Colonization and extinction rates can be considered effective
rates in the sense that they are average approximations to the
intrinsic individual-level processes driving species-specific dynamics.
This function includes three simple stochastic population models
simulated with Gillepie’s exact algorithm (Gillespie 1977). All three
models assume individuals as discrete entities subject to a range of
processes. Our aim is to show the correspondence between parameters
driving individual deaths and births, and colonization-extinction rates
at the population level. The population models included in function
ibd_models
are: the seminal model by Kendall (1948), a
mainland-island model by Alonso & McKane (2002) and a basic
population model with density-dependent deaths by Haegeman & Loreau
(2010). The three models have three basic processes that differ in their
parametrization: inmigration (arrival of new individuals from outside
the population), individual births and individual deaths. In the
following table, we specify the processes and the transitions (with
probability rates in units of Time⁻¹) associated with each model.
Process | Transition | Kendall (1948) | Alonso & McKane (2002) | Haegeman & Loreau (2010) |
---|---|---|---|---|
Inmigration | ∅ → A | μ | μ(K − n) | μ |
Birth | A → A + A | βn | $\beta n (1 - \frac{n}{K})$ | βn |
Death | A → ∅ | δn | δn | $n (\delta + (\beta - \delta) \frac{n}{K})$ |
Please note that Kendall’s model may explode if the birth rate is higher than the death rate. Notice also that the death rate in the Haegeman & Loreau model may become ill-defined, this is, negative for death rate values higher than the value for the birth rate, given that probability rates can never be negative.
The function ibd_models
allows to simulate the
stochastic population dynamics described in the previous section. The
function requires that we specify arguments n0
(initial
population size), beta
(birth rate), delta
(death rate), mu
(inmigration rate), and K
(carrying capacity) when required. We also need to specify a vector of
sampling times time_v
and the model we plan to use via
argument type
. To illustrate its stochastic nature, the
following code simulates the dynamics of Alonso and McKane (2002) model,
with equal birth and death rates and low inmigration.
In the following section, we illustrate the use of colonization and
extinction rates as effective parameters reflecting the underlying
species dynamics. We used the Alonso & McKane model implemented in
function ibd_models
to examine the effect of varying
carrying capacity K on our
colonization and extinction rates for a given set of parameters, showing
that changes in carrying capacity can drastically change the
colonization and extinction rates obtained.
ts <- 0:100 #Time-vector
ccc <- seq(10, 100, 10) #Carrying capacities
out <- NULL #Initializing output
for (i in ccc){
pops <- matrix(nrow = 100, ncol = 101)
for (j in 1:100){
sim <- ibd_models(n0 = 0, beta = 0.2, delta = 0.3, mu = 0.004, K = i, time_v = ts,
type = "Alonso") #Simulations
pops[j, ] <- (sim[, 2] > 0) * 1.0
}
out <- rbind(out, c(i, regular_sampling_scheme(pops, 1:101)))
}
#Plotting
plot(out[, 1], out[, 2], type = "b", xlab = "Carrying capacity", ylab = "Rate",
col = "darkgreen", main = "Effect of changes in the underlying population dynamics
over colonization and extinction rates")
lines(out[, 1], out[, 5], type = "b", col = "magenta")
legend(10, .35, legend=c("Colonization", "Extinction"),
col=c("darkgreen", "magenta"), pch = 21, lty=1, pt.bg = "White", cex=0.8)
In order to generate more realistic simulations, we can add a
detectability filter to the output of function ibd_models
.
For the sake of simplicity, we assume that the detectability of a
species is a function of the number of individuals present in the
population, as described by the following equation: dn = 1 − (1 − d)n
where dn
is the probability of finding the species, d is the detection probability of
one individual, and n is the
number of individuals present in the population. This assumes that
individuals are detected independently from each other with the same
constant probability d.
The next example follows the same procedure as in the previous section,
with the added step of sampling population at some detectability level.
It illustrates how changes in population-level parameters make an
influence on colonization and extinction estimates.
ts <- seq(0, 49, 7) #Time-vector
ccc <- seq(10, 100, 10) #Carrying capacities
out <- NULL
for (i in ccc){
pops <- matrix(nrow = 100, ncol = 24)
for (j in 1:100){
sim <- ibd_models(n0 = sample(c(0,1), 1), beta = 0.24, delta = 0.3, mu = 0.004, K = i, time_v = ts,
type = "Alonso")
# Applying the detectability filter and preparing the data for sss_cedp
filter1 <- (runif(8) < 1 - (1 - 0.7)^sim[, 2]) * 1.0
filter2 <- (runif(8) < 1 - (1 - 0.7)^sim[, 2]) * 1.0
filter3 <- (runif(8) < 1 - (1 - 0.7)^sim[, 2]) * 1.0
filtered <- cbind(filter1, filter2, filter3)
filtered2 <- c(t(filtered))
pops[j, ] <- filtered2
}
out <- rbind(out, c(i, unlist(sss_cedp(pops, seq(0, 49, 7), rep(3, 8), Colonization = 0.1, Extinction = 0.1, Phi_Time_0 = 0.5, Detectability = 0.7))))
}
plot(out[, 1], out[, 2], type = "b", xlab = "Carrying capacity", ylab = "Rate or probability",
col = "darkgreen", main = "Effect of changes in the underlying population dynamics
over cedp parameters", ylim = c(0, 1))
lines(out[, 1], out[, 3], type = "b", col = "magenta")
lines(out[, 1], out[, 4], type = "b", col = "blue")
lines(out[, 1], out[, 5], type = "b", col = "brown")
legend(80, .8, legend=c("Colonization", "Extinction", "Detectability", "P0"),
col=c("darkgreen", "magenta", "blue", "brown"), pch = 21, lty=1, pt.bg = "White", cex=0.8)