ARTICLE IN PRESS
Journal of Theoretical Biology 251 (2008) 210–226
www.elsevier.com/locate/yjtbi
Evolution of dominance under frequency-dependent
intraspecific competition
Stephan Peischla, Reinhard Bürgera,b,
a
Department of Mathematics, University of Vienna, Nordbergstrasse 15, 1090 Wien, Austria
Program for Evolutionary Dynamics, Harvard University, One Brattle Square, Cambridge, MA 02138, USA
b
Received 19 June 2007; received in revised form 15 October 2007; accepted 14 November 2007
Available online 19 November 2007
Abstract
A population-genetic analysis is performed of a two-locus two-allele model, in which the primary locus has a major effect on a
quantitative trait that is under frequency-dependent disruptive selection caused by intraspecific competition for a continuum of
resources. The modifier locus determines the degree of dominance at the trait level. We establish the conditions when a modifier allele can
invade and when it becomes fixed if sufficiently frequent. In general, these are not equivalent because an unstable internal equilibrium
may exist and the condition for successful invasion of the modifier is more restrictive than that for eventual fixation from already high
frequency. However, successful invasion implies global fixation, i.e., fixation from any initial condition. Modifiers of large effect can
become fixed, and also invade, in a wider parameter range than modifiers of small effect. We also study modifiers with a direct,
frequency-independent deleterious fitness effect. We show that they can invade if they induce a sufficiently high level of dominance and if
disruptive selection on the ecological trait is strong enough. For deleterious modifiers, successful invasion no longer implies global
fixation because they can become stuck at an intermediate frequency due to a stable internal equilibrium. Although the conditions for
invasion and for fixation if sufficiently frequent are independent of the linkage relation between the two loci, the rate of spread depends
strongly on it. The present study provides further support to the view that evolution of dominance may be an efficient mechanism to
remove unfit heterozygotes that are maintained by balancing selection. It also demonstrates that an invasion analysis of mutants of very
small effect is insufficient to obtain a full understanding of the evolutionary dynamics under frequency-dependent selection.
r 2007 Elsevier Ltd. All rights reserved.
Keywords: Frequency dependence; Disruptive selection; Intraspecific competition; Balancing selection; Stable underdominance; Evolution of genetic
architecture; Dominance modifier
1. Introduction
Frequency-dependent intraspecific competition has been
invoked in the explanation of a number of important
evolutionary phenomena. These include the maintenance
of high levels of genetic variation (Cockerham et al., 1972;
Clarke, 1979; Asmussen and Basnayake, 1990; Gavrilets
and Hastings, 1995), in particular, in quantitative traits
(Bulmer, 1974; Slatkin, 1979; Christiansen and Loeschcke,
1980; Loeschcke and Christiansen, 1984; Bürger
Corresponding author at: Department of Mathematics, University of
Vienna, Nordbergstrasse 15, 1090 Wien, Austria.
E-mail addresses: stephan.peischl@univie.ac.at (S. Peischl),
reinhard.buerger@univie.ac.at (R. Bürger).
0022-5193/$ - see front matter r 2007 Elsevier Ltd. All rights reserved.
doi:10.1016/j.jtbi.2007.11.014
2002a, b, 2005; Bürger and Gimelfarb, 2004; Schneider,
2006), the evolution of sexual dimorphism (Slatkin, 1984;
Bolnick and Doebeli, 2003; Van Dooren et al., 2004), the
evolutionary splitting of assortatively mating populations
(Drossel and McKane, 2000; Bolnick, 2004; Kirkpatrick
and Nuismer, 2004; Bürger and Schneider, 2006; Bürger et
al., 2006; Schneider and Bürger, 2006), the evolution of
assortative mating and sympatric speciation (Maynard
Smith, 1966; Udovic, 1980; Doebeli, 1996; Dieckmann and
Doebeli, 1999; Dieckmann et al., 2004; Matessi et al.,
2001; Kirkpatrick and Ravigné, 2002; Gavrilets, 2003,
2004; Polechová and Barton, 2005), and the evolution
of genetic architecture (van Doorn and Dieckmann,
2006; Kopp and Hermisson, 2006; Schneider, 2007).
