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Appendix 1
Derivation of the parasite map
In this appendix, we suppress the w subscripts. The map governing average parasite per juvenile dynamics, P(t + 1) = βΔkλ(1 − Δ)P(t) A(t + 1), represents two processes, growth and transmission. For sea lice, problems of transmission (Krkošek et al. 2005; Frazer 2008) and growth (Stien et al. 2005; Revie et al. 2005; Krkošek 2010; Frazer 2009) have been studied in detail; however, the transmission models are spatially explicit descriptions of dynamics occurring in fjordic habitats over small time scales, and the growth models consider details of parasite age structure. We neglect the details of these formulations in favour of generality, assuming only that transmission results from low-probability infection events occurring in a well-mixed environment. Here, we derive the map used above to approximate a mass action process in a well-mixed environment that is valid when transmission is based on low-probability attachment events. Additionally, we assume that parasites grow without density dependence and have no age structure.
Each year includes a short infection window Δ, the period of wild adult and juvenile summer sympatry. During the remainder of the year, the maturation period, (1 − Δ), juveniles J(t) become adults A(t + 1) and parasite population growth occurs. The total number of adult-associated parasites at the end of the maturation period, which we denote \({\mathcal {P}}_{\rm adult}\) using a calligraphic “P” to differentiate from the variables for average parasite abundance used elsewhere, is reduced by host death due to parasitism and other factors, and increased by parasite reproduction and growth. Assuming the parasites are uniformly distributed on hosts, decline in host population from juvenile to adults due to parasites (\(1 - e^{-P_w}\)) affects the parasite population proportionally. Parasite population increase is expressed as a geometric growth in the average parasites per host at rate λ over the time (1 − Δ). Then, the number of adult-associated parasites at the end of maturation and the onset of transmission is given by
$$ {\cal P}_{\rm adult}(t+(1-\Delta)) = \lambda (1 -\Delta)P_w(t) \cdot A(t+1), $$
(8a)
$$ = \lambda (1 -\Delta)P_w(t) J(t) e^{-aP(t)-c_1A(t)}. $$
(8b)
We consider transmission during the infection window Δ in continuous time τ. Specifically, we consider the process of infective parasites, ψ, attaching to juvenile fish, F, during an infection window of length Δ. Because Δ is short, we treat number of juveniles F as constant and ignore production or immigration of new infective parasites ψ, of which we assume there are an initial quantity proportional to the number of adult-associated parasites at the beginning of transmission,
$$ \psi_{0}= k {\cal P}_{\rm adult} , $$
(9)
which relates back to model (Eq. 1) through the definition of \({\cal P}_{\rm adult}\) in Eq. 8. We further assume that infective parasites ψ become attached parasites \({\cal P}\) independently from one another at a constant rate β. Finally, for consistency with Eq. 1, where the units of P are motile parasites per fish, we track \(P = {\cal P}/F\) the average attached parasites per fish. This gives the following equations for τ ∈ (0, Δ),
$$ \dot \psi = -\beta \psi F $$
(10a)
$$ \dot {\cal P} = \beta \psi F $$
(10b)
$$ \dot P =\frac{\dot {\cal P}}{F}= \beta \psi, $$
(10c)
The equation for the change in parasites per fish, \(\dot P\), comes from dividing the equation for total attached parasites \(\dot {\cal P}\) by F. Note that attachment rate β implicitly includes mortality of infective parasites. This is similar to equations underlying the macroparasite model of Anderson and May (1978), but here considered only over a short time scale.
