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Digital Life Laboratory, California Institute of Technology, Pasadena, California 91125
1 Present address: Keck Graduate Institute, 535 Watson Dr., Claremont, CA 91711.
E-mail: wilke{at}kgi.edu
| ABSTRACT |
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X174 and G4 (BULL et al. 2000; KICHLER HOLDER and BULL 2001). Early studies of clonal interference date back to Kimura and coworkers (CROW and KIMURA 1965; KIMURA and OHTA 1971). These authors considered the same effect s for all beneficial mutations. GERRISH and LENSKI (1998) were the first to consider a distribution of beneficial effects, but neglected deleterious mutations. The results of GERRISH and LENSKI (1998) were later generalized by ORR (2000) to include deleterious mutations. In the works of both GERRISH and LENSKI (1998) and ORR (2000), the final results (formulas for the expected substitution rate and for the mean effect of fixed mutations) were given in the form of unwieldy double integrals, which are difficult to interpret. [However, GERRISH and LENSKI (1998) gave explicit expressions for the unrealistic case of uniformly distributed beneficial mutations.] From these integrals, we cannot easily estimate for what parameter settings the interference effect becomes important, and it is unknown how the speed of adaptation behaves for very large N. Moreover, even numerical evaluation of the integrals can be tricky, because the integrand is strongly peaked. ROZEN et al. (2002) gave an explicit expression for the distribution of beneficial effects of fixed mutations at large N. However, this expression also does not lead to a simple expression for the mean.
Here, I derive asymptotic expansions for the expected rate of adaptation and for the mean beneficial effect of fixed mutations, under the assumption that beneficial mutations are distributed exponentially. This assumption is reasonable and has good theoretical support from extreme-value theory (GILLESPIE 1983, 1991; ORR 2003). I find that for very large N, the expected rate of adaptation approaches a limiting value that is given by the mean selective advantage of new beneficial mutations. The mean beneficial effect of fixed mutations, on the other hand, does not reach a hard limit, but continues to grow with the logarithm of the population size.
| MATERIALS AND METHODS |
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U for small pb). The effects of both beneficial and deleterious mutations are drawn from probability distributions; all mutations act multiplicatively. I use a slightly simplified notation for beneficial and deleterious effects of mutations in comparison to ORR (2000): By s, I denote the effect of a particular mutation, either beneficial (in which case fitness is increased by a factor 1 + s) or deleterious (in which case fitness is decreased by a factor 1 s). The mean effect of beneficial mutations is sb, and the mean effect of deleterious mutations is sd. The harmonic mean of the distribution of deleterious mutations is sH. At equilibrium (when all beneficial mutations have gone to fixation), the frequency of the class of individuals with the highest fitness is approximately P0 = exp(U/sH) (ORR 2000). I assume that beneficial mutations are exponentially distributed; that is, beneficial effects are drawn from a distribution with probability density function f(s) = exp(s/sb)/sb. The analytic calculations make no assumption about the distribution of deleterious mutations, but all simulations have been carried out with a truncated exponential distribution (see Simulation methods). I assume that on average deleterious mutations have a much larger effect than beneficial mutations (sb << sd), such that beneficial mutations rarely compensate deleterious mutations.
Simulation methods:
I carried out simulations of the model described in the previous subsection. In the simulations, N sequences were propagated in discrete generations. The number of offspring sequences of a sequence i in the next generation was binomially distributed with mean wi/
w
, where wi is the fitness of sequence i and
w
is the average fitness of the population. Each offspring sequence suffered kb beneficial and kd deleterious mutations, where kb and kd were Poisson distributed with means Upb and U(1 pb), respectively. Each beneficial mutation increased the fitness of a sequence by a factor of 1 + s, where s was drawn from an exponential distribution with mean sb. Each deleterious mutation decreased the fitness of a sequence by a factor of 1 s, where s was drawn from a truncated exponential distribution with parameter a. The distribution was truncated both to the left and to the right. The left truncation was necessary to avoid a zero harmonic mean sH. (For sH = 0, the predicted frequency of the unmutated individuals is P0 = 0, and the theory breaks down.) I used as a cutoff for the left truncation the value 0.01. The right truncation is necessary to avoid negative fitness, and here I used the cutoff value 1. As a parameter for the truncated exponential distribution, I used a = 0.1, which results in sd = 0.11 and sH = 0.05.