The latter includes the evolution of dominance, the topic
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to which this work is devoted. For a recent review of
various evolutionary responses to disruptive selection, see
Rueffler et al. (2006).
Evolution of dominance has been a controversial issue in
population genetics which has its origin in the famous
dispute between Fisher and Wright beginning in 1928; for a
review see Mayo and Bürger (1997). Theories explaining
dominance and its modification within a biochemical
framework are discussed in Bürger and Bagheri (2008).
The idea common to models of dominance evolution is that
if some heterozygous and homozygous genotypes differ in
fitness, dominance should evolve such that the phenotype
associated with the disadvantageous genotype resembles
the superior phenotype. However, a dominance modifier
can attain an evolutionarily significant selective advantage
only if heterozygotes are sufficiently frequent. This may
occur during a selective sweep (e.g., Haldane, 1956;
Wagner and Bürger, 1985), if there is heterozygous
advantage (Sheppard, 1958; Bürger, 1983; Otto and
Bourguet, 1999), under disruptive selection (Clarke and
Sheppard, 1960), under frequency-dependent selection
(e.g., Clarke, 1964; O’Donald, 1968) or, more generally,
if heterozygotes are maintained at high frequency by some
form of balancing selection, such as migration-selection
balance or spatially varying selection (Fisher, 1931; Van
Dooren, 1999; Otto and Bourguet, 1999). As noted by
Mayo and Bürger (1997), most well-documented empirical
examples for the evolution of dominance originate from
studies of genetic variation in a relatively well-understood
ecological context.
Wilson and Turelli (1986) found stable underdominance
in a model of differential utilization of two resources and
argued that evolution of dominance would be an efficient
mechanism for removing unfit heterozygotes. Also strong
intraspecific competition for a single, continuously distributed resource is known to cause stable polymorphism
and disruptive selection (e.g., Bulmer, 1974; Christiansen
and Loeschcke, 1980). In related contexts, evolution of
dominance has been demonstrated theoretically in subdivided populations (Otto and Bourguet, 1999) and in a
heterogeneous environment (Van Dooren, 1999). Evolution of dominance caused by pesticide resistance may be a
case in point (Otto and Bourguet, 1999). In both models,
frequency-dependent disruptive selection results from
variation in the direction of selection among the patches.
Thus, under appropriate conditions balancing selection
maintains heterozygotes at high frequency.
It is tempting to speculate about evolution of dominance
caused by intraspecific competition for resources in the
African finch Pyrenestes (Smith, 1993), where two morphs
differ substantially in lower mandible width. Apparently,
these morphs are randomly breeding with respect to these
traits. Disruptive selection is most likely related to seed
quality, because large morphs feed more efficiently on a
hard-seeded species of sedge and small morphs on a softseeded species. The trait under putative disruptive selection
shows a distinct bimodal distribution, and there is evidence
211
that the bill-size polymorphism is caused by a single
autosomal diallelic locus with complete dominance for the
large-bill morph. Although the seed distribution is strongly
bimodal, a putative ancestral generalist (Rueffler et al.,
2006) may have had highest fitness under low population
density or weak competition. Another example, where
negative frequency-dependent selection on a single gene
maintains a polymorphism, is the foraging gene in larvae of
Drosophila melanogaster (Fitzpatrick et al., 2007). Also in
this case, heterozygous larvae are similar to one of the
homozygotes (to the rovers). A further example may be the
jaw asymmetry in the scale-eating cichlid Perissodus
microlepis (Hori, 1993).
In this paper, we perform a population-genetic analysis
of a two-locus two-allele model, in which the primary locus
has a major effect on a quantitative trait that is under
frequency-dependent selection caused by intraspecific
competition for a continuum of resources. The modifier
locus determines the degree of dominance at the trait level.