With a constant number of juveniles F, we have \(\psi(\tau) = \psi_{0}e^{-\beta F \tau}\) and \(P(\tau) = \beta \psi_{0}\int_{0}^{\tau}e^{-\beta F s}{\rm d} s\) on τ ∈ (0, Δ). This expresses average parasites per fish at the end of the infection window as a function of juveniles, initial infective parasites, the transmission rate, and the length of the window: \(P(\Delta) = \frac{\psi_{0}}{F}[1-e^{-\beta \Delta F}]\). If βΔF ≪ 1 a first-order Taylor approximation yields P (Δ) ≈ βΔψ
0. For \(F < \frac{1}{\beta\Delta}\), the error in this approximation is bounded by \(\frac{\psi_0 \beta \Delta}{e}\) (where e is Euler’s constant). Using Eqs. 8 and 9 to relate this approximation back to the variables in Eq. 1,
$$ P(t+1) = \beta \Delta k\lambda(1-\Delta) P(t) J(t) e^{-a P(t)-c_1 A(t)}, $$
(11)
we also note that the relevant quantity of juveniles is J(t + 1). We use this equation under the assumption that the number of juveniles falls below a threshold \(J(t+1) < \frac{1}{\beta \Delta}\), which is an inverse measure of the strength of inter-lineage transmission. When inter-lineage transmission is very weak, β is very low and \(\frac{1}{\beta \Delta}\) is very large.
Appendix 2
Analysis of farm-free system
Using both analytical techniques from dynamical systems and numerical bifurcation analysis we find regions where line dominance occurs in the two-dimensional space of parameters governing (1) negative density-dependent interactions between host lineages and (2) host productivity. Line dominance corresponds to mathematical two cycles and arises from stable equilibria through period-doubling so we focus on defining boundaries of the region where period-doubling occurs in parameter space. In the results of the main text, we report how these boundaries shift with the introduction of farm hosts.
Recall that we treat the low-juvenile case, where \(N_0 \le \frac{1}{\beta_w\Delta_f}\). We introduce a scaling of Eq. 1 to obtain the non-dimensional equations,
$$ N_0(t+1) = N_1(t) e^{r-N_1(t)- \tilde c_0N_0(t)}, $$
(12a)
$$ N_1(t+1) = N_0(t) e^{-\tilde c_{1}N_1(t) - P(t)}, $$
(12b)
$$ P(t+1) = \eta P(t) N_{0}(t) e^{-\tilde c_{1}N_1(t) - P(t)}, $$
(12c)
where non-dimensional parameters \(\tilde c_0 = \frac{c_0}{s_1 b}\), \(\tilde c_1 = \frac{c_1}{b}\) relate to inter-cohort density dependence. Dynamical variables are N
0 = b
s
1
J, N
1 = b
A, and P = a
w
P
w
. Host growth rate is \(e^r = s_0s_1s_2 f\). The non-dimensional parameter for parasite-mediated density dependence is \(\eta = \frac{\beta_w \Delta_f k\lambda(1-\Delta_f)}{b}\). For the remainder of the appendix we suppress tildes on \(\tilde c_i\). The model (Eq. 12) exhibits positive invariance to \(\mathbb R^3_+\). To see this, define N (
t) as \(\left(N_0 (t), N_1(t), P(t)\right)\) then take N(
t
0
) > 0 as initial data at time t
0. Applying Eq. 12 once, N (
t
0
+ 1) > 0 and repeated application of Eq. 12 results in N(
t) > 0 for all t > t
0.
We assume that parameters r and η are positive thereby restricting attention to cases where wild adult–juvenile transmission occurs. Furthermore, we focus attention on changes in parameters governing negative density-dependent inter-lineage interactions that result in two cycles in Eq. 12. Mathematically, these are period-doubling bifurcations of stable equilibria.
Standard linearized stability analysis requires solving Eq. 12 for equilibria. The analytical tractability of Eq. 12 depends on the values of the parameters describing general negative density-dependent interactions c
i
. We assume c
i
are non-negative and treat several cases. In two of these, one parameter is zero and at least some analytical treatment is possible: (1) when c
0 = 0 but c
1 > 0 and maturation range inter-lineage interactions are possible, and (2) when c
0 > 0 but c
1 = 0. In case (3) where both maturation range and nursery range inter-lineage interactions are possible, i.e. c
i
> 0, but the fixed points of Eq. 12 are not expressible in terms of elementary functions. We do not consider this case further. Biologically, this means that we treat cases where negative density-dependent interactions occur between lineages either in ocean habitat (c
1) or in breeding habitat (c
0), but not in both.
