Random walks on Apollonian network with a single trap

Random walks on the Apollonian network with a single trap

Zhongzhi Zhang 1 1 School of Computer Science, Fudan University, Shanghai 200433, China
Shanghai Key Lab of Intelligent Information Processing, Fudan University, Shanghai 200433, China
Department of Computer Science and Technology, Tongji University, 4800 Cao’an Road, Shanghai 201804, China122 zhangzz@fudan.edu.cn
   Jihong Guan 2 33 jhguan@tongji.edu.cn    Wenlei Xie 1 School of Computer Science, Fudan University, Shanghai 200433, China
Shanghai Key Lab of Intelligent Information Processing, Fudan University, Shanghai 200433, China
Department of Computer Science and Technology, Tongji University, 4800 Cao’an Road, Shanghai 201804, China122
   Yi Qi 1 School of Computer Science, Fudan University, Shanghai 200433, China
Shanghai Key Lab of Intelligent Information Processing, Fudan University, Shanghai 200433, China
Department of Computer Science and Technology, Tongji University, 4800 Cao’an Road, Shanghai 201804, China122
   Shuigeng Zhou 3 1 School of Computer Science, Fudan University, Shanghai 200433, China
Shanghai Key Lab of Intelligent Information Processing, Fudan University, Shanghai 200433, China
Department of Computer Science and Technology, Tongji University, 4800 Cao’an Road, Shanghai 201804, China122 sgzhou@fudan.edu.cn 1 School of Computer Science, Fudan University, Shanghai 200433, China
Shanghai Key Lab of Intelligent Information Processing, Fudan University, Shanghai 200433, China
Department of Computer Science and Technology, Tongji University, 4800 Cao’an Road, Shanghai 201804, China12233
11
22
33
August 29, 2019
Abstract

Explicit determination of the mean first-passage time (MFPT) for trapping problem on complex media is a theoretical challenge. In this paper, we study random walks on the Apollonian network with a trap fixed at a given hub node (i.e. node with the highest degree), which are simultaneously scale-free and small-world. We obtain the precise analytic expression for the MFPT that is confirmed by direct numerical calculations. In the large system size limit, the MFPT approximately grows as a power-law function of the number of nodes, with the exponent much less than 1, which is significantly different from the scaling for some regular networks or fractals, such as regular lattices, Sierpinski fractals, T-graph, and complete graphs. The Apollonian network is the most efficient configuration for transport by diffusion among all previously studied structure.

pacs:
05.40.Fb
pacs:
89.75.Hc
pacs:
05.60.Cd

Random walks and Levy flights Networks and genealogical trees Classical transport

1 Introduction

Trapping is an integral major theme of random walks (diffusion) [1, 2, 3], which is relevant to a wide range of applications and has led to a growing number of theoretical and practical investigation over the past decades [4, 5, 6, 7, 8, 9]. The trapping problem, first introduced in [10], is in fact a random-walk issue, where a trap is positioned at a given location, which absorbs all particles visiting it. The primarily interesting quantity closely related to trapping problem is the average trapping time, also referred to as the mean first-passage time (MFPT), which is useful in the study of transport-limited reactions [11, 12], target search [13, 14] and other physical problems.

An important question in the study of trapping is how the MFPT scales with the size of the system. There are some well-known results providing answers to the corresponding questions in the cases of some graphs with simple topology, including regular lattices [10], Sierpinski fractals [15, 16], T-fractal [17], and so on. However, these graphs are not suitable to describe real systems [18] encountered in everyday experience, most of which are scale-free [19] and small-world [20] that have been shown to influence profoundly various dynamical processes running on networks [21, 22]. Thus, it is natural and interesting to explore the trapping problem on networks with general structure embedded in real life. Although a lot of activities have been devoted to studying random walks on complex networks[23, 24, 25, 26, 27], work about trapping problem on scale-free small-world graphs is much less [28].

In the paper, we investigate the trapping problem on the Apolloian network [29, 30] with scale-free and small-world properties. We focus on a specific aspect of random walks in the presence of a single trap situated at a given node with the largest degree (hub node). We obtain an exact analytical solution for the MFPT and the dependence of this primary quantity on the system size. We show that the Apolloian network is a preferred architecture that minimizes the increase of MFPT with network size, compared with regular networks and fractals.

