrm {d}s_2\mathrm {d}s_1 \\&\quad \le Ct^3 \max _{0\le s\le 1}\int _{\mathcal {O}_i}\int _{{\mathcal {M}}_{\mathbf {y}}^t}R_t(\mathbf {x},\mathbf {y})\left| D^{2,3}u({\varPhi }_{i}(\alpha +s \xi ))\right| ^2\mathrm {d}\mu _\mathbf {x}\mathrm {d}\mu _\mathbf {y}, \end{aligned}$$
where we use the fact that \(J(\mathbf {y})=i,\; \mathbf {y}\in \mathcal {O}_i\) and
$$\begin{aligned} \left| D^{2,3}u(\mathbf {x})\right| ^2=\sum _{j,j',j''=1}^d|\nabla ^{j''}\nabla ^{j'}\nabla ^ju(\mathbf {x})|^2 +\sum _{j,j'=1}^d|\nabla ^{j'}\nabla ^ju(\mathbf {x})|^2. \end{aligned}$$
Let \(\mathbf {z}_i={\varPhi }_i(\alpha +s \xi ),\; 0\le s\le 1\), then for any \(\mathbf {y}\in \mathcal {O}_i\subset B_{\mathbf {q}_i}^\delta \) and \(\mathbf {x}\in {\mathcal {M}}_{\mathbf {y}}^t\),
$$\begin{aligned} |\mathbf {z}_i-\mathbf {y}|\le 2s|\xi |\le 4s|\mathbf {x}-\mathbf {y}|\le 8s\sqrt{t},\quad |\mathbf {z}_i-\mathbf {q}_i|\le |\mathbf {z}_i-\mathbf {y}|+|\mathbf {y}-\mathbf {q}_i|\le \delta +8s\sqrt{t}. \end{aligned}$$
We can assume that t is small enough such that \(8\sqrt{t}\le \delta \), then we have
$$\begin{aligned} \mathbf {z}_i\in B_{\mathbf {q}_i}^{2\delta }. \end{aligned}$$
After changing of variable, we obtain
$$\begin{aligned}&\int _{\mathcal {O}_i}\int _{{\mathcal {M}}_{\mathbf {y}}^t}R_t(\mathbf {x},\mathbf {y})\left| D^{2,3}u({\varPhi }_i(\alpha +s \xi ))\right| ^2\mathrm {d}\mu _\mathbf {x}\mathrm {d}\mu _\mathbf {y}\\&\quad \le \frac{C}{\delta _0} \int _{\mathcal {O}_i}\int _{B_{\mathbf {q}_i}^{2\delta }}\frac{1}{s^k}R\left( \frac{|\mathbf {z}_i-\mathbf {y}|^2}{128s^2t}\right) \left| D^{2,3}u(\mathbf {z}_i)\right| ^2\mathrm {d}\mu _{\mathbf {z}_i}\mathrm {d}\mu _\mathbf {y}\\&\quad =\frac{C}{\delta _0} \int _{\mathcal {O}_i}\frac{1}{s^k}R\left( \frac{|\mathbf {z}_i-\mathbf {y}|^2}{128s^2t}\right) \mathrm {d}\mu _\mathbf {y}\int _{B_{\mathbf {q}_i}^{2\delta }}\left| D^{2,3}u(\mathbf {z}_i)\right| ^2\mathrm {d}\mu _{\mathbf {z}_i} \\&\quad \le C \int _{B_{\mathbf {q}_i}^{2\delta }}\left| D^{2,3}u(\mathbf {x})\right| ^2\mathrm {d}\mu _{\mathbf {x}}. \end{aligned}$$
This estimate would give us that
$$\begin{aligned} \Vert r_1(\mathbf {x})\Vert _{L^2({\mathcal {M}})}\le Ct^{1/2}\Vert u\Vert _{H^3({\mathcal {M}})} \end{aligned}$$
Now, we turn to estimate the gradient of \(r_1\).
$$\begin{aligned} \int _{\mathcal {M}}|\nabla _\mathbf {x}r_1(\mathbf {x})|^2\mathrm {d}\mu _\mathbf {x}\le & {} C\int _{\mathcal {M}}\left| \int _{\mathcal {M}}\nabla _\mathbf {x}R_t(\mathbf {x},\mathbf {y})\mathrm{d}(\mathbf {x},\mathbf {y}) \mathrm {d}\mu _\mathbf {y}\right| ^2\mathrm {d}\mu _\mathbf {x}\\&+C\int _{\mathcal {M}}\left| \int _{\mathcal {M}}R_t(\mathbf {x},\mathbf {y})\nabla _\mathbf {x}\mathrm{d}(\mathbf {x},\mathbf {y}) \mathrm {d}\mu _\mathbf {y}\right| ^2\mathrm {d}\mu _\mathbf {x}, \end{aligned}$$
where \(\nabla _\mathbf {x}\) is the gradient in \({\mathcal {M}}\) with respect to \(\mathbf {x}\).
Using the same techniques in the calculation of \(\Vert r_1(\mathbf {x})\Vert _{L^2({\mathcal {M}})}\), we get that the first term of right-hand side can bounded as follows
$$\begin{aligned} \int _{\mathcal {M}}\left| \int _{\mathcal {M}}\nabla _\mathbf {x}R_t(\mathbf {x},\mathbf {y})\mathrm{d}(\mathbf {x},\mathbf {y}) \mathrm {d}\mu _\mathbf {y}\right| ^2\mathrm {d}\mu _\mathbf {x}\le C \Vert u\Vert _{H^3({\mathcal {M}})}^2. \end{aligned}$$
The estimation of second term is a little involved. First, we have
$$\begin{aligned} \int _{\mathcal {M}}\left| \int _{\mathcal {M}}R_t(\mathbf {x},\mathbf {y})\nabla _\mathbf {x}\mathrm{d}(\mathbf {x},\mathbf {y}) \mathrm {d}\mu _\mathbf {y}\right| ^2\mathrm {d}\mu _\mathbf {x}\le & {} C\int _{\mathcal {M}}\left( \int _{\mathcal {M}}R_t(\mathbf {x},\mathbf {y})|\nabla _\mathbf {x}\mathrm{d}(\mathbf {x},\mathbf {y})|^2\mathrm {d}\mu _\mathbf {y}\right) \mathrm {d}\mu _\mathbf {x}\\= & {} C\sum _{i=1}^N \int _{\mathcal {O}_i}\left( \int _{{\mathcal {M}}_{\mathbf {y}}^t}R_t(\mathbf {x},\mathbf {y})|\nabla _\mathbf {x}\mathrm{d}(\mathbf {x},\mathbf {y})|^2\mathrm {d}\mu _\mathbf {x}\right) \mathrm {d}\mu _\mathbf {y}. \end{aligned}$$
Also using Newton–Leibniz formula, we have
$$\begin{aligned} \mathrm{d}(\mathbf {x},\mathbf {y})= & {} \xi ^{i}\xi ^{i'}\int _0^1\int _0^1s_1\left( \partial _{i}{\varPhi }^j(\alpha + s_1\xi )\partial _{i'}{\varPhi }^{j'}(\alpha +s_2 s_1\xi )\right. \\&\left. \times \nabla ^{j'}\nabla ^ju({\varPhi }(\alpha +s_2s_1 \xi ))\right) \mathrm {d}s_2\mathrm {d}s_1 \\&-\xi ^{i}\xi ^{i'}\int _0^1\int _0^1s_1\left( \partial _{i}{\varPhi }^j(\alpha )\partial _{i'}{\varPhi }^{j'}(\alpha )\nabla ^{j'}\nabla ^ju({\varPhi }(\alpha ))\right) \mathrm {d}s_2\mathrm {d}s_1 \end{aligned}$$
Then, the gradient of \(\mathrm{d}(\mathbf {x},\mathbf {y})\) has following representation,
$$\begin{aligned} \nabla _\mathbf {x}\mathrm{d}(\mathbf {x},\mathbf {y})= & {} \xi ^{i}\xi ^{i'}\nabla _\mathbf {x}\left( \int _0^1\int _0^1s_1\left( \partial _{i}{\varPhi }^j(\alpha + s_1\xi )\partial _{i'}{\varPhi }^{j'}(\alpha +s_2 s_1\xi ) \right. \right. \\&\times \left. \left. \nabla ^{j'}\nabla ^ju({\varPhi }(\alpha +s_2s_1 \xi ))\right) \mathrm {d}s_2\mathrm {d}s_1\right) \\&+\nabla _\mathbf {x}\left( \xi ^{i}\xi ^{i'}\right) \int _0^1\int _0^1\int _0^1s_1\frac{d}{d s_3}\left( \partial _{i}{\varPhi }^j(\alpha + s_3s_1\xi )\partial _{i'}{\varPhi }^{j'}(\alpha +s_3s_2 s_1\xi ) \right. \\&\times \left. \nabla ^{j'}\nabla ^ju({\varPhi }(\alpha +s_3s_2s_1 \xi ))\right) \mathrm {d}s_3\mathrm {d}s_2\mathrm {d}s_1 \\= & {} d_1(\mathbf {x},\mathbf {y})+d_2(\mathbf {x},\mathbf {y}). \end{aligned}$$
For \(d_1\), we have
$$\begin{aligned}&\int _{\mathcal {O}_i}\left( \int _{{\mathcal {M}}_{\mathbf {y}}^t}R_t(\mathbf {x},\mathbf {y})|d_1(\mathbf {x},\mathbf {y})|^2\mathrm {d}\mu _\mathbf {x}\right) \mathrm {d}\mu _\mathbf {y}\\&\quad \le Ct^2\max _{0\le s\le 1} \int _{\mathcal {O}_i}\left( \int _{{\mathcal {M}}_{\mathbf {y}}^t}R_t(\mathbf {x},\mathbf {y})|D^{2,3}u({\varPhi }_i(\alpha +s \xi ))|^2\mathrm {d}\mu _\mathbf {x}\right) \mathrm {d}\mu _\mathbf {y}, \end{aligned}$$
which means that
$$\begin{aligned} \int _{\mathcal {O}_i}\left( \int _{{\mathcal {M}}_{\mathbf {y}}^t}R_t(\mathbf {x},\mathbf {y})|d_1(\mathbf {x},\mathbf {y})|^2\mathrm {d}\mu _\mathbf {x}\right) \mathrm {d}\mu _\mathbf {y}\le C \int _{B_{\mathbf {q}_i}^{2\delta }}|D^{2,3}u(\mathbf {x})|^2\mathrm {d}\mu _\mathbf {x}\end{aligned}$$
For \(d_2\), we have
$$\begin{aligned} d_2(\mathbf {x},\mathbf {y})= & {} \nabla _\mathbf {x}\left( \xi ^{i}\xi ^{i'}\right) \int _{[0,1]^3}s_1\frac{\mathrm{d}}{\mathrm{d} s_3}\left( \partial _{i}{\varPhi }^j(\alpha + s_3s_1\xi )\partial _{i'}{\varPhi }^{j'}(\alpha +s_3s_2 s_1\xi ) \right. \\&\times \left. \nabla ^{j'}\nabla ^ju({\varPhi }(\alpha +s_3s_2s_1 \xi ))\right) \mathrm {d}s_3\mathrm {d}s_2\mathrm {d}s_1 \\= & {} \nabla _\mathbf {x}\left( \xi ^{i}\xi ^{i'}\right) \xi ^{i''}\int _{[0,1]^3} s_1^2s_2\partial _{i}{\varPhi }^j(\alpha +s_3 s_1\xi )\partial _{i''}\partial _{i'}{\varPhi }^{j'}(\alpha +s_3s_2 s_1\xi ) \\&\times \nabla ^{j'}\nabla ^ju({\varPhi }(\alpha +s_3s_2s_1 \xi )) \mathrm {d}s_3\mathrm {d}s_2\mathrm {d}s_1 \\&+\nabla _\mathbf {x}\left( \xi ^{i}\xi ^{i'}\right) \xi ^{i''}\int _{[0,1]^3}s_1^2 \partial _{i''}\partial _{i}{\varPhi }^j(\alpha +s_3 s_1\xi )\partial _{i'}{\varPhi }^{j'}(\alpha +s_3s_2 s_1\xi ) \\&\times \nabla ^{j'}\nabla ^ju({\varPhi }(\alpha +s_3s_2s_1 \xi )) \mathrm {d}s_3\mathrm {d}s_2\mathrm {d}s_1 \\&+\nabla _\mathbf {x}\left( \xi ^{i}\xi ^{i'}\right) \xi ^{i''}\int _{[0,1]^3} s_1^2s_2\partial _{i} {\varPhi }^j(\alpha +s_2 s_1\xi )\partial _{i'} \\&\times {\varPhi }^{j'}(\alpha +s_3s_2 s_1\xi )\partial _{i''}{\varPhi }^{j''}(\alpha +s_3s_2 s_1\xi ) \\&\times \nabla ^{j''}\nabla ^{j'}\nabla ^ju({\varPhi }(\alpha +s_3s_2s_1 \xi ))\mathrm {d}s_3\mathrm {d}s_2\mathrm {d}s_1 \end{aligned}$$
This formula tells us that
$$\begin{aligned}&\int _{\mathcal {O}_i}\left( \int _{{\mathcal {M}}_{\mathbf {y}}^t}R_t(\mathbf {x},\mathbf {y})|d_2(\mathbf {x},\mathbf {y})|^2\mathrm {d}\mu _\mathbf {x}\right) \mathrm {d}\mu _\mathbf {y}\\&\quad \le Ct^2\max _{0\le s\le 1} \int _{\mathcal {O}_i}\left( \int _{{\mathcal {M}}_{\mathbf {y}}^t}R_t(\mathbf {x},\mathbf {y})|D^{2,3}u({\varPhi }(\alpha +s \xi ))|^2\mathrm {d}\mu _\mathbf {x}\right) \mathrm {d}\mu _\mathbf {y}. \end{aligned}$$
Using the same arguments as that in the calculation of \(\Vert r_1\Vert _{L^2({\mathcal {M}})}\), we have
$$\begin{aligned} \int _{\mathcal {O}_i}\left( \int _{{\mathcal {M}}_{\mathbf {y}}^t}R_t(\mathbf {x},\mathbf {y})|d_2(\mathbf {x},\mathbf {y})|^2\mathrm {d}\mu _\mathbf {x}\right) \mathrm {d}\mu _\mathbf {y}\le C \int _{B_{\mathbf {q}_i}^{2\delta }}|D^3u(\mathbf {x})|^2\mathrm {d}\mu _\mathbf {x}\end{aligned}$$
Combining (24) and (25), we have