Equilibria
Bifurcations of equilibria from fixed points to two cycles through period-doubling occur from both parasite-free N
PFE
and coexistence N
*
equilibria. The cases treated here differ in their potential for period-doubling bifurcations from these two types of equilibria. For cases (1) and (2), parasite-free equilibria are given in Table 3. Only for case (1) can the coexistence equilibria be obtained analytically in terms of elementary functions; given in Table 3.
Table 3 Fixed points of model for analytically tractable cases
In case (2), when c
0 > 0 and c
1 = 0, the coexistence equilibria of Eq. 12 are defined by transcendental equations. Specifically, let \(\mathbf N^{(2)}_{*} := (N^*_0, N^*_1, P^*)\) denote the equilibrium in this case. Dividing Eq. 12c through by P
*, we see \(1 = \eta N^*_0 e^{-P^*}\). Substituting this relation into Eq. 12b,
$$ N^*_1 = \frac{1}{\eta}. $$
By substituting into Eq. 12a, we see that
$$ N^*_0 = \frac{1}{\eta}e^{r - c_0 N^*_0 - \frac{1}{\eta}}, $$
a transcendental equation for \(N^*_0\). This equation does have a unique solution, which expressible in terms of the Lambert W function (see, e.g., Corless et al. 1996), and is given in Table 3.
Stability
Standard linearized stability also requires linearizing the system (Eq. 12). The linearization is expressed through the Jacobian matrix of the system:
$${\begin{array}{rll} &\mathbf D(t) \\ &=\left(\scriptsize\begin{matrix} - N_{1} c_{0} e^{r - N_{1} - N_{0} c_{0}} & (1- N_{1})e^{r - N_{1} - N_{0} c_{0}}& 0\\ e^{- P - N_{1} c_{1}} & - N_{0} c_{1} e^{- P - N_{1} c_{1}} & - N_{0} e^{- P - N_{1} c_{1}}\\ P \eta e^{- P - N_{1} c_{1}} & - N_{0} P \eta c_{1} e^{- P - N_{1} c_{1}} & (1-P)N_{0} \eta e^{- P - N_{1} c_{1}} \end{matrix}\right). \end{array}} $$
(13)
We use standard local stability analysis of dynamical systems. For discrete-time systems, linear stability requires that each eigenvalue of the Jacobian matrix (Eq. 13) evaluated at an equilibrium lies within the unit circle in the complex plane. If the linearized system at a particular equilibria satisfies this requirement, then it is stable. For analysis of the parasite-free equilibrium, N
PFE
we are able to analytically compute the eigenvalues of Eq. 13 evaluated at the equilibrium and thus verify stability. For the coexistence equilibrium, N
*
, we use Jury’s criteria, which provide necessary and sufficient conditions on the characteristic polynomial of the Jacobian for stability. We do not focus on the stability of equilibria per se, but instead on the location in parameter space where stability is lost, through bifurcation. Thus, results of our stability analysis are described below in our bifurcation analysis.
Bifurcations
Throughout we focus on behaviour for moderate values of host reproduction, i.e. r < 2, that correspond to the situation of biological interest. This eliminates possible period-doubling bifucations due to the host reproduction parameter r. Such bifurcations occur in the classical Ricker model, as part of a period doubling cascade to chaos as outlined in May and Oster (1976). Because our concern is line dominance, we focus on period-doubling bifurcations that occur with changes in parameters governing negative density-dependent inter-lineage interactions, including general interactions c
i
and parasite-mediated interactions governed by the inter-lineage transmission term η.