I let the population equilibrate for 1000 generations at pb = 0 before I set pb to its desired value and started measuring the rate of adaptation. Simulations were continued for up to 50,000 generations, depending on population size (the smaller the population size, the longer the simulation run), and replicated between 5 and 50 times (the smaller the population size, the more replicates). For each sequence in the population, I kept track of the number of beneficial mutations it had accumulated. At the end of a simulation run, I subdivided the final population into classes with equal numbers of beneficial mutations and determined the most abundant class. The number of beneficial mutations n in the most abundant class divided by the number of generations since equilibration
t served as an estimator for the rate of substitution k. I averaged k over all replicates to obtain the result reported for E[k]. To obtain an estimate for the change in log fitness over time d log w(t)/dt, I determined the sequence with the least number of deleterious mutations in the most abundant class and divided the logarithm of the sequence's fitness by
t. Again, I averaged over all replicates to arrive at the values reported here. To test whether this approach was comparable to a direct measurement of the change in population fitness, I fitted for several exemplary runs a straight line to the logarithm of the average population fitness as a function of time, from the end of the equilibration time to the end of the simulation run, and took the slope of that line as the value for d log w(t)/dt. The differences in the results obtained with these two alternative approaches were minute.
| RESULTS |
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![]() | (1) |
(ORR 2000). When beneficial mutations interfere with each other, then their probability of fixation is reduced by a factor of eI(s), with
(GERRISH and LENSKI 1998; ORR 2000). I(s) is the expected number of new mutations of effect larger than s that occur in the time interval of length t = (2/s) ln N during which a mutation of effect s goes to fixation. The form of I(s) that I use throughout this article assumes that beneficial mutations are distributed exponentially. The general form for arbitrary distributions is given in GERRISH and LENSKI (1998) and ORR (2000). The expected rate of substitution is obtained by integrating over all beneficial mutations. Again using the assumption that beneficial mutations are exponentially distributed, one finds that
![]() | (2) |
(GERRISH and LENSKI 1998; ORR 2000).
In APPENDIX A, I show that for large N, the substitution rate becomes
![]() | (3) |
In the limit of N
, this expression simplifies to
![]() | (4) |
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![]() | (5) |
![]() | (6) |
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2NUpbP0sb (Equation 1), while for very large N, we have E[k] = sb. On the basis of these two equations, we can derive a simple estimate for the parameter regions in which clonal interference is relevant: We are certainly in the clonal-interference regime if the estimate of E[k] for small N exceeds that for large N, that is, if
![]() | (7) |
This result has a simple interpretation: Clonal interference becomes relevant ifon averageone beneficial mutation arises in the zero-mutation class at least every other generation. Note that the mean effect of deleterious mutations enters this result (through P0), but not the mean effect of beneficial mutations.
The estimate Equation 7 is fairly conservative, in the sense that when N > 1/(2UpbP0), we are sure that clonal interference is important, but clonal interference starts having some effect already for smaller N. In APPENDIX A, I show that an improved estimate is
![]() | (8) |
Figure 1 illustrates where the two estimates Equations 7 and 8 lie with respect to the exact expression and the approximations for E[k].
Speed of adaptation:
The expected substitution rate is in general not an accurate measure for the speed of adaptation, because it disregards the beneficial effect of the fixed mutations. A better measure is the change in fitness (or log fitness, which is more appropriate for a multiplicative model) over time. Clearly, the faster fitness increases, the faster a population adapts to its environment.