2 Introduction to the Apollonian network

We first introduce the Apollonian packing [31], from which the Apollonian network is derived. There are two commonly used Apollonian packings that differ mainly in initial configurations. The first packing is constructed by starting with three mutually touching disks, the interstice of which is a curvilinear triangle. In the first generation a disk is inscribed, touching all the sides of this curvilinear triangle. For subsequent generations we indefinitely repeat the packing process for all the new curvilinear triangles. In the limit of infinite generations, an Apollonian packing is obtained. The left panel of figure 1 displays the first three generations of this Apollonian packing.

Figure 1: (Left panel) The first three generations of the first Apollonian packing of disks. (Right panel) An Apollonian network corresponding to the packing shown in the left panel.

The other frequently used Apollonian packing has a initial configuration with three mutually touching disks inscribed inside a circular space. The interstices of the initial disks and circle are four curvilinear triangles to be filled. Then in each subsequent generation, we add one disk to each interstice (curvilinear triangle), so that the added disk touches all the three sides of the corresponding curvilinear triangle. The first several processes are shown in figure 2.

Figure 2: The first several generations of the second Apollonian packing of disks within a circle.

The above two Apollonian packings can be easily mapped to networks, usually called as Apollonian networks [29, 30]. The translation from Apollonian packing construction to Apollonian network generation is quite straightforward. Each node (vertex, site) corresponds to a disk, and two nodes are linked to each other if their corresponding disks are tangent. Note that for the second Apollonian packing, the initial circle also corresponds to a node. The right panel of figure 1 shows an example of the network. Since the resulting networks associated with the two packings have similar structural features, except for the initial disks, in this paper we will focus on the network based on the second Apollonian packing, which is convenient for analytically deriving the network properties.

Figure 3: The initial construction of Apollonian network.

According to the foregoing mapping, one can introduce a general algorithm [32, 33] to create the Apollonian network, denoted by after generation evolutions. For , is a tetrahedron with four faces or triangles, see figure 3. For , is obtained from . For each of the existing triangles of that is created at generation , a new node is added and connected to all the three nodes of this triangle. Figure 4 illustrates the construction process for the first two generations of the initial four faces as shown in figure 3.

Figure 4: The Apollonian network of generation 2 and the labeling of its nodes.

According to the network construction, one can see [30, 33] that at the th () generation, the number of newly introduced nodes is . From this result, we can easily compute the total number of nodes in network (hereafter called the network order):

(1)

For convenient use in the next section, we distinguish different nodes of by labeling them sequentially as follows. The four nodes (i.e., nodes , , , and in figure 3) created at initial generation are labeled as 1, 2, 3, and 4, respectively. Then, in each new generation, we only label the new nodes added at this generation, while keep the labels of pre-existing nodes unchanged. That is to say, we label new nodes progressively as , in which is the total number of the pre-existing nodes and is the number of newly-added nodes. Eventually, every node is labeled by a unique integer, all nodes in are labeled from 1 to , see figure 4.

Let be the degree of a node at generation , which entered the network at the generation of (). Then [30, 33]

(2)

From equation (2), one can easily see that at each step the degree of a node doubles, i.e.,

(3)

The Apollonian network presents the typical characteristics of real-life networks [29, 30, 32, 33, 34]. It has a power-law degree distribution with the exponent . Its average path length, defined as the mean of shortest distance between all pairs of nodes, increases logarithmically with network order [34]. In the large network order limit, the average clustering coefficient tends to . Thus, the Apollonian network exhibits small-world effect [20]. In addition, the network is disassortative [30]. In view of its structural properties similar to those of real networks and its intrinsic interest, Apollonian network is a good substrate network for studying criticality phenomena and dynamical processes [35, 36, 37, 38, 39, 40, 41, 42, 43]. In what follows we will investigate the MFPT for random walks with an immobile trap on the Apollonian network.

3 Formulation of the problem

In this section we formulate the problem of a simple random walk of a particle on Apollonian network in the presence of a trap or a perfect absorber positioned on a given node. To this end, we first specify by its adjacency matrix (hereafter we neglect the subscript) of order , which completely describes network . The element of A is defined as follows: if the pair of node and node is connected by a link (edge, bond), otherwise . The degree of node is , and the diagonal degree matrix is given by . Then, the normalized Laplacian matrix of is given by and its entry is , where I is an identity matrix.