Period-doubling (PD) bifurcations of maps must satisfy two criteria (Iooss 1979, p. 12):
Theorem 1
Consider the map
\((\mu, X_{i}) \!\mapsto\! f_\mu (X_i): \mathbb R^4 \to\)
\( \mathbb R^3\)
where
\(X_{i} \in \mathbb R^3\)
are dynamical variables and
\(\mu \in \mathbb R\)
is a parameter. If f
μ
is of class C
k
for k ≥ 2 near a fixed point X
*
, then a period doubling bifurcation exists at μ = μ
*
if the following conditions are satisfied:
-
(PD1)
Eigenvalue location The Jacobian
\(D f_\mu (X^*)\)
has an eigenvalue λ
0(μ) with
\(\lambda_0(\mu^*) = -1\)
and
\(|\lambda_i(\mu^*)|<1\)
for i = 1,2; and
-
(PD2)
Transversal \(\frac{d |\lambda(\mu^*)|}{d\mu} < 0\).
Specifically, there exists a unique one-sided bifurcated branch of fixed points of order 2, (μ(s), X
j
(s), j = 1, 2) for f
μ
such that μ(X
*) = X
*
, μ( − s) = μ(s), X
1( − s) = X
2(s),\(\frac{d_{X_1}}{ds}(0) = 1\),\(X_j(0) = X^*\),\(f_\mu (X_j) = X_{j^{\prime;}}, j \ne j^{\prime}\). The functions μ
and X
j
are C
k − 1.
Bifurcation from parasite-free equilibrium
For the parasite-free equilibria N
PFE
, we characterized period-doubling bifurcations for both case (1) and case (2).
In case (1), c
0 = 0 the Jacobian (Eq. 13) evaluated at N
PFE
from Table 3 is given by
$$ \left(\begin{matrix}0 & - \displaystyle\frac{r e^{r - \frac{r}{1 + c_{1}}}}{1 + c_{1}} + e^{r - \frac{r}{1 + c_{1}}} & 0\\[12pt]e^{- \frac{c_{1} r}{1 + c_{1}}} & - \displaystyle\frac{c_{1} r}{1 + c_{1}} & - \displaystyle\frac{r}{1 + c_{1}}\\[12pt]0 & 0 & \displaystyle\frac{\eta r}{1 + c_{1}}\end{matrix}\right). $$
(14)
The characteristic equation of Eq. 14 is
$$\begin{array}{rll} \lambda^{3} &+& \lambda^{2} \left(\frac{c_{1} r}{1 + c_{1}} - \frac{\eta r}{1 + c_{1}}\right) \notag\\ &-& \lambda \left(1 - \frac{r}{1 + c_{1}} + \frac{\eta c_{1} r^{2}}{\left(1 + c_{1}\right)^{2}}\right)\notag\\ &+& \frac{\eta r}{1 + c_{1}} - \frac{\eta r^{2}}{\left(1 + c_{1}\right)^{2}} =0. \end{array}$$
(15)
The polynomial on the right hand side of Eq. 15 can be factored,
$$\begin{array}{lll} \left(\!\lambda - \frac{\eta r}{1+c_1}\!\right)\\ \quad \cdot\left(\!\lambda + \frac{c_{1} r}{2 + 2 c_{1}}- \frac{1}{2} \sqrt{4 - 4 \frac{r}{1 + c_{1}} + \frac{c_{1}^{2} r^{2}}{\left(1 + c_{1}\right)^{2}}}\right)\\ \quad \cdot \left(\lambda + \frac{c_{1} r}{2 + 2 c_{1}} + \frac{1}{2} \sqrt{4 - 4 \frac{r}{1 + c_{1}} + \frac{c_{1}^{2} r^{2}}{\left(1 + c_{1}\right)^{2}}}\right). \end{array} $$
To find potential curves in parameter space where period-doubling occurs, we set one root of the characteristic equation (Eq. 15) to negative unity. The resulting curve is c
1 = 1. Along this curve, one eigenvalue of Eq. 14, i.e. root of Eq. 15, is negative unity. The eigenvalue of Eq. 14
$$ \lambda_{PD(i)} = - \frac{c_{1} r}{2 + 2 c_{1}} - \frac{1}{2} \sqrt{4 - 4 \frac{r}{1 + c_{1}} + \frac{c_{1}^{2} r^{2}}{\left(1 + c_{1}\right)^{2}}} $$
(16)
evaluates to negative unity when c
1 = 1. The other roots of Eq. 15 have absolute value less than unity when conditions on η and r are satisfied: the root \(\frac{\eta r}{1+c_0}\), has absolute value less than unity when η is sufficiently small, i.e. \(\eta < \frac{2}{r} = \frac{1+c_1}{r}\); the other root is the complex conjugate of Eq. 16, and has absolute value less than unity for values of r considered here, i.e. r < 2. Thus the eigenvalue location (PD1) criterion is satisfied for r < 2 and sufficiently small values of η. For this eigenvalue,
$$ \frac{\partial \lambda_{PD(i)} (c_1)}{\partial c_1}{\Big\rvert}_{c_1=1} = - \frac{1}{8} r - \frac{1}{8}\frac{4 r + r^{2}}{r -4}, $$
thus satisfying the transversal (PD2) criterion for values of r considered here, i.e. r < 2.
