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Density dependence

Density dependence refers to the process in whereby the growth rate of a varies as a function of its , often through interactions that regulate and prevent unbounded growth. This phenomenon typically manifests as negative density dependence, where increasing leads to reduced individual via intensified for resources, heightened predation risk, or elevated transmission, thereby stabilizing populations around a . In contrast, positive density dependence, also known as the , occurs at low densities when individual improves with rising numbers, such as through facilitated mate finding or cooperative behaviors that enhance survival. Key mechanisms of negative density dependence include for limited resources like and , which dilutes nutritional quality and slows growth rates even when remains available, as observed in large populations. Predation and also intensify with density, as higher concentrations of prey or hosts make them easier targets, while waste accumulation from dense groups can degrade local environments and increase mortality. For positive density dependence, component Allee effects arise from specific fitness correlates, such as reduced predation through group defense in species like fish or improved efficiency in at higher densities. Empirical examples illustrate these dynamics across taxa; in Adélie penguins (Pygoscelis adeliae), limited breeding habitat imposes density-dependent constraints on growth rates, forcing colonies to occupy steeper slopes and altering occupancy patterns in . Similarly, in parasitic worms like , higher host densities correlate with reduced egg production per individual, demonstrating fecundity regulation. Allee effects are evident in declining populations, where low densities exacerbate mating challenges and elevate extinction risk. Density dependence is central to models of , such as the logistic growth equation, which incorporates a density-dependent term to predict stabilization rather than exponential increase. It underpins understanding of , invasion biology, and conservation, as ignoring it can mispredict range expansions or collapse thresholds, particularly in fragmented habitats where Allee effects amplify vulnerability. Ongoing research emphasizes its role in multispecies interactions and responses to , highlighting the need for density-explicit frameworks in predictive ecology.

Fundamentals

Definition and Historical Context

Density dependence refers to the phenomenon in where the per capita growth rate of a population varies as a function of its density, such that changes in population size influence vital rates like birth, , or dispersal. This contrasts with density-independent factors, which impact absolute rates uniformly across densities, such as weather events or that affect individuals regardless of how crowded the population is. The concept underscores how interactions can regulate populations by creating , where growth accelerates at low densities and slows at high ones. The intellectual roots of density dependence trace back to Thomas Malthus's 1798 essay, which posited exponential limited by arithmetic increases in resources, implying inherent checks on unchecked expansion. In the early , this evolved into more formalized ecological models; Raymond Pearl and Lowell Reed introduced the logistic growth equation in 1920, using U.S. census data to describe S-shaped population trajectories where growth rates decline with increasing density due to resource limitations. Pearl's work marked a shift from purely Malthusian exponential models to ones incorporating density-mediated constraints, influencing subsequent ecological theory. By the 1930s, A.J. Nicholson advanced these ideas in his seminal 1933 paper "The Balance of Animal Populations," arguing that animal populations achieve through and biotic factors like predation, which intensify with density to maintain balance rather than climate alone driving fluctuations. Nicholson emphasized density-dependent regulation in insect populations, proposing that competition curves ensure populations oscillate around an equilibrium density. The term "density dependence" itself was coined shortly after by Harry S. Smith in 1935, who distinguished biotic factors (density-dependent) from abiotic ones (density-independent) in controlling population densities, particularly in entomological contexts. This framework solidified density dependence as a cornerstone of , bridging theoretical models with empirical observations.

Role in Population Dynamics

Density dependence is fundamental to population regulation, primarily by modulating growth rates in relation to . Negative density dependence typically reduces these rates as populations approach or exceed limits, creating a feedback mechanism that stabilizes growth and prevents overexploitation of the , ultimately capping populations at a where net growth approaches zero. This process ensures long-term persistence by balancing demographic rates against ecological constraints. Conversely, at low densities, positive density dependence can elevate growth rates, often by facilitating processes like location or group defense that become more efficient as numbers increase slightly from near-extinction levels. Such enhancement supports and contrasts with the regulatory role at higher densities. In terms of stability, density dependence generally promotes equilibrium in , fostering bounded fluctuations around and serving as a key distinction from density-independent , which lacks such self-limitation. However, delayed density dependence—where effects manifest over multiple time steps—can introduce destabilizing forces, leading to oscillatory or cyclic patterns rather than steady states. To detect density dependence empirically, researchers commonly use time-series data to examine relationships between and . A standard approach involves regressing the rate, expressed as \log\left(\frac{N_{t+1}}{N_t}\right), against the logarithm of current , \log(N_t); a significantly negative indicates density-dependent , as it demonstrates declining with rising . This graphical and statistical method has proven effective across diverse taxa, revealing the prevalence of such feedbacks in natural populations.

