Abstract 1 Introduction 2 Preliminaries 3 Review of Previous Algorithm 4 Linear-Time Influence Spread Computation 5 Discussion 6 Conclusion References

Linear-Time Exact Computation of Influence Spread on Bounded-Pathwidth Graphs

Kengo Nakamura ORCID Communication Science Laboratories, NTT, Inc., Kyoto, Japan    Masaaki Nishino ORCID Communication Science Laboratories, NTT, Inc., Kyoto, Japan
Abstract

Given a network and a set of vertices called seeds to initially inject information, influence spread is the expected number of vertices that eventually receive the information under a certain stochastic model of information propagation. Under the commonly used independent cascade model, influence spread is equivalent to the expected number of vertices reachable from the seeds on a directed uncertain graph, and the exact evaluation of influence spread offers many applications, e.g., influence maximization. Although its evaluation is a #P-hard task, there is an algorithm that can precisely compute the influence spread in O(mnωp22ωp2) time, where ωp is the pathwidth of the graph. We improve this by developing an algorithm that computes the influence spread in O((m+n)ωp22ωp2) time. This is achieved by identifying the similarities in the repetitive computations in the existing algorithm and sharing them to reduce computation. Although similar refinements have been considered for the probability computation on undirected uncertain graphs, a greater number of similarities must be leveraged for directed graphs to achieve linear time complexity.

Keywords and phrases:
Influence spread, bounded pathwidth, network reliability, linear time algorithm
Copyright and License:
[Uncaptioned image] © Kengo Nakamura and Masaaki Nishino; licensed under Creative Commons License CC-BY 4.0
2012 ACM Subject Classification:
Theory of computation Parameterized complexity and exact algorithms
; Networks Network algorithms
Related Version:
Full Version: https://arxiv.org/abs/2604.13526
Funding:
This work was supported by JSPS KAKENHI Grant Number JP26K02906.
Editor:
Pierre Fraigniaud

1 Introduction

Given a network and seed set S, which is a set of vertices that are initially injected information, influence spread [5] σ(S) is the expected number of vertices that eventually receives the information under a stochastic model of information propagation. Influence spread is implemented in viral marketing applications with the aim of evaluating the influence of a particular node within a social network. Currently, it is also a keystone for other network applications such as network monitoring [11], rumor control [23], target advertisement [13], and social recommendation [24]. Among several information diffusion models, the most basic and commonly used one is the independent cascade (IC) model [6]. In this model, a network is modeled as a directed graph G=(V,E), where each edge eE is associated with a probability pe. When a vertex v receives information, it stochastically propagates the information along every outgoing edge e independently with a given probability pe.

The influence spread σ(S) under the IC model is equivalent to the expected number of vertices reachable from at least one vertex in S on a directed uncertain graph. Given directed graph G=(V,E) and probability pe for every edge eE, we consider an uncertainty in which each edge eE is present with probability pe and absent with probability 1pe. We assume that each edge’s presence or absence is stochastically independent of the other edges. Accordingly, the probability that a subgraph (V,E)(EE) appears is

Pr(E)eEpeeEE(1pe). (1)

Here, a directed path from some sS to vertex v on the subgraph (V,E) corresponds to the route of information propagation from s to v. Therefore, given SV and vV, the probability that v receives information is equal to the probability Pr(Sv) that v can be reached from some vertices in S under uncertainty. Here, Pr(Sv)=ESvPr(E), where Sv is the family of subsets E of edges such that v can be reached from some vertices in S on (G,E). Finally, the influence spread can be represented as σ(S)=vVSPr(Sv).

Example 1.1.

Figure 1a depicts examples of the probabilities Pr(E) of subgraphs (V,E)(EE). For this uncertain graph, there are 15 subgraphs in which v=4 is reachable from {S}=1 (Figure 1b); thus, Pr({1}4) is the sum of Pr(E) over all these subgraphs. By evaluating Pr({1}2), Pr({1}3), and Pr({1}4) as in Figure 1c, σ({1}) can be computed as their sum.

Figure 1: (a) Example of directed uncertain graph and probabilities of subgraphs. (b) All 15 subgraphs in which v=4 is reachable from {S}=1. Pr({1}4) is the sum of probabilities of these subgraphs. (c) σ({1}) is computed as the sum of Pr({1}v)s for v=2,3,4.

Since evaluating the influence spread σ(S) is a #P-hard task [3], most studies have relied on Monte Carlo simulation for evaluating σ(S) [7, 10, 11, 18]. However, exact computation of σ(S) is important for the following reasons. First, this allows us to more accurately evaluate the influence spread in larger networks, since real networks often consist of small communities; the exact computation of influence spread in each small community will improve overall evaluation quality. Second, this allows us to rank the influential vertices in descending order of influence spread. For this purpose, Monte Carlo simulations are not sufficient because Ω(1/ε2) samples are needed to obtain (1±ε)-approximation with high probability [18]; to distinguish every vertex’s influence spread, high accuracy such as ε105 is sometimes needed, which is costly for Monte Carlo methods.

Maehara et al. [15] proposed the only non-trivial algorithm to exactly compute σ(S) under the IC model. Given seed set S and v, it efficiently computes Pr(Sv), i.e., the probability that v receives information. Given the path decomposition of G whose width is ωp, this probability for a single v can be computed in O(mωp22ωp2) time, where m is the number of edges. Hereafter, we mean the pathwidth of a directed graph G in the sense of the pathwidth of the underlying undirected graph of G as used in the literature [15, 20]. The influence spread σ(S)=vVSPr(Sv) can be computed in O(mnωp22ωp2) time, where n is the number of vertices.

Here, even for bounded-pathwidth graphs, obtaining the σ(S) value requires super-linear (O(mn)) time. Since there are similarities in the repetitive computation for different vertices v using this algorithm, we investigated the use of these similarities to refine their algorithm and thus improve the running time for computing σ(S).

1.1 Our Contribution

In this paper, we propose an algorithm for computing σ(S) for given S under the IC model. Specifically, the proposed algorithm simultaneously computes Pr(Sv) in an uncertain directed graph for all vertices v. Our main result can be expressed as follows.

Theorem 1.2.

Given directed graph G, seed set S, each edge’s probability pe of presence, and the path decomposition of G whose width is ωp, the probability Pr(Sv) for every vertex v can be computed in O((m+n)ωp22ωp2) time in total.