As mentioned by JOHNSON and BARTON (2002), the change in log fitness is given by
![]() | (9) |
Using E[k] = sb and E[s] as given in Equation 6, we find for large N
![]() | (10) |
This equation predicts two different regimes for d log w(t)/dt, depending on the values of sb and N. If sb << 1, and N is only moderately large (but sufficiently large such that E[k]
sb), then we can approximate ln(1 + E[s]) with E[s] and find
![]() | (11) |
In this regime, the speed of adaptation depends logarithmically on N. If on the other hand N is extremely large and sb is not extremely small, then
![]() | (12) |
In this regime, the speed of adaptation depends double-logarithmically on N.
For comparison, I now calculate the speed of adaptation for small N. For small N, clonal interference can be neglected, and therefore the mean beneficial effect corresponds to the mean effect of beneficial mutations that have survived drift. The distribution of these mutations is
(OTTO and JONES 2000; ROZEN et al. 2002), and the mean is E[s] = 2sb. Using ln(1 + E[s])
E[s], we find for small N
![]() | (13) |
To summarize, the speed of adaptation grows linearly in N for small N and logarithmically or double-logarithmically in N for large N. Interestingly, in the clonal interference regime, growth in the speed of adaptation comes from the fixation of mutations with increasingly larger effects, rather than from the fixation of increasingly more beneficial mutations. Hence, clonal interference slows down the speed of adaptation, but it does not lead to a hard speed limit as long as beneficial mutations of increasingly larger effect are accessible.
Simulation results:
I have carried out extensive simulations to test the accuracy of the clonal interference theory. GERRISH and LENSKI (1998) mentioned that they found good agreement between theory and simulations, but they did not report any simulation results or the parameter regions they had considered. ORR (2000) reported some simulation results, but his simulations were not in the clonal interference regime (as defined by Equation 8).
Figure 3 shows the expected substitution rate as a function of the mutation rate U, both as predicted by Equation 2 and as found in simulations. Below the optimal mutation rate U = sH at which the substitution rate assumes its maximum (ORR 2000), agreement between theory and data is good over a wide range of population sizes. Above U = sH, the theory underestimates E[k]. This effect is caused by the accumulation of slightly deleterious mutations in the simulations. The theory assumes that only those beneficial mutations that arise in backgrounds free from deleterious mutations can go to fixation. However, for large U, sequences that carry one or several slightly deleterious mutations become so frequent that it becomes likely that one of them acquires a beneficial mutation of sufficiently large effect to compensate the deleterious background and goes to fixation. The degree to which the theory underestimates E[k] increases as sH decreases. In the limit of sH = 0, the theory predicts that E[k] = 0, while simulations show that the true results (with identical sb and sd) are not substantially different from those shown in Figure 3 (data not shown). Surprisingly, the theory accurately predicts the change in log fitness d ln w(t)/dt even in the regime of large U, as long as d ln w(t)/dt is not negative (Figure 4). [For very high U, Muller's ratchet (MULLER 1964; FELSENSTEIN 1974; HAIGH 1978; GORDO and CHARLESWORTH 2000) becomes the predominant force in the dynamic of the evolving population, and the change in log fitness can assume negative values.] Apparently, in the regime of large U, the theory underestimates E[k] and overestimates E[s], in such a way that the two effects nearly cancel each other.
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0.001 the theory underestimates E[k] and overestimates E[s], in such a way that the two effects cancel each other (data not shown).
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1, which means that d ln w(t)/dt should appear approximately as a straight line with slope 2 in the double-logarithmic plot. We see that the simulation data agree very well with the theory as long as sb
sd, but start to diverge slowly as sb grows larger than sd.
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| DISCUSSION |
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My results hinge on the assumption that new beneficial mutations are exponentially distributed. If beneficial mutations are distributed such that large effects are absent, then the rate of adaptation will most likely reach an upper limit for large N. If on the other hand beneficial effects follow a distribution with a long tail (such as a power-law or Cauchy distribution), then the speed of adaptation may grow even faster than predicted by Equation 10 for large N. To date, we do not have a good understanding of the true distribution of beneficial effects in experimental systems. However, an exponential distribution has good theoretical support (GILLESPIE 1983, 1991; ORR 2003), has led to good agreement between theory and experiment in E. coli (ROZEN et al. 2002), and overall seems to be a reasonable choice.