In case (2), c
1 = 0, the Jacobian (Eq. 13) evaluated at N
PFE
from Table 3 is given by
$$ \left(\begin{matrix}- \displaystyle\frac{c_{0} r e^{r - \frac{r}{1 + c_{0}} - \frac{c_{0} r}{1 + c_{0}}}}{1 + c_{0}} & - \displaystyle\frac{r e^{r - \frac{r}{1 + c_{0}} - \frac{c_{0} r}{1 + c_{0}}}}{1 + c_{0}} + e^{r - \frac{r}{1 + c_{0}} - \frac{c_{0} r}{1 + c_{0}}} & 0\\ 1 & 0 & - \frac{r}{1 + c_{0}}\\ 0 & 0 & \frac{\eta r}{1 + c_{0}} \end{matrix}\right)\!. $$
(17)
The characteristic equation of Eq. 17 is
$$ \begin{array}{rll} \lambda^{3}&+&\lambda^{2} \left(\frac{c_{0} r}{1 + c_{0}} - \frac{\eta r}{1 + c_{0}}\right)\\ &-& \lambda \left(1 - \frac{r}{1 + c_{0}} + \frac{\eta c_{0} r^{2}}{\left(1 + c_{0}\right)^{2}}\right)\\ &+& \frac{\eta r}{1 + c_{0}} - \frac{\eta r^{2}}{\left(1 + c_{0}\right)^{2}} =0. \end{array} $$
(18)
The polynomial on the right hand side of Eq. 17 can be factored,
$$ \begin{array}{lll} \left(\lambda - \frac{\eta r}{1+c_0}\right)\\ \quad \cdot \left(\lambda + \frac{c_{0} r}{2 + 2 c_{0}} -\frac{1}{2} \sqrt{4 - 4 \frac{r}{1 + c_{0}} + \frac{c_{0}^{2} r^{2}}{\left(1 + c_{0}\right)^{2}}}\right)\\ \quad \cdot \left(\lambda + \frac{c_{0} r}{2 + 2 c_{0}}+ \frac{1}{2} \sqrt{4 - 4 \frac{r}{1 + c_{0}} + \frac{c_{0}^{2} r^{2}}{\left(1 + c_{0}\right)^{2}}}\right). \end{array} $$
To find potential curves in parameter space where period-doubling occurs, we set one root of the characteristic equation (Eq. 18) to negative unity. The resulting curve is c
0 = 1. Along this curve, one eigenvalue of Eq. 17, i.e. root of Eq. 18, is negative unity. The eigenvalue of Eq. 17
$$ \lambda_{PD(ii)} = - \frac{c_{0} r}{2 + 2 c_{0}} - \frac{1}{2} \sqrt{4 - 4 \frac{r}{1 + c_{0}} + \frac{c_{0}^{2} r^{2}}{\left(1 + c_{0}\right)^{2}}} $$
(19)
evaluates to negative unity when c
0 = 1. The other roots of Eq. 18 have absolute value less than unity when conditions on η and r are satisfied: the root \(\frac{\eta r}{1+c_0}\), has absolute value less than unity when η is sufficiently small, i.e. \(\eta < \frac{2}{r} = \frac{1+c_0}{r}\); the other root is the complex conjugate of Eq. 19, and has absolute value less than unity for values of r considered here, i.e. r < 2. Thus the eigenvalue location (PD1) criterion is satisfied for r < 2 and sufficiently small values of η.
