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VOLUME 93, N UMBER 15 PHYSICA L R EVIEW LET T ERS week ending 8 OCTOBER 2004 Stabilization of Large Generalized Lotka-Volterra Foodwebs By Evolutionary Feedback G. J. Ackland* and I. D. Gallagher School of Physics, The University of Edinburgh, Mayfield Road, Edinburgh EH9 3JZ, United Kingdom (Received 25 June 2004; published 8 October 2004) Conventional ecological models show that complexity destabilizes foodwebs, suggesting that foodwebs should have neither large numbers of species nor a large number of interactions. However, in nature the opposite appears to be the case. Here we show that if the interactions between species are allowed to evolve within a generalized Lotka-Volterra model such stabilizing feedbacks and weak interactions emerge automatically. Moreover, we show that trophic levels also emerge spontaneously from the evolutionary approach, and the efficiency of the unperturbed ecosystem increases with time. The key to stability in large foodwebs appears to arise not from complexity per se but from evolution at the level of the ecosystem which favors stabilizing (negative) feedbacks. DOI: 10.1103/PhysRevLett.93.158701 Ecosystems are a classic example of complexity [1–7], being formed from a myriad of interactions between various species. The mathematical study of ecosystems has a long history, dating back to the work of Lotka and of Volterra [8,9]. Such models tread a delicate balance between including so much detail that they lose the capability to make qualitative predictions, and being so simple as to be wholly wrong. Striking features of ecosystems are their tendency to be arranged into a hierarchical structure with different trophic levels, their development of many complex interactions, and their chaotic population dynamics. In setting up a model, it is necessary to decide which of these observed qualities will be built into the model, and which (one hopes) will emerge from solving the model. For example, May’s early work based on random matrices did not assume trophic structure, but did assume the number of interactions and their distribution of strengths. These simple ecosystem models exhibit chaotic population dynamics and stability [2,3]. Further work by Pimm and co-workers [1,7,10,11] showed that webs with an imposed hierarchical trophic structure (i.e., the absence of ‘‘trophic cycles,’’ formally defined by loops in the directed graph) were more stable than random webs. However, large or highly connected model foodwebs tended towards instability in both models. Subsequently, investigation has been done on webs created by continuous introduction and extinction of species of preset trophic level and interactions, with success depending on population dynamics [12,13]. These foodwebs evolve [14] to contain large numbers of species and are persistent even though species are continually being introduced and going extinct. However, in all of these models increasing connectivity (the number of interactions per species) leads to instability. McCann et al. addressed this latter issue by investigating simple webs with weak interactions added based on studies of interaction strengths in real foodwebs [6]. This work showed that weak interactions act to dampen oscillations and stabilize highly connected systems. 158701-1 0031-9007=04=93(15)=158701(4)$22.50 PACS numbers: 87.23.Kg, 05.65.+b, 89.75.Hc It has been suggested [15] that nontrophic effects such as cooperation or competition may be required to stabilize large systems. These effects are undoubtedly important in real ecosystems, but here we show that large, stable, highly connected trophic foodwebs with chaotic dynamics and many weak interactions arise from a generalized Lotka-Volterra (GLV) model with evolution of the interaction strengths [16,17]. Such evolution may arise from various biological phenomena, including genetic and behavioral evolution, predator choice, and changes in the spatial overlap of populations [14]. The interaction strength represents the balance of power between the species. Species tend to evolve [14] more effective means of dealing with the other, but the interaction strengths, representing differences in effectiveness may increase or decrease. Interactions cannot, of course, change sign as the role of predator and prey cannot be reversed. We assume that the overall effect is that large populations of predators become less well adapted to capturing rare prey, since other food sources are available, while small populations of prey become better able to avoid their major predators. Thus we simulate coupled population and evolutionary dynamics, starting with a pool of species and eliminating any whose population drops below a minimum threshhold (extinction). Lotka-Volterra-type models [1] consider populations of species as their basic objects, modeling the interactions between the various populations. The Lotka-Volterra model [8,9] considers two species with populations x1 (prey/autotroph) and x2 (predator/heterotroph). x2 has a constant death rate c and per capita reproduction proportional to the amount of prey, effectiveness of predation (M), and birth efficiency (b). x1 has a per capita death rate due to predation by x2 and a regeneration