Before proceeding further, let us introduce the so-called simple random walk [1, 2, 3] on network . At each time step (taken to be unity), the walker moves from its current location to any of its nearest neighbors with equal probability. According to this rule, at time , a walker at a node will hop to one of its neighbors, say , with the transition probability . Suppose that the walker starts from node at , then the jumping probability of going from to at time is governed by the following master equation:

(4)

We next focus a random walk on with a trap. We locate the trap at node 1, represented as . It should be pointed out that thanks to the symmetry, the trap can be also situated at node 2, 3, or 4, which has no influence on MFPT. The particular selection for the trap location allows one to calculate analytically the MFPT, which will be addressed in detail in the next section. At each time step, the walker, starting from any node except the trap , jumps to any of its nearest neighbors with equal probability.

Let be mean transmit time (first-passage time, trapping time, or the mean time to absorption) for a walker, starting from node , to first arrive at the trap . Thus, . Then, the set of these interesting quantities follows the recurrence equation [44]

(5)

where . Equation (5) may be also rewritten in matrix notation as

(6)

where and are two ()-dimensional vectors, and is the fundamental matrix of the Markov chain representing such unbiased random walk. In fact, is a sub-matrix of the normalized discrete Laplacian matrix whose first row and column, corresponding to the trap node, have been removed.

Then, the mean first-passage time, or the average of the mean time to absorption, , which is the average of over all nodes distributed uniformly over nodes in other than the trap, is given by

(7)

Equation (7) can be easily explained by looking at the random walk from the perspective of a Markov chain. Actually, the entry of the fundamental matrix of the Markov process expresses the average number of times that a walker starting at node will be at node , and the row sum is exactly , the total times a particle starting at node will traverse all other nodes before being absorbed by the trap.

Equation (7) shows that the problem of determining is reduced to finding the sum of all elements of the fundamental matrix of order , which can be obtained by utilizing a standard software package, Mathematica 5.0. Irrespective of the seemingly compact expression of equation (7), since increases exponentially with , for large , it becomes difficult to obtain through direct calculation from this equation, because of the limitations of time and computer memory. Therefore, one can compute directly the MFPT only for the first generations, see table 1. However, the particular construction of the Apollonian network allows one to calculate analytically MFPT to obtain a rigorous solution. Details of derivation will be provided below.

          
0 4
1 8
2 20
3 56
4 164
5 488
6 1460
Table 1: The MFPT obtained by direct calculation from equation (7) by using a standard software package, Mathematica 5.0. Since for large networks, the computation of the MFPT from equation (7) is prohibitively time and memory consuming, we calculate the MFPT for the first several generations.

4 Exact solution for mean first-passage time

Before deriving the general formula for MFPT, , we first establish the scaling relation dominating the evolution of with generation , where is the trapping time for a walk originating at node on the th generation of Apollonian network.

4.1 Evolution scaling for trapping time

  (2,3,4)   (5,6,7)   (8) (9,10,12,13,15,16)  (11,14,17)  (18,19,20)
0
1
2
3
4
5
6
Table 2: Mean time to absorption for a random walker starting from node on the Apollonian network for various . Notice that owing to the obvious symmetry, nodes in a parenthesis are equivalent, since they have the same trapping time. All the values are calculated straightforwardly from equation (7).

We begin by recording the numerical values of . Obviously, for all , ; for , it is a trivial case, we have . For , the values of can be obtained straightforwardly via equation (7). Table 2 lists the numerical values of for some nodes up to . The numerical values listed in table 2 show that for a given node we have . That is to say, upon growth of the Apollonian network from to generation , the mean time to first reach the trap increases by a factor . This is a basic character of random walks on the Apollonian network, which can be established from the arguments below [1, 25].

Consider an arbitrary node in the Apollonian network after generation evolution. From equation (2), we know that upon growth of the Apollonian network to generation , the degree of node doubles. Thus, at generation , node has old neighbors (born at generation or earlier) and new neighbors (generated at generation ). Let the mean transmit time for going from node to any of its old neighbors be ; and let the mean transmit time for going from any of its new neighbors to one of the old neighbors be . Then we can establish the following underlying backward equations (see figure 5)

(8)

which leads to . That is to say, the passage time from any node () to any node () increases by a factor of , upon the network growth from generation to generation . Thus, we have , which will be useful for deriving the formula for the mean first-passage time in the following text.