$$\begin{aligned} \Vert \nabla r_1(\mathbf {x})\Vert _{L^2({\mathcal {M}})}\le C\Vert u\Vert _{H^3({\mathcal {M}})} \end{aligned}$$
For \(r_2\), first, notice that
$$\begin{aligned} \nabla ^j\bar{R}_t(\mathbf {x},\mathbf {y})= & {} \frac{1}{2t}\partial _{m'}{\varPhi }^j(\alpha ) g^{m'n'}\partial _{n'}{\varPhi }^i(\alpha ) (x^i-y^i)R_t(\mathbf {x}, \mathbf {y}), \\ \frac{\eta ^j}{2t}R_t(\mathbf {x},\mathbf {y})= & {} \frac{1}{2t}\partial _{m'}{\varPhi }^j(\alpha ) g^{m'n'}\partial _{n'}{\varPhi }^i(\alpha ) \xi ^{i'}\partial _{i'}{\varPhi }^iR_t(\mathbf {x}, \mathbf {y}). \end{aligned}$$
Then, we have
$$\begin{aligned}&\nabla ^j\bar{R}_t(\mathbf {x},\mathbf {y})-\frac{\eta ^j}{2t}R_t(\mathbf {x},\mathbf {y}) \\&\quad =\frac{1}{2t}\partial _{m'}{\varPhi }^i g^{m'n'}\partial _{n'}{\varPhi }^j \left( x^j-y^j-\xi ^{i'}\partial _{i'}{\varPhi }^j\right) R_t(\mathbf {x}, \mathbf {y})\\&\quad = \frac{1}{2t}\xi ^{i'}\xi ^{j'}\partial _{m'}{\varPhi }^i g^{m'n'}\partial _{n'}{\varPhi }^j \left( \int _0^1\int _0^1s\partial _{j'}\partial _{i'}{\varPhi }^j(\alpha +\tau s \xi )\mathrm {d}\tau \mathrm {d}s\right) R_t(\mathbf {x}, \mathbf {y})\end{aligned}$$
Thus, we get
$$\begin{aligned} \left| \nabla ^j\bar{R}_t(\mathbf {x},\mathbf {y})-\frac{\eta ^j}{2t}R_t(\mathbf {x},\mathbf {y})\right|\le & {} \frac{C|\xi |^2}{t}R_t(\mathbf {x}, \mathbf {y})\\ \left| \nabla _\mathbf {x}\left( \nabla ^j\bar{R}_t(\mathbf {x},\mathbf {y})-\frac{\eta ^j}{2t}R_t(\mathbf {x},\mathbf {y})\right) \right|\le & {} \frac{C|\xi |}{t}R_t(\mathbf {x}, \mathbf {y})+\frac{C|\xi |^3}{t^2}|R'_t(\mathbf {x},\mathbf {y})|. \end{aligned}$$
Then, we have following bound for \(r_2\),
$$\begin{aligned}&\int _{{\mathcal {M}}}|r_2(\mathbf {x})|^2\mathrm {d}\mu _\mathbf {x}\nonumber \\&\quad \le Ct\int _{\mathcal {M}}\left( \int _{\mathcal {M}}R_t(\mathbf {x}, \mathbf {y})|D^2u(\mathbf {y})| \mathrm {d}\mu _\mathbf {y}\right) ^2\mathrm {d}\mu _\mathbf {x}\nonumber \\&\quad \le Ct\int _{\mathcal {M}}\left( \int _{\mathcal {M}}R_t(\mathbf {x}, \mathbf {y})\mathrm {d}\mu _\mathbf {y}\right) \int _{\mathcal {M}}R_t(\mathbf {x}, \mathbf {y})|D^2u(\mathbf {y})|^2 \mathrm {d}\mu _\mathbf {y}\mathrm {d}\mu _\mathbf {x}\nonumber \\&\quad \le Ct \max _{\mathbf {y}}\left( \int _{\mathcal {M}}R_t(\mathbf {x}, \mathbf {y})\mathrm {d}\mu _\mathbf {x}\right) \int _{\mathcal {M}}|D^2u(\mathbf {y})|^2 \mathrm {d}\mu _\mathbf {y}\nonumber \\&\quad \le Ct\Vert u\Vert _{H^2({\mathcal {M}})}^2. \end{aligned}$$
Similarly, we have
$$\begin{aligned}&\int _M |\nabla r_2(\mathbf {x})|^2\mathrm {d}\mu _\mathbf {x}\nonumber \\&\quad \le Ct\int _{\mathcal {M}}\left( \int _{\mathcal {M}}\nabla _\mathbf {x}R_t(\mathbf {x}, \mathbf {y})\mathrm {d}\mu _\mathbf {y}\right) \int _{\mathcal {M}}\nabla _\mathbf {x}R_t(\mathbf {x}, \mathbf {y})|D^2u(\mathbf {y})|^2 \mathrm {d}\mu _\mathbf {y}\mathrm {d}\mu _\mathbf {x}\nonumber \\&\quad \le C\sqrt{t} \max _{\mathbf {y}}\left( \int _{\mathcal {M}}\nabla _\mathbf {x}R_t(\mathbf {x}, \mathbf {y})\mathrm {d}\mu _\mathbf {x}\right) \int _{\mathcal {M}}|D^2u(\mathbf {y})|^2 \mathrm {d}\mu _\mathbf {y}\nonumber \\&\quad \le C\Vert u\Vert _{H^2({\mathcal {M}})}^2. \end{aligned}$$
\(r_3\) is relatively easy to estimate by using the well known Gauss formula.
$$\begin{aligned} r_3(\mathbf {x})&=\int _{\partial \mathcal {M}}n^{j}\eta ^{i}(\nabla ^{i} \nabla ^{j}u(\mathbf {y})) \bar{R}_t(\mathbf {x}, \mathbf {y})\mathrm {d}\tau _\mathbf {y}=\tilde{I}_{bd}, \end{aligned}$$
where \(\tilde{I}_{bd}=\int _{\partial \mathcal {M}}n^{j}\eta ^{i}(\nabla ^{i} \nabla ^{j}u(\mathbf {y})) \bar{R}_t(\mathbf {x}, \mathbf {y})\mathrm {d}\tau _\mathbf {y}\).
Now, we turn to bound the last term \(r_4\). Notice that
$$\begin{aligned} \nabla ^j\left( \nabla ^{j}u(\mathbf {y})\right)&=(\partial _{k'} {\varPhi }^j)g^{k'l'}\partial _{l'}\left( (\partial _{m'}{\varPhi }^j)g^{m'n'}(\partial _{n'} u )\right) \nonumber \\&=(\partial _{k'}{\varPhi }^j)g^{k'l'}\left( \partial _{l'}(\partial _{m'}{\varPhi }^j)\right) g^{m'n'}(\partial _{n'}u)\nonumber \\&\quad +(\partial _{k'}{\varPhi }^j)g^{k'l'}(\partial _{m'}{\varPhi }^j)\partial _{l'} \left( g^{m'n'}(\partial _{n'}u)\right) \nonumber \\&=\frac{1}{\sqrt{\det G}}(\partial _{m'}\sqrt{\det G}) g^{m'n'}(\partial _{n'}u)+\partial _{m'}\left( g^{m'n'}(\partial _{n'}u)\right) \nonumber \\&=\frac{1}{\sqrt{\det G}}\partial _{m'}\left( \sqrt{\det G} g^{m'n'}(\partial _{n'}u)\right) ={\varDelta }_{\mathcal {M}}u(\mathbf {y}), \end{aligned}$$
where \(\det G\) is the determinant of G and \(G=(g_{ij})_{i,j=1,\ldots ,k}\). Here, we use the fact that
$$\begin{aligned} (\partial _{k'}{\varPhi }^j)g^{k'l'}\left( \partial _{l'}(\partial _{m'}{\varPhi }^j)\right)&=(\partial _{k'}{\varPhi }^j)g^{k'l'}\left( \partial _{m'}(\partial _{l'}{\varPhi }^j)\right) \\&=(\partial _{m'}(\partial _{k'}{\varPhi }^j))g^{k'l'}(\partial _{l'}{\varPhi }^j) \\&=\frac{1}{2}g^{k'l'}\partial _{m'}(g_{k'l'}) \\&=\frac{1}{\sqrt{\det G}}(\partial _{m'}\sqrt{\det G}). \end{aligned}$$
Moreover, we have
$$\begin{aligned}&g^{i'j'}(\partial _{j'}{\varPhi }^{j})(\partial _{i'}\xi ^{l}) (\partial _{l}{\varPhi }^{i})(\nabla ^{i}\nabla ^{j}u(\mathbf {y}))\nonumber \\&\quad =- g^{i'j'}(\partial _{j'}{\varPhi }^{j})(\partial _{i'}{\varPhi }^{i})(\nabla ^{i}\nabla ^{j}u(\mathbf {y}))\nonumber \\&\quad = - g^{i'j'}(\partial _{j'}{\varPhi }^{j})(\partial _{i'}{\varPhi }^{i})(\partial _{m'} {\varPhi }^{i})g^{m'n'}\partial _{n'}\left( \nabla ^{j}u(\mathbf {y}) \right) \nonumber \\&\quad = - g^{i'j'}(\partial _{j'}{\varPhi }^{j})\partial _{i'}\left( \nabla ^{j}u(\mathbf {y})\right) \nonumber \\&\quad = - \nabla ^{j}\left( \nabla ^{j}u(\mathbf {y})\right) , \end{aligned}$$
where the first equalities are due to that \(\partial _{i'}\xi ^l = -\delta _{i'}^l\). Then we have
$$\begin{aligned}&\text{ div } \; \left( \eta ^i(\nabla ^i\nabla ^j u(\mathbf {y}))\right) +{\varDelta }_{\mathcal {M}}u(\mathbf {y}) \\&\quad = \frac{1}{\sqrt{\det G}}\,\partial _{i'}\left( \sqrt{\det G}\,g^{i'j'}(\partial _{j'}{\varPhi }^j) \xi ^{l}(\partial _l {\varPhi }^i)(\nabla ^i\nabla ^j u(\mathbf {y}))\right) \\&\qquad -\,g^{i'j'}(\partial _{j'}{\varPhi }^{j})(\partial _{i'}\xi ^{l}) (\partial _{l}{\varPhi }^{i})(\nabla ^{i}\nabla ^{j}u(\mathbf {y})) \\&\quad = \frac{\xi ^l}{\sqrt{\det G}}\,\partial _{i'}\left( \sqrt{\det G}\,g^{i'j'}(\partial _{j'}{\varPhi }^j) (\partial _l {\varPhi }^i)(\nabla ^i\nabla ^j u(\mathbf {y}))\right) . \end{aligned}$$
Here, we use the equalities (30), (31), \(\eta ^i = \xi ^{l} \partial _{i'}{\varPhi }^l\) and the definition of \(\text{ div }\),
$$\begin{aligned} \text{ div }X = \frac{1}{\sqrt{\det G}}\partial _{i'} (\sqrt{\det G}\,g^{i'j'}\partial _{j'}{\varPhi }^k X^k), \end{aligned}$$
where X is a smooth tangent vector field on \({\mathcal {M}}\) and \((X^1,\ldots ,X^d)^t\) is its representation in embedding coordinates.
$$\begin{aligned} r_4(\mathbf {x})=\int _\mathcal {M}\frac{\xi ^l}{\sqrt{\det G}}\,\partial _{i'}\left( \sqrt{\det G}\,g^{i'j'} (\partial _{j'}{\varPhi }^j) (\partial _l {\varPhi }^i)(\nabla ^i\nabla ^j u(\mathbf {y}))\right) \bar{R}_t(\mathbf {x}, \mathbf {y})\mathrm {d}\mu _\mathbf {y}. \end{aligned}$$
Then, it is easy to get that
$$\begin{aligned} \Vert r_4(\mathbf {x})\Vert _{L^2({\mathcal {M}})}\le & {} C t^{1/2}\Vert u\Vert _{H^3({\mathcal {M}})},\end{aligned}$$
$$\begin{aligned} \Vert \nabla r_4(\mathbf {x})\Vert _{L^2({\mathcal {M}})}\le & {} C\Vert u\Vert _{H^3({\mathcal {M}})}. \end{aligned}$$
By combining (23), (26), (27), (28), (29), (33), (34), we know that
$$\begin{aligned} \Vert r-\tilde{I}_{bd}\Vert _{L^2({\mathcal {M}})}\le & {} C t^{1/2}\Vert u\Vert _{H^3({\mathcal {M}})},\end{aligned}$$
$$\begin{aligned} \Vert \nabla (r-\tilde{I}_{bd})\Vert _{L^2({\mathcal {M}})}\le & {} C\Vert u\Vert _{H^3({\mathcal {M}})}. \end{aligned}$$
Using the definition of \(I_{bd}\) and \(\tilde{I}_{bd}\), we obtain
$$\begin{aligned} I_{bd}-\tilde{I}_{bd}=\int _{\partial \mathcal {M}}n^{j}(\mathbf {y})(\mathbf {x}-\mathbf {y}-\eta (\mathbf {x},\mathbf {y}))\cdot (\nabla \nabla ^{j}u(\mathbf {y})) \bar{R}_t(\mathbf {x}, \mathbf {y})\mathrm {d}\tau _\mathbf {y}. \end{aligned}$$
Using the definition of \(\eta (\mathbf {x},\mathbf {y})\), it is easy to check that
$$\begin{aligned} |\mathbf {x}-\mathbf {y}-\eta (\mathbf {x},\mathbf {y})|=O(|\mathbf {x}-\mathbf {y}|^2),\quad |\nabla _{\mathbf {x}}(\mathbf {x}-\mathbf {y}-\eta (\mathbf {x},\mathbf {y}))|=O(|\mathbf {x}-\mathbf {y}|), \end{aligned}$$
which implies that
$$\begin{aligned} \Vert I_{bd}-\tilde{I}_{bd}\Vert _{L^2({\mathcal {M}})}\le & {} C t^{3/4}\Vert u\Vert _{H^2({\mathcal {M}})}, \end{aligned}$$
$$\begin{aligned} \Vert \nabla (I_{bd}-\tilde{I}_{bd})\Vert _{L^2({\mathcal {M}})}\le & {} Ct^{1/4}\Vert u\Vert _{H^3({\mathcal {M}})}. \end{aligned}$$
The theorem is proved by putting (35), (36), (37), (38) together.