rate constrained by environmental resources as described by the logistic map. This gives the following equations for two species: dx1 gx1 gx21 =K Mx2 x1 ; dt 2004 The American Physical Society (1) 158701-1 VOLUME 93, N UMBER 15 PHYSICA L R EVIEW LET T ERS dx2 Mbx1 cx2 : dt (2) This model can be readily generalized to N species: for autotrophs, with x0 setting the limit on the population and Mij always negative: X dxi xi x2i =x0 Mij xi xj (3) dt j for heterotrophs, which may predate on some species and be predated on by others so that Mij may be positive or negative: X dxi cxi Mij xi xj : (4) dt j We take death rate c 0:01 and draw the initial Mij randomly from a flat distribution between 0 and 1. Predation is not efficient, and following Lotka-Volterra we assume that for positive Mij , Mji bMij with a birth efficiency b, typically 0.1. This foodweb forms a directed graph where the species form nodes connected by interactions of strength Mij . We define the resource flow (Fig. 1) into the network as the sum of positive terms in Eqs. (3) and (4) and flow out as sum of negative terms. Ensemble averaged values of these quantities must balance in the steady state, but their absolute value is not determined. We also allow for evolution of the link strengths Mij themselves. The Mij represent the probability of predation between individuals of two species and its change therefore incorporates all genetic or behavioral changes which affect this probability. The driving force for change in Mij FIG. 1. Time series of the populations of typical species in a typical evolving foodweb. Autotrophs are shown by thick lines, heterotrophs by thin lines. Units of population (N) are arbitrary; time is related to the death rate of 0.01 for heterotrophs (i.e., 100 is a mean life-span). Both population dynamics and the dynamics of interaction strengths (not shown) are chaotic. The dynamics can be explored using an applet [18]. 158701-2 week ending 8 OCTOBER 2004 is proportional to the number and strength of interactions per individual of the species. Since Mij affects two species, its actual change is the difference in evolution of the two species: if both predator and prey are becoming better adapted at the same rate, no change in Mij occurs. dMij Ni Nj Mij ; dt (5) where sets the rate of change. We set an upper limit of 1 on the efficiency Mij —without this it is possible for species to evolve so as to exist on vanishingly small amounts of prey. In our calculations we iterate Eqs. (3) – (5) in time, eliminating any species for which Ni < 0. Preliminary calculations with constant interaction strengths showed that this strategy produces large, feasible, viable foodwebs, but that the complexity of the interaction network remains low, on average just one link per species, independent of web size. This is consistent with previous numerical work on evolved webs [12,13] and the exact result for random webs [1]. Hence, as with all previous models, selection by extinction of failing species does not reproduce the observed complexity. In our main calculations where the interactions evolve, we introduce one new parameter and eliminate two assumptions— neither the number of interactions per species nor the distribution of interaction strengths need be determined a priori—the system is able to evolve its interactions or make them so weak as to effectively remove them altogether. The model also does not preassign trophic levels to heterotrophs or (almost equivalently) preclude trophic cycles. We find that in our evolving-interaction model, when very weak interactions (less than 0.0001 of the maximum) are neglected, a cycle-free trophic structure with chaotic dynamics almost invariably emerges (Fig. 2). The emergent absence of effective trophic cycles (e.g., A eats B, B eats C, C eats A) is a particularly striking result — the random allocation of Mij to autotrophs means that such cycles are present initially, but the dynamics is always such as either to eliminate one of the species in the cycle or to make one of the Mij negligibly small (eliminating it is not possible in the model). Consideration of the flow of resource helps us to understand this: a trophic cycle would have a flow of resource around it, dissipated by b at each interaction, but cannot have any generation of resource. Moreover, the distribution of interaction strengths (Fig. 3) is a power law with an exponent of 1 (within error), independent of web size for large webs. This means that at any one time the predators are obtaining their resources both from a few strong interactions and from many weak interactions, which also serve to stabilize the web, particularly by becoming stronger in times of declining population. 