Since even inputting the entire graph requires linear time, this algorithm is asymptotically optimal for graphs with a bounded pathwidth when the constant factor is ignored. Moreover, the exponential factor of the pathwidth, hidden in the constant, remains the same as in the algorithm of Maehara et al. [15]: the dependence on the graph sizes is improved from O(mn) to O(m+n) while the dependence on the pathwidth is kept the same.

Our algorithm shares certain ideas with the existing algorithm for simultaneously computing the probabilities of connection in undirected graphs [16] in that both use similarities in the computation of the previous algorithms [8, 15] for different vertices. However, there is a non-trivial gap in extending that algorithm [16] to directed graphs due to the difference between connectivity in undirected graphs and reachability in directed graphs. We fill this gap by finding additional similarities in computing σ(S) with the previous algorithm [15]; details are discussed in Section 5.

1.2 Related Work

Influence maximization.

The most well-studied problem related to influence spread is influence maximization [10], that is, the problem of choosing a seed set S to maximize the influence spread. This has attracted much attention over the past two decades [12, 14, 19]. Although the influence maximization problem under most diffusion models including the IC model is NP-hard [10], a simple greedy algorithm [10] can achieve a (11/e)-approximation provided that every σ(S) is computed exactly. Various methods, e.g., the sketch-based methods described in a survey [12], have improved this greedy algorithm. However, if we resorted to using Monte Carlo simulation to evaluate σ(S), we could not obtain a deterministic approximation bound for influence maximization, even with greedy or more sophisticated algorithms. Moreover, although many studies have used an alternative proxy for σ(S) to speed up the computation (e.g., proxy-based methods [12] and learning-based methods [14]), they also lack approximation bounds. This situation accentuates the theoretical importance of an exact evaluation of influence spread.

Network reliability.

Computing the probability that some vertices are connected in an uncertain graph has been traditionally studied as network reliability evaluation in the network community. Most studies on network reliability evaluation have modeled the network as an undirected graph and, given a vertex set K and the probability pe of presence for every edge, they computed the probability that the vertices in K are connected. Even for undirected graphs, computing this probability is #P-complete [22]. Nevertheless, Hardy et al. [8] developed an algorithm that could compute this probability in linear time for graphs with bounded pathwidth. Another line of research has attempted to compute the expected number of vertices connected to vertex u [17], which is an analogue of the influence spread under the IC model for undirected graphs. Nakamura et al. [16] proposed an algorithm that could compute the probability that a vertex u is connected to v for every vV in linear time for an undirected graph with bounded pathwidth. By summing all the probabilities for every v, it is also possible to compute the expected number of vertices connected to v in linear time. This algorithm uses the similarities in the computation of the probability that u and v are connected with Hardy’s algorithm [8] for different v; therefore, it shares similar ideas with our work. However, we cannot straightforwardly extend this algorithm to handle directed graphs, as described in Section 1; detailed discussions are given in Section 5. Note that these algorithms [8, 16] also run in polynomial time for graphs with bounded pathwidth, indicating the importance of algorithms dealing with bounded-pathwidth graphs.

2 Preliminaries

For sets U,W of vertices, UGW means that u can reach w, i.e., w can be reached from u, for some uU and wW in directed graph G. If U (or W) consists of only a single vertex u (w), we simply write, e.g., uGW and uGw instead of {u}GW and {u}G{w}. When it is clear from the context, we omit the subscript G.

A directed graph is called strongly connected if uv for every ordered pair (u,v) of vertices. We say vertex subset C is a strongly connected component (SCC) of G if the vertex-induced subgraph of G induced by C is strongly connected but that induced by V{v} is not strongly connected for any vVC. It is known that, given directed graph G, all SCCs in G can be computed in linear time in the size of G [21]. Throughout this paper, n and m denote the number of vertices and edges, respectively, in the input graph G.

We formally define the problems to solve as follows.

Problem 2.1.

Given a directed graph G, probabilities {pe}eE, and a seed set SV, compute the probability Pr(Sv) for every vVS.

For convenience, we assume that G contains no self-loops and the underlying undirected graph of G is connected. Note that if G contains self-loops, we can safely remove it, since it would never affect reachability. If G is disconnected, we can solve the problem individually for each connected component.

3 Review of Previous Algorithm

3.1 Decomposition of Probability

In the following, we review Maehara’s algorithm [15] for exactly computing Pr(Sv) for a given S,v. Although the literature [15] only showed the algorithm for the case |S|=1, here we show the general S case because it can be easily extended.

The basic idea in evaluating Pr(Sv) is to decompose Pr(Sv) into terms that can be easily computed. For E,E′′E such that EE′′=, let Pr(E,E′′¯) be the conditional probability given that the edges in E are present and those in E′′ are absent. From the case analysis of whether eE(EE′′) is present or absent,

Pr(SvE,E′′¯)=pePr(SvE{e},E′′¯)+(1pe)Pr(SvE,E′′{e}¯). (2)

By ordering edges as e1,,em, Pr(Sv) can be decomposed by recursively applying (2):

Pr(Sv) =pe1Pr(Sv{e1},¯)+(1pe1)Pr(Sv,{e1}¯)
=pe1pe2Pr(Sv{e1,e2},¯)+pe1(1pe2)Pr(Sv{e1},{e2}¯)+
(1pe1)pe2Pr(Sv{e2},{e1}¯)+(1pe1)(1pe2)Pr(Sv,{e1,e2}¯)
==EE<iPr<i(E)Pr(SvE,E<iE¯)=, (3)
where E<i{e1,,ei1},Pr<i(E)eEpeeE<iE(1pe).

This expansion eventually reaches the definition Pr(Sv)ESvPr(E). Therefore, by using this decomposition naively, we have O(2m) terms, which incurs exponential complexity of the graph size in evaluating it.

To prevent this, we attempt to detect the equality among probabilities, i.e., to find subsets E,FE<i(EF) such that Pr(SvE,E<iE¯)=Pr(SvF,E<iF¯). If such equality can be detected, we simply need to further decompose only one among the equal probabilities, which reduces the number of terms. If the following condition (#) holds, we can confirm Pr(SvE,E<iE¯)=Pr(SvF,E<iF¯):

(#) For any HEiEE<i, S(V,EH)v if and only if S(V,FH)v.