Our approach differs in important respects from related
ones. Motivated by molecular-genetic considerations, Van
Dooren (1999) assumed a single locus and considered two
specific genotype–phenotype maps for which dominance
interactions between alleles derive from their promoter
affinities. His population inhabits a heterogeneous environment according to a Levene model with two demes and
soft selection. His analysis is within the adaptive-dynamics
framework, i.e., successive invasion is studied of single
mutants that change the dominance relation, each by a
small amount. Otto and Bourguet (1999) investigated a
population-genetic model similar in spirit to the present
one, but had two habitats connected by migration and
alternative alleles selectively favored in the two habitats.
We explore the conditions under which an allele
modifying the dominance relations at the primary locus
can invade and when it becomes fixed if already frequent.
These conditions are often not equivalent because an
internal equilibrium may exist. In the case of asymmetric
selection, depending on the direction, the induced dominance effect may have to be sufficiently strong for a
modifier to be able to invade. In contrast to most previous
studies, we admit modifiers with a (frequency-independent)
deleterious effect on fitness. We show that modifiers with a
modest deleterious effect can invade and rise to fixation if
their modifying effect is sufficiently large.
2. The model
Our model follows closely that of Bürger (2005). We
consider a sexually reproducing population of diploid
organisms with discrete generations. Both sexes have the
same genotype distribution and are treated as indistinguishable. The population size N may be density regulated,
but is sufficiently large so that random genetic drift can be
ignored. Natural selection acts through differential viabilities on a quantitative trait. Individual fitness depends on
two components: frequency-independent stabilizing selec-
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tion on this trait, and frequency- and density-dependent
competition among individuals of similar phenotype. A
single locus with two alleles contributes to the trait. Alleles
on a second locus, the modifier locus, determine the
dominance relations on the primary locus.
2.1. Ecological assumptions
The first fitness component of the quantitative trait is
frequency independent and may reflect some sort of direct
selection on the trait, for example, by differential supply of
a resource whose utilization efficiency is phenotype
dependent. We ignore environmental variation and deal
directly with the fitnesses of genotypic values. For
simplicity, we use the words genotypic value and phenotype synonymously.
Stabilizing selection is modeled by the quadratic
function
SðgÞ ¼ 1 sðg yÞ2 ,
(1)
where sX0 measures the strength of stabilizing selection
and y is the position of the optimum. Of course, SðgÞ is
assumed positive on the range of possible phenotypes,
which is scaled to ½1; 1. Thus, we have the constraint
0pspð1 þ jyjÞ2 . In addition, we restrict attention to the
case jyjo1, so there is always stabilizing selection.
The second component of fitness is frequency dependent.
We assume that competition between phenotypes g and h
can be described by
aðg; hÞ ¼ 1 cðg hÞ2 ,
(2)
where 0pcp14. This implies that competition between
individuals of similar phenotype is stronger than between
individuals of very different phenotype, as it will be the
case if different phenotypes preferentially utilize
different food resources. Large c implies a strong
frequency-dependent effect of competition whereas in
the limit c ! 0, frequency dependence vanishes. Let PðhÞ
denote the relative frequency of individuals with phenotype
h. Then the intraspecific competition function āðgÞ,
which measures the strength of competition experienced
by phenotype g if the population distribution is P, is
given by
X
āðgÞ ¼
aðg; hÞPðhÞ
h
and calculated to
āðgÞ ¼ 1 c½ðg ḡÞ2 þ V .