Types

Positive Density Dependence

Positive density dependence occurs when the per capita growth rate of a population increases as density rises, typically up to a threshold beyond which other factors may dominate. This contrasts with the more commonly observed negative density dependence, where growth rates decline at higher densities. In ecological contexts, positive density dependence often arises from cooperative behaviors or mutual benefits that enhance individual fitness in groups, such as improved resource acquisition or reduced predation risk. A key manifestation of positive density dependence is the Allee effect, defined as a positive association between average individual fitness and either population density or size over some interval of density or size. Allee effects can be classified as strong or weak: strong Allee effects feature a critical threshold population size below which the per capita growth rate is negative, increasing extinction risk, whereas weak Allee effects show positive density dependence without such a threshold, merely elevating growth rates at higher densities. Additionally, Allee effects are distinguished as component or demographic; component Allee effects involve positive correlations with specific fitness components like survival or fecundity, while demographic Allee effects occur when these components translate to a positive relationship between per capita population growth rate and density. These distinctions, formalized in seminal work, highlight how positive density dependence can destabilize small populations through mechanisms like mate limitation or cooperative defense. Examples of positive density dependence abound in species reliant on social interactions. In greater prairie chickens (Tympanuchus cupido pinnatus), low population densities hinder mate finding at leks, reducing fertilization rates and exemplifying a strong component on ; translocations to bolster numbers have reversed declines by facilitating encounters. In fish larvae, like those of (Gadus morhua), at higher densities accelerates growth of surviving individuals, reducing their vulnerability to external predators and inducing a demographic by boosting overall cohort survival rates.

Negative Density Dependence

Negative density dependence occurs when the per capita growth rate of a population declines as density increases, promoting self-limitation and preventing expansion. This process arises primarily from intraspecific interactions that intensify with crowding, such as for essential resources or , ultimately capping population size at levels sustainable by the . In ecological terms, it represents a key regulatory mechanism that balances birth and death rates against available . Negative density dependence manifests in two main forms: direct and indirect. Direct forms involve active interference among individuals, where physical or behavioral confrontations limit to resources, such as through aggressive exclusion from optimal patches. Indirect forms stem from exploitative , where increased depletes shared resources like or nutrients, reducing availability for all without direct conflict. Within these, can be classified as or . features equal but diluted resource partitioning among all individuals, often leading to uniform declines across the . In contrast, allows dominant individuals to monopolize resources, leaving subordinates with minimal shares and exacerbating inequality in survival and reproduction. A prominent example of direct negative density dependence is observed in song sparrows (Melospiza melodia) on Mandarte Island, , where territorial behavior regulates population size. As densities rise, males defend smaller territories through increased aggression, reducing per capita food access and nesting success, which in turn lowers recruitment rates and stabilizes the population. This contest-like highlights how behavioral interference enforces density limits in avian systems. In microbial systems, indirect negative density dependence is exemplified by nutrient exhaustion in closed batch cultures of yeast (Saccharomyces cerevisiae). During exponential growth, cells rapidly consume available sugars, but as density approaches the nutrient threshold—typically around 10^8 cells per milliliter—per capita division rates plummet due to resource scarcity, transitioning the population into a stationary phase. This scramble-type process underscores exploitative limits in unicellular organisms, mirroring broader patterns in resource-constrained environments.