To check condition (#), we focus on the reachability relation on the subgraph (V,E). If u(V,E)w and w(V,F)v are equivalent for any u,wV, we can confirm that (#) holds. In brief, this is because, given a path from sS to v on (V,EH), we can construct a path from s to v on (V,FH) by using the above equivalence, and vice versa.

Maehara et al. [15] indicated that only a limited subset of vertices called frontier vertices is important for checking (#).

Definition 3.1.

Given edge ordering e1,,em, (i-th) frontier vertices Wi are those appearing in both E<i and Ei.

We consider the reachability relations among WiS{v} on (V,E) as follows.

Definition 3.2.

Let WiS(E){wWiS(V,E)w} (frontier vertices reachable from S) and Wiv(E){wWiw(V,E)v} (those that can reach v). A binary matrix Φiv(E) is defined as follows: (I) It is indexed by (WiWiS(E){S})×(WiWiv(E){v}). (II) Φiv(E)uw=1 if and only if u(V,E)w. Here, S is treated as a special (single) row index, and v is treated as a column index. We call Φiv(E) a transversal configuration (TC).

We can then prove the following.

Lemma 3.3.

Φiv(E)=Φiv(F) is a sufficient condition for (#), meaning that Pr(SvE,E<iE¯)=Pr(SvF,E<iF¯). Note that Φiv(E)=Φiv(F) means that the indices of matrices as well as their entries are equal.

This can be shown by transforming a u-v directed path on (V,EH) for some uS to a u-v directed path on (V,FH) for some uS. Now we can rewrite Pr(SvE,E<iE¯) as Pr(SvΦiv(E)).

Example 3.4.

On the graph in Figure 2a with v=5, we examine {e1,e4},{e1,e2,e3,e4}, {e1,e2,e4,e6},{e2,e5,e6}E<8 corresponding to the four edge subgraphs of Figure 2b. These subsets have an identical TC Φ85 because W8={4,5}. Thus, the conditional probabilities of S5 are all equal for these subsets.

Algorithm 1 Previous algorithm [15].
Figure 2: (a) Example of input graph G. Red vertex is included in S. (b) Example of different edge subsets of E<8 leading to the same TC Φ85.

Moreover, Φiv() has the following property: if Φiv(E)=Φiv(F) for E,FE<i, both Φi+1v(E)=Φi+1v(F) and Φi+1v(E{ei})=Φi+1v(F{ei}) hold. Thus, there exist transition functions 𝗅𝗈v,𝗁𝗂v from Φiv to Φi+1v satisfying 𝗅𝗈v(Φiv(E))=Φi+1v(E) and 𝗁𝗂v(Φiv(E))=Φi+1v(E{ei}) for any EE<i. By combining this fact and (2), we have, for any Φ=Φiv(E)(EE<i),

Pr(SvΦ)=pePr(Sv𝗁𝗂v(Φ))+(1pe)Pr(Sv𝗅𝗈v(Φ)). (4)

Using this decomposition recursively, Pr(Sv) can be decomposed as follows:

Pr(Sv) =Pr(SvΦ1v())
=pe1Pr(Sv𝗁𝗂v(Φ1v()))+(1pe1)Pr(Sv𝗅𝗈v(Φ1v()))
==Φ𝒩iPr(Φ)Pr(SvΦ)=, (5)
where Pr(Φ)EE<i:Φiv(E)=ΦPr<i(E),𝒩i{Φiv(E)EE<i}. (6)

In other words, Pr(Φ) is the probability that TC Φ appears and 𝒩i is the set of all TCs of the subsets of E<i. We later show that |𝒩i| is bounded by a constant if the pathwidth is bounded in Lemma 4.15. This is the main reason to achieve O(m) time complexity in computing Pr(Sv).

For some TCs Φ, we can confirm that Sv must hold or must not hold, i.e., Pr(SvΦ)=1 or 0. For such TCs, we do not need to further decompose Pr(SvΦ) with (4). We define such base cases with the following -pruning and -pruning as follows. Let iu be the largest index i such that one of the endpoints of ei is u and let iSmaxuSiu.

  • If 𝗁𝗂v(Φ)Sv=1, determining the presence of ei confirms Sv, i.e., Pr(Sv𝗁𝗂v(Φ))=1. In such a case, we let 𝗁𝗂v(Φ)=, a special TC meaning that Sv must hold (-pruning).

  • Suppose that iiS and 𝗅𝗈v(Φ)Su=0 for any u, or that iiv and 𝗅𝗈v(Φ)uv=0 for any u. In these cases, no further vertices can be reached from S or reach v by determining the absence of ei, i.e., Pr(Sv𝗅𝗈v(Φ))=0. Thus, we let 𝗅𝗈v(Φ)=, which is a special TC meaning that Sv must not hold (-pruning)111Although the original version [15] uses different pruning rules, they require a pre-computation of transitive closures of (V,Ei), which takes cubic time. We use an alternative pruning rule that can be checked in linear time.. We also let 𝗁𝗂v(Φ)= if -pruning does not occur and 𝗁𝗂v(Φ) satisfies the same condition as above.

Eventually, all the TCs are transformed into either or , and (5) reaches Pr(Sv)=Pr()1+Pr()0=Pr(). Thus, computing Pr() is sufficient for evaluating Pr(Sv).

3.2 Procedure and Complexity

Now we describe the procedure to compute Pr(). We again use the transition of TCs. By considering the pruning described above, we redefine the set of TCs as 𝒩1{Φ1v()} and 𝒩i(Φ𝒩i1{𝗁𝗂v(Φ),𝗅𝗈v(Φ)}){,}, i.e., we remove the pruned TCs from 𝒩i. Then, from the definition of Pr(Φ) (Eq. (6)), we have

Pr(Φ)=piΦ𝒩i1:𝗁𝗂(Φ)=ΦPr(Φ)+(1pi)Φ𝒩i1:𝗅𝗈(Φ)=ΦPr(Φ). (7)

To compute Pr(), we can use a similar formula:

Pr()=piΦ𝒩1𝒩m:𝗁𝗂(Φ)=Pr(Φ)+(1pi)Φ𝒩1𝒩m:𝗅𝗈(Φ)=Pr(Φ). (8)

Starting from 𝒩1={Φ1v()}, we can generate 𝒩i+1 from 𝒩i recursively using transition functions 𝗁𝗂v,𝗅𝗈v. By recording the transition, we can compute every Pr(Φ) and Pr() with (7) and (8).