6 Error analysis of the discretization (Theorem 3)

In this section, we estimate the discretization error introduced by approximating the integrals in (14) that is to prove Theorem 3. To simplify the notation, we introduce an intermediate operator defined as follows,
$$\begin{aligned} L_{t, h}u(\mathbf {x}) = \frac{1}{t}\sum _{j=1}^n R_t(\mathbf {x}, \mathbf{p }_j)(u(\mathbf {x}) - u(\mathbf{p }_j))V_j. \end{aligned}$$
If \(u_{t,h}=I_{\mathbf {f}}(\mathbf {u})\) with \(\mathbf {u}\) satisfying equation (10), one can verify that the following equation is satisfied,
$$\begin{aligned} L_{t, h}u_{t,h}(\mathbf {x}) = \sum _{j=1}^n \bar{R}_t(\mathbf {x}, \mathbf{p }_j)f(\mathbf{p }_j)V_j. \end{aligned}$$
We introduce a discrete operator \(\mathcal {L}: \mathbb {R}^n\rightarrow \mathbb {R}^n\) where \(n=|P|\). For any \(\mathbf{u }=(u_1,\ldots ,u_n)^t\), denote
$$\begin{aligned} \left( \mathcal {L}\mathbf {u}\right) _i = \frac{1}{t}\sum _{j=1}^n R_t(\mathbf{p }_i,\mathbf{p }_j)(u_i - u_j)V_j. \end{aligned}$$
For this operator, we have the following important theorem.

