Integrating coevolution into the tree of life 0 ๐๐ ๐๐ ๐๐ Scott L. Nuismer What is coevolution? Species 1 Species 2 Coevolution: Reciprocal evolutionary change in interacting species (Janzen, 1980) "Thus I can understand how a flower and a bee might slowly become, either simultaneously or one after the other, modified and adapted to each other in the most perfect manner, by the continued preservation of all the individuals which presented slight deviations of structure mutually favourable to each other." โ Charles Darwin, The Origin of Species The importance of coevolution Much of what we know about coevolution comes from mathematical models A key assumption of coevolutionary theory A key assumption of comparative methods The current state of affairs Coevolutionary theory ignores phylogeny Phylogenetic comparative methods ignore coevolution This raises two important questions Question 1: Do coevolution and phylogeny interact to shape contemporary trait values? Question 2: Can we predict contemporary rates of interaction? Our goal is to use a mathematical model to answer these questions Merging coevolution and evolutionary history Species 1 Species 2 + A general modeling approach First time interval Second time interval Third time interval (no coevolution) (2-way coevolution) (3-way coevolution) Our approach will be agnostic with respect to the process of speciation How do traits mediate interactions? Model 1: Phenotype Differences ๐๐๐ = 1 1 + ๐ธ๐ฅ๐[๐ผ ๐ง๐ โ ๐ง๐ ] How do traits mediate interactions ๐๐๐ ๐ง๐ ๐ง๐ Best suited for interactions that depend on interference competition How do traits mediate interactions? Model 2: Phenotype Matching 2 ๐๐,๐ = ๐ธ๐ฅ๐[โ๐ผ ๐ง๐ โ ๐ง๐ ] How do traits mediate interactions ๐๐,๐ ๐ง๐ ๐ง๐ Best suited for interactions that depend on exploitation of shared resources Predicting trait coevolution Individual fitness ๐ ๐๐ = 1 โ ๐ ๐ ๐๐ ๐๐๐ ๐=1 Random encounters among individuals Gaussian trait distributions Classical quantitative genetics โ๐ ๐ = ๐ฎ ๐ ๐ ๐๐พ๐ + ๐บ๐ ๐พ๐ ๐๐๐ Coevolutionary dynamics on a star phylogeny