Mechanisms

Resource Competition and Interference

Resource competition represents a primary intraspecific mechanism underlying negative density dependence, wherein individuals of the same species contend for limiting resources like , water, or , resulting in diminished growth, survival, or reproduction as rises. This process intensifies with increasing density because resource supply remains fixed while demand escalates, leading to a feedback that stabilizes populations below . Resource competition manifests in two distinct forms: exploitative and . Exploitative competition arises indirectly through the shared depletion of resources, where higher densities accelerate resource exhaustion without direct contact between competitors. For instance, in populations feeding on sap, elevated densities cause rapid host plant depletion, reducing nymphal rates and by up to 50% at high infestation levels. competition, conversely, involves direct antagonistic behaviors such as , territorial , or physical exclusion, which escalate in frequency and intensity as increases due to more frequent encounters. In ( elaphus), rutting males exhibit heightened fighting and displacement as population increases, incurring elevated injury risks and energetic costs that lower . Intraspecific contexts amplify these effects because all competitors share identical requirements and cannot niches as in interspecific scenarios, making a direct driver of strength. As rises, the probability of resource overlap or confrontations grows nonlinearly, often shifting from dominance at low densities to prevalence at high ones. This amplification manifests in reduced individual metrics, such as body condition or offspring production, which collectively impose stronger regulatory pressure on . Mathematical representations of intraspecific resource competition adapt the Lotka-Volterra competition framework by setting interspecific coefficients to zero and focusing on self-limitation, yielding the logistic model: \frac{dN}{dt} = rN \left(1 - \frac{N}{K}\right) Here, r denotes intrinsic growth rate, N is , and K is ; the term \left(1 - \frac{N}{K}\right) quantifies density-dependent inhibition from , where the competition coefficient \alpha_{ii} (implicitly 1) reflects equivalent impact on conspecifics. This formulation captures how resource scarcity at high N curtails growth, with empirical validations showing close fits to observed trajectories in controlled populations. Empirical studies in plant systems provide robust evidence for these dynamics through self-thinning laws, which describe density-dependent mortality in crowded stands where competition for light, water, and nutrients enforces an upper biomass-density boundary. In even-aged forests like those of Pinus sylvestris, self-thinning follows the power-law relation N \cdot M^{3/2} = c (where M is average individual biomass and c is a constant), with densities declining from over 10,000 stems/ha at early stages to below 1,000/ha as trees mature, directly linking competition intensity to yield regulation. Such patterns underscore how intraspecific resource competition maintains stand structure and productivity across diverse taxa.

Predation, Disease, and Allee Effects

Predation represents a key extrinsic mechanism of density dependence in , where the rate at which predators consume prey often varies nonlinearly with prey density. This relationship is captured by the , which describes how an individual predator's consumption rate changes as prey abundance increases. A classic example is the Holling Type II functional response, in which the per-predator consumption rate rises asymptotically with prey density due to and handling times, leading to density-dependent as per-prey mortality decreases at higher densities while remaining elevated at low ones to prevent rapid . In the Royale - system, long-term observations have demonstrated this Type II response, where wolf kill rates on moose exhibit satiation effects that contribute to population without driving prey to . Disease provides another biotic mechanism through which density influences , primarily via increased contact rates among hosts at higher densities. In mass-action models of disease spread, the force of infection is proportional to the product of susceptible and infected host densities, assuming encounters occur at a rate scaled by overall ; this results in higher per capita infection probabilities as host numbers rise. The foundational SIR (Susceptible-Infectious-Recovered) model illustrates this density dependence, where the term \beta S I (with \beta as the ) drives epidemics more rapidly in dense populations, as evidenced by wildlife time-series data showing transmission scaling linearly with host density for directly transmitted pathogens like in foxes. Such dynamics underscore how pathogens can act as stabilizing forces in population regulation, particularly in species with limited mobility or territorial behaviors. Allee effects introduce positive density dependence through extrinsic factors, where individual fitness declines at low population densities due to heightened vulnerability to biotic threats. In predation contexts, grouping behaviors enable dilution effects, reducing the per capita risk of attack by spreading predator attention across multiple targets; for instance, in schooling fish like clupeids, larger schools dilute the probability of any single being captured, as predators select prey at random within the group, thereby enhancing survival rates at higher densities. This extrinsic Allee effect manifests as a component-level benefit in per capita mortality, contributing to overall in . Similarly, cooperative group living can foster positive density dependence in disease resistance, as seen in social mammals where collective grooming and vigilance reduce parasite loads and infection risks more effectively in larger groups, amplifying through shared defensive behaviors.00069-6)