For this eigenvalue,
$$ \frac{\partial \lambda_{PD(ii)} (c_0)}{\partial c_0}{\Big\rvert}_{c_0=1} = - \frac{1}{8} r - \frac{1}{8}\frac{4 r + r^{2}}{r -4}, $$
thus satisfying the transversal (PD2) criterion for values of r considered here, i.e. r < 2.
Bifurcation from coexistence equilibrium
For the coexistence equilibrium, N
*
, in case (1), the Jacobian (Eq. 13) evaluated at N
* from Table 3 is given by
$$ \left(\begin{smallmatrix}0 & - \displaystyle\frac{e^{r - \frac{1}{\eta}}}{\eta} + e^{r - \frac{1}{\eta}} & 0\\ e^{- r + \frac{1}{\eta}} & - \displaystyle\frac{c_{1}}{\eta} & - \displaystyle\frac{1}{\eta}\\ \eta \left(r - \displaystyle\frac{1}{\eta} - \displaystyle\frac{c_{1}}{\eta}\right) e^{- r + \frac{1}{\eta}} & - c_{1} \left(r - \displaystyle\frac{1}{\eta} - \displaystyle\frac{c_{1}}{\eta}\right) & 1 - r + \displaystyle\frac{1}{\eta} + \displaystyle\frac{c_{1}}{\eta} \end{smallmatrix}\right) $$
(20)
The characteristic equation of Eq. 20 is
$$ \lambda^{3}+\lambda^{2} \left(r - 1 - \frac{1}{\eta}\right) + \lambda \left(\frac{1-c_{1}}{\eta} -1\right) +1- \frac{1}{\eta} = 0 $$
(21)
To find potential curves in parameter space where period-doubling occurs, we set one root of the characteristic polynomial (Eq. 21) to negative unity. The resulting curve is \(r = \frac{3 - c_1}{\eta}\). Along this curve, one eigenvalue of Eq. 20 is negative unity and thus part of the eigenvalue location (PD1) criterion is satisfied. The roots of Eq. 21 are obtainable through the formula for the roots of a cubic. The formulae that result from these roots, however, are very long and would be tedious to treat analytically. We use Jury’s criteria, which provide necessary and sufficient conditions on the characteristic polynomial of the Jacobian for stability, to verify that the remaining eigenvalues fall within the unit circle. We state Jury’s stability criteria from (Cain 2007):
Theorem 2
(Jury stability test) All roots of the polynomial
$$ q(x) = a_m x^m + a_{m-1} + \dots + a_1 x + a_0 $$
(22)
lie in the open disc in the complex plane if and only if
-
(J1)
a
m
q(1) > 0,
-
(J2)
\((-1)^m a_m q(-1) > 0\)
, and
-
(J3.j)
|r
j
| < 1 for j = 1, 2, ...m, where r
j
are given by the following iterative procedure. First, set b
j
= a
m − j
for j = 0, 1, ...m and define r
m
= b
m
/a
m
. Then, define
\(a^{\rm new}_{j-1} = a_j - {\rm r}_m b_j\)
for j = 1, 2, ...m. This gives the coefficients
a
m − 1, a
m − 2 ...a
0
for the next iteration.