Arguments for an exponential distribution of new deleterious mutations are not as strong. At the same time, the theory is much less dependent on the particulars of the distribution of deleterious mutations. As long as we have an accurate expression for P0, and beneficial mutations are unlikely to compensate deleterious mutations, the theory should work. In practice, this means that the theory should work with any distribution that does not produce an excessive amount of slightly deleterious mutations. (Neutral mutations could be dealt with by considering them as a reduction in the overall mutation rate U.)
DE VISSER et al. (1999) measured the speed of adaptation in E. coli, varying both the population size and the mutation rate each over approximately two orders of magnitude. They found that the speed of adaptation did not grow in proportion to increases in population size or mutation rate. In fact, apart from the experiments carried out at the lowest mutation rate, the speed of adaptation changed only very little with population size or mutation rate. These results indicate that the populations with the larger size and higher mutation rates could not benefit from the additional beneficial mutations that must have appeared. The results of DE Visser et al. (1999) thus provide good support for the clonal interference model on a qualitative level. Quantitatively, however, their data seem to disagree with the model analyzed here: Figure 2A of DE VISSER et al. (1999) suggests that the speed of adaptation runs quickly into a hard limit, whereas the model predicts that the speed should continue to grow logarithmically, at least with respect to population size.
Two reasons may have caused this discrepancy: First, DE VISSER et al. (1999) plotted the speed of adaptation vs. the relative mutation-supply rate (which is the product of population size and relative mutation rate). Such a plot is problematic, because the mutation-supply rate does not uniquely specify the speed of adaptation in the clonal interference model. (For the mutation-supply rate to uniquely specify the speed of adaptation, population size and mutation rate would have to enter the equations always as a product, which is not the case. In Equation 10, for example, the term P0 depends on U but not on N, while the term ln N does not depend on U.) The model predicts that the speed of adaptation should increase with increasing N, whereas it should reach a maximum and then decrease with increasing U. Thus, a plot of the speed of adaptation vs. population size (at fixed U) is inherently more informative than a plot of the speed of adaptation vs. mutation rate (at fixed N). In the latter case, a decline in the increase of the speed of adaptation may also indicate that the mutation rate approaches the optimal mutation rate U = sH. Since DE VISSER et al. (1999) studied only two different population sizes (and three mutation rates), it is not possible to replot a subset of their data vs. population size at fixed U and obtain a quantitative comparison to the model.
Second, the speed of adaptation at a high mutation-supply rate may have been reduced (thus giving the impression of a hard speed limit) in part because the populations began to run out of beneficial mutations. de Visser et al. propagated the populations for 1000 generations and determined the speed of adaptation from the total fitness increase over these 1000 generations. In particular for the large population size, it seems that adaptation slowed down considerably after 500 generations (DE VISSER et al. 1999, Figure 1B). [Note, however, that this argument does not invalidate the overall conclusion of DE VISSER et al. (1999). The fitness increase after 200 generations in their Figure 1 shows strong dependence on the mutation rate for the small population size and weak dependence on the mutation rate for the large population size, which agrees very well with the predictions of the clonal interference model.] A related explanation for the apparent slowdown in the speed of adaptation at large population size is that the large populations may have found mutations of large beneficial effect earlier in the experiments than the small populations, as predicted by the clonal interference model.
The clonal interference model assumes an infinite supply of beneficial mutations, and this assumption is of course unrealistic. Nevertheless, we can expect good agreement between model and experiment if the experiment is restricted to a relatively short number of generations, or if only the effect of the first fixed mutation is measured. An experiment of the latter kind was carried out by ROZEN et al. (2002), who found that the measured distribution of beneficial effects in E. coli was in good agreement with the distribution as predicted by the clonal interference model.