Algorithm 1 formally presents the procedures. Lines 1–7 recursively generate the successive TCs using transition functions 𝗅𝗈v,𝗁𝗂v while executing ,-pruning. This process can be seen as constructing a diagram of TCs as in Figure 3. Every Φ except for , has two outgoing edges heading to 𝗅𝗈v(Φ) and 𝗁𝗂v(Φ). In Algorithm 1, each Φ has two entries Φ.𝗅𝗈 and Φ.𝗁𝗂 that store the pointer to 𝗅𝗈v(Φ) and 𝗁𝗂v(Φ). Here, 𝒩i stores the TCs of the subsets of E<i as a hash map; pruned TCs are not stored. Along this diagram, we can compute every Pr(Φ) with simple dynamic programming (DP) in lines 8–13; this simulates the formulas (7) and (8). The array p[Φ] for Φ𝒩i is prepared to store Pr(Φ). Note that even if an identical TC Φ appears in 𝒩i and 𝒩j (ij), we distinguish Φ𝒩i and Φ𝒩j in computing p[]. After computing all p[Φ], Pr(Sv)=Pr() is stored in p[].

Next, we analyze the complexity of this algorithm. For each TC Φ, computing 𝗅𝗈v(Φ) and 𝗁𝗂v(Φ) takes O((|Wi|+|Wi+1|)2) time; details are in Lemma 4.14 of Section 4.4. If every 𝒩i is implemented as a hash map, storing or searching a TC also takes O(|Wi|2) time. The number of patterns on Φiv can be bounded by O(2|Wi|2); since this was not rigorously proved [15], we prove it in Lemma 4.15 of Section 4.4. The overall complexity can be bounded by O(i(|Wi|+|Wi+1|)22|Wi|2)=O(mω22ω2), where ω=maxi|Wi|.

In fact, ω is related to the pathwidth of a graph. Given a path decomposition of G with width ωp, we can generate an edge ordering with ωωp in linear time [9]. Since we can construct a path decomposition in linear time for a graph with bounded pathwidth [2], we have a linear time algorithm for computing Pr(Sv) on a graph with bounded pathwidth. However, computing σ(S) requires O(mnω22ω2) time by computing Pr(Sv) for vVS.

Figure 3: (a)(b) Upper four levels of diagrams constructed from graph in Figure 2a with v=4 and v=5. (c)(d) Parts of lower levels of diagrams constructed from graph in Figure 2a with v=2 and v=3; (c) depicts part below Φ82({e2,e5,e6}) and (d) depicts part below Φ83({e1,e4,e7}). Solid arcs indicate connection from Φ to Φ.𝗁𝗂, while dashed arcs indicate connection from Φ to Φ.𝗅𝗈.

4 Linear-Time Influence Spread Computation

We now describe the proposed algorithm for Problem 2.1. First, we explain the high-level concept of the proposed algorithm. In computing σ(S) with the algorithm described in Section 3, different diagrams of TCs are generated for different vVS in computing Pr(Sv). To argue the similarities among these diagrams, we divide each of them into three parts: upper levels, lower levels, and middle levels. More specifically, let AiV be the vertices that only appear in E<i and do not appear in Ei, and BiV be those that only appear in Ei and do not appear in E<i. Ai, Bi, and Wi (Definition 3.1) constitute a partition of V. Moreover, since E<iE<i+1 and EiEi+1 for i=1,,m, V=B1Bm+1= and =A1Am+1=V. Thus, by fixing v, the diagram of TCs Φiv() made from the reachability to v can be divided into three parts according to i: levels i s.t. vBi (upper levels), those s.t. vWi (middle levels), and those s.t. vAi (lower levels).

We first find that upper levels of these diagrams exhibit an identical structure, i.e., diagrams of Φiv and Φiw exhibit an identical structure as long as v,wBi (Observation 4.2); we extract the essential information to build this identical diagram as a shared transversal configuration (STC) Ψ=Ψi(E). We can also confirm that middle levels of these diagrams were also governed by the STCs (Lemma 4.8). Thus, by considering STCs Ψi(), we can have a similar formula to (5) using the STCs when vBiWi:

Pr(Sv)=ΨiPr(Ψ)Pr(SvΨ), (9)
wherePr(Ψ)EE<i:Ψi(E)=ΨPr<i(E),i{Ψi(E)EE<i}.

For every v, there exists i such that vBiWi. Thus, for every v, if Pr(Ψ) and Pr(SvΨ) are efficiently computed for all Ψ=Ψi() with the above i, we can compute Pr(Sv) with (9). Here, since Pr(Ψ) has a similar recursion as Pr(Φ) (Lemma 4.9), all Pr(Ψ)s can be computed in a manner similar to that used in Section 3 by building a diagram of STCs from i=1 to m+1. Since |i| is constant for a graph with bounded pathwidth (Lemma 4.16), it can be performed in O(m) time.

Indeed, when vWi (middle levels), Pr(SvΨ) for Ψ=Ψi() can also be computed efficiently. To compute this, we use the lower levels of the diagram of TCs Ψiv(). Although naively constructing the diagrams of TCs Φ for every v costs O(mn) time, we find that the lower levels of these diagrams have many identical substructures (Lemma 4.5). By using this, we can build all possible substructures of diagrams that appear in the lower level of these diagrams in O(m) time. In addition, we again use middle levels’ equivalence (Lemma 4.8) to compute Pr(SvΨ) on middle levels in O(m) time. Here we use the recursion on Pr(SvΨ) (Lemmas 4.11 and 4.12).

Eventually, for every v and i where vWi, we obtain Pr(Ψ) and Pr(SvΨ) for Ψ=Ψi(). Thus, by choosing i such that vWi, we can compute Pr(Sv) with (9). Since (9) contains O(|i|) terms, which is constant for bounded-pathwidth graphs, the computation of Pr(Sv) for every v costs O(n) time in total. The overall time complexity is bounded by O(m+n) for a graph with bounded pathwidth. Note that, for every v, there exists i such that vWi if v has degree more than 1. For vertices with degree 1, such i might not exist, but we can easily compute Pr(Sv) for such vertices, as described later.