158701-2 VOLUME 93, N UMBER 15 week ending 8 OCTOBER 2004 PHYSICA L R EVIEW LET T ERS The behavior of our foodwebs can be monitored by the flow of resources through the system over time [1]. We monitored this during our simulations and found a remarkable result —the total flow of resource (and hence total biomass) increases with time reaching a plateau after many thousands of steps —the steady-state linkstrength ensemble distribution appears to be the one which maximizes the use of resource. This type of optimization is consistent with what has been observed in other ecological models [19,20]. If the model is recast in terms of flow and dissipation, the maximization principle is equivalent to maximum entropy production [21]: the mathematical equivalent of ‘‘entropy production’’ is just the total death rate, and hence the flow out. Unfortunately, as with many systems described by maximum entropy, it is not possible to determine analytically what the maximum flow actually is, and the principle can only be inferred by the increase with time as the steady state is approached. Most results described here are robust against changing initial conditions, varying b and c, or making them species dependent. However, the power-law distribution of link strengths depends on the existence of chaotic population dynamics, which in general arises from either finite time step or a sharp upper limit on Mij . The switch from a power law to an exponential distribution is also understandable in terms of the central limit theorem —in both cases the distribution of average values for individual populations over time is distributed normally—in the fixed point case this is also the instantaneous average. The presence of instantaneous power-law distributions is consistent with the maximum entropy production [21]. If we take an alternate evolution of the interactions for which Mij is self-limiting, replacing Eq. (5) with the more complex form and use an infinitesimal time step, then the dynamics tend to one of many fixed points rather than the chaotic state. Trophic level structure and high numbers of weak interactions still occur in this model, but curiously, the evolved link strengths are now exponential rather than power-law distributed. Eliminating the maximum allowed value of Mij has a similar mathematical effect, although it makes little biological sense to allow a predator to extract unlimited resource from a given prey. The switch between chaotic and steady behavior when going from discrete to continuous dynamics could be anticipated, being typical of many systems, including the logistic map. It is possible to construct different, more complex, models with alternative relations between Mij and Mji reflecting mutualism (both positive) or competition (both negative); however, these are not essential to stability. For example, Kondoh [17] recently considered restricting the evolution to the predator only, essentially replacing Eq. (5) with dMij =dt Nj Mij (7) for Mij > 0. In this model the feedback also stabilized realistic highly connected webs. Generalized Lotka-Volterra models are widely used in economics as well as in ecology, and it is worth noting that the fixed point of our system does not represent a Nash equilibrium. Mij contains both evolution of the predator to catch its prey and that of the prey to avoid its predator. The fixed point means that each species is becoming better adapted to combat the other at the same rate: the so-called ‘‘red queen’’ effect. 8 dMij =dt 1=Ni dNi =dt 1=Nj dNj =dtMij (6) 6 log(Number of Links) Population [log] 10 1 0.1 0.01 4 2 0 0.001 0 2000 4000 6000 8000 Time 10000 12000 14000 FIG. 2 (color online). Graph of total population as a function of time for a typical evolving web with 100 species, and flow of resources in and out of the web (see the text for definition). The graph of inward flow in broadened for clarity: it lies close to (and leads) the outward flow throughout. 158701-3 −2 −7 −6 −5 −4 −3 −2 −1 0 log(link strength) FIG. 3. Plot of the (log) number of links against their (log) strength. The histogram is averaged over many snapshots from many stable webs of size 100 species. In each stable web the link strength varies with time —the interaction strengths are instantaneous, not time-averaged values. 158701-3 VOLUME 93, N UMBER 15 PHYSICA L R EVIEW LET T ERS In sum, we have shown that simply by allowing the strength of interactions to evolve in a GLV model, several features of observed foodwebs emerge spontaneously. These include chaotic dynamics, maximal use of resources, stability engendered by many weak links, and the absence of trophic cycles. While previous models have shown some of these phenomena, in general one or more have been be assumed in the formulation of the models. This work uses a minimal number of assumptions to show the powerful effect of evolution in structuring the foodweb patterns of nature, focusing the system onto stable states via a feedback process. *Electronic address: [email protected] [1] S. L. Pimm, Food Webs (Chapman and Hall, London, 1982) (republished by University of Chicago Press, Chicago, 2002). [2] R. M. May, Stability and Complexity in Model Ecosystems (Princeton University Press, Princeton, 1974). [3] R. M. May, Ecology 54, No. 3, 638 (1973). [4] R. M. May, Nature (London) 238, 413 (1972). [5] X. Chen and J. E. Cohen, Proc. R. Soc. London B 286, 869 (2001). [6] K. McCann, A. Hastings, and G. R. Huxel, Nature (London) 395, 794 (1998). [7] S. L. Pimm, Nature (London) 307, 321 (1984). 158701-4 week ending 8 OCTOBER 2004 [8] A. J. Lotka, Elements of Mathematical Biology (Williams and Wilkins, Baltimore, 1925) [republished as Elements of Mathematical Biology (Dover, New York, 1956)]. [9] V. 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