Abstract
Power laws are cornerstone relationships in ecology and evolutionary biology. The density-mass allometry (DMA), which predicts an allometric scaling of population abundance, and Taylor’s law (TL), which predicts a decrease in the population abundance variation along with a decrease in population density, have enhanced our knowledge of inter- and intra-specific variation in population abundance. When combined, these two power laws led to the variance-mass allometry (VMA), which states that larger species have lower spatial variation in population density than smaller species. The VMA has been predicted through theoretical models, however few studies have investigated if this law is also supported by empirical data. Here, to formally test the VMA, we have used the population density estimates obtained through worldwide camera trapping studies for an emblematic and ecologically important carnivorous taxa, the Felidae family. Our results showed that the VMA law hold in felids, as well as the TL and the DMA laws; bigger cat species showed less variation for the population density than smaller species. These results have important implications for the conservation of wildlife population and confirm the validity of important ecological concepts, like the allometric scaling of population growth rate and the slow-fast continuum of life history strategies.
Highlights
Power laws are cornerstone relationships in ecology and evolutionary biology
Based on an exhaustive review of population density estimates over multiple study sites from camera-trap studies on felids worldwide, we demonstrated that the spatial variance-mass allometry (VMA) was supported for Felidae, and variation in population density decreases with increasing body mass
The VMA was already found for another population parameter across mammalian species as Sinclair[61] reported an inverse allometric relationship between the standard deviation of the maximum population growth rate and body mass
Summary
Power laws are cornerstone relationships in ecology and evolutionary biology. The density-mass allometry (DMA), which predicts an allometric scaling of population abundance, and Taylor’s law (TL), which predicts a decrease in the population abundance variation along with a decrease in population density, have enhanced our knowledge of inter- and intra-specific variation in population abundance. Power laws have greatly contributed to our understanding of the large-scale variations of population abundance[3,4,5] or of variation of metabolism across the body mass continuum in animals and p lants[6,7,8] In this context, one of the first power law ascertained in ecology is the Taylor’s law (hereafter, TL), which positively links the variance in population density to the mean density of populations[3,9] with the following equation: VarDi = a · (MeanDi)b, with a > 0, and, 1 ≤ b ≤ 2 in numerous empirical examples where Di is the population density in study site i. The VMA scaling exponent has been theoretically predicted by combining the TL scaling exponent (∼ 2) and the DMA exponent (∼ − 0.75), giving an exponent for the VMA of ∼ − 3/21,34
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