In the following, we first identify the similarities in the previous algorithm [15] for different v in Section 4.1. Then, we derive DP formulas for computing Pr(Sv) in Section 4.2. Finally, we explain the main procedures and the complexity in Sections 4.3 and 4.4.

4.1 Equivalence of Diagrams for Different Vertices

We formally state the equivalence of different diagrams of TCs for upper levels (vBi), lower levels (vAi), and middle levels (vWi).

Upper level equivalence.

First, we consider the case v,wBi. No edges in E<i are incident to v, meaning that no vertex in Wi can reach v on (V,E<i). Furthermore, no vertex in S can reach v on (V,E<i). Therefore, for any EE<i, Φiv(E)uv=0 for any u. This means we need to consider the reachability relations among only Wi{S}, not Wi{S,v}.

Definition 4.1.

Let Ψi(E) be a binary matrix indexed by (WiWiS(E){S})×Wi, where Ψi(E)ux=1 if and only if u(V,E)x. Here, S is treated as a special (single) row index. We call Ψi() a shared transversal configuration (STC).

Since vBi, we can recover Φiv(E) from Ψi(E) by Φiv(E)ux=Ψi(E)ux for any u as well as xv and Φiv(E)uv=0 for any u. In other words, the diagram structure is completely determined by the transition of Ψi() instead of Φiv() when vBi. The above argument also holds for the other wBi. Therefore, the following observation holds.

Observation 4.2.

Consider the diagrams generated using Algorithm 1 with different v,w. If v,wBi, the diagrams above any TCs Φiv(E) and Φiw(E) are identical. Moreover, we can instead use STC Ψi() in building the diagram.

Example 4.3.

Figures 3a and 3b show the upper four levels of the diagram generated using Algorithm 1 with the graph of Figures 2a and v=4 or v=5. Since 4,5B4, the first four levels are identical, as depicted in these figures.

Lower level equivalence.

Next, we consider the case v,wAi. Recall that Φiv() captures the reachability among Wi{S,v}, and Φiw() captures those among Wi{S,w}. Since v,wAi, all edges incident to v and w are in E<i, meaning that all incident edges are determined when the edges in E<i are determined. Thus, intuitively, if Φiv and Φiw are “identical,” i.e., the reachability relations are identical by substituting v with w, Sv and Sw can be regarded as equivalent events. We formally define such an equivalence.

Definition 4.4.

For E,FE<i, consider two TCs Φiv(E) and Φiw(F), where v,wAi. We say these TCs are identical if Φiv(E)ux=Φiw(F)ux for any u and xv,w and Φiv(E)uv=Φiw(F)uw for any u. This means that Φiv(E) and Φiw(F) are identical matrices, except for the column indices being different.

Lemma 4.5.

Suppose Φiv(E) and Φiw(F) are identical for v,wAi and E,FE<i. Then, for any HEi, S(V,EH)v if and only if S(V,FH)w.

Proof.

Fix HEi and suppose that S(V,EH)v. There is then a directed walk P from some sS to v in (V,EH). The walk P can be divided into small walks P=P0P1P2P2k1P2k satisfying the conditions that P2j consists of only the edges in EE<i and that P2j+1 consists of only the edges in HEi. Let pj be the contact vertex of Pj and Pj+1. Note that P0 may be empty when sWiBi; in such a case, we set p0=s. Since pj(j1) is incident to both edges in EE<i and those in HEi, pjWi. If P0 is nonempty, p0 is also in Wi. We can also assume that p1,p2,,p2k2WiS(E); otherwise, we can take a directed walk P from some sS to pj within (V,E) and consider a walk PPj+1P2k instead. With a similar argument, we can assume that p1,p2,,p2k2Wiv(E). Now, we constitute a directed walk P from some sS to w in (V,FH). First, when P0 is not empty, Φiv(E)Sp0=1. Since Φiv(E) and Φiw(F) are identical, Φiw(F)Sp0=1; thus, there is a directed walk P0 from some sS to p0 in (V,F). This also holds when P0 is empty; in such a case, s=s=p0 and P0 is also empty. Next, for 1jk1, P2j’s existence and identity indicate Φiv(E)p2j1p2j=1=Φiw(F)p2j1p2j, meaning that there is a directed walk P2j from p2j1 to p2j in (V,F). Finally, P2k’s existence and identity indicate Φiv(E)p2k1v=1=Φiw(F)p2k1w, meaning that there is a directed walk P2k from p2k1 to w in (V,F). Now P=P0P1P2P2k1P2k is a directed walk from sS to w in (V,FH), indicating S(V,FH)w.

In the same manner, we can show the reverse direction. Thus, the lemma holds. This indicates that Pr(SvΦiv)=Pr(SwΦiw) when Φiv and Φiw are identical.

Observation 4.6.

Consider the diagrams generated using Algorithm 1 with different v,w. If v,wAi and identical TCs Φiv,Φiw appear in each diagram, the diagram structures below Φiv and below Φiw are identical.

Example 4.7.

Figures 3c and 3d show parts of the last four levels of the diagrams below Φ82({e2,e5,e6}) (v=2) and below Φ83({e1,e4,e7}) (v=3). Since 2,3A8 and these TCs are identical, these diagram structures are also identical.

Middle level equivalence.

Finally, we examine the case v,wWi. In this case, the TC Φiv() captures the reachability among Wi{S,v}=Wi{S}. In addition, the STC Ψi() also captures the reachability among Wi{S}. Thus, we can recover Φiv(E) from Ψi(E) by removing the columns corresponding to Wiv(E). In other words, if Ψi(E)=Ψi(F), then E,FE<i satisfy condition (#).

For Ψ=Ψi(E), let WiS(Ψ) be the set of vertices in Wi that can be reached from S under Ψ, which is determined by the missing row indices of Ψ. Consider a graph Gi(Ψ)(WiWiS(Ψ),Ei(Ψ)), where Ei(Ψ){(u,x)u,xWiWiS(Ψ),Ψux=1}. In other words, when Ψ=Ψi(E), Gi(Ψ) is the subgraph of the transitive closure of (V,E) induced by WiWiS(Ψ). Then, we can prove the following.

Lemma 4.8.