The characteristic polynomial of Eq. 20 is given by the left-hand side of the characteristic equation (Eq. 21). To apply Theorem 2 to the linearization (Eq. 20), we identify coefficients of the polynomial from Eq. 21 with coefficients a
j
of Eq. 22:
$$ \begin{array}{rll} a_3 &=& 1,\\ a_2 &=& r - 1 - \frac{1}{\eta},\\ a_1 &=& \frac{1-c_1}{\eta} - 1,\\ a_0 &=& 1 - \frac{1}{\eta}. \end{array} $$
The full set of Jury’s criteria from Theorem 2 for N
*
in case (1) are given in Table 4. Equality in condition J2 of Table 4 corresponds to the curve \(r = \frac{3-c_1}{\eta}\). Condition J1 is satisfied along this curve for c
1 < 1, and condition J3.1 is satisfied for \(\eta > \frac{1}{2}\). Thus, along the curve \(r = \frac{3-c_1}{\eta}\), for r < 2, \(\eta > \frac{1}{2}\), and c
1 < 1, when criteria J3.2 and J3.2 are also met, the full eigenvalue location criterion (PD1) is satisfied.
Table 4 Conditions for existence and stability of N
*
in case (1)
Because we did not explicitly compute the eigenvalues of Eq. 21, we could not verify the transversal condition analytically. Using the numerical continuation tool Cl_matcontM (Dhooge et al. 2003), however, we verified that the system undergoes a period-doubling bifurcation along the dashed line of Fig. 2a. This tool, like many software packages for numerical analysis of bifurcations, solves equations that define a bifurcation type, e.g. period-doubling, and computes corresponding normal forms to identify the bifurcation (Dhooge et al. 2003; Kuznetsov 2004).
Thus, equality in the conditions of Table 5 defines boundaries between regions in which the coexistence and parasite-free equilibria are stable and those in which two cycles occur. For c
i
< 1 period-doubling bifurcations from a stable coexistence equilibrium are possible. The dashed lines in Fig. 2 represent curves where the eigenvalue location (PD1) criterion is satisfied for the coexistence equilibrium N
*
. Numerical computations using Cl_matcontM (Dhooge et al. 2003) confirm these curves represent the location of period-doubling bifurcations with increasing η. In this case, the dynamics undergo a qualitative transition from stable endemic equilibrium to dominance through period doubling with increase in either η or c
1.
Table 5 Conditions that, if violated, result in loss of stability through period-doubling of parasite-free N
PFE
and coexistence N
*
fixed points; for analytically tractable cases
The ηr stability plane, i.e. Fig. 2a in the main text, shows curves based on the applying Jury’s criteria to N
*
for case (1), i.e. Table 4, and results from numerical continuation. The structure shown in this figure indicate that the governing of dynamics by r is also typical for η > 0. For fixed r, e.g. r = r
* = 1.2 the empirical estimate for pink salmon (Myers et al. 1999), as η becomes very large, a bifurcation across the dotted line of Fig. 2a to higher-order cycles is possible. This line corresponds to Neimark–Sacker bifurcation, i.e. a Hopf bifurcation for maps (Hale and Kocak 1991). Bifurcation in η is shown in Fig. 3a. The character of the bifurcation in η is a single period doubling. In contrast to the “cascade to chaos” familiar from the Ricker model (May and Oster 1976), the period-two regime is present for a large range, η ≈ 2.5 to η ≥ 100 (not shown).
Appendix 3
Differential mortality between lines when dominance occurs
If dominance occurs in Eq. 1, the less-abundant lineage experiences 40% mortality (or greater) due to negative density-dependent inter-lineage interactions, while the dominant lineage experiences less mortality. Figure 5a shows the equilibrium mortality of juvenile hosts due to general negative density dependence and parasitism at the edge of the dominance region, i.e. dashed lines in Fig. 2. The degree of overall mortality due to both factors decreases slightly as the general negative density dependent , c
1/b, interaction strength is increased. The figure was computed for a system with where negative density-dependent effects occur between lineages only based on adult abundance (c
1 > 0, c
0 = 0). In the “dominance” region of Fig. 2a, mortality for the more-abundant lineage falls below the curves given, while mortality for the less-abundant lineage is above the curve.
As the strength of general negative density-dependent interactions is increased, the amount of parasite-mediated negative density-dependent mortality needed to maintain dominance decreases. Figure 5b shows this effect, plotting the mortality due to parasite-mediated effects alone that is needed to maintain line dominance plotted against the strength of general negative density-dependent inter-lineage interactions c
1/b.