The data of ROZEN et al. (2002) also allow us to estimate the onset of clonal interference in E. coli. By fitting the theoretical prediction for the distribution of beneficial effects to their data, ROZEN et al. (2002) derived estimates for the mean beneficial effect of new mutations sb and for the beneficial mutation rate Upb. They found sb = 0.024 and Upb = 5.9 x 108. Having an estimate for the beneficial mutation rate, we can use Equation 8 to estimate the population size in these E. coli populations at which clonal interference becomes important. Since we do not have a good estimate for the mutational load in these populations, we set P0 = 1, which means that we neglect the effect of deleterious mutations. [See ORR (2000) for a discussion of this problem and its implications for the estimates of sb and Upb.] As a consequence, we most likely underestimate the population size at which clonal interference becomes important. Further, instead of the factor 2 in front of Upb, we use 0.6. This factor takes into account that the E. coli populations fluctuate in size under standard laboratory conditions; see ROZEN et al. (2002), p. 1044. Thus, we use for our estimate N ln N > 1/(0.6 x 5.9 x 108). This condition simplifies to N > 2 x 106. [Using a less accurate method based on only the expected substitution rate and mean beneficial effect of fixed mutations, GERRISH and LENSKI (1998) had earlier derived an estimate of Upb = 2 x 109, which leads to N > 4.7 x 107.] ROZEN et al. (2002) carried out their experiments at an effective population size of N = 3.3 x 107, which means that clonal interference probably had an effect on their results. This reasoning is consistent with the observation that the mean beneficial effect of fixed mutations is clearly >2sb in their data (ROZEN et al. 2002, Figure 3).
Clonal interference has been studied not only in E. coli, but also in vesicular stomatitis virus (VSV). Following DE VISSER et al. (1999), MIRALLES et al. (1999) fitted a linear and a hyperbolic model to the rate of fitness change in VSV as a function of population size and found that the hyperbolic model provided the better fit. However, their data do not plateau at high N, and visual inspection of their Figure 1 suggests that a logarithmic model might fit their data as well. On the other hand, the multiplicity of infection was changed along with the population size in these experiments, so that a slowdown in the speed of adaptation could also be due to increased virus-virus interactions within cells, rather than to clonal interference (WILKE and NOVELLA 2003).
My simulations have shown that the theory of clonal interference works well for small to moderate mutation rates, but fails at high mutation rates, when Muller's ratchet becomes important. Another effect at high mutation rates that is neglected in the theory (but was also absent from the simulations) is the evolution of mutational robustness: If the distribution of deleterious mutations itself can change, then at a high mutation rate there is a selective pressure to minimize the mutational load of the population (VAN NIMWEGEN et al. 1999; WILKE et al. 2001; WILKE and ADAMI 2003). This effect will increase the mean fitness of the population and will also increase the potential for further adaptation by increasing P0. In general, at a high mutation rate we have to consider that a mutation will be combined with additional mutations on the way to fixation. Therefore, we cannot simply assume that a mutation of beneficial effect s has probability of fixation 2s, but have to use fairly complicated mathematical tools (such as multitype branching processes) to calculate the fixation probability (BARTON 1995; JOHNSON and BARTON 2002; WILKE 2003; IWASA et al. 2004). As a consequence, it is unlikely that we will ever have a simple closed-form expression for the speed of adaptation at a high mutation rate.
A second regime in which the theorynot surprisinglybreaks down is when sb exceeds sd. In this regime, we cannot simply neglect all beneficial mutations that do not arise on genetic backgrounds free of deleterious mutations. JOHNSON and BARTON (2002) have recently studied this situation, but not in the clonal interference regime. In the clonal interference regime, there are two opposing effects to be considered: On the one hand, the total number of competing mutations should increase, since now beneficial mutations on deleterious backgrounds compete for fixation as well. On the other hand, the total fitness effect of many of the mutations that are competing for fixation is smaller than what we expect from the distribution of new beneficial mutations, because the beneficial effects are reduced by deleterious backgrounds. Without a detailed analysis, it is unclear which of the two effects is more important. However, if the results from the present study are an indication, in the clonal interference regime the number of competing mutations will be less important than the distribution of their beneficial effects, which means that the present theory should overestimate the rate of adaptation for sb > sd. Indeed, I observed exactly this behavior in my simulations (Figure 6).