Suppose Ψi(E)=Ψi(F)Ψ for E,FE<i and v,wWiWiS(E) are in the same SCC of Gi(Ψ). Then, for any HEi, S(V,EH)v if and only if S(V,FH)w.

Proof.

Fix HEi. We can prove the equivalence of S(V,EH)v and S(V,FH)v from Ψi(E)=Ψi(F) with almost the same argument as that in the proof of Lemma 4.5. Since v and w are in the same SCC of Gi(Ψ), v(V,F)w and w(V,F)v. Consequently, S(V,FH)v indicates S(V,FH)w and vice versa. This concludes S(V,EH)vS(V,FH)w.

4.2 New Decomposition and DP Formulas

Decomposition formula.

Using the equivalences described above, we derive a formula for Pr(Sv) using the STCs. Since we confirmed that Φiv(E) can be recovered from Ψi(E) when vAiWi, we can derive the decomposition formula (9). If vWi, it can be further transformed. Based on Lemma 4.8, we can rewrite Pr(SvΨ) as Pr(SCΨ(v)Ψ), where CΨ(v) is the SCC of Gi(Ψ) containing v when vWiS(Ψ). If vWiS(Ψ), we immediately have Pr(SvΨ)=1. Now (9) can be further transformed into

Pr(Sv) =Ψi{Pr(Ψ)(vWiS(Ψ))Pr(Ψ)Pr(SCΨ(v)Ψ)(vWiWiS(Ψ)). (10)

If we can obtain Pr(Ψ) and Pr(SCΨ) for every STC Ψ and every SCC C of Gi(Ψ), we can compute every Pr(Sv) by choosing i such that vWi and then use (10). Note that if all vertices have degree not less than 2, there must exist index i such that vWi, since G contains no self-loops. The Pr(Sv) value for degree 1 vertices can be easily obtained; details are given in Section 4.3.

DP formulas.

Since TCs can be recovered from STCs and admit transition functions 𝗁𝗂v,𝗅𝗈v, STCs also admit transition functions 𝗅𝗈 and 𝗁𝗂 satisfying that, for any EE<i, 𝗅𝗈(Ψi(E))=Ψi+1(E) and 𝗁𝗂(Ψi(E))=Ψi+1(E{ei}). Here, we set 𝖿(Ψ)= for 𝖿{𝗁𝗂,𝗅𝗈} when iiS and 𝖿(Ψ)Su=0 for any u, which confirms Pr(Sw𝖿(Ψ))=0 for any further vertices wWi+1Bi+1 (-pruning). Now Pr(Ψ) can be computed in the same manner as described in Section 3: From the definition of Pr(Ψ) (Eq. (9)), we have the following.

Lemma 4.9.

For Ψ=Ψi(E) for some EE<i, we have

Pr(Ψ)=piΨi1:𝗁𝗂(Ψ)=ΨPr(Ψ)+(1pi)Ψi1:𝗅𝗈(Ψ)=ΨPr(Ψ), (11)

where 1{Ψ1()} and i(Ψi1{𝗁𝗂(Ψ),𝗅𝗈(Ψ)}){}, i.e., we remove pruned STCs from i.

It remains to be explained how to compute Pr(SCΨ) for an SCC C of Gi(Ψ). If there exists uC such that uWi+1, we can decompose it using the case analysis of ei: If ei is present, Pr(SCΨ) equals Pr(SC𝗁𝗂(Ψ)), where C is the SCC of Gi+1(𝗁𝗂(Ψ)) containing u. If ei is absent, Pr(SCΨ) equals Pr(SC′′𝗅𝗈(Ψ)), where C′′ is the SCC of Gi+1(𝗅𝗈(Ψ)) containing u. Here, the relation between C and C,C′′ can be seen as the transition from C to successive SCCs C,C′′. By considering the pruned cases, we formally define the successive SCCs as follows.

Definition 4.10.

For SCC C of Gi(Ψ), we define successive SCC 𝖿(C) for 𝖿{𝗅𝗈,𝗁𝗂} as follows. (i) If 𝖿=𝗁𝗂, and ei=(u,v) with uWiS(Ψ)S and vC, 𝗁𝗂(C), meaning that C can be reached from S by determining the presence of ei. (ii) If (i) does not hold and 𝖿(Ψ)=, 𝖿(C), meaning that C cannot be reached from S. (iii) If neither (i) nor (ii) holds and there exists uC such that uWi+1, 𝖿(C)C𝖿(Ψ)(u). (iv) Otherwise, 𝖿(C), meaning that there is no successive SCC.

Lemma 4.11.

If there exists uC such that uWi+1, i.e., successive SCCs exist, we can decompose Pr(SCΨ) for Ψ=Ψi(E) and SCC C of Gi(Ψ) as follows:

Pr(SCΨ)=peiPr(S𝗁𝗂(C)𝗁𝗂(Ψ))+(1pei)Pr(S𝗅𝗈(C)𝗅𝗈(Ψ)). (12)

Note that if uWi+1S(𝗁𝗂(Ψ)), since Pr(Su𝗁𝗂(Ψ))=1, we replace Pr(SC𝗁𝗂(Ψ)(u)𝗁𝗂(Ψ)) in the above formula with 1. This replacement is reflected in case (i) of Definition 4.10.

What can be done when such a vertex u does not exist? In this case, we attempt to use the original TC. We observe in Section 4.1 that if uWi, we can recover Φ=Φiu(E) from Ψi(E) with an appropriate transformation. Thus, by fixing some uC and letting Φu be a TC recovered from STC Ψ, we have the following case analysis: If ei is present, Pr(SCΨ)=Pr(SuΦu) equals Pr(Su𝗁𝗂u(Φu)). If ei is absent, Pr(SCΨ) equals Pr(Su𝗅𝗈u(Φu)). This leads to the following decomposition.

Lemma 4.12.

For Ψ=Ψi(E) and SCC C of Gi(Ψ), suppose that successive SCCs do not exist. Let uC and Φu be a TC recovered from STC Ψ. Then,

Pr(SCΨ)=peiPr(Su𝗁𝗂u(Φu))+(1pei)Pr(Su𝗅𝗈u(Φu)). (13)

To compute the terms in the right-hand-side of (13), we can use the previous algorithm in Section 3. However, naively computing these terms for every uV requires O(mnωp22ωp2) time, since this amounts to constructing a diagram of the previous algorithm for every u.