Mathematical Models

Discrete-Time Models

Discrete-time models describe density-dependent population growth over distinct time intervals, such as annual breeding cycles or non-overlapping generations, using difference equations of the form N_{t+1} = f(N_t), where N_t is the at time t and f incorporates density dependence to at high densities. These models are particularly useful for with synchronized reproduction, like many or , and can exhibit including oscillations and , unlike smoother continuous-time approximations. The Ricker model, introduced in the context of fish stock-recruitment relationships, is given by N_{t+1} = N_t \exp\left(r \left(1 - \frac{N_t}{K}\right)\right), where r > 0 is the intrinsic growth rate and K > 0 is the carrying capacity. This formulation arises from assuming that per capita growth declines exponentially with density due to factors like competition or predation, leading to an overcompensatory response where recruitment drops sharply beyond K. For low r (typically r < 2), the equilibrium at N = K is stable, with populations converging monotonically or via damped oscillations. As r increases beyond approximately 2, the equilibrium becomes unstable through a period-doubling bifurcation, giving rise to stable 2-cycles, then 4-cycles, and eventually chaos for r > 2.57, where population trajectories become unpredictable and sensitive to initial conditions. These chaotic dynamics highlight how discrete-time models can produce irregular fluctuations even in single-species systems, a phenomenon observed in some empirical time series of population abundances. In contrast, the Beverton-Holt model assumes a compensatory but non-overcompensatory form of density dependence, expressed as N_{t+1} = \frac{r N_t}{1 + (r-1) \frac{N_t}{K}}, where r > 1 is the maximum reproductive rate and K is the carrying capacity. Derived for exploited fish populations, this model reflects scenarios where density dependence acts additively on survival or fecundity, resulting in a smooth approach to the asymptote at K without overshooting. The equilibrium N = K is globally asymptotically stable for all parameter values, ensuring convergence to the carrying capacity regardless of initial population size (above zero), which makes it suitable for modeling sustainable fisheries yields. This stability stems from the model's monotonic increasing and concave-down shape, preventing cycles or chaos. Both models can be derived from per capita growth rates that decline with density. In general, if the per capita rate is \lambda(N_t) = \frac{N_{t+1}}{N_t} = g(1 - \frac{N_t}{K}) for some decreasing function g, then N_{t+1} = N_t g(1 - \frac{N_t}{K}). For the Ricker model, g(x) = e^{r x}, yielding exponential decline in per capita recruitment at high densities. For Beverton-Holt, a hyperbolic form g(x) = \frac{r}{1 + (r-1)x} is used, representing saturation of resources or space. These derivations emphasize how the shape of the per capita function determines dynamic behavior: overcompensatory (like exponential) leads to potential instability, while undercompensatory (hyperbolic) promotes stability. Bifurcation analysis in these models reveals transitions in stability as parameters vary. In the Ricker model, plotting equilibria or cycles against r shows a cascade of period-doubling leading to , with the onset quantified by the Feigenbaum \delta \approx 4.669, universal across similar maps. The Beverton-Holt model lacks such , maintaining a single stable equilibrium, but extensions like the sigmoid Beverton-Holt can introduce multiple equilibria or Allee effects under certain conditions. These analyses underscore the sensitivity of discrete-time dynamics to the form of density dependence, informing predictions of population cycles in empirical data.

Continuous-Time Models

Continuous-time models of density dependence describe population growth using ordinary differential equations, which assume overlapping generations and continuous time, making them suitable for species with frequent reproduction events. These models capture how per capita growth rates decline as population density increases, leading to an equilibrium carrying capacity. The foundational example is the logistic equation, originally proposed by Pierre-François Verhulst in 1838 to model self-limiting population growth. The logistic equation is given by \frac{dN}{dt} = r N \left(1 - \frac{N}{K}\right), where N(t) is at time t, r > 0 is the intrinsic rate, and K is the . This can be derived by assuming density-dependent birth and death rates: the birth rate decreases linearly with density as b(N) = b_0 (1 - N/K), while the per capita death rate is constant at d, yielding r = b_0 - d and net dN/dt = [b(N) - d] N. The explicit solution is N(t) = \frac{K}{1 + \left(\frac{K}{N_0} - 1\right) e^{-rt}}, where N_0 = N(0) is the initial population size; populations approach K asymptotically from below if N_0 < K or from above if N_0 > K. The equilibrium at N = K is stable for r > 0, as small perturbations decay exponentially toward it, while N = 0 is unstable. A key limitation of the logistic model is its assumption of constant r, which implies symmetric density dependence in birth and death rates and may not reflect varying environmental or demographic responses. To address this, the theta-logistic model generalizes the form to \frac{dN}{dt} = r N \left(1 - \left(\frac{N}{K}\right)^\theta \right), where \theta > 0 modulates the strength and shape of density dependence: \theta = 1 recovers the logistic, \theta < 1 yields a sigmoidal growth curve with slower initial decline, and \theta > 1 accelerates it near K. Introduced by Gilpin and Ayala in 1973, this extension better fits empirical data where density effects are nonlinear, such as in laboratory Drosophila populations.