W ðgÞ ¼ 1 sðg yÞ2 þ sf ½ðg ḡÞ2 þ V ,
(4)
(5)
where the dependence of W ðgÞ on P is omitted (Bürger,
2005). There, it was shown that W ðgÞ is the weak-selection
approximation of fitness (i.e., to first order in s) in most
models of intraspecific competition for a continuum of
resources, e.g., in those of Bulmer (1974), Slatkin (1979),
Christiansen and Loeschcke (1980), Loeschcke and Christiansen (1984), Doebeli (1996), Dieckmann and Doebeli
(1999), Bürger (2002a, b), Bolnick and Doebeli (2003),
Bolnick (2004), Bürger and Gimelfarb (2004), Gourbiere
(2004), Kirkpatrick and Nuismer (2004), Schneider (2006),
Schneider and Bürger (2006). Therefore, the present results
are representative for a large class of functional forms for
fitness if selection is not too strong. Density dependence
will be treated in Section 3.6.
Because W ðgÞ is quadratic in g, selection is disruptive if
W ðgÞ is convex and the minimum is within the range of
phenotypic values, ½1; 1. For a given population distribution P, ḡ and V are constants and W ðgÞ is twice
differentiable. By straightforward calculation, we obtain
that W ðgÞ is convex if and only if f 41. The minimum lies
in the interior of the phenotypic range if and only if
f4
1þy
1 þ ḡ
and
f4
1y
.
1 ḡ
(6)
If both conditions are satisfied, f 41 holds. Therefore, the
conditions (6) are necessary and sufficient for selection to
be disruptive for every population distribution with mean
ḡ. Hence, if f 41, then selection is disruptive if ḡ is
sufficiently close to y, otherwise it is directional. If ḡ ¼ y,
then f 41 is necessary and sufficient for selection to be
disruptive. Therefore, we call intraspecific competition
strong if f 41, and weak if f o1.
2.2. Genetic assumptions and evolutionary dynamics
We consider a simple model, in which the trait value, g,
is determined by a single, diallelic locus, which we shall call
the primary locus. We label the two alleles a and A. The
alleles at the modifier locus are m and M, and they affect
the dominance relations on the primary locus as follows:
mm
(3)
Here, ḡ and V denote the mean and variance, respectively,
of the distribution P of genotypic values. In the following,
it will be convenient to measure the strength of frequencydependent competition relative to the strength of stabilizing selection. Therefore, we define
f ¼ c=s.
We shall treat f and s as independent parameters and
assume f X0.
First, we ignore density dependence and assume that
relative fitness is given by
mM
MM
aa
1
1
1
aA
a
AA
1
b
g
1
1:
(7)
We assume 0pjajobpgp1, where a can be positive or
negative. Thus, we assume that M induces a higher degree
of dominance than m. If a ¼ 0, the case to which we pay
most attention, the alleles a and A contribute additively to
the trait if M is absent. For biological purposes, it may be
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more natural to assume yX0 and to admit positive and
negative values of b and g because dominance may be
modified in either direction. In the Discussion we
reformulate our main results for this scenario. Mathematically, it is equivalent to the one used here and below
because gXb40 and yo0 is equivalent to gpbo0 and
y40. Admitting y 2 ð1; 1Þ and restricting b and g to
positive values allows a more efficient formulation and
visualization of many results. Modifiers with a direct
deleterious effect on fitness will be treated in Section 3.3.
The frequencies of the gametes am, Am, aM, and AM are
denoted by p1 , p2 , p3 , and p4 , respectively. Due to the
assumption of random mating and because gamete
frequencies are measured after reproduction and before
selection, we can use Hardy–Weinberg proportions and it
is sufficient to follow gamete frequencies. We denote the
recombination rate between the primary locus and the
modifier locus by r, and linkage disequilibrium by
D ¼ p1 p4 p2 p3 . The marginal fitness of gamete i is
denoted by W i and can be calculated from (7) and (5).
For instance, we have W 1 ¼ W ð1Þp1 þ W ðaÞp2 þ
W ð1Þp3 þ W ðbÞp4 . Mean fitness is
X
W¼
W i pi ¼ 1 sðḡ yÞ2 þ 2sfV ,
(8)
213
15 randomly chosen initial conditions, subject to the
constraint that the minimum Euclidean distance between
any pair is 0.2. More precisely, for several combinations of
s, b, and g a fine grid of values of y and f was chosen. The
equilibria and their properties were recorded. In addition
to these iterations, results were also checked by solving the
equilibrium equations numerically and by computing the
eigenvalues.