To overcome this, we use Lemma 4.5. Since we only need to compute Pr(SvΦv) for the case vAi, we can share identical TCs, as in Observation 4.6. Accordingly, we do not need to construct different diagrams for every v to compute Pr(SvΦv), that is, if identical TCs Φv and Φw from different v,w appear, we share them. This enables us to compute all Pr(SvΦv)s in linear time.

4.3 Procedure

We formally describe the proposed method in Algorithm 2. Lines 1–6 construct the diagram of STCs Ψ. Ψ.𝖿 stores a pointer to 𝖿(Ψ). We consider the successive SCCs in lines 7–11. If a successive SCC of C exists, C.𝖿 stores the pointer to it. Otherwise, following the approach of Section 4.2, we recover the original TC Φu, where uC, and then carry out transition 𝗅𝗈u or 𝗁𝗂u on it. Φu(Ψ) recovers the original TC by removing every column x satisfying Ψxu=1 from Ψ, that is, we remove columns whose indices can reach u. If a pruning occurs by considering Φ=𝖿u(Φu(Ψ)), C.𝖿 stores or . Otherwise, C.𝖿 stores a pointer to 𝖼𝗁𝖺𝗇𝗀𝖾t(Φ), where 𝖼𝗁𝖺𝗇𝗀𝖾t() changes the column index u to t. Here, t is an imaginary vertex that is assumed to be contained within Ai. Since Observation 4.6 confirms that the transitions of identical TCs are identical, we standardize the column index u by changing it to t. We build a diagram of Φit() in Lines 12–15.

Lines 17–19 compute p[Ψ]=Pr(Ψ) for every Ψi in the same manner as Algorithm 1, and lines 20–22 compute q[Φ]=Pr(StΦ) for every Φ𝒩i in a bottom-up manner. Lines 23–26 compute r[Ψ,C]=Pr(SCΨ) for every Ψ and every SCC C of Gi(Ψ). Here, c ? x : y stands for a conditional operator that returns x if c is satisfied or y otherwise. When C.𝖿 is either an original TC Φt or ,, we use the q value; otherwise, we use the r value. Finally, lines 27–31 compute every res[v]=Pr(Sv) using (10).

Algorithm 2 Proposed algorithm for computing Pr(Sv) for every v.

Here, we confirm the correctness of Algorithm 2.

Lemma 4.13.

After executing Algorithm 2, res[v] equals Pr(Sv).

Proof.

First, we confirm p[Ψ]=Pr(Ψ). Starting from p[Ψ1()]=Pr(Ψ1())=1 for Ψ1()1, lines 17–19 compute every Pr(Ψ) value for 2,,m according to (11).

Second, we confirm q[Φ]=Pr(StΦ), but this is much simpler; with the case analysis of whether ei is present or absent, we have

Pr(StΦ)=piPr(St𝗁𝗂t(Φ))+(1pi)Pr(St𝗅𝗈t(Φ)). (14)

Starting from q[]=Pr(St)=0 and q[]=Pr(St)=1, lines 20–22 compute every Pr(StΦ) value for 𝒩m,𝒩m1, according to (14).

Third, we confirm r[Ψ,C]=Pr(SCΨ). If there exists uC such that uWi+1, i.e., a successive SCC exists, we can apply (12). Otherwise (i.e., a successive SCC does not exist), we can apply (13). Here, without considering the pruning, C.𝖿 stores a pointer to 𝖿(C) if a successive SCC exists or, otherwise, to 𝖼𝗁𝖺𝗇𝗀𝖾t(𝗅𝗈u(Φu)). Consequently, lines 23–26 correctly compute r[Ψ,C] according to (12) if a successive SCC exists or to (13) otherwise. For the latter case, we use Lemma 4.5; i.e., Pr(Su𝗅𝗈u(Φu))=Pr(St𝖼𝗁𝖺𝗇𝗀𝖾t(𝗅𝗈u(Φu)))=q[𝖼𝗁𝖺𝗇𝗀𝖾t(𝗅𝗈u(Φu))].

Finally, by choosing i such that vWi, res[v]=Pr(Sv) is correctly computed using (10) through lines 27–30.

Treatment of degree 𝟏 vertices.

We finally describe how to deal with degree 1 vertices. By obtaining the Pr(Sv) values for all vertices with degree not less than 2, we can easily obtain the Pr(Sv) values for degree 1 vertices. Let vVS be a vertex whose degree is 1. Let ev be the unique edge incident to v. If ev=(v,w) for some wV, i.e., v is the tail of ev, we have Pr(Sv)=0 because v has no incoming edges. Otherwise (i.e., v is the head of ev), we have Pr(Sv)=pevPr(Sw) because every path from some sS to v must go through w, thus ev. Since G is connected and thus w has degree at least 2 except for the trivial case where ev is the only edge of G, we can obtain Pr(Sv) for v whose degree is 1 from the value of Pr(Sw).

4.4 Complexity

To analyze the complexity, we again use ω=maxi|Wi|. First, we consider the diagram construction. The key lemma is as follows.

Lemma 4.14.

Given Φ=Φiv(E) for some EE<i, we can compute the transitions 𝗅𝗈v(Φ) and 𝗁𝗂v(Φ) in O((|Wi|+|Wi+1|)2) time. Similarly, given Ψ=Ψi(E) for some EE<i, we can also compute 𝗅𝗈(Ψ) and 𝗁𝗂(Ψ) in O((|Wi|+|Wi+1|)2) time.

The full proof is deferred to the full version; here, we describe the ideas for computing transitions. For TC Φ, we build a graph G=(Wi{S,v},E), where S is regarded as an individual special vertex and E={(u,w)Φuw=1}. By adding and removing edges and vertices according to the transition and computing the transitive closure, we can obtain the updated graph, whose adjacency matrix constitutes 𝗁𝗂(Φ) or 𝗅𝗈(Φ). The transition of STC Ψ can be computed in very similar way.