Phenotype differences Phenotype matching ๐ โ๐ง๐ โ ๐บ๐ ๐ ๐๐ ๐๐ + ๐๐ ๐=1 How do traits mediate interactions โ๐ง๐ โ ๐บ๐ ๐๐ ๐๐ ๐ง๐ โ ๐ง๐ + ๐๐ ๐=1 How do traits evolve? Integrating evolutionary history: Phenotype differences ๐๐๐ = 1 1 + ๐ธ๐ฅ๐[๐ผ ๐ง๐ โ ๐ง๐ ] How do traits mediate interactions ๐๐๐ ๐ง๐ ๐ง๐ Best suited for interactions that depend on interference competition Integrating evolutionary history First interval: After speciation Before speciation ๐1,๐1 = ๐1,0 2 ๐1,๐ 1 = ๐บ ๐ ๐1 ๐1,๐1 = ๐1,0 ๐2,๐1 = ๐1,0 2 ๐1,๐ = ๐บ ๐ ๐1 1 2 ๐2,๐ = ๐บ ๐ ๐1 1 ๐12,๐1 = ๐บ ๐ ๐1 0 ๐๐ Integrating evolutionary history After speciation Second interval: ๐1,๐2 = ๐1,0 + ๐บ๐ ๐2 โ ๐1 Before speciation ๐2,๐2 = ๐1,0 + ๐บ๐ ๐2 โ ๐1 ๐1,๐2 = ๐1,0 + ๐บ๐ ๐2 โ ๐1 ๐3,๐2 = ๐1,0 + ๐บ๐ ๐2 โ ๐1 ๐2,๐2 = ๐1,0 + ๐บ๐ ๐2 โ ๐1 2 ๐1,๐ = ๐บ ๐ ๐2 2 2 ๐1,๐ = ๐บ ๐ ๐2 2 2 ๐2,๐ = ๐บ ๐ ๐2 2 2 ๐2,๐ = ๐บ ๐ ๐2 2 ๐12,๐2 = ๐บ ๐ ๐1 2 ๐3,๐ = ๐บ ๐ ๐2 2 ๐12,๐2 = ๐บ ๐ ๐1 ๐13,๐2 = ๐บ ๐ ๐2 ๐23,๐2 = ๐บ ๐ ๐1 0 ๐๐ ๐๐ Integrating evolutionary history Third interval: ๐1,๐2 = ๐1,0 + ๐บ๐ ๐3 โ ๐1 ๐2,๐2 = ๐1,0 + ๐บ๐ ๐3 โ ๐1 ๐3,๐2 = ๐1,0 + ๐บ๐ ๐3 โ ๐1 2 ๐1,๐ = ๐บ ๐ ๐3 2 2 ๐2,๐ = ๐บ ๐ ๐3 2 2 ๐3,๐ = ๐บ ๐ ๐3 2 ๐12,๐2 = ๐บ ๐ ๐1 ๐13,๐2 = ๐บ ๐ ๐2 0 ๐๐ ๐๐ ๐๐ ๐23,๐2 = ๐บ ๐ ๐1 This result can be easily generalized for any phylogeny โฏ Coevolution and phylogeny do not interact Phylogeny explains phenotypic similarity Coevolution explains expected trait values Contemporary interactions can be predicted Expected outcome? Expected asymmetry? 1 ๐๐๐ โ 2 ๐ผ2 ๐บ ๐ดโ ๐ โ ๐๐๐ 2 ๐ ๐ How do traits mediate interactions How do traits evolve? Integrating evolutionary history: Phenotype matching 2 ๐๐,๐ = ๐ธ๐ฅ๐[โ๐ผ ๐ง๐ โ ๐ง๐ ] How do traits mediate interactions ๐๐,๐ ๐ง๐ ๐ง๐ Best suited for interactions that depend on exploitation of shared resources Integrating evolutionary history First interval: After speciation Before speciation ๐1,๐1 = ๐1,0 2 ๐1,๐ 1 = ๐บ ๐ ๐1 ๐1,๐1 = ๐1,0 ๐2,๐1 = ๐1,0 2 ๐1,๐ = ๐บ ๐ ๐1 1 2 ๐2,๐ = ๐บ ๐ ๐1 1 ๐12,๐1 = ๐บ ๐ ๐1 0 ๐๐ Integrating evolutionary history After speciation Second interval: ๐1,๐2 = ๐1,0 Before