Applications

Population Regulation and Stability

Density dependence serves as a primary mechanism for population regulation in ecological systems, exerting that maintains equilibria by curbing at high densities and facilitating at low densities. This regulatory effect bounds population fluctuations, reducing the risk of unbounded expansion or in variable environments. Compensatory density dependence, the dominant form observed in natural populations, manifests when per capita growth rates decline as density increases, often through heightened mortality, reduced , or slowed development that collectively stabilize population sizes. In contrast, depensatory density dependence—where per capita rates rise with density—can amplify fluctuations and promote instability, though it is less prevalent. These compensatory processes ensure that populations self-regulate around carrying capacities, with mortality or reproductive rates adjusting inversely to density changes. Stability in density-dependent populations is analyzed through local and global criteria in mathematical frameworks. Local stability is determined by the eigenvalues of the Jacobian matrix at equilibrium, where all eigenvalues must have absolute values less than one for perturbations to decay in discrete-time systems, as explored in dedicated modeling sections. In the classic logistic model, the positive equilibrium representing carrying capacity exhibits global stability, attracting trajectories from diverse initial conditions and underscoring density dependence's role in long-term persistence. Empirical evidence from long-term studies highlights these regulatory dynamics. The population on Island, monitored since 1957, experiences recurrent density-driven crashes, where high autumn densities exceeding 200 individuals per square kilometer trigger elevated over-winter mortality rates up to 70%, preventing sustained overabundance despite favorable conditions. This pattern, driven by and exacerbated by weather, illustrates how compensatory mortality enforces , with post-crash rebounds maintaining the population's persistence over decades.

Parasite and Host Dynamics

In host-parasite systems, density dependence plays a critical role in the transmission of macroparasites, such as helminths, where the rate of new infections increases with population size. The seminal Anderson and May model captures this through a describing the interaction between host population size H and total parasite abundance P. The host dynamics are given by \frac{dH}{dt} = (a - b) H - \alpha P, where a is the host birth rate, b the natural host death rate, and \alpha P represents parasite-induced host mortality proportional to total parasite load. The parasite dynamics incorporate density-dependent transmission as \frac{dP}{dt} = \beta H P - (\mu + \alpha + b) P, where \beta H P is the recruitment term reflecting the production and uptake of infective stages, with \beta encapsulating the effective transmission coefficient (including egg production rate \lambda, infective stage survival, and infection probability), \mu the parasite natural mortality rate, and the other terms accounting for parasite loss due to host death and parasite-induced host mortality. This density-dependent form arises because higher host population size H (implying higher density in fixed habitat) facilitates greater contact between hosts and free-living parasite stages, amplifying transmission. Additionally, macroparasites often exhibit aggregated distributions within hosts, modeled using a negative binomial distribution with aggregation parameter k, where lower k values indicate higher overdispersion; this aggregation modulates the per capita impact of parasites on hosts and stabilizes coexistence by reducing the average harm per parasite at high intensities. For microparasites, such as or viruses that multiply within , density dependence manifests in susceptible-infected-susceptible () or susceptible-infected-recovered () models through contact rates that scale with population size. In the basic framework, the dynamics are \frac{dI}{dt} = \beta H I - (\gamma + \mu) I, where I is the number of infected , H total population size (with susceptibles S \approx H assuming low ), \beta the transmission rate (incorporating density effects via fixed area), \gamma the recovery rate, and \mu the death rate; the term \beta H I reflects density-dependent contacts driving new . Similarly, SIR models extend this by including a recovered class R, with term \beta H S (where S + I + R = H), emphasizing how higher population sizes accelerate spread until or depletion intervenes. These formulations highlight how density-dependent transmission can lead to thresholds below which microparasites cannot invade sparse populations. In , density dependence influences helminth infections profoundly, as seen in populations where elevated densities enhance environmental contamination with eggs, boosting and overall egg output from the parasite population. For instance, in (Lagopus lagopus scoticus) infected with the Trichostrongylus tenuis, higher grouse densities correlate with increased fecal egg counts and larval availability, driving cycles of parasite abundance that regulate host numbers. Conversely, positive density dependence emerges in low-density host refugia, where sparse populations fall below the for effective , allowing parasite and creating parasite-free zones that buffer against reinvasion; this is evident in fragmented habitats, such as isolated deer herds, where low densities foster refugia for hosts against macroparasite establishment.