Figure 5: Growth of trapping time in going from to . Node has neighbor nodes in generation () and new neighbor nodes in generation (). A new node has a degree of 3, and is linked to and its two old neighbor nodes.

4.2 Formula for the mean first-passage time

Having obtained the scaling of mean transmit time for old nodes, we now determine the mean first-passage time, with an aim to derive an exact solution. We represent the set of nodes in as , and denote the set of nodes created at generation by . Thus we have . For the convenience of computation, we define the following quantities for :

(9)

and

(10)

Then, we have

(11)

Next we will explicitly determine the quantity . To this end, we should firstly determine .

We examine the mean time to absorption for the first several generations of Apollonian network. In the case of , by the very construction of Apollonian network, it follows that

Thus,

(12)

Similarly, for case, it is easy to obtain

(13)

Proceeding analogously, it is not difficult to derive that

(14)

and

(15)

where and are actually the numbers of nodes generated at generations and , respectively. Equation (15) minus equation (14) times and making use of the relation , one gets

(16)

Using , equation (16) is solved inductively

(17)

Substituting equation (17) for into equation (11) and using , we have

(18)

Considering the initial condition , equation (18) is resolved by induction to yield

(19)

Plugging the last expression into equation (7), we arrive at the accurate formula for the average of the mean time to absorption at the trap located at node 1 on the th of Apollonian network:

(20)

We have checked our analytic formula against numerical values quoted in Table 1. For the range of , the values obtained from equation (20) completely agree with those numerical results on the basis of the direct calculation through equation (7). This agreement serves as an independent test of our theoretical formula.

From equation (1), we have . Hence, for large network (i.e., ), we obtain

(21)

where the exponent . Thus, in the large limit of network order , the MFPT increases algebraically with increasing order of the network.

Generally, finite-size effect plays a crucial role in critical phenomena and dynamical processes on networks [45]. In order to study the finite-size effect in the scaling behavior of MFPT for the Apollonian network, we plot a figure to show the MFPT with order for small networks, see figure 6. Surprisingly, it is observed from figure 6 that the finite-size effect has little influence on the scaling.

Figure 6: Mean first-passage time versus network order on a log-log scale. The solid line is a guide to the eye.

Previous studies showed that for regular lattices [10], Sierpinski fractals [15, 16], and T-graph [17] with large order , their MFPT behaves as with . Even in a complete graph of nodes, , the MFPT grows linearly with as . Actually, linear scaling of the MFPT with is the best that has been reported so far. From equation (21), one can see that the MFPT of the Apollonian network increases as a fractional power of network order , which implies that Apollonian network has a faster transmit time than any other analytically soluble media. In other words, the Apollonian network has the best structure for fast diffusion one can see heretofore.

We argue that the heterogeneous topology of the Apollonian network may be responsible for the high efficiency for transport. In the Apollonian network, there are some nodes with high degree, which are linked to one another and to most other nodes in the network. These ‘large’ nodes can be easily visited by a walker starting from an arbitrary location. Since ‘large’ nodes, including the trap node, are connected to one another, so the walker can find the trap in a very short time.

5 Conclusions

In summary, we have studied trapping problem on the Apollonian network exhibiting remarkable features (scale-free behavior and small-world effects) of a variety of real networks. We have obtained an analytical closed-form solution for the MFPT for random walks with a trap located at a hub node, which is consistent with the numerical computation. The rigorous result indicates that the MFPT on the Apollonian network shows a very distinct behavior, which is compared with those results previously reported for regular lattices, Sierpinski fractals, T-graph, and complete graph. We have shown that Apollonian network is the most efficient network for transport by diffusion, in contrast to other studied structure. We hope that the current study may cast some light on trapping problem in some real networks, that present similar topologies as the Apollonian network.

6 Acknowledgment

This research was supported by the National Basic Research Program of China under grant No. 2007CB310806, the National Natural Science Foundation of China under Grant Nos. 60704044, 60873040 and 60873070, Shanghai Leading Academic Discipline Project No. B114, and the Program for New Century Excellent Talents in University of China (NCET-06-0376).

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