Theorem 6

Under the assumptions in Assumption 1, there exist constants \(C>0,\, C_0>0\), \(T_0\) independent on t so that for any \(\mathbf{u } = (u_1, \ldots , u_n)^t \in \mathbb {R}^d\) with \(\sum _{i=1}^n u_iV_i = 0\), \(t\le T_0\) and sufficient small \(\frac{h(P,\mathbf {V},{\mathcal {M}})}{\sqrt{t}}\)
$$\begin{aligned} \left\langle \mathbf{u }, {\mathcal {L}} \mathbf{u } \right\rangle _{\mathbf {V}} \ge C\left( 1-\frac{C_0h(P,\mathbf {V},{\mathcal {M}})}{\sqrt{t}}\right) \left\langle \mathbf{u }, \mathbf{u }\right\rangle _{\mathbf {V}}, \end{aligned}$$
where \(\left<\mathbf{u }, \mathbf{v }\right>_{\mathbf {V}} = \sum _{i=1}^n u_iv_iV_i\) for any \(\mathbf{u } = (u_1, \ldots , u_n), \mathbf{v } =(v_1, \ldots , v_n)\).

The proof of the above theorem is deferred to “Appendix D.”

It has an easy corollary which gives a priori estimate of \(\mathbf {u}=(u_1, \ldots , u_n)^t\) solving the discrete problem (10).

Lemma 1

Suppose \(\mathbf {u}=(u_1, \ldots , u_n)^t\) with \(\sum _i u_i V_i = 0\) solves the problem (10) and \(\mathbf{f }=(f(\mathbf{p }_1), \ldots , f(\mathbf{p }_n))^t\) for \(f\in C(\mathcal {M})\),

there exists a constant \(C>0\) such that
$$\begin{aligned} \left( \sum _{i=1}^nu_i^2V_i\right) ^{1/2}\le C\Vert f\Vert _\infty , \end{aligned}$$
provided t and \(\frac{h(P,\mathbf {V},{\mathcal {M}})}{\sqrt{t}}\) are small enough.


From Theorem 6, we have
$$\begin{aligned} \sum _{i=1}^{n} u_i^2 V_i\le & {} \sum _{i=1}^{n} \left( \sum _{j=1}^n \bar{R}_t(\mathbf{p }_i, \mathbf{p }_j)f_jV_j \right) u_iV_i \\\le & {} \left( \sum _{i=1}^{n} u_i^2V_i\right) ^{1/2} \left( \sum _{i=1}^{n} \left( \Vert f\Vert _\infty \sum _{p_j \in P} \bar{R}_t(\mathbf{p }_i, \mathbf{p }_j)V_j \right) ^2 V_i\right) ^{1/2} \\\le & {} C\left( \sum _{i=1}^{n} u_i^2V_i\right) ^{1/2} \Vert f\Vert _\infty . \end{aligned}$$
This proves the lemma.

We are now ready to prove Theorem 3.

Proof of Theorem 3

$$\begin{aligned} u_{t,h}(\mathbf {x}) = \frac{1}{w_{t,h}(\mathbf {x})}\left( \sum _{j=1}^nR_t(\mathbf {x},\mathbf{p }_j)u_jV_j -t\sum _{j=1}^n\bar{R}_t(\mathbf {x},\mathbf{p }_j)f_jV_j\right) , \end{aligned}$$
where \(\mathbf {u}=(u_1, \ldots , u_n)^t\) with \(\sum _{i=1}^n u_i V_i = 0\) solves the problem (10), \( f_j = f(\mathbf{p }_j)\) and \(w_{t,h}(\mathbf {x})=\sum _{j=1}^nR_t(\mathbf {x},\mathbf{p }_j)V_j\). For convenience, we set
$$\begin{aligned} a_{t,h}(\mathbf {x})= & {} \frac{1}{w_{t,h}(\mathbf {x})}\sum _{j=1}^nR_t(\mathbf {x},\mathbf{p }_j)u_jV_j, \\ c_{t,h}(\mathbf {x})= & {} -\frac{t}{w_{t,h}(\mathbf {x})}\sum _{j=1}^n\bar{R}_t(\mathbf {x},\mathbf{p }_j)f(\mathbf{p }_j)V_j, \end{aligned}$$
and thus \(u_{t,h} = a_{t, h} +c_{t, h}\).

In the proof, to simplify the notation, we denote \(h=h(P,\mathbf {V},{\mathcal {M}})\) and \(n=|P|\).

First we upper bound \(\Vert L_t(u_{t,h}) - L_{t, h}(u_{t, h})\Vert _{L^2({\mathcal {M}})}\). For \(c_{t, h}\), we have
$$\begin{aligned}&\left| \left( L_tc_{t, h} - L_{t, h}c_{t, h}\right) (\mathbf {x})\right| \\&\quad = \frac{1}{t} \left| \int _{\mathcal {M}}R_t(\mathbf {x},\mathbf {y})(c_{t,h}(\mathbf {x})-c_{t,h}(\mathbf {y})) \mathrm {d}\mu _\mathbf {y}-\sum _{j=1}^nR_t(\mathbf {x},\mathbf{p }_j)(c_{t,h}(\mathbf {x})-c_{t,h}(\mathbf{p }_j))V_j\right| \\&\quad \le \frac{1}{t} \left| c_{t,h}(\mathbf {x})\right| \left| \int _{\mathcal {M}}R_t(\mathbf {x},\mathbf {y}) \mathrm {d}\mu _\mathbf {y}-\sum _{j=1}^nR_t(\mathbf {x},\mathbf{p }_j)V_j\right| \\&\qquad + \frac{1}{t}\left| \int _{\mathcal {M}}R_t(\mathbf {x},\mathbf {y})c_{t,h}(\mathbf {y}) \mathrm {d}\mu _\mathbf {y}-\sum _{j=1}^nR_t(\mathbf {x},\mathbf{p }_j)c_{t,h}(\mathbf{p }_j)V_j\right| \\&\quad \le \frac{Ch}{t^{3/2}}\left| c_{t,h}(\mathbf {x})\right| + \frac{Ch}{t^{3/2}} \Vert c_{t,h}\Vert _{C^1({\mathcal {M}})} \\&\quad \le \frac{Ch}{t^{3/2}}t\Vert f\Vert _\infty + \frac{Ch}{t^{3/2}}(t\Vert f\Vert _\infty + t^{1/2}\Vert f\Vert _{\infty })\le \frac{Ch}{t}\Vert f\Vert _{\infty }. \end{aligned}$$
For \(a_{t, h}\), we have
$$\begin{aligned}&\int _{\mathcal {M}}\left( a_{t,h}(\mathbf {x})\right) ^2\left| \int _{\mathcal {M}}R_t(\mathbf {x},\mathbf {y}) \mathrm {d}\mu _\mathbf {y}-\sum _{j=1}^nR_t(\mathbf {x},\mathbf{p }_j)V_j\right| ^2\mathrm {d}\mu _\mathbf {x}\nonumber \\&\quad \le \frac{Ch^2}{t}\int _{\mathcal {M}}\left( a_{t,h}(\mathbf {x})\right) ^2\mathrm {d}\mu _\mathbf {x}\le \frac{Ch^2}{t} \int _{\mathcal {M}} \left( \frac{1}{w_{t, h}(\mathbf {x})} \sum _{j=1}^nR_t(\mathbf {x},\mathbf{p }_j)u_jV_j \right) ^2 \mathrm {d}\mu _\mathbf {x}\nonumber \\&\quad \le \frac{Ch^2}{t} \int _{\mathcal {M}} \left( \sum _{j=1}^nR_t(\mathbf {x},\mathbf{p }_j)u_j^2V_j \right) \left( \sum _{j=1}^nR_t(\mathbf {x},\mathbf{p }_j)V_j \right) \mathrm {d}\mu _\mathbf {x}\nonumber \\&\quad \le \frac{Ch^2}{t} \left( \sum _{j=1}^{n}u_j^2V_j \int _{\mathcal {M}}R_t(\mathbf {x},\mathbf{p }_j) \mathrm {d}\mu _\mathbf {x}\right) \le \frac{Ch^2}{t}\sum _{j=1}^{n}u_j^2V_j. \end{aligned}$$
$$\begin{aligned} A= & {} C_t\int _{\mathcal {M}}\frac{1}{w_{t, h}(\mathbf {y})}R\left( \frac{|\mathbf {x}-\mathbf {y}|^2}{4t}\right) R\left( \frac{|\mathbf{p }_i-\mathbf {y}|^2}{4t}\right) \mathrm {d}\mu _\mathbf {y}\\&- C_t\sum _{j=1}^n \frac{1}{w_{t, h}(\mathbf{p }_j)}R\left( \frac{|\mathbf {x}-\mathbf{p }_j|^2}{4t}\right) R\left( \frac{|\mathbf{p }_i-\mathbf{p }_j|^2}{4t}\right) V_j. \end{aligned}$$
We have \(|A|<\frac{Ch}{t^{1/2}}\) for some constant C independent of t. In addition, notice that only when \(|\mathbf {x}-\mathbf{p }_i|^2\le 16t \) is \(A\ne 0\), which implies
$$\begin{aligned} |A| \le \frac{1}{\delta _0}|A|R\left( \frac{|\mathbf {x}-\mathbf{p }_i|^2}{32t}\right) . \end{aligned}$$
Then, we have
$$\begin{aligned}&\int _{\mathcal {M}}\left| \int _{\mathcal {M}}R_t(\mathbf {x},\mathbf {y})a_{t,h}(\mathbf {y}) \mathrm {d}\mu _\mathbf {y}-\sum _{j=1}^nR_t(\mathbf {x},\mathbf{p }_j)a_{t,h}(\mathbf{p }_j)V_j\right| ^2\mathrm {d}\mu _\mathbf {x}\nonumber \\&\quad = \int _{\mathcal {M}}\left( \sum _{i=1}^{n}C_tu_iV_i A \right) ^2\mathrm {d}\mu _\mathbf {x}\le \frac{Ch^2}{t} \int _{\mathcal {M}}\left( \sum _{i=1}^{n} C_t|u_i|V_i R\left( \frac{|\mathbf {x}-\mathbf{p }_i|^2}{32t}\right) \right) ^2 \mathrm {d}\mu _\mathbf {x}\nonumber \\&\quad \le \frac{Ch^2}{t} \int _{\mathcal {M}} \left( \sum _{i=1}^{n} C_t R\left( \frac{|\mathbf {x}-\mathbf{p }_i|^2}{32t}\right) u^2_iV_i\right) \left( \sum _{\mathbf{p }_i\in P} C_t R\left( \frac{|\mathbf {x}-\mathbf{p }_i|^2}{32t} \right) V_i \right) \mathrm {d}\mu _\mathbf {x}\nonumber \\&\quad \le \frac{Ch^2}{t} \sum _{i=1}^{n} \left( \int _{\mathcal {M}} C_t R\left( \frac{|\mathbf {x}-\mathbf{p }_i|^2}{32t}\right) \mathrm {d}\mu _\mathbf {x}\left( u^2_iV_i\right) \right) \le \frac{Ch^2}{t} \left( \sum _{i=1}^{n}u_i^2V_i\right) . \end{aligned}$$
Combining Eqs. (45), (46) and Lemma 1,
$$\begin{aligned}&\Vert L_ta_{t, h} - L_{t, h}a_{t, h}\Vert _{L^2({\mathcal {M}})} \\&\quad = \left( \int _M \left| \left( L_t(a_{t, h}) - L_{t, h}(a_{t, h})\right) (\mathbf {x})\right| ^2 \mathrm {d}\mu _\mathbf {x}\right) ^{1/2} \\&\quad \le \frac{1}{t}\left( \int _{\mathcal {M}}\left( a_{t,h}(\mathbf {x})\right) ^2\left| \int _{\mathcal {M}}R_t(\mathbf {x},\mathbf {y}) \mathrm {d}\mu _\mathbf {y}-\sum _{j=1}^nR_t(\mathbf {x},\mathbf{p }_j)V_j\right| ^2\mathrm {d}\mu _\mathbf {x}\right) ^{1/2} \\&\qquad + \frac{1}{t}\left( \int _{\mathcal {M}}\left| \int _{\mathcal {M}}R_t(\mathbf {x},\mathbf {y})a_{t,h}(\mathbf {y}) \mathrm {d}\mu _\mathbf {y}-\sum _{j=1}^nR_t(\mathbf {x},\mathbf{p }_j)a_{t,h}(\mathbf{p }_j)V_j\right| ^2\mathrm {d}\mu _\mathbf {x}\right) ^{1/2} \\&\quad \le \frac{Ch}{t^{3/2}} \left( \sum _{i=1}^{n}u_i^2V_i\right) ^{1/2} \le \frac{Ch}{t^{3/2}}\Vert f\Vert _\infty . \end{aligned}$$
Assembling the parts together, we have the following upper bound.
$$\begin{aligned}&\Vert L_tu_{t, h} - L_{t, h}u_{t, h}\Vert _{L^2({\mathcal {M}})} \nonumber \\&\quad \le \Vert L_ta_{t, h} - L_{t, h}a_{t, h}\Vert _{L^2({\mathcal {M}})} + \Vert L_tc_{t, h} - L_{t, h}c_{t, h}\Vert _{L^2({\mathcal {M}})} \nonumber \\&\quad \le \frac{Ch}{t^{3/2}}\Vert f\Vert _\infty + \frac{Ch}{t}\Vert f\Vert _{\infty } \le \frac{Ch}{t^{3/2}} \Vert f\Vert _\infty \end{aligned}$$
At the same time, since \(u_t\) respectively \(u_{t,h}\) solves equation (14) respectively equation (40), we have
$$\begin{aligned}&\Vert L_t(u_{t}) - L_{t, h}(u_{t, h})\Vert _{L^2({\mathcal {M}})} \nonumber \\&\quad = \left( \int _{\mathcal {M}}\left( \left( L_tu_{t} - L_{t, h}u_{t, h}\right) (\mathbf {x})\right) ^2 \mathrm {d}\mu _\mathbf {x}\right) ^{1/2} \nonumber \\&\quad = \left( \int _{\mathcal {M}}\left( \int _{\mathcal {M}}\bar{R}_t(\mathbf {x},\mathbf {y})f(\mathbf {y}) - \sum _{j=1}^n\bar{R}_t(\mathbf {x},\mathbf{p }_j)f(\mathbf{p }_j)V_j\right) ^2 \mathrm {d}\mu _\mathbf {x}\right) ^{1/2}\nonumber \\&\quad \le \frac{Ch}{t^{1/2}}\Vert f\Vert _{C^1({\mathcal {M}})}. \end{aligned}$$
The complete \(L^2\) estimate follows from Eqs. (47) and (48).