Whether the assumption sb < sd is reasonable is not yet resolved. (Likely, the answer to this question will also depend on the particular species under study and on the concrete selection regime.) Several authors found that deleterious mutations were frequent but had a very small effect (MUKAI et al. 1972; OHNISHI 1977; KIBOTA and LYNCH 1996; SHABALINA and KONDRASHOV 1997; ELENA and MOYA 1999), while others found that deleterious mutations were less frequent but of larger effect (KEIGHTLEY 1996; FERNáNDEZ and LóPEZ-FANJUL 1996; GARCíA-DORADO 1997; KEIGHTLEY and CABALLERO 1997). If the first set of results is representative, then beneficial mutations may indeed have on average a larger effect on fitness than deleterious mutations. While it is reasonably straightforward to study the distribution of deleterious mutations in mutation-accumulation experiments, it is much harder to measure the distribution of new beneficial mutations (as opposed to the distribution of fixed beneficial mutations, which is skewed toward mutations of large effect). However, evidence from experimental evolution with viruses shows that in some cases, beneficial mutations must have very large effects: WICHMAN et al. (1999) found a several-thousand-fold increase in population growth after 10 days of selection in phage
X174, and NOVELLA et al. (1995) found fitness increases by a factor of 10 or more within 510 generations in vesicular stomatitis virus. In both cases, the observed fitness increase within a very short time frame can be explained only by a large supply of beneficial mutations of large effect.
To summarize, in this article I have found the following novel conclusions:
| APPENDIX A |
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![]() | (A1) |
Therefore, the shape of E[k] as a function of N or U is independent of the value of sb.
We are interested in an asymptotic expansion of the integral in Equation A1 for large N. For the asymptotic expansion to work, N needs to be so large that A is large. Clearly, for any given UpbP0, we can always choose N sufficiently large such that A is large. Because of the exponential factor in the integrand, the main contribution to the integral comes from values of x for which A(1 + 1/x)ex + x is small. Since the first term decays exponentially with x while the second term grows linearly, in general the main contribution to the integral will come from small x. However, for large A, the first term becomes small only when x is substantially larger than one. In this regime, we can neglect the term 1/x, and the integral in Equation A1 is then identical to the integral Jn(A) defined in APPENDIX B with n = 1. Using the expression for J1(A) given in Equation B4, we find
![]() | (A2) |
In the limit of very large N, we obtain the even simpler expression E[k]
sb.
Using a reasoning similar to that for the expected substitution rate, we find that the expected beneficial effect (as given in Equation 5) also depends linearly on sb and simplifies for large N to E[s] = sbJ2(A)/J1(A) (again with A = 2UpbP0N ln N). Using the expressions given in Equations B3 and B4, we find
![]() | (A3) |
In the limit of very large N, the second term disappears, and we end up with
![]() | (A4) |
Estimating the onset of clonal interference:
We can derive an estimate of the parameter region in which clonal interference becomes important by calculating the point at which the approximation for E[k] for small N (Equation 1) comes the closest to the approximation for E[k] for large N, Equation 3. Since the shape of E[k] is not influenced by sb (see above), we can set sb = 1 for this calculation. Further, we write C = 2UpbP0. Now, we have to find the minimum of the function
![]() | (A5) |
We find
g(C, N)/
C = N 1/(C ln N), which leads to the condition
![]() | (A6) |
| APPENDIX B: |
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![]() | (B1) |
![]() | (B2) |
The main contribution to the remaining integral comes from small z, while A is large in the cases considered here. Therefore, we can replace the upper limit of integration with
. For the three relevant cases k = 0, k = 1, and k = 2, the integrals are
,
,
, where
0.5772 is the Euler constant. Thus, we find approximately
![]() | (B3) |
![]() | (B4) |
| ACKNOWLEDGEMENTS |
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