Similar to Φiv, we can compute the transition 𝗅𝗈,𝗁𝗂 of Ψ in O(ω2) by recomputing the transitive closure. Note that we can also compute the SCCs and their successive SCCs within this process, as described in the proof of Lemma 4.14. Thus, the total time for diagram construction is bounded by O(ω2)O(i(|i|+|𝒩i|)) time. Here, we can bound the number of possible patterns on Φiv and Ψi, i.e., |𝒩i| and |i|, as follows. Since the proofs of Lemmas 4.15 and 4.16 are much similar; the proof of Lemma 4.16 is put on the full version.

Lemma 4.15.

|i|=|{Φiv(E)EE<i}| is bounded by O(2|Wi|2).

Proof.

If we fix WiS(E) and Wiv(E), some entries of Φiv(E) are determined as follows: Φiv(E)Sw=1 if wWiS(E) or 0 if wWiWiS(E), and Φiv(E)uv=1 if uWiv(E) or 0 if uWiWiv(E). Therefore, the possible patterns on Φiv(E) is bounded by O(2(|Wi||WiS(E)|)(|Wi||Wiv(E)|)) because Φiv(E) is a binary matrix of size (|Wi||WiS(E)|+1)×(|Wi||Wiv(E)|+1), and the entries of one row and one column are already determined.

We conduct a case analysis of k=|WiS(E)|+|Wiv(E)| when fixing WiS(E) and Wiv(E). When k=0, the bound is O(2|Wi|2). When k=1, the bound is O(2|Wi|2|Wi|), and the number of patterns on (WiS(E),Wiv(E)) is bounded by O(|Wi|). When k2, since (|Wi||WiS(E)|)(|Wi||Wiv(E)|)(|Wi|1)(|Wi|1)=|Wi|22|Wi|+1 (supposing that |Wi|3), the number of possible patterns is bounded by O(2|Wi|22|Wi|). The number of possible patterns on (WiS(E),Wiv(E)) is bounded by 2|Wi|2|Wi| because WiS,WivWi. Thus, the total number of patterns on Φiv(E) is bounded by O(2|Wi|2)+O(|Wi|2|Wi|2|Wi|)+O(22|Wi|)O(2|Wi|22|Wi|)=O(2|Wi|2)+O(2|Wi|2+log|Wi||Wi|)+O(2|Wi|2)=O(2|Wi|2).

Lemma 4.16.

|𝒩i|=|{Ψi(E)EE<i}| is bounded by O(2|Wi|2).

Therefore, |i|=|𝒩i|=O(2ω2), and the total time complexity for diagram construction can be bounded by O(mω22ω2).

Next, we consider the DP. Each value can be computed in constant time. The number of values to compute for Ψi and Φiv is bounded by O(|i|+|Wi||i|+|𝒩i|)=O(ω2ω2+2ω2)=O(ω2ω2). Thus, the total complexity is O(mω2ω2).

Finally, computing each Pr(Sv) using (10) requires O(|i|)=O(2ω2) time. Thus, it needs O(n2ω2) time in total for all Pr(Sv) values.

Proposition 4.17.

Given directed graph G, seed set S, each edge’s probability pe of presence, and the edge ordering e1,,em, the probability Pr(Sv) for every vertex v can be computed in O((m+n)ω22ω2) time in total.

Since we can generate an edge ordering with ωωp from a path decomposition of width ωp [9] in linear time, we achieve Theorem 1.2. Moreover, with the linear-time path-decomposition algorithm for a bounded-pathwidth graph [2], we have the following.

Theorem 4.18.

Given directed graph G, seed set S, and each edge’s probability pe of presence, suppose that G’s pathwidth is bounded by a constant. Then, Pr(Sv) for every vertex v can be computed in O(m+n) time in total.

The previous algorithm [15] requires O(mω22ω2) time for computing Pr(Sv), as discussed in Section 3. Thus, it takes O(nmω22ω2) time for computing σ(S). In contrast, the proposed algorithm takes O((n+m)ω22ω2) time. Therefore, in terms of time complexity, our algorithm reduces the dependence on the graph size from O(mn) to O(m+n) while the dependence on ω=maxi|Wi| is kept the same.

5 Discussion

Here, we point out the differences between the proposed algorithm and the existing algorithm that computes the probability of connection for undirected graphs [16]. These algorithms basically share the same idea: In computing the probability of reachability (or connectivity in the undirected graphs) of every vertex, the previous top-down style algorithms, like that in Section 3, generate similar diagrams for different vertices v, so they attempt to share equivalent structures. The algorithm for undirected graphs uses connected components (CCs) among frontier vertices to efficiently compute the conditional probabilities, similar to Pr(SCΨ) in our algorithm. The difference comes from the computation of conditional probability when a successive SCC or CC does not exist. In undirected graphs, if a successive CC does not exist, the current CC is disconnected from any further vertex, so we immediately have the conditional probability 0 (or 1 in an exceptional case). In contrast, in directed graphs, even if a successive SCC does not exist, the current SCC may still reach or be reached from further vertices because it can reach or be reached from the frontier vertices. This makes the computation of the conditional probabilities difficult because we cannot immediately determine them when no successive SCC exists. We resolve this issue by focusing on the equivalence of lower levels of diagrams (Lemma 4.5). This enables us to compute the conditional probabilities using a constant number of diagrams (STCs Ψ and TCs Φt of imaginary vertex t) without breaking the linear complexity.

6 Conclusion

We proposed an algorithm for computing the influence spread under IC model exactly in O((m+n)ωp22ωp2) time. For graphs with bounded pathwidth ωp, we improved the complexity from O(mn) to O(m+n), linear in the graph size, while the dependence on the pathwidth ωp is kept the same.

Finally, we mention some future directions. First, a more efficient exact evaluation of influence spread, suitable for the greedy algorithm [10], should be investigated. Chen et al. [4] developed an algorithm that simultaneously approximates σ(S{v})σ(S) for all vVS, which corresponds to one iteration of the greedy algorithm. Nakamura et al. [17] developed an algorithm for undirected graphs that exactly and simultaneously computes the expected number of connected vertices for all vertices. This algorithm is promising for adoption with directed graphs as a way to simultaneously compute σ(S{v}) for all vVS exactly. Second, we should investigate whether a linear time algorithm for computing σ(S) is possible for graphs with bounded treewidth. A roadmap for achieving this may be to fit the diagram construction method based on tree decomposition [1] to the computation of influence spread and then observe the equivalences. However, such an improvement may not be straightforward due to the complicated nature of these algorithms.

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