The estimate of the gradient, \(\Vert \nabla (L_t(u_{t}) - L_{t, h}(u_{t, h}))\Vert _{L^2({\mathcal {M}})}\), can be obtained similarly. The details can be found in “Appendix E.”

7 Stability analysis (Theorems 2 and 5)

To prove Theorem 2 and 5, we need following two theorems regarding the coercivity of the operator \(L_t\).

Theorem 7

For any function \(u\in L^2(\mathcal {M})\), there exists a constant \(C>0\) independent on t and u, such that
$$\begin{aligned} \left<u,L_t u\right>_{\mathcal {M}}\ge C\int _\mathcal {M} |\nabla v|^2 \mathrm {d}\mu _\mathbf {x}, \end{aligned}$$
where \(\left<f, g\right>_{\mathcal {M}} = \int _{\mathcal {M}} f(\mathbf {x})g(\mathbf {x})\mathrm {d}\mu _\mathbf {x}\) for any \(f, g\in L_2(\mathcal {M})\), and
$$\begin{aligned} v(\mathbf {x})=\frac{C_t}{w_t(\mathbf {x})}\int _{\mathcal {M}}R\left( \frac{|\mathbf {x}-\mathbf {y}|^2}{4t}\right) u(\mathbf {y})\mathrm {d}\mu _\mathbf {y}, \end{aligned}$$
and \(w_t(\mathbf {x}) = C_t\int _{\mathcal {M}}R\left( \frac{|\mathbf {x}-\mathbf {y}|^2}{4t}\right) \mathrm {d}\mu _\mathbf {y}\).

Theorem 8

Assume both \({\mathcal {M}}\) and \(\partial {\mathcal {M}}\) are \(C^\infty \). There exists a constant \(C>0\) independent on t so that for any function \(u\in L_2({\mathcal {M}})\) with \(\int _{\mathcal {M}}u(\mathbf {x})\mathrm {d}\mu _\mathbf {x}= 0\) and for any sufficient small t
$$\begin{aligned} \left<u, L_tu \right>_{\mathcal {M}} \ge C\Vert u\Vert _{L_2({\mathcal {M}})}^2. \end{aligned}$$

Theorem 2 is a direct corollary of following two lemmas.

Lemma 2

For any function \(u\in L^2(\mathcal {M})\), there exists a constant \(C>0\) independent on t and u, such that
$$\begin{aligned} \frac{C_t}{t}\int _\mathcal {M}\int _{\mathcal {M}}R\left( \frac{|\mathbf {x}-\mathbf {y}|^2}{32t}\right) (u(\mathbf {x})-u(\mathbf {y}))^2\mathrm {d}\mu _\mathbf {x}\mathrm {d}\mu _\mathbf {y}\ge C\int _\mathcal {M} |\nabla v|^2 \mathrm {d}\mu _\mathbf {x}, \end{aligned}$$
where v is the same as defined in (50).

Lemma 3

If t is small enough, then for any function \(u\in L^2(\mathcal {M})\), there exists a constant \(C>0\) independent on t and u, such that
$$\begin{aligned}&\int _\mathcal {M}\int _{\mathcal {M}}R\left( \frac{|\mathbf {x}-\mathbf {y}|^2}{32t}\right) (u(\mathbf {x})-u(\mathbf {y}))^2\mathrm {d}\mu _\mathbf {x}\mathrm {d}\mu _\mathbf {y}\\&\quad \le C \int _\mathcal {M}\int _{\mathcal {M}}R\left( \frac{|\mathbf {x}-\mathbf {y}|^2}{4t}\right) (u(\mathbf {x})-u(\mathbf {y}))^2\mathrm {d}\mu _\mathbf {x}\mathrm {d}\mu _\mathbf {y}. \end{aligned}$$
The proofs of the above two lemmas are put in “Appendix B” and “C.” Once we have Lemmas 2 and 3, Theorem 7 becomes obvious by noticing that:
$$\begin{aligned} \left<u,L_tu\right>_{\mathcal {M}}= & {} \int _\mathcal {M}\int _{\mathcal {M}}R\left( \frac{|\mathbf {x}-\mathbf {y}|^2}{4t}\right) u(\mathbf {x})(u(\mathbf {x})-u(\mathbf {y}))\mathrm {d}\mu _\mathbf {y}\mathrm {d}\mu _\mathbf {x}\\= & {} -\int _\mathcal {M}\int _{\mathcal {M}}R\left( \frac{|\mathbf {x}-\mathbf {y}|^2}{4t}\right) u(\mathbf {y})(u(\mathbf {x})-u(\mathbf {y}))\mathrm {d}\mu _\mathbf {y}\mathrm {d}\mu _\mathbf {x}\\= & {} \frac{1}{2}\int _\mathcal {M}\int _{\mathcal {M}}R\left( \frac{|\mathbf {x}-\mathbf {y}|^2}{4t}\right) (u(\mathbf {x})-u(\mathbf {y}))^2\mathrm {d}\mu _\mathbf {y}\mathrm {d}\mu _\mathbf {x}. \end{aligned}$$
Now, we turn to prove Theorem 51.