3.1. Equilibrium and stability structure for neutral modifiers
We exclude the degenerate case f ¼ 1 in which a
manifold of equilibria exists which, apparently, attracts
all trajectories. For f a0, the complexity of the model
precludes explicit calculation of all possible equilibria. We
have been able to determine all equilibria on the boundary
of the state space, which is the simplex S4 (Fig. 1). In
addition, an internal, i.e., fully polymorphic, equilibrium
may exist. Our numerical results suggest that at most one
stable internal equilibrium can exist, which is always in
linkage equilibrium. Table 1 lists the types of equilibria
found. Their properties are summarized below. A full
i
where ḡ ¼ ðp2 þ p4 Þ2ðp1 þ p3 Þ2 þ 2ap1 p2 þ 2bðp1 p4 þp2 p3 Þ
þ2gp3 p4 and V ¼ ðp2 þp4 Þ2 þðp1 þ p3 Þ2 þ2a2 p1 p2 þ 2b2 ðp1 p4
þp2 p3 Þ þ2g2 p3 p4 ḡ2 .
The genetic dynamics is given by the well known system
of recursion relations
W p0i ¼ pi W i ri W ðbÞD;
i ¼ 1; 2; 3; 4,
(9)
where r1 ¼ r4 ¼ r and r2 ¼ r3 ¼ r.
3. Results
Of prime interest are the conditions when a modifier of
dominance (M) can invade and when it becomes fixed in
the population. To this aim, we find the possible equilibria
and establish their stability properties. First, we assume a
neutral modifier and a population of constant size, for
instance, at demographic equilibrium. After considering
several special cases in Section 3.2, we relax the condition
of neutrality in Section 3.3 and investigate modifiers with a
direct deleterious effect. Whereas in Sections 3.1–3.3,
absence of dominance ða ¼ 0Þ is assumed at the primary
locus in the presence of mm, the case aa0 is the subject of
Section 3.4. The effect of recombination and the rate of
evolution are treated in Section 3.5. Finally, in Section 3.6,
we briefly report results for a neutral modifier if densitydependent population growth is admitted. Throughout, we
restrict our attention to positive recombination, r40.
Because not all properties of interest could be proved
analytically, we complement the analytical work by
numerical results. These were obtained primarily by
iterating the recursion relations (9) for a large number of
combinations of the parameters s; b; g; y, and f, each from
Fig. 1. Schematic drawing of all possible equilibria for r40.
Table 1
The five types of equilibria
(a)
(b)
(c)
(d)
(e)
Fixation of allele a, every point on the edge p1 þ p3 ¼ 1, in
particular, the monomorphic equilibria p1 ¼ 1 and p3 ¼ 1
Fixation of allele A, every point on the edge p2 þ p4 ¼ 1, in
particular, the monomorphic equilibria p2 ¼ 1 and p4 ¼ 1
A single-locus polymorphism at the primary locus with modifier
allele m fixed, i.e., p1 þ p2 ¼ 1 and 0op1 o1; denoted p^ ðmÞ
A single-locus polymorphism at the primary locus with modifier
allele M fixed, i.e., p3 þ p4 ¼ 1 and 0op3 o1; denoted p^ ðMÞ
An internal equilibrium in linkage equilibrium, i.e., D ¼ 0,
where both loci are polymorphic; denoted by p^ LE
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account of the mathematical results together with proofs is
given in the Appendix A.
3.1.1. The edge equilibria, (a) and (b)
They exist always because if the primary locus is fixed for
either A or a, modifier alleles have no effect and there is no
mutation. In general, only the stability conditions for the
monomorphic equilibria, i.e., pi ¼ 1, can be given explicitly
(Appendix A.1). Those for the equilibria on the edges can
be determined approximately by assuming weak selection,
i.e., s5r. In this case and if f 41, there is one eigenvalue
41 (and one is always 1 because these are manifolds of
equilibria), hence none can be stable if f 41 (Appendix
A.2). Our numerical results suggest that this is true for
every admissible s. Stability of any of these equilibria
implies the possible loss of all genetic variation on
the primary locus. If all edge equilibria are unstable,
there is a protected polymorphism at the primary locus.