Implications

Conservation and Management

Density dependence plays a critical role in by influencing risks through Allee effects, where positive density dependence at low sizes can create thresholds below which populations decline further rather than recover.01684-5) These effects increase vulnerability by reducing growth rates, mating success, or cooperative behaviors when densities fall critically low, often leading to a size estimated in the hundreds to thousands of individuals depending on the and environmental factors. Below this critical density, recovery fails due to intensified predation, , or resource access issues, amplifying probabilities in fragmented or small populations. In management strategies, density dependence informs sustainable harvesting models, such as those based on the logistic growth equation, which predict a at half the to balance exploitation with population regulation. often applies these principles to set quotas that account for density-dependent recruitment and growth, preventing while maximizing long-term yields. For reintroduction programs, recognizing positive density dependence guides efforts to release sufficient individuals to surpass Allee thresholds, enhancing establishment success in like or mammals where low initial densities hinder breeding. A prominent is the collapse of the northern Atlantic (Gadus morhua) stock off Newfoundland in the early , where overharvesting ignored density-dependent dynamics, driving the population below Allee-effect thresholds and contributing to a slow and challenging . Predation-driven Allee effects exacerbated the decline, as low cod densities reduced anti-predator schooling and increased juvenile mortality, illustrating how neglecting density dependence can lead to severe population crashes. As of 2025, the stock shows signs of improvement, with spawning stock biomass estimated at 524,000 tonnes—double the limit reference point—and a more than doubled total allowable catch of 38,000 tonnes following the end of the moratorium in 2024, though it remains below historical levels and faces ongoing pressures like predation. This event prompted revised management frameworks emphasizing precautionary density-based assessments to avoid similar outcomes in exploited fisheries.

Distribution Patterns

Density dependence plays a crucial role in by influencing the and spatial structure of populations across fragmented habitats. In source-sink models, local populations are categorized as sources, where reproduction exceeds mortality due to favorable conditions, and , where the opposite occurs, with net required for sink . Density-dependent dispersal enhances this framework by increasing rates from high-density source patches, thereby redistributing individuals to and stabilizing overall occupancy. This mechanism prevents in sources and rescues from , as demonstrated in experimental systems with fragmented landscapes where density-dependent processes regulated local most strongly in homogeneous environments. Adaptations of the classic Levins model incorporate density dependence to better capture realistic spatial variation. The original Levins model assumes constant and rates, but extensions introduce density-dependent rates that decline with increasing , reflecting resource or among patches. These modifications predict higher metapopulation persistence thresholds under density-dependent dispersal, where from crowded patches promotes without overwhelming sinks. For instance, nonlinear density dependence in dispersal rates can lead to inflationary effects, amplifying in marginal habitats and altering risks in dynamic patch networks. In patchy environments, negative density dependence often results in clumped spatial distributions of population abundances, as growth rates slow in high-density areas, leading to uneven aggregation across the landscape. This pattern is empirically captured by Taylor's , where the variance in (V) scales as a power function of the mean density (M), expressed as V \propto M^b with b > 1 indicating aggregation due to localized and dispersal limitations. Such clumping arises because in dense patches limits expansion, while sparser areas remain underpopulated until dispersal equalizes abundances imperfectly, as observed in time-series data from neutrally modeled populations where density dependence generates and power-law relationships. For parasite distributions, the R_0—the expected number of secondary infections from a single infected in a susceptible —varies directly with under density-dependent . In low- , R_0 < 1 prevents parasite establishment, resulting in sparse or absent distributions, whereas higher densities push R_0 > 1, enabling and aggregation at invasion fronts. This shapes spatial , as seen in disease systems where rates and advancing fronts accelerate nonlinearly with , concentrating parasites in high- zones while leaving low- areas uninvaded. In -parasite models, such dynamics underscore how negative dependence in can stabilize parasite persistence by modulating efficiency across heterogeneous landscapes.

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