speciation ๐1,๐2 = ๐1,0 2 ๐2,๐ = 2 ๐บ โ1 + ๐ 4๐ ๐2 โ๐1 + 4๐ ๐1 + ๐2 8๐๐ ๐บ โ1 + ๐ 4๐ ๐12,๐2 = ๐3,๐2 = ๐1,0 2 ๐1,๐ 2 ๐2,๐2 = ๐1,0 2 ๐1,๐ = 2 ๐2,๐2 = ๐1,0 ๐2 โ๐1 + 4๐ ๐1 + ๐2 = 2 ๐2,๐ = 2 2 ๐3,๐ = 2 ๐บ โ1 + ๐ 4๐ ๐บ 1โ๐ + 4๐ ๐1 + ๐2 8๐๐ ๐บ โ1 + ๐ ๐บ โ1 + ๐ 4๐ ๐2 โ๐1 ๐๐ ๐๐ + 4๐ ๐1 + ๐2 8๐๐ ๐12,๐2 = ๐13,๐2 = ๐23,๐2 = 0 + 4๐ ๐1 + ๐2 8๐๐ 4๐ ๐2 โ๐1 8๐๐ 4๐ ๐2 โ๐1 ๐2 โ๐1 ๐บ 1โ๐ + 4๐ ๐1 + ๐2 8๐๐ + 4๐ ๐1 + ๐2 4๐ ๐2 โ๐1 8๐๐ + 4๐ ๐1 + ๐2 ๐บ 1โ๐ 4๐ ๐2 โ๐1 ๐บ 1โ๐ 4๐ ๐2 โ๐1 8๐๐ + 4๐ ๐1 + ๐2 8๐๐ Integrating evolutionary history Third interval: ๐1,๐3 = ๐1,0 ๐2,๐3 = ๐1,0 ๐3,๐3 = ๐1,0 3 2 ๐1,๐ 3 1 ๐บ(โ17 + ๐ 4๐(๐2 โ๐1 ) โ 4๐ 2๐(๐3 โ๐2 ) + 12๐ 3๐(๐3 โ๐2 ) + 4๐ ๐(๐2 +3๐3 โ4๐1 ) + 4๐ 2๐(5๐2 +3๐3 โ8๐1 ) + 12๐(3๐1 + ๐2 + 2๐3 )) = 72๐๐ 2 ๐2,๐ = 3 ๐บ(โ17 + ๐ 4๐ ๐2 โ๐1 3 โ 8๐ 2๐ ๐3 โ๐2 1 + 16๐ ๐ ๐2 +3๐3 โ4๐1 โ 8๐ 2๐(5๐2 +3๐3 โ8๐1 ) + 12๐(3๐1 + ๐2 + 2๐3 )) 72๐๐ 3 2 ๐3,๐ 3 ๐12,๐3 = ๐13,๐2 = ๐23,๐3 = 0 ๐๐ ๐๐ 1 ๐บ(โ17 + ๐ 4๐(๐2 โ๐1 ) โ 4๐ 2๐(๐3 โ๐2 ) + 12๐ 3๐(๐3 โ๐2 ) + 4๐ ๐(๐2 +3๐3 โ4๐1 ) + 4๐ 2๐(5๐2 +3๐3 โ8๐1 ) + 12๐(3๐1 + ๐2 + 2๐3)) = 72๐๐ 3 ๐บ(7 + ๐ 4๐ ๐2 โ๐1 + 2๐ 2๐ ๐บ(7 + ๐ 4๐ ๐2 โ๐1 โ 4๐ 2๐ ๐บ(7 + ๐ 4๐ ๐2 โ๐1 + 2๐ 2๐ 3 3 1 ๐3 โ๐2 โ 8๐ ๐ โ 2๐ 2๐(5๐2 +3๐3 โ8๐1 ) + 12๐(3๐1 + ๐2 + 2๐3 )) 72๐๐ ๐3 โ๐2 โ 12๐ 3๐(๐3 โ๐2 ) + 4๐ ๐(๐2 +3๐3 โ4๐1 ) + 4๐ 2๐(5๐2 +3๐3 โ8๐1 ) + 12๐(3๐1 + ๐2 + 2๐3 )) 72๐๐ ๐3 โ๐2 โ 8๐ ๐ ๐2 +3๐3 โ4๐1 1 1 โ 2๐ 2๐(5๐2 +3๐3 โ8๐1 ) + 12๐(3๐1 + ๐2 + 2๐3 )) 72๐๐ ๐2 +3๐3 โ4๐1 ๐๐ Unfortunately, this result cannot easily be generalized Coevolution and phylogeny interact Phylogeny creates a template of phenotypic similarity And coevolution modifies this template Contemporary interactions can be predicted Expected intensity of competition (without coevolution) Expected intensity of competition (with coevolution) If we also have information about the historical strength of coevolution Conclusion 1: Coevolution leaves a signature Conclusion 2: Interactions can be predicted We can predict asymmetries How do traits evolve? We can predict intensity Acknowledgements Funding National Science Foundation Luke Harmon
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