This is always the case if f 41, the situation we are most
interested in.
3.1.2. The equilibrium (c)
^ ðmÞ
This equilibrium satisfies p^ ðmÞ
3 ¼p
4 ¼ 0, and the frequency of allele A is
1
y
^ ðmÞ
,
(10)
p^ ðmÞ
A ¼p
2 ¼ þ
2 1þf
where we denote allele frequencies by the corresponding
subscripts. It exists, i.e., satisfies 0op^ ðmÞ
A o1, if and only if
f 42jyj 1.
(11)
Hence, p^ ðmÞ exists whenever jyjo12 or f 41. We note that if
f 41, then (11) is equivalent to underdominance, whereas it
is equivalent to overdominance if f o1.
Stability of this equilibrium determines if a modifier
allele that induces dominance can invade, i.e., invasion
occurs if this equilibrium is unstable. If the optimum is
symmetric, i.e., if y ¼ 0, the condition for local stability is
simply f o1. In general, we set
f2 ¼
2y
1.
b
(12)
Then, p^ ðmÞ exists and is asymptotically stable if and only if
either
maxð0; 2jyj 1; f 2 Þof o1,
(13a)
which requires b4y, or
1of of 2 ,
(13b)
which requires boy (see Appendix A.3). To put it
otherwise, if f 41, then invasion of the modifier allele M
occurs if and only if
f 4f 2 .
(14)
Notably, the invasion condition is independent of the
recombination rate.
A simple calculation yields ḡ ¼ 2y=ð1 þ f Þ at p^ ðmÞ , and
conditions (6) show that disruptive selection acts on the
equilibrium distribution if and only if f 41. Thus, any
modifier allele with b40 can invade if yp0, whereas
sufficiently large b (or f) is required if y40. Rearrangement
of (14) shows that a modifier invades if and only if either
bo0 or b42y=ðf þ 1Þ. This condition is easily shown to be
equivalent to
W ðbÞ4W ð0Þ,
(15)
where fitnesses are evaluated at p^ ðmÞ . Thus, if y40, only
modifiers can invade that either have negative b or a
sufficiently large b, such that the fitness valley can be
crossed and a fitness gain is achieved. For graphical
illustrations, see Fig. 2.
3.1.3. The equilibrium (d)
ðMÞ
It satisfies p^ ðMÞ
¼ p^ ðMÞ
¼ 0. In general, p^ A
¼ p^ ðMÞ
is a
1
2
4
complicated solution of a cubic which does not give much
insight. In Appendix A.4.1 it is shown that p^ ðMÞ exists if
and only if
2y 1 g g 1 2y
f 4f 0 ¼ max 0;
;
.
(16)
1g
1þg
We note that f 41 implies f 4f 0 because we assume jyjo1.
If MM causes complete dominance, i.e., g ¼ 1, then p^ ðMÞ is
of much simpler form and a local stability analysis can be
performed; see Section 3.2.3.
Fig. 2. Fitness at the equilibrium p^ ðmÞ as a function of the trait value g. The positions of the resident genotypes are indicated on the horizontal axis and
thick lines correspond to values of b such that a modifier M can invade. In the left panel the modifier is neutral ðt ¼ 0Þ and in the right panel deleterious
ðt ¼ 0:01Þ. The other parameters are s ¼ 0:1; y ¼ 0:5; f ¼ 1:5 and a ¼ 0.
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Stability of equilibrium (d) determines if a modifier
inducing dominance becomes fixed if sufficiently frequent.
If it is asymptotically stable, then this is the case. Since, as
already noted, p^ ðMÞ is of very complicