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Efficiency of random swap clustering
Journal of Big Data volume 5, Article number: 13 (2018)
Abstract
Random swap algorithm aims at solving clustering by a sequence of prototype swaps, and by finetuning their exact location by kmeans. This randomized search strategy is simple to implement and efficient. It reaches good quality clustering relatively fast, and if iterated longer, it finds the correct clustering with high probability. In this paper, we analyze the expected number of iterations needed to find the correct clustering. Using this result, we derive the expected time complexity of the random swap algorithm. The main results are that the expected time complexity has (1) linear dependency on the number of data vectors, (2) quadratic dependency on the number of clusters, and (3) inverse dependency on the size of neighborhood. Experiments also show that the algorithm is clearly more efficient than kmeans and almost never get stuck in inferior local minimum.
Introduction
The aim of clustering is to group a set of N data vectors {x_{i}} in Ddimensional space into k clusters by optimize a given objective function f. Each cluster is represented by its prototype, which is usually the centroid of the cluster. Kmeans performs the clustering by minimizing the distances of the vectors to their cluster prototype. This objective function is called sumofsquared errors (SSE), which corresponds to minimizing withincluster variances. The output of clustering is the set of cluster labels {p_{i}} and the set of prototypes {c_{i}}.
Kmeans was originally defined for numerical data only. Since then, it has also been applied to other types of data. The key is to define the distance or similarity between the data vectors, and to be able to define the prototype (center). It is not trivial how to do it, but if properly solved, then kmeans can be applied. In case of categorical data, several alternatives were compared including kmedoids, kmodes, and kentropies [1].
Quality of clustering depends on several factors. The first step is to choose the attributes and the objective function according to the data. They have the biggest influence on the clustering result, and their choice is the most important challenge for practitioners. The next step is to deal with missing attributes and noisy data. If the number of missing attributes is small, we can simply exclude these data vectors from the process. Otherwise some data imputation technique should be used to predict the missing values; for some alternatives see [2].
Noise and outliers can also bias the clustering especially with the SSE objective function. Detection of outliers is typically considered as a separate preprocessing step. Another approach is to perform the clustering first, and then label points that did not fit into any cluster as outliers. Outlier removal can also be integrated in the clustering directly by modifying the objective function [3]. After the preprocessing steps, the main challenge is to optimize the clustering so that the objective function would be minimized. In this paper, we focus on this problem.
We use the centroid index (CI) as our primary measure of success [4]. It counts how many real clusters are missing a prototype, and how many have too many prototypes. The CIvalue is the higher of these two numbers. It is demonstrated in Fig. 1 where four real clusters are missing a prototype. This value provides a clear intuition about the result. Specifically, if CI = 0, the result is correct clustering. Sometimes we normalize CI by the number of clusters, and report the relative CIvalue (CI/k). If the ground truth is not available, the result can be compared with the global minimum (if available), or with the best available solution used as gold standard.
Kmeans is very good in finetuning the cluster boundaries locally but it is unable to solve the cluster locations globally. In the solution in Fig. 2 (current solution), most prototypes are in correct locations, except at the top there are two prototypes but only one would be needed; one prototype is also missing in the middle. This solution has value CI = 1. Kmeans is not able to fix it as the two regions are spatially separated, and there is one stable cluster between the two problematic ones. Gradual changes cannot therefore happen by kmeans iterations. This kind of problems is typical especially when the data contains wellseparated clusters.
On the other hand, the correct locations of the prototypes can be solved by a sequence of prototype swaps, and leaving the finetuning of their exact location to kmeans. In Fig. 2, only one swap is needed to fix the solution. An important observation is that it is not even necessary to swap one of the redundant prototypes but simply removing any prototype in their immediate neighborhood is enough since kmeans can finetune their exact location locally. Also, the exact location where the prototype is relocated is not important, as long as it is in the immediate neighborhood where the prototype is needed.
Several swapbased clustering algorithms have been considered in literature. Deterministic swap selects the prototype to be swapped as the one that increases the objective function value f least [5,6,7], or by merging two existing clusters [8, 9] following the spirit of agglomerative clustering. The new location of the prototype can be chosen by considering all possible data vectors [7], splitting an existing cluster [7, 10], or by using some heuristic such as selecting the cluster with the largest variance [5]. The swapbased approach has also been used for solving pmedian problem [11].
The main drawback of these methods is their computational complexity. Much simpler but effective approach is random swap strategy: select the prototype to be removed randomly and replace it to the location of a randomly selected data vector. This trialanderror approach was first used in the tabu search algorithm presented in [12], and later simplified to a method called randomized local search (RLS) [13]. The main observation was that virtually the same clustering quality is reached independent of the initial solution. The same conclusion was later confirmed in [14]. CLARANS is another variant of this technique using medoids instead of centroids [15].
The main reason why random swap approach is not so widely used is the lack of theoretical results of its properties. Our experiments, however, have shown that it works much better than kmeans in practice, and in most cases, is also more efficient [16,17,18,19,20]. Its main limitation is that there is no clear rule how long the algorithm should be iterated and this parameter needs to be selected experimentally.
In this paper, we formulate the random swap (RS) as a probabilistic algorithm. We show that the expected time complexity to find the correct cluster allocation of the prototypes is polynomial. The processing time of the algorithm depends on how many iterations (trial swaps) are needed, and how much time each iteration takes. We will show that for a given probability of failure (q), the time complexity of the algorithm is upper bounded by a function that has linear O(N) dependency on the number of data vectors, quadratic O(k^{2}) dependency on the number of clusters, and inverse dependency on the size of neighborhood.
The main advantage of random swap clustering is that it is extremely simple to implement. If kmeans can be implemented for the data, random swap is only a small extension. Kmeans consists of two steps (partition step and centroid step), and the random swap method has only one additional step: prototype swap. In most cases, this step is independent on the data and the objective function. It is also trivial to implement, which makes it highly useful for practical applications.
Besides the theoretical upper bound, we compare the efficiency experimentally against kmeans, repeated kmeans, kmeans++, xmeans, global kmeans, agglomerative clustering and genetic algorithm. With our clustering benchmark data sets, we compare the results to the known ground truth and observe that random swap finds the correct cluster allocation every time. In case of image data, we use genetic algorithm (GA) as golden standard, as it is the most accurate algorithm known.
The rest of the paper is organized as follows. In “Random swap clustering” section, we recall kmeans and random swap algorithms and analyze their time complexities. In “Number of iterations” section, we study the number of iterations and derive the expected time complexity of the algorithm. The optimality of the algorithm is also discussed. In “Neighborhood size” section, we define the concept of neighborhood. Experimental studies are given in “Experiments” section to demonstrate the results in practice. Conclusions are drawn in “Conclusions” section.
Random swap clustering
The clustering problem is defined as follows. Given a set of N data vectors x in Ddimensional space, partition the vectors into k clusters so that sum of squared error SSE (intra cluster variance) is minimized. For consistency to our previous works, we normalize the sum per vector and per dimension. In this way, the function represents how much error the clustering causes per single attribute (dimension). In image processing context, it is also natural to normalize the value per pixel (N vectors in image, D pixels in vector). It is calculated as follows:
Kmeans algorithm starts with a set of randomly selected vectors as the initial prototypes. It then improves this it initial solution iteratively by the following two steps. In the first step, optimal partition is solved in respect to the given set of prototypes by mapping each data vector to its nearest prototype:
In the second step, a new set of prototypes is calculated based on the new partition:
These steps are iteratively performed for a fixed number of iterations, or until convergence.
Random swap algorithm
Random swap removes one existing cluster and creates a new one to a different part of the data space. This is done by selecting a randomly chosen prototype C_{ s }, and replacing it by a randomly selected data vector x_{ i }:
This generates a global change in the clustering structure. An alternative implementation of the swap would be to create the new cluster by first choosing an existing cluster randomly, and then by selecting a random data vector within this cluster. We use the first approach for simplicity but the second approach is useful for the analysis of the swap.
After the swap, local repartition is performed to update the partition. This local repartition is not obligatory as the solution will anyway be tuned by kmeans afterwards, but it merely speedups the process. First, vectors of the removed cluster are repartitioned to their nearby clusters. This is done by comparing the distances to all other prototypes (including the new cluster) and selecting the nearest:
Second, the new cluster is created by attracting vectors from nearby clusters by calculating the distance of all vectors to the new prototype. If the distance is smaller than the distance to the prototype of the current cluster, the vector will join the new cluster:
The new solution is then modified by two iterations of kmeans to adjust the partition borders locally. The overall process is a trialanderror approach: a new solution is accepted only if it improves the objective function (1).
Pseudo code of the algorithm is sketched in Fig. 3. In brief, random swap is a simpler wrapper, in which any existing kmeans library can be used. One can also leave out the local repartition step as kmeans will anyway fix the partition. The purpose of the local repartition is merely to speedup the process as it basically implements a half iteration of kmeans but faster. Otherwise, it has no significance in the algorithm. To sum up, the only additions random swap have to kmeans are the swap and the comparison (IF–THEN). They are both trivial to implement. Therefore, if kmeans can be applied to the data, so can random swap.
The process of the algorithm is demonstrated in Fig. 4 with T = 5000 trial swaps. Eight of the trial swaps improves the sum of squared error (SSE) and are thus accepted. Among the accepted swaps, three reduces the CIvalue (iterations 1, 3 and 16). The rest of the accepted swaps provide minor improvement in SSE via local finetuning (iterations 2, 9, 28, 58, 121). After that, no further improvement is found. In this example, 16 iterations were needed to solve the correct clustering (CI = 0), and 121 iterations to complete the local finetuning. However, the algorithm does not know when to stop, and we therefore need to estimate how many iterations (trial swaps) should be applied.
Implementations are available in our web pages in C, Matlab, Java, Javascript, R and Python:
There are also video lecture (youtube), presentation material (ppt), flash animation (animator) and web page (Clusterator) where anyone can upload data in text format and obtain quick clustering result in just a 5 s, or alternatively, use longer 5 min option for higher quality. It is currently limited to numerical data only but we plan to extend it to other data types in future.
Time complexity of a swap
Time complexity of a single iteration depends on the implementation of the following steps:

1.
Swap of the prototype.

2.
Removal of the old cluster.

3.
Creation of the new cluster.

4.
Updating affected prototypes.

5.
Kmeans iterations.
Step 1 consists of two random number generations and one copy operation, which take O(1) time. For simplicity, we assume here that the dimensionality is constant d = O(1). In case of very high dimensions, the complexities should be multiplied by d due to the distance calculations.
In step 2, a new partition is found for every vector in the removed cluster. The time complexity depends on the size of the removed cluster. In total, there are N data vectors divided into k clusters. Since the cluster is selected randomly, its expected size is N/k. Processing of a vector requires k distance calculations and k comparisons. This multiplies to 2k·N/k = 2N. Note that the expected time complexity is independent on the size of the cluster.
In step 3, distance of every data vector to the newly created prototype is calculated. There are N vectors to be processed, each requiring 2 distance calculations. Thus, the time complexity of this step sums up to 2N, which is also independent on the size of the cluster.
In step 4, new prototypes are generated by calculating cumulative sums of the vectors in each cluster. To simplify the implementation, the cumulative sums are calculated already during the steps 2 and 3. One addition and one subtraction are needed per each vector that changes its cluster. The sums of the affected clusters (the removed, the new and their neighbors) are then divided by the size of the cluster. There are N/k vectors both in the removed and in the new cluster, on average. Thus, the number of calculations sums up to 2N/k + 2N/k + 2α = O(N/k) where α denotes to the neighborhood size (see “Neighborhood size” section).
The time complexity of the kmeans iterations is less trivial to analyze but the rule of thumb is that only local changes appear due to the swap. In a straightforward implementation, O(Nk) time would be required for every kmeans iteration. However, we use the reduced search variant [21], where full search is needed only for the vectors in the affected clusters. For the rest of the vectors, it is enough to compute distances only to the prototypes of the affected clusters. We estimate that the number of the affected clusters equals to the size of neighborhood of the removed and the added clusters, which is 2α. The expected number of vectors in those clusters is 2α·(N/k). The time complexity of one kmeans iteration is therefore 2α·(N/k)·k for the full searches, and (N − (2α·(N/k)))·2α ≤ N·2α for the rest. These sum up roughly to 4αN = O(αN) for two kmeans iterations.
Table 1 summarizes the time complexity and shows also real observed numbers for the Bridge data set (see “Experiments” section). These numbers are reasonably close to the expected time complexities; only kmeans iterations take twice more than what expected. The reason is that we apply only two iterations whereas the fast kmeans variant in [21] does not become fully effective during the first two iterations. It is the more effective the less the prototypes are moving. This can be seen in Fig. 5; 1st iteration takes 53% share of the total processing time, but 2nd iteration only 39%. Nevertheless, the theoretical estimates are still well within the order of the magnitude bounds.
Figure 5 shows the distribution of the processing times between the steps 1–4 (swap + local repartition) and the step 5 (kmeans). The number of processing time required by kmeans is somewhat higher in the early iterations. The reason is the same as above: there are more prototypes moving in the early stage but the movements soon reduce to the expected level. The time complexity function predicts that kmeans step would take 4αN/(2N + 2N + 4αN) = 89% proportion of the total processing time with Bridge. The observed number of the steps gives 197,327/215,718 = 91% at the 500 iterations, and the actual measured processing times of kmeans takes 0.53 + 0.39 = 92%. For BIRCH_{1}, the time complexity predicts 85% proportion whereas the actual is 97% but it drops to 94% around 500 iterations after all the prototypes have found their correct location.
Further speedup of kmeans could be obtained by using the activitybased approach jointly with kdtree [22], or by exploiting the activity information together with triangular inequality rule for eliminating candidates in the nearest neighbor search [23]. This kind of speedup works well for data where the vectors are concentrated along the diagonal but generalizes poorly when the data is distributed uniformly [21, 24]. It is also possible to eliminate those prototypes from the full search whose activity is smaller than a given threshold and provide further speedup at the cost of decreased quality [25, 26].
Number of iterations
We define three different types of swap:

Trial.

Accepted.

Successful.
One trial swap is made in every iteration but only a swap that improves the objective function is called accepted swap. However, in the following analysis we are interested not all accepted swaps but only those that also reduces CIvalue. In other words, swaps that correct one error in the global prototype allocation; minor finetunings do not count in this analysis. We therefore define a swap as successful if it reduces the CIvalue.
In the example in Fig. 4, among the 5000 thousand trial swaps, 8 are accepted of which 3 we consider successful. Another example is shown in Fig. 6 where the swap in the middle improves objective function and is therefore accepted. However, it does not fix any problem in the prototype allocation, and is therefore not considered as a successful swap. In the rightmost case, the prototype is moved elsewhere and it fixes one more cluster location (CI changes from 2 to 1). This swap shows also significant reduction in the objective function (from 20.12 to 15.87). Larger scale examples are shown in Fig. 7; one with CI = 4 and another one with CI = 9.
Successful swaps
To achieve a successful swap, the algorithm must succeed in three independent tasks:

Select a proper prototype to be removed.

Select a proper location for the prototype.

Perform local finetuning successfully.
The first two are more important, but we will show that the finetuning can also play a role in finding a successful swap. We analyze next the expected number of iterations to fix one prototype location, and then generalize the result to the case of multiple swaps.
To make successful swap to happen, we must remove one prototype from an overpartitioned region and relocate it to an underpartitioned region, and the finetuning must relocate the prototype so that it fills in one real cluster (pigeonhole). All of this must happen during the same trial swap.
Assume that CI = 1. It means that there is one real cluster missing a prototype, and another cluster overcrowded by having two prototypes. We therefore have two favorable prototypes to be relocated. The probability for selecting one of these prototypes by a random choice is 2/k as there are k prototypes to choose from. To select the new location, we have N data vectors to choose from and the desired location is within the real cluster lacking prototype. Assume that all the clusters are of the same sizes, and that the mass of the desirable cluster is twice that of the others (it covers two real clusters). With this assumption, the probability that a randomly selected vector belongs the desired cluster is 2(N/k)/N = 2/k. The exact choice within the cluster is not important because kmeans will tune the prototype locations locally within the cluster.
At first sight, the probability for a successful swap appears to be 2/k·2/k = O(1/k^{2}). However, the finetuning capability of kmeans is not limited within the cluster but it can also move prototypes across neighboring clusters. We define here that two clusters are kmeans neighbors if kmeans can move prototypes from a cluster to its neighbor. In order this to happen, the clusters must be both spatial neighbors and also in the vicinity of each other. This concept of neighborhood will be discussed more detailed in “Neighborhood size” section.
Note that it is also possible that the swap solves one allocation problem but creates another one elsewhere. However, this not considered a successful swap because it does not change the CIvalue. It is even possible that CIvalue occasionally increases even when objective function decreases but this is also not important for the analysis. In fact, by accepting any swap that decreases the objective function, we guarantee that the algorithm will eventually converge; even if the algorithm itself does not know when it happens. We will study this more detailed in “Experiments” section.
Probability of successful swap
To keep the analysis simple, we introduce a datadependent variable α to represent the size of the kmeans neighborhood (including the vector itself). Although it is difficult to calculate exactly, it provides a useful abstraction that helps to analyze the behavior of the algorithm. Mainly α depends on the dimensionality (d) and structure of the data, but also on the size (N) and number of clusters (k). The worst case is when all clusters are isolated (α = 1). An obvious upper limit is α ≤ k.
By following the intuition that any kmeans neighbor of the desired cluster is good enough (both for the removal and for the addition) we estimate the probability of a successful swap as:
In total, there are O(α) clusters to choose from, but both the removal and addition must be made within the neighborhood. This probability becomes lower when the number of clusters (k) increases, but higher when the dimensionality (d) increases. The exact dependency on dimensionality is not trivial to analyze. Results from literature imply that the number of spatial neighbors increases exponentially with the dimensionality: α = O(2^{d}) [27]. However, the data is expected to be clustered and has some structure; it usually has lower intrinsic dimensionality than its actual dimensionality.
Analysis for the number of iterations
We study next the probability that the algorithm can fix one cluster in T iterations. We refer the probability of success as p, and the probability of failure as q = 1 − p. If only one swap is needed, the probability of failure equals to the probability of selecting T unsuccessful swaps in a row:
We can estimate the number of iterations (trial swaps) needed to find the successful swap with the probability of q as follows:
For example, we have visually estimated that the size of neighborhood in Fig. 2 is 4, on average. This estimate leads to the probability of a favorable swap as (α/k)^{2} = (4/15)^{2} ≈ 7%. The dependency of T on p and q is demonstrated in Fig. 8.
Bounds for the number of iterations
We derive tight bounds for the required number of iterations for (8) as follows.
Theorem
Proof for upper limit
According to [28, p. 54]:
This inequality is strict when x = 0. From the second part of (10), we can derive inequality:
Applying this result to (8) with x = (α/k)^{2}, we derive an upper bound as:
Proof for lower limit
In a similar manner, we can derive another inequality from the first part of (10):
Applying this to (8), we derive a lower bound as:
Since the same function is both the upper (11) and lower bound (12), the theorem is proven.□
Multiple swaps
The above analysis was made only if one prototype is incorrectly located. In case of the S_{1–4} datasets, 1 swap is needed in 60% cases of a random initialization, and 2 swaps in 38% cases. Only very rarely (< 2%) three or more swaps are required.
The result of “Analysis for the number of iterations” section can be generalized to multiple (w) swaps as follows. It is known that T ≫ w and p ≥ α^{2}/k^{2} independent on the number of swaps. An upper bound for the probability for performing less than w successful swaps in T iterations can be calculated by the binomial probability:
The idea is that there is a sequence of T swaps of which (i < w) are successful. The expected number of iterations for this would be:
The only difference to the case of single swap is the logarithmic term (log_{2} w), which depends only on the number of swaps needed. Even this is a too pessimistic estimation since the probability of the first successful swap is up to w^{2} times higher than that of the last swap. This is because there are potentially w times more choices for the successful removal and addition. Experimental observations show that 2.7 swaps are required with S_{1}–S_{4}, on average, and the number of iterations is multiplied roughly by a factor of 1.34, when compared to the case of a single swap. However, the main problem of using the Eq. (13) in practice is that the number of swaps (w) is unknown.
Overall time complexity
The total processing time is the number of iterations multiplied by the time required for a single iteration (αN). Based on the results in section combined with (11–13), it can be estimated as:
The expected processing time is derived accordingly multiplying (14) by αN:
From (16), we can make the following observations about the time complexity:

Linear dependency on N.

Quadratic dependency on k.

Logarithmic dependency on w.

Inverse dependency onα.
The main result is that the time complexity has only linear dependency on the size of data, but quadratic on the number of clusters (k). Although k is relatively small in typical clustering problems, the algorithm can become slow in case of large number of clusters.
The size of the neighborhood affects the algorithm in two ways. On one hand, it increases the time required by the kmeans iterations. On the other hand, it also increases the probability for finding successful swaps, and in this way, it reduces the total number of iterations. Since the latter one dominates the time complexity, the final conclusion becomes somewhat surprising: the larger the neighborhood (α) the faster the algorithm.
Furthermore, since α increases with the dimensionality, the algorithm has inverse dependency on dimensionality. The higher the dimensionality implies the algorithm being faster. In this sense, data having low intrinsic dimensionality represent the worst case. For example, BIRCH_{2} (see “Experiments” section) has onedimensional structure (D = 1) having small neighborhood size (α = 3).
Optimality of the random swap
So far we have assumed that the algorithm finds the correct cluster allocation every time (CI = 0). This can be argued by the pigeonhole principle: there are k pigeons and k pigeonholes. In a correct solution, exactly one pigeon (prototype) occupies one pigeon hole (cluster). The solution for this problem can be found by a sequence of swaps: by swapping pigeons from overcrowded holes to the empty ones. It is just a matter of how many trial swaps are needed to make it happen. We do not have formal proof that this would always happen but it is unlikely that the algorithm would get stuck in suboptimal solution with wrong cluster allocation (CI > 0). With all our data having known ground truth and unique global minimum, random swap always finds it in our experiments.
A more relevant question is what happens with real world data that does not necessarily have clear clustering structure. Can the algorithm also find the global optimum minimizing SSE? According to our experiments, this is not the case. Higher dimensional image data can have—not exactly multiple optima—but multiple plateaus with virtually the same SSEvalues. In such cases, random swap ends up to any of the alternative plateaus all having nearoptimal SSEvalues. Indirect evidence in [4] showed that two highly optimized solutions with the same cluster allocation (CI = 0) have also virtually the same objective function value (SSE = 0.1%) with significantly different allocations of the prototypes (5%).
We constructed similar experience here using three different random initial solutions: A, B and C, see Fig. 9. We first performed one million trial swaps (A1, B1, C1) and then continued further to 8 million trial swaps, in total (A8, B8, C8). As expected, all solutions have very similar SSEvalues (< 0.3% difference). Despite of this, their cluster level differences (CIvalues) remain significantly high: A8 and B8 had 24/256 ≈ 9% differences. This indicates that the random swap algorithm will find one of the nearoptimal solutions but not necessarily the one minimizing SSE.
To sum up: proof of optimality (or nonoptimality) of the cluster level allocation (CIvalue) remains an open problem. For minimizing SSE, the algorithm finds either the optimal solution (if unique) or one of the alternative nearoptimal solutions all having virtually equal quality.
Neighborhood size
In the previous analysis, we introduced the concept of kmeans neighborhood. The size of this neighborhood (including the vector itself) is denoted by α. It is defined as the average over the entire data set. In practice, it is not possible to calculate or even estimate α accurately without actually performing kmeans. The value is bounded to the range α∈[1,k], and the worst case is α = 1 when all clusters are isolated from each other. We next discuss how the size of this neighborhood could be analyzed in the context of multidimensional data.
Voronoi neighbors
One way to analyze whether clusters are neighbors is to calculate Voronoi partition of the vector space [29, 30] according to a given set of prototypes, and define two clusters as neighbors if they share a common Voronoi facet. An example of Voronoi partition is shown in Fig. 10 (left).
For 2D data, an upper limit for the number of Voronoi surfaces has been shown to be 3k − 6 [30]. Since every Voronoi surface separates two neighbor partitions, we can derive an upper limit for the average number of neighbors as 2·(3k − 6)/k = 6 − 12/k, which approaches to 6 when k becomes large. In our 2D data sets (S_{1}–S_{4}), there are 4 Voronoi neighbors, on average, varying from 1 to 10. For Ddimensional data, the number of Voronoi surfaces is upper bounded by \({\text{O}}(k^{{\left \!{\overline {\, D \,}} \right. /\left. {\overline {\, 2 \,}}\! \right }} )\) [30]. Respectively, an upper bound for the Voronoi neighbors is \({\text{O}}( 2\cdot k^{{\left \!{\overline {\, D \,}} \right. /\left. {\overline {\, 2 \,}}\! \right }} /k)\, = \,{\text{O}}( 2\cdot k^{{\left \!{\overline {\, D \,}} \right. /\left. {\overline {\, 2 \,}}\! \right  1}} )\).
However, such upper bounds estimates are far from reality. Firstly, there cannot be more neighbors than there are clusters (α ≤ k). Secondly, kmeans cannot solve the local optimization if the distance between the clusters is greater than the longest distance within the clusters because no vector can then change partition by kmeans iterations. So we have the following bounds derived both from theory and from data:
 Theory for 2dim::

α ≤ 6 − 12/k
 Theory for Ddim::

\(\upalpha \le {\text{O}}( 2\cdot k^{{\left \!{\overline {\, D \,}} \right. /\left. {\overline {\, 2 \,}}\! \right  1}}\)
 Data limit::

α ≤ k
According to our experiments (“Estimating α and T” section), the theoretical bounds are reasonable for 2D but not for higher dimensions. For example, our highest dimensional (D = 74) dataset KDD04Bio has only 33.3 neighborhood size whereas the theoretical upper bound is 10^{118}, and the data limit 2000. The DIM32 dataset is even more extreme; there are almost no neighbors because the clusters are well separated.
Data  Dim  k  Theory  Reality 

S _{2}  2  15  5.2  4.5 
Bridge  16  256  10^{17}  5.4 
DIM32  32  16  10^{19}  1.1 
KDD04Bio  74  2000  10^{118}  33.3 
To sum up, the number of Voronoi neighbors is significantly higher than the size of the kmeans neighborhood. A better estimator for the size of neighborhood is therefore needed.
Estimation algorithm
For the sake of analysis, we introduce an algorithm to estimate the average size of the kmeans neighborhood. We use it merely to approximate the expected number of iterations (14) for a given data set in experiments in “Experiments” section. The idea is to first to find Voronoi neighbors and then analyze whether they are also kmeans neighbors. However, Voronoi can be calculated fast in O(k·log k) only in case of 2dimensional data. In higher dimensions it takes \({\text{O}}(k^{{\left \!{\overline {\, D \,}} \right. /\left. {\overline {\, 2 \,}}\! \right }} )\) time [31]. We therefore apply the following procedure.
First, we perform random swap clustering for a small number of iterations (T = 5) to obtain an initial clustering. We then compare each pair of prototypes c_{ a } and c_{ b } to conclude whether the two clusters a and b are neighbors. We use the XNN graph introduced in [32]:

1.
Calculate the half point of the prototypes: hp←(c_{a} + c_{b})/2.

2.
Find the nearest prototype (nc) for hp.

3.
If nc = c_{ a } or nc = c_{ b } then (a, b) are neighbors.
Every pair of prototypes that pass this test, are detected as spatial neighbors. We then calculate all vector distances across the two clusters. If any distance is smaller than the distance of the corresponding vector to its own cluster prototype, it is evidence that kmeans has potential to operate between the clusters. Accordingly, we define the clusters as kmeans neighbors. Although this does not give any guarantee, it is reasonable indicator for our purpose.
Experiments
We next test the theory and the assumptions using the data sets summarized in Table 2 and visualized in Fig. 11. The vectors in the first set (Bridge) are 4 × 4 nonoverlapping blocks taken from a grayscale image, and in the second set (Miss America) 4 × 4 difference blocks of two subsequent frames in video sequence. The third data set (House) consists of color values of the RGB image. Europe consists of differential coordinates from a large vector map. The number of clusters in these is fixed to k = 256. We also use several generated data sets such as BIRCH [33], the highdimensional data sets from [24], and the datasets S_{1}–S_{4} with varying overlap of the clusters. KDD04Bio is a largescale highdimensional data set [34].
Ground truth clustering results exist for all the generated data. For the rest, we iterate random swap algorithm for 1 million iterations, and use the final result as the reference solution (golden standard) when applicable. To measure the goodness of the result, we calculate the centroid index (CI) against the ground truth (or reference) solution. Value CI = 0 indicates that the cluster level structure is correct.
All tests have been performed on a Dell PowerEdge R920 Server with four Xeon E74860 v2 processors having 1 TB memory and using RedHat Enterprise Linux 7 operating system.
Estimating α and T
Table 3 reports the estimated neighborhood sizes when calculated by the algorithm of “Estimation algorithm” section and that of the full data. For our analysis, it does not make a big difference at which stage (T = 0, T = 5, T = 5000) the estimation is made. Even if the value was calculated from a random clustering (T = 0) it still provides a useful estimate. In the following experiments, we use the values calculated at T = 5.
We estimate the number of iterations (trial swaps) required to find the clustering for three given probabilities of failure (10, 1, 0.1%). The estimated number of iterations is small for data with few clusters (S_{1}–S_{4}, Unbalance). Even the highest confidence level (q = 0.1%) requires only 97–137 iterations for S_{1}–S_{4}, and 167 for Unbalance. The clusters in the Dim dataset are isolated, which makes the size of the neighborhood very small (1.1). It therefore has larger estimates (about 1700). For the image datasets the estimates are significantly higher because of large number of clusters.
We next study how these predicted numbers compare to reality. For this, we run the algorithm for each dataset exactly the number of times estimated in Table 4. The runs are then repeated 10,000 times, and we record how many times the algorithm actually found the correct clustering (CI = 0). The results for Dim and S datasets in Fig. 12 show that the estimates are slightly overoptimistic for S_{1}–S_{4}. For example, for S_{1} the predicted number of iterations are T = (46, 92, 137) for the failure values q = (10, 1, 0.1%), whereas the algorithm actually failed 18, 4 and 0.6% times. For the Dim sets the results are much closer to the estimates.
The inaccuracies originate from two factors: the estimate of α is somewhat overoptimistic, and the fact that we apply only two iterations of kmeans. To understand the significance of these we plot the distribution of the iterations (trial swaps) required in Fig. 13 as observed in the reality. In 90% of cases, the algorithm requires less than 70 (S_{1}) and 50 (S_{4}) iterations. The corresponding estimates (q = 10%) are 46 (S_{1}) and 34 (S_{4}). Thus, the number of iterations needed is roughly 1.5 than what is estimated. This is well within the order of magnitude of the estimates of Eqs. (15) and (16).
The worst case behavior is when α = 1, meaning that all clusters are isolated. If we left α out of the equations completely, this would lead to estimates of T ≈ 700 for S_{1}–S_{4} even with q = 10%. With this number of iterations we always found the correct clustering and the maximum number of iterations ever observed was 322 (S_{1}) and 248 (S_{4}) at the end of the tail of the distribution. To sum up, the upper bounds hold very well in practice even if we ignored α.
Expected number of iterations
Next we study how well the Eq. (16) can predict the expected number of iterations. We use the same test setup and run the algorithm as long as needed to reach the correct result (CI = 0). Usually the last successful swap is the most time consuming, so we study separately how many iterations are needed from CI = 1 to 0 (last swap), and how many in total (all swaps). The estimated and the observed numbers are reported in Table 4. The number of successful swaps needed (w) is experimentally obtained from the data sets.
a. Estimated iterations
The expected results are again somewhat overoptimistic compared to the reality but still well within the order of magnitude of the time complexity results. For S sets, the algorithm is iterated about 50% longer [26, 29, 35] than estimated [18, 20, 21, 24]. For BIRCH data, the estimates for the last swap are slightly too pessimistic as it overestimates the iterations by about 30%. The difference becomes bigger in case of all swaps. Unbalance has the biggest difference, almost 5 times, so let us focus on it a little bit more.
The creation of a new cluster assumes that all clusters are roughly of the same size. However, this assumption does not hold for the Unbalance data, which has three big clusters of size 2000 and five small ones of size 100. By random sampling, it is much more likely to allocate prototype in a bigger cluster. On average, random initialization allocates 7 prototypes within the three big clusters, and only one within the five small clusters. Starting from this initial solution, a successful swap must select a vector from any of the small clusters because the big clusters are too far and they are not kmeans neighbors with the small ones. The probability for this is 500/6500 = 7.7% in the beginning (when w = 4 swaps needed), and 200/6500 = 3% for the last swap. The estimate is 1/k = 1/8 = 12.5%.
Despite this inaccuracy, the balance cluster assumption itself is usually fair because the time complexity result is still within the order of the magnitude. We could make even more relaxed assumption by considering the cluster sizes following arithmetic series cN, 2cN,…, kcN, where c is a constant in range [0,1]. The analysis in [36] shows that the time complexity result holds both with the balance assumption and with the arithmetic case. The extreme case still exists though: cluster size distribution of (1, 1, 1,…, N − k) would lead to higher time complexity of O(Nk^{3}) instead of O(Nk^{2}). However, balance assumption is still fair because such tiny clusters are usually outliers.
b. Kmeans iterations
Another source of inaccuracy is that we apply only two kmeans iterations. It is possible that kmeans sometimes fails to make the necessary finetuning if the number of iterations is fixed too low. This can cause overestimation of α. However, since the algorithm is iterated long, much more trial swaps can be tested within the same time. A few additional failures during the process is also compensated by the fact that kmeans tuning also happens when a swap is accepted even if it is not considered as successful swap by the theory.
We tested the algorithm also using 10 kmeans iterations to see whether it affects the estimates of T, see column Real^{10} in Table 4. The estimates are closer to the reality with the S sets having cluster overlap. This allows kmeans to operate better between the clusters. However, the estimates are not significantly more accurate, and especially with datasets like Dim and Unbalance where clusters are well separated, the difference is negligible. The value of the kmeans iterations is therefore not considered as important.
However, since kmeans step is a bottleneck in terms of absolute running time, we studied its timedistortion efficiency with values 1, 2, 3, 4, 5, 10, 20 and 100. Earlier studies quite unanimously support that two iterations is the best choice [12, 13, 16], and our results here in Fig. 14 confirm this; two iterations is slightly better but the exact value is not critical. One kmeans iteration is slightly inferior to two iterations. However, three or more iterations do not provide enough additional benefit to compensate the extra time spent. We observe the same trend with all data sets. Only exception is if we iterate the algorithm extremely long; several hours or even several days. Then applying 100 kmeans iterations eventually provides the lower SSEvalues with better time efficiency but this kind of result has no practical relevance.
c. Number of swaps
From Table 4, we can also observe that more time is spent for the last successful swap than to all previous ones together. It indicates that the logarithmic dependency on the number of swaps needed is too pessimistic estimation. We therefore study next how much more work is done by all the other swaps in addition to the last one. Results are summarized in Table 5 by measuring the factor between the number of iterations requires by the last swap relative to that of all swaps.
Overall trend is that the log w term is slightly too high estimate when compared to the reality. In case of S sets, the log w value indicates 1.5 total work, whereas the reality is between 1.27 and 1.34. For example, S_{1} requires 33 swaps in total, of which 26 are spent for the last swap. In BIRCH datasets, the difference is much more visible. About 20 swaps are needed, which indicates extra work by a factor of about 4. In reality, only 50% more is required. The corresponding numbers for unbalance (2.0 vs. 2.09) and Dim sets (1.9 vs. 1.41–1.61) show also mild overestimate.
Overall, our conclusion is that for datasets with clear clustering structure, the last swap is the bottleneck and the additional work for all the previous swaps at most doubles the total work load. We therefore conclude that knowing the exact number of swaps needed is not very important to have a good estimate for the required number of iterations.
d. Effect of N and k
We perform one more analysis by varying the size of the data (N) and the number of clusters (k). We reduce the size of BIRCH_{2} in two alternative ways. First we generated random subsamples by eliminating 1000 random vectors at a time to create a series of subsets with N = 1000–100,000. Second we eliminated one cluster at a time to create a series of subsets with k = 1–100. For these subsets, we ran the algorithm until it found the correct clustering (CI = 0). Results are summarized in Fig. 15. We observe that the number of iterations needed has almost no dependency on the size of data but there it has strong quadratic correlation with k. These observations correspond directly to our theory in Eq. (14).
Timedistortion efficiency in practice
We next compare timedistortion performance of the random swap (RS) algorithm to repeated kmeans (RKM) in practice. It is well known that kmeans often gets stuck into an inferior local minimum, and because of this, most practitioners repeat the algorithm. The number of repeats is similar parameter as the number of iterations in RS. We consider 10–100 repeats but it can be easily extended to much higher. Open questions are how many repeats should one use, and whether RKM will also find the correct global allocation.
We first let both RS and RKM run extremely long: RS 1 million iterations, and repeat RKM 500–25,000 times depending on the data. Timedistortion results are summarized in Fig. 16 showing also the number of trial swaps (RS) and repeats (RKM). The number of remaining successful swaps needed is shown by red and blue colors. In case of real data, we use the result of RS after 1 million iterations as reference. This is not necessarily the global optimum but merely as a point of comparison. The dashed line shows the point when the expected number of iterations is reached.
The results show that RS is significantly more efficient than RKM. It usually achieves the same quality equally fast as kmeans, and outperforms it when kept iterating longer. In case of artificial data with clear clusters (Birch_{1}, Birch_{2}, Unbalanced), RS finds the correct clustering (CI = 0) in all cases. For the same data, kmeans has (CI = 7, CI = 18, CI = 3) and repeated kmeans (CI = 3, CI = 9, CI = 1). RS achieves the correct clustering in less than 1 min using (606, 2067, 98) trial swaps. Repeated kmeans is successful only with the Unbalance dataset. It finds the correct result 60% of the trials if repeated 20,000 times. On average, it took 17,538 repeats to reach CI = 0 by RKM.
Multidimensional image data sets do not have clear clustering structure. The clustering can therefore endup with significantly different cluster allocation (10% different clusters) despite having virtually the same SSEvalue (see “Optimality of the random swap” section). The number of missing swaps is therefore less intuitive what it means in practice, but the superiority of RS in comparison to the repeated Kmeans is still clear. The toughest data set is Europe, for which RS outperforms RKM only after running several minutes (after about 2000 swaps).
The expected number of iterations (dashed vertical line) gives a reasonable estimate when the algorithm has succeeded in case of S and BIRCH datasets. For the image datasets, it is just like a line drawn into water without any specific meaning. Since they lack clear clustering structure, the algorithm keeps on searching—and also keeps on finding—better allocations of the prototypes. It seems not to reach any local or global minimum. Additional tests revealed that it seems to stabilize somewhere before 10 M iterations, which corresponds roughly about 3 weeks of processing—way beyond any practical significance.
As a second test, we run RS several times with T = 5000 iterations. Histograms of the resulting values are shown in Fig. 17. In case of S and BIRCH datasets, RS always found the correct clustering. In case of image data sets, there are some variations but even the worst run of RS is always better than the best run of kmeans. Based on the SSEvalues, it is difficult to conclude how significant the difference would be for practical application. However, the CIvalues with BIRCH demonstrate it better. Among the k = 100 clusters, kmeans fails in case of 7% with BIRCH_{1}, and 18% with BIRCH_{2}. Repeated kmeans reaches levels 3 and 9% but it requires 1000 repeats, which takes several minutes. Reaching CI = 0 by RKM seems unrealistic, indicating that it is not capable to solve the global cluster allocation in general.
Finally, we tested the optimality of the random swap using the datasets with known ground truth (S, Birch, Dim, Unbalance). We let the algorithm run until it reached the correct clustering (CI = 0), and then restarted it from scratch. We let it run 10,000 times for Birch sets and 1,000,000 times for S, Dim and Unbalance sets. The algorithm found CI = 0 result every time and never got stuck into a suboptimal solution even once.
Comparison to other algorithms
Since random swap is not the only good clustering algorithm around, we next put the results in wider perspective. Table 6 summarizes the quality and the processing times of a few selected algorithms including the best known and some popular ones: kmeans (KM), repeated kmeans (RKM), kmeans++ [37], xmeans [38], agglomerative clustering (AC) [35], random swap (RS) [13], global kmeans [7], and genetic algorithm [39]. For all kmeans variants, we use the fast variant presented in [21]. For detailed description and more comprehensive quality comparison, we refer to [6]. For RS we use both 5000 iterations (RS_{5000}) and the number of iterations estimated for failure probability q = 0.1% (RS_{x}) from Table 3. RKM is repeated 100 times. KM, KM++ and XM are results of individual runs. The clustering quality is measured by the Centroid Index (CI).
The results show that all kmeans variants (KM, RKM, KM++, XM) fail to find the correct result in more than 50% of the cases. Kmeans++ and xmeans work better than kmeans but not significantly better than RKM. Better algorithms (AC, RS, GKM, GA) are successful in all cases with the exception of AC, which makes one error with S_{4}. RS is simplest to implement. AC is also relatively simple but requires the fast variant from [35] since a straightforward school book or Matlab implementations would be an order of magnitude slower. GA [39] is composed of the same AC and kmeans components.
The down side of using the better algorithms is their slower running time. Three algorithms (AC, RS, GA) work in reasonable time for data sets of size N = 5000 but require already several minutes for the Birch sets of size N = 100,000. GKM is slow in all cases.
Conclusions
Random swap is an efficient algorithm for solving clustering, and unlike kmeans, it does not converge to an inferior local minimum [40, 41]. In this paper, we have analyzed the number of iterations (trial swaps) needed to solve the global allocation of the clusters. Our main results are that the expected processing time, O(Nk^{2}logw/α), depends on the following factors:

Linear O(N) dependency on the size of data.

Quadratic O(k^{2}) dependency on the number of clusters.

Inverse O(1/α) dependency on the neighborhood size.

Logarithmic O(log w) dependency on the number successful swaps needed.
The main limitation is that no practical stopping criterion can be reliably derived from the theory. Previously a fixed number of iterations has been used, such as T = 5000, or another rule of thumb such as T = N. Here we used w = 1 and estimated α using the preliminary clustering after T = 5 iterations. This works ok in practice, but a better estimation would still be desired. Nevertheless, if the quality of the clustering is the main concern, one can simply iterate the algorithm as long as there is time.
The worst case of the algorithm is when the clusters are isolated (α = 1), which leads to O(Nk^{2}) time for one swap. The number of successful swaps needed (w) is unknown but it has at most logarithmic additional cost. Empirical results indicate that the last swap is the most timeconsuming. Theoretical upper limit would be O(Nk^{2}logk) assuming that w = k swaps were needed. Due to the quadratic dependency on k, a faster algorithm such as deterministic swap [20] or divisive clustering [10] might be more useful if the number of clusters is very high.
Implementation of random swap is publicly available in C, Matlab, Java, Javascript, R and Python. We also have web page (http://cs.uef.fi/sipu/clusterator/) where anyone can upload data in text format and obtain quick clustering result in a 5 s, or alternatively use longer 5 min option. As future work, we plan to extend the Clusterator to solve the number of clusters, and also to support nonnumerical data. Importing random swap to other machine learning platforms like Spark MLlib will be considered, including a parallel variant to provide better support for big data.
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Pasi Fränti received the M.Sc. and Ph.D. degrees from the University of Turku, 1991 and 1994 in Computer Science. Since 2000, he has been a professor of Computer Science at the University of Eastern Finland. He has published 72 journal and 159 conference papers, including 14 IEEE transaction papers. His current research interests are in clustering and locationaware applications.
Acknowledgements
The author thanks Dr. Olli Virmajoki for his efforts on the earlier drafts: let’s shed more sweat and tears in future!
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Fränti, P. Efficiency of random swap clustering. J Big Data 5, 13 (2018). https://doi.org/10.1186/s405370180122y
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DOI: https://doi.org/10.1186/s405370180122y