Proof of Theorem 51

By Theorem 7 and the Poincaré inequality, there exists a constant \(C>0\), such that
$$\begin{aligned} \int _\mathcal {M} (v(\mathbf {x})-\bar{v})^2\mathrm {d}\mu _\mathbf {x}\le \frac{CC_t}{t}\int _\mathcal {M}\int _{\mathcal {M}} R\left( \frac{|\mathbf {x}-\mathbf {y}|^2}{4t}\right) (u(\mathbf {x})-u(\mathbf {y}))^2\mathrm {d}\mu _\mathbf {x}\mathrm {d}\mu _\mathbf {y}, \end{aligned}$$
where \(\bar{v}=\frac{1}{|\mathcal {M}|}\int _\mathcal {M} v(\mathbf {x})\mathrm {d}\mu _\mathbf {x}\) and
$$\begin{aligned} v(\mathbf {x})=\frac{C_t}{w_t(\mathbf {x})}\int _{\mathcal {M}}R\left( \frac{|\mathbf {x}-\mathbf {y}|^2}{4t}\right) u(\mathbf {y})\mathrm {d}\mu _\mathbf {y}. \end{aligned}$$
At the same time, we have
$$\begin{aligned} |\mathcal {M}||\bar{v}|= & {} \left| \int _\mathcal {M} v(\mathbf {x})\mathrm {d}\mu _\mathbf {x}\right| \\= & {} \left| \int _\mathcal {M}\int _\mathcal {M}\frac{C_t}{w_t(\mathbf {x})}R\left( \frac{|\mathbf {x}-\mathbf {y}|^2}{4t}\right) (u(\mathbf {y})-u(\mathbf {x}))\mathrm {d}\mu _\mathbf {y}\mathrm {d}\mu _\mathbf {x}\right| \\\le & {} \left( \int _\mathcal {M}\int _\mathcal {M}\frac{C_t}{w_t(\mathbf {x})} R\left( \frac{|\mathbf {x}-\mathbf {y}|^2}{4t}\right) \mathrm {d}\mu _\mathbf {y}\mathrm {d}\mu _\mathbf {x}\right) ^{1/2} \\&\left( \int _\mathcal {M}\int _\mathcal {M}\frac{C_t}{w_t(\mathbf {x})} R\left( \frac{|\mathbf {x}-\mathbf {y}|^2}{4t}\right) (u(\mathbf {y})-u(\mathbf {x}))^2\mathrm {d}\mu _\mathbf {y}\mathrm {d}\mu _\mathbf {x}\right) ^{1/2} \\\le & {} C|\mathcal {M}|^{1/2}\left( C_t\int _\mathcal {M}\int _\mathcal {M} R\left( \frac{|\mathbf {x}-\mathbf {y}|^2}{4t}\right) (u(\mathbf {y})-u(\mathbf {x}))^2\mathrm {d}\mu _\mathbf {y}\mathrm {d}\mu _\mathbf {x}\right) ^{1/2}, \end{aligned}$$
where the second equality comes from \(\int _{{\mathcal {M}}} u(\mathbf {x})\mathrm {d}\mu _\mathbf {x}= 0\). This enables us to upper bound the \(L_2\) norm of v as follows. For t sufficiently small,
$$\begin{aligned} \int _\mathcal {M} (v(\mathbf {x}))^2\mathrm {d}\mu _\mathbf {x}&\le 2\int _M (v(\mathbf {x}) - \bar{v})^2 \mathrm {d}\mathbf {x}+ 2 \int _M \bar{v}^2 \mathrm {d}\mu _\mathbf {x}\\&\le \frac{CC_t}{t}\int _\mathcal {M}\int _{\mathcal {M}} R\left( \frac{|\mathbf {x}-\mathbf {y}|^2}{4t}\right) (u(\mathbf {x})-u(\mathbf {y}))^2\mathrm {d}\mu _\mathbf {x}\mathrm {d}\mu _\mathbf {y}. \end{aligned}$$
Let \(\delta =\frac{w_{\min }}{2w_{\max }+w_{\min }}\) where \(w_{\min }=\min _\mathbf {x}w_t(\mathbf {x})\) and \(w_{\max }=\max _\mathbf {x}w_t(\mathbf {x})\). If u is smooth and close to its smoothed version v, in particular,
$$\begin{aligned} \int _\mathcal {M} |v(\mathbf {x})|^2\mathrm {d}\mu _\mathbf {x}\ge \delta ^2 \int _\mathcal {M} |u(\mathbf {x})|^2\mathrm {d}\mu _\mathbf {x}, \end{aligned}$$
then the theorem is proved.
Now, consider the case where (52) does not hold. Note that we now have
$$\begin{aligned} \Vert u-v\Vert _{L^2({\mathcal {M}})}&\ge \Vert u\Vert _{L_2({\mathcal {M}})}-\Vert v\Vert _{L_2({\mathcal {M}})}> (1-\delta )\Vert u\Vert _{L_2({\mathcal {M}})} \\&>\frac{1-\delta }{\delta }\Vert v\Vert _{L_2({\mathcal {M}})}=\frac{2w_{\max }}{w_{\min }}\Vert v\Vert _{L_2({\mathcal {M}})}. \end{aligned}$$
Then, we have
$$\begin{aligned}&\frac{C_t}{t}\int _\mathcal {M}\int _{\mathcal {M}} R\left( \frac{|\mathbf {x}-\mathbf {y}|^2}{4t}\right) (u(\mathbf {x})-u(\mathbf {y}))^2\mathrm {d}\mu _\mathbf {x}\mathrm {d}\mu _\mathbf {y}\\&\quad =\frac{2C_t }{t}\int _\mathcal {M} u(\mathbf {x})\int _{\mathcal {M}} R\left( \frac{|\mathbf {x}-\mathbf {y}|^2}{4t}\right) (u(\mathbf {x})-u(\mathbf {y}))\mathrm {d}\mu _\mathbf {y}\mathrm {d}\mu _\mathbf {x}\\&\quad =\frac{2 }{t}\left( \int _\mathcal {M} u^2(\mathbf {x})w(\mathbf {x})\mathrm {d}\mu _\mathbf {x}-\int _{\mathcal {M}}u(\mathbf {x})v(\mathbf {x})w(\mathbf {x})\mathrm {d}\mu _\mathbf {x}\right) \\&\quad =\frac{2 }{t}\left( \int _\mathcal {M} (u(\mathbf {x})-v(\mathbf {x}))^2w(\mathbf {x})\mathrm {d}\mu _\mathbf {x}+ \int _{\mathcal {M}}(u(\mathbf {x})-v(\mathbf {x}))v(\mathbf {x})w(\mathbf {x})\mathrm {d}\mu _\mathbf {x}\right) \\&\quad \ge \frac{2 }{t}\int _\mathcal {M} (u(\mathbf {x})-v(\mathbf {x}))^2w(\mathbf {x})\mathrm {d}\mu _\mathbf {x}\\&\qquad -\frac{2 }{t} \left( \int _{\mathcal {M}}v^2(\mathbf {x})w(\mathbf {x})\mathrm {d}\mu _\mathbf {x}\right) ^{1/2} \left( \int _{\mathcal {M}}(u(\mathbf {x})-v(\mathbf {x}))^2w(\mathbf {x})\mathrm {d}\mu _\mathbf {x}\right) ^{1/2}\\&\quad \ge \frac{2 w_{\min }}{t}\int _\mathcal {M} (u(\mathbf {x})-v(\mathbf {x}))^2\mathrm {d}\mu _\mathbf {x}\\&\qquad -\frac{2 w_{\max }}{t} \left( \int _{\mathcal {M}}v^2(\mathbf {x})\mathrm {d}\mu _\mathbf {x}\right) ^{1/2} \left( \int _{\mathcal {M}}(u(\mathbf {x})-v(\mathbf {x}))^2\mathrm {d}\mu _\mathbf {x}\right) ^{1/2} \\&\quad \ge \frac{ w_{\min }}{t}\int _\mathcal {M} (u(\mathbf {x})-v(\mathbf {x}))^2\mathrm {d}\mu _\mathbf {x}\ge \frac{ w_{\min }}{t}(1-\delta )^2\int _\mathcal {M} u^2(\mathbf {x})\mathrm {d}\mu _\mathbf {x}. \end{aligned}$$
This completes the proof for the theorem.

7.1 Proof of Theorem 2

With Theorem 7 and 51, the proof of Theorem 2 is straightforward.

Proof of Theorem  2

Using Theorem 51, we have
$$\begin{aligned} \Vert u\Vert _{L^2({\mathcal {M}})}^2&\le C \left<u,L_tu\right> = C\int _{\mathcal {M}}u(\mathbf {x})(r(\mathbf {x})-\bar{r})\mathrm {d}\mu _\mathbf {x}\nonumber \\&\le C\Vert u\Vert _{L^2({\mathcal {M}})}\Vert r\Vert _{L^2({\mathcal {M}})}. \end{aligned}$$
To show the last inequality, we use the fact that
$$\begin{aligned} |\bar{r}|=\frac{1}{|{\mathcal {M}}|}\left| \int _{\mathcal {M}}r(\mathbf {x})\mathrm {d}\mu _\mathbf {x}\right| \le C\Vert r\Vert _{L^2({\mathcal {M}})}. \end{aligned}$$
This inequality (53) implies that
$$\begin{aligned} \Vert u\Vert _{L^2({\mathcal {M}})}\le C\Vert r\Vert _{L^2({\mathcal {M}})}. \end{aligned}$$
Now, we turn to estimate \(\Vert \nabla u\Vert _{L^2({\mathcal {M}})}\). Notice that we have the following expression for u, since u satisfies the integral equation (14).
$$\begin{aligned} u(\mathbf {x})=v(\mathbf {x})+\frac{t}{w_t(\mathbf {x})}\,(r(\mathbf {x}) - \bar{r}), \end{aligned}$$
$$\begin{aligned} v(\mathbf {x})=\frac{1}{w_t(\mathbf {x})}\int _{{\mathcal {M}}}R_t(\mathbf {x},\mathbf {y})u(\mathbf {y})\mathrm {d}\mu _\mathbf {y},\quad w_t(\mathbf {x})=\int _{{\mathcal {M}}}R_t(\mathbf {x},\mathbf {y})\mathrm {d}\mu _\mathbf {y}. \end{aligned}$$
By Theorem 7, we have
$$\begin{aligned} \Vert \nabla u\Vert _{L^2({\mathcal {M}})}^2&\le 2\Vert \nabla v\Vert _{L^2({\mathcal {M}})}^2+ 2t^2\left\| \nabla \left( \frac{r(\mathbf {x}) - \bar{r}}{w_t(\mathbf {x})}\right) \right\| _{L^2({\mathcal {M}})}^2 \\&\le C \left<u,L_tu\right> + Ct\Vert r\Vert _{L^2({\mathcal {M}})}^2+Ct^2\Vert \nabla r\Vert _{L^2({\mathcal {M}})}^2 \\&\le C\Vert u\Vert _{L^2({\mathcal {M}})}\Vert r\Vert _{L^2({\mathcal {M}})}+ Ct\Vert r\Vert _{L^2({\mathcal {M}})}^2+Ct^2\Vert \nabla r\Vert _{L^2({\mathcal {M}})}^2 \\&\le C\Vert r\Vert _{L^2({\mathcal {M}})}^2+Ct^2\Vert \nabla r\Vert _{L^2({\mathcal {M}})}^2 \\&\le C\left( \Vert r\Vert _{L^2({\mathcal {M}})}+t\Vert \nabla r\Vert _{L^2({\mathcal {M}})}\right) ^2. \end{aligned}$$
This completes the proof.

7.2 Proof of Theorem 5

The proof of Theorem 5 is more involved.


First, we denote
$$\begin{aligned} r(\mathbf {x})&=\int _{\partial {\mathcal {M}}}\mathbf {b}(\mathbf {y})\cdot (\mathbf {x}-\mathbf {y})\bar{R}_t(\mathbf {x}, \mathbf {y})\mathrm {d}\tau _\mathbf {y},\\ \bar{r}&=\frac{1}{|{\mathcal {M}}|}\int _{\mathcal {M}}\left( \int _{\partial {\mathcal {M}}}\mathbf {b}(\mathbf {y})\cdot (\mathbf {x}-\mathbf {y})\bar{R}_t(\mathbf {x}, \mathbf {y})\mathrm {d}\tau _\mathbf {y}\right) \mathrm {d}\mathbf {x}, \end{aligned}$$
where \(|{\mathcal {M}}|=\int _{\mathcal {M}}\mathrm {d}\mu _\mathbf {y}\).
The key point of the proof is to show that
$$\begin{aligned} \left| \int _{\mathcal {M}}u(\mathbf {x})\left( r(\mathbf {x})-\bar{r}\right) \mathrm {d}\mu _\mathbf {x}\right| \le C\sqrt{t} \;\Vert \mathbf {b}\Vert _{H^1({\mathcal {M}})} \Vert u\Vert _{H^1({\mathcal {M}})}. \end{aligned}$$
First, notice that
$$\begin{aligned} |\bar{r}|\le C\sqrt{t}\;\Vert \mathbf {b}\Vert _{L^2(\partial {\mathcal {M}})}\le C\sqrt{t}\;\Vert \mathbf {b}\Vert _{H^1({\mathcal {M}})}. \end{aligned}$$
Then, it is sufficient to show that
$$\begin{aligned} \left| \int _{\mathcal {M}}u(\mathbf {x})\left( \int _{\partial {\mathcal {M}}}\mathbf {b}(\mathbf {y})\cdot (\mathbf {x}-\mathbf {y})\bar{R}_t(\mathbf {x},\mathbf {y}) \mathrm {d}\tau _\mathbf {y}\right) \mathrm {d}\mu _\mathbf {x}\right| \le C\sqrt{t} \;\Vert \mathbf {b}\Vert _{H^1({\mathcal {M}})} \Vert u\Vert _{H^1({\mathcal {M}})}. \end{aligned}$$
Direct calculation gives that
$$\begin{aligned} |2t\nabla \bar{\bar{R}}_t(\mathbf {x}, \mathbf {y})-(\mathbf {x}-\mathbf {y})\bar{R}_t(\mathbf {x},\mathbf {y})|\le C|\mathbf {x}-\mathbf {y}|^2\bar{R}_t(\mathbf {x}, \mathbf {y}), \end{aligned}$$
where \(\bar{\bar{R}}_t(\mathbf {x}, \mathbf {y})=C_t\bar{\bar{R}}\left( \frac{\Vert \mathbf {x}-\mathbf {y}\Vert ^2}{4t}\right) \) and \(\bar{\bar{R}}(r)=\int _{r}^{\infty }\bar{R}(s)\mathrm {d}s\). This implies that
$$\begin{aligned}&\left| \int _{\mathcal {M}}u(\mathbf {x}) \int _{\partial {\mathcal {M}}}\mathbf {b}(\mathbf {y})\left( (\mathbf {x}-\mathbf {y})\bar{R}_t(\mathbf {x},\mathbf {y})+2t\nabla \bar{\bar{R}}_t(\mathbf {x}, \mathbf {y})\right) \mathrm {d}\tau _\mathbf {y}\mathrm {d}\mu _\mathbf {x}\right| \nonumber \\&\quad \le C\int _{\mathcal {M}}|u(\mathbf {x}) |\int _{\partial {\mathcal {M}}}|\mathbf {b}(\mathbf {y})||\mathbf {x}-\mathbf {y}|^2\bar{R}_t(\mathbf {x}, \mathbf {y})\mathrm {d}\tau _\mathbf {y}\mathrm {d}\mu _\mathbf {x}\nonumber \\&\quad \le Ct\Vert \mathbf {b}\Vert _{L^2(\partial {\mathcal {M}})} \left( \int _{\partial {\mathcal {M}}}\left( \int _{\mathcal {M}}\bar{R}_t(\mathbf {x}, \mathbf {y})\mathrm {d}\mu _\mathbf {x}\right) \left( \int _{\mathcal {M}}|u(\mathbf {x})|^2\bar{R}_t(\mathbf {x}, \mathbf {y})\mathrm {d}\mu _\mathbf {x}\right) \mathrm {d}\tau _\mathbf {y}\right) ^{1/2}\nonumber \\&\quad \le Ct\Vert \mathbf {b}\Vert _{H^1({\mathcal {M}})} \left( \int _{{\mathcal {M}}} |u(\mathbf {x})|^2 \left( \int _{\partial {\mathcal {M}}} \bar{R}_t(\mathbf {x}, \mathbf {y})\mathrm {d}\tau _\mathbf {y}\right) \mathrm {d}\mu _\mathbf {x}\right) ^{1/2}\nonumber \\&\quad \le Ct^{3/4}\Vert \mathbf {b}\Vert _{H^1({\mathcal {M}})}\Vert u\Vert _{L^2({\mathcal {M}})}. \end{aligned}$$
On the other hand, using the Gauss integral formula, we have
$$\begin{aligned}&\int _{\mathcal {M}}u(\mathbf {x}) \int _{\partial {\mathcal {M}}}\mathbf {b}(\mathbf {y})\cdot \nabla \bar{\bar{R}}_t(\mathbf {x}, \mathbf {y})\mathrm {d}\tau _\mathbf {y}\mathrm {d}\mu _\mathbf {x}\nonumber \\&\quad = \int _{\partial {\mathcal {M}}} \int _{{\mathcal {M}}}u(\mathbf {x}) T_\mathbf {x}(\mathbf {b}(\mathbf {y}))\cdot \nabla \bar{\bar{R}}_t(\mathbf {x}, \mathbf {y})\mathrm {d}\mu _\mathbf {x}\mathrm {d}\tau _\mathbf {y}\nonumber \\&\quad = \int _{\partial {\mathcal {M}}} \int _{\partial {\mathcal {M}}}\mathbf {n}(\mathbf {x})\cdot T_\mathbf {x}(\mathbf {b}(\mathbf {y}))u(\mathbf {x})\bar{\bar{R}}_t(\mathbf {x}, \mathbf {y})\mathrm {d}\tau _\mathbf {x}\mathrm {d}\tau _\mathbf {y}\nonumber \\&\qquad -\int _{\partial {\mathcal {M}}} \int _{{\mathcal {M}}}\text {div}_\mathbf {x}[u(\mathbf {x}) T_\mathbf {x}(\mathbf {b}(\mathbf {y}))]\bar{\bar{R}}_t(\mathbf {x}, \mathbf {y})\mathrm {d}\mu _\mathbf {x}\mathrm {d}\tau _\mathbf {y}. \end{aligned}$$
Here, \(T_\mathbf {x}\) is the projection operator to the tangent space on \(\mathbf {x}\). To get the first equality, we use the fact that \(\nabla \bar{\bar{R}}_t(\mathbf {x}, \mathbf {y})\) belongs to the tangent space on \(\mathbf {x}\), such that \(\mathbf {b}(\mathbf {y})\cdot \nabla \bar{\bar{R}}_t(\mathbf {x}, \mathbf {y})=T_\mathbf {x}(\mathbf {b}(\mathbf {y}))\cdot \nabla \bar{\bar{R}}_t(\mathbf {x}, \mathbf {y})\) and \(\mathbf {n}(\mathbf {x})\cdot T_\mathbf {x}(\mathbf {b}(\mathbf {y}))=\mathbf {n}(\mathbf {x})\cdot \mathbf {b}(\mathbf {y})\) where \(\mathbf {n}(\mathbf {x})\) is the out normal of \(\partial {\mathcal {M}}\) at \(\mathbf {x}\in \partial {\mathcal {M}}\).
For the first term, we have
$$\begin{aligned}&\left| \int _{\partial {\mathcal {M}}} \int _{\partial {\mathcal {M}}}\mathbf {n}(\mathbf {x})\cdot T_\mathbf {x}(\mathbf {b}(\mathbf {y}))u(\mathbf {x})\bar{\bar{R}}_t(\mathbf {x}, \mathbf {y})\mathrm {d}\tau _\mathbf {x}\mathrm {d}\tau _\mathbf {y}\right| \nonumber \\&\quad = \left| \int _{\partial {\mathcal {M}}} \int _{\partial {\mathcal {M}}}\mathbf {n}(\mathbf {x})\cdot \mathbf {b}(\mathbf {y})u(\mathbf {x})\bar{\bar{R}}_t(\mathbf {x}, \mathbf {y})\mathrm {d}\tau _\mathbf {x}\mathrm {d}\tau _\mathbf {y}\right| \nonumber \\&\quad \le C\Vert \mathbf {b}\Vert _{L^2(\partial {\mathcal {M}})} \left( \int _{\partial {\mathcal {M}}} \left( \int _{\partial {\mathcal {M}}}|u(\mathbf {x})|\bar{\bar{R}}_t(\mathbf {x}, \mathbf {y})\mathrm {d}\tau _\mathbf {x}\right) ^2 \mathrm {d}\tau _\mathbf {y}\right) ^{1/2}\nonumber \\&\quad \le C\Vert \mathbf {b}\Vert _{H^1({\mathcal {M}})} \left( \int _{\partial {\mathcal {M}}} \left( \int _{\partial {\mathcal {M}}}\bar{\bar{R}}_t(\mathbf {x}, \mathbf {y})\mathrm {d}\tau _\mathbf {x}\right) \left( \int _{\partial {\mathcal {M}}}|u(\mathbf {x})|^2\bar{\bar{R}}_t(\mathbf {x}, \mathbf {y})\mathrm {d}\tau _\mathbf {x}\right) \mathrm {d}\tau _\mathbf {y}\right) ^{1/2}\nonumber \\&\quad \le Ct^{-1/2}\; \Vert \mathbf {b}\Vert _{H^1({\mathcal {M}})} \Vert u\Vert _{L^2(\partial {\mathcal {M}})}\le Ct^{-1/2}\; \Vert \mathbf {b}\Vert _{H^1({\mathcal {M}})} \Vert u\Vert _{H^1({\mathcal {M}})}. \end{aligned}$$
We can also bound the second term on the right-hand side of (57). By using the assumption that \({\mathcal {M}}\in C^\infty \), we have
$$\begin{aligned}&|\text {div}_\mathbf {x}[u(\mathbf {x}) T_\mathbf {x}(\mathbf {b}(\mathbf {y}))]| \\&\quad \le |\nabla u(\mathbf {x})||T_\mathbf {x}(\mathbf {b}(\mathbf {y}))|| | +|u(\mathbf {x})||\text {div}_\mathbf {x}[T_\mathbf {x}(\mathbf {b}(\mathbf {y}))]|| |+|\nabla ||u(\mathbf {x})T_\mathbf {x}(\mathbf {b}(\mathbf {y}))| \\&\quad \le C(|\nabla u(\mathbf {x})|+|u(\mathbf {x})|)|\mathbf {b}(\mathbf {y})| \end{aligned}$$
where the constant C depends on the curvature of the manifold \({\mathcal {M}}\).
Then, we have
$$\begin{aligned}&\left| \int _{\partial {\mathcal {M}}} \int _{{\mathcal {M}}}\text {div}_\mathbf {x}[u(\mathbf {x})T_\mathbf {x}(\mathbf {b}(\mathbf {y}))]\bar{\bar{R}}_t(\mathbf {x}, \mathbf {y})\mathrm {d}\mu _\mathbf {x}\mathrm {d}\tau _\mathbf {y}\right| \nonumber \\&\quad \le C \int _{\partial {\mathcal {M}}}\mathbf {b}(\mathbf {y}) \int _{{\mathcal {M}}}(|\nabla u(\mathbf {x})|+|u(\mathbf {x})|)\bar{\bar{R}}_t(\mathbf {x}, \mathbf {y})\mathrm {d}\mu _\mathbf {x}\mathrm {d}\tau _\mathbf {y}\nonumber \\&\quad \le C \Vert \mathbf {b}\Vert _{L^2(\partial {\mathcal {M}})} \left( \int _{{\mathcal {M}}} (|\nabla u(\mathbf {x})|^2+|u(\mathbf {x})|^2) \left( \int _{\partial {\mathcal {M}}}\bar{\bar{R}}_t(\mathbf {x}, \mathbf {y})\mathrm {d}\tau _\mathbf {y}\right) \mathrm {d}\mu _\mathbf {x}\right) ^{1/2}\nonumber \\&\quad \le C t^{-1/4}\;\Vert \mathbf {b}\Vert _{H^1({\mathcal {M}})} \Vert u\Vert _{H^1({\mathcal {M}})}. \end{aligned}$$
Then, the inequality (55) is obtained from (56), (57), (58) and (59). Now, using Theorem 51, we have
$$\begin{aligned} \Vert u\Vert _{L^2({\mathcal {M}})}^2\le C \int _{\mathcal {M}}u(\mathbf {x})L_tu(\mathbf {x}) \mathrm {d}\mu _\mathbf {x}\le C\sqrt{t}\;\Vert \mathbf {b}\Vert _{H^1({\mathcal {M}})} \Vert u\Vert _{H^1({\mathcal {M}})}. \end{aligned}$$
Note \(r(\mathbf {x})=\int _{\partial {\mathcal {M}}}(\mathbf {x}-\mathbf {y})\cdot \mathbf {b}(\mathbf {y})\bar{R}_t(\mathbf {x},\mathbf {y}) \mathrm {d}\tau _\mathbf {y}\). Direct calculation gives us that
$$\begin{aligned} \Vert r(\mathbf {x})\Vert _{L^2({\mathcal {M}})}\le & {} Ct^{1/4}\Vert \mathbf {b}\Vert _{H^1({\mathcal {M}})},~\text {and}\\ \Vert \nabla r(\mathbf {x})\Vert _{L^2({\mathcal {M}})}\le & {} Ct^{-1/4}\Vert \mathbf {b}\Vert _{H^1({\mathcal {M}})} . \end{aligned}$$
The integral equation \(L_t u=r-\bar{r}\) gives that
$$\begin{aligned} u(\mathbf {x})=v(\mathbf {x})+\frac{t}{w_t(\mathbf {x})}\,(r(\mathbf {x})-\bar{r}), \end{aligned}$$
$$\begin{aligned} v(\mathbf {x})=\frac{1}{w_t(\mathbf {x})}\int _{{\mathcal {M}}}R_t(\mathbf {x},\mathbf {y})u(\mathbf {y}) \mathrm {d}\mu _\mathbf {y},\quad w_t(\mathbf {x})=\int _{{\mathcal {M}}}R_t(\mathbf {x},\mathbf {y}) \mathrm {d}\mu _\mathbf {y}. \end{aligned}$$
By Theorem 7, we have
$$\begin{aligned}&\Vert \nabla u\Vert _{L^2({\mathcal {M}})}^2 \nonumber \\&\quad \le 2\Vert \nabla v\Vert _{L^2({\mathcal {M}})}^2+ 2t^2\left\| \nabla \left( \frac{r(\mathbf {x})-\bar{r}}{w_t(\mathbf {x})}\right) \right\| _{L^2({\mathcal {M}})}^2\nonumber \\&\quad \le C \int _{\mathcal {M}}u(\mathbf {x})L_tu(\mathbf {x}) \mathrm {d}\mu _\mathbf {x}+ Ct\Vert r\Vert _{L^2({\mathcal {M}})}^2+Ct^2\Vert \nabla r\Vert _{L^2({\mathcal {M}})}^2\nonumber \\&\quad \le C\sqrt{t}\;\Vert \mathbf {b}\Vert _{H^1({\mathcal {M}})} \Vert u\Vert _{H^1({\mathcal {M}})}+ Ct\Vert r\Vert _{L^2({\mathcal {M}})}^2+Ct^2\Vert \nabla r\Vert _{L^2({\mathcal {M}})}^2\nonumber \\&\quad \le C\Vert \mathbf {b}\Vert _{H^1({\mathcal {M}})} \left( \sqrt{t}\Vert u\Vert _{H^1({\mathcal {M}})}+ Ct^{3/2}\right) . \end{aligned}$$
Using (60) and (61), we have
$$\begin{aligned} \Vert u\Vert _{H^1({\mathcal {M}})}^2\le C\Vert \mathbf {b}\Vert _{H^1({\mathcal {M}})} \left( \sqrt{t}\Vert u\Vert _{H^1({\mathcal {M}})}+ Ct^{3/2}\right) , \end{aligned}$$
which proves the theorem.

8 Discussion and future work

We have proven the convergence of the point integral method for Poisson equations on submanifolds that are isometrically embedded in Euclidean spaces. Our analysis shows that the convergence rate of PIM is \(h^{1/4}\) in \(H^1\) norm. However, our experimental results in [33] show that the empirical convergence rate is approximately linear. In some parts in our analysis, we believe that the error bounds could be improved.

Nevertheless, the quadrature rule we used in the point integral method is of low accuracy. If we have more information, such as the local mesh or local hypersurface, we could use high-order quadrature rule to improve the accuracy of the point integral method.

Based on the convergence result in this paper, we can show that the spectra of the graph Laplacian with proper normalization converge to the spectra of \({\varDelta }_{\mathcal {M}}\) with the Neumann boundary condition. Moreover, we can obtain an estimate of the rate of spectral convergence. The point integral method also applies to Poisson equation with Dirichlet boundary. Moreover, we can also show the convergence of the point integral method for the Dirichlet boundary. These results will be reported in the subsequent papers.

Another interesting problem is generalizing PIM to solve other type of PDEs. PIM can handle elliptic equations with anisotropic or discontinuous coefficients. The generalization to the diffusion equation seems to be natural. If the equation is dominated by convection term, it may need more careful study.


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Authors’ Affiliations

Yau Mathematical Sciences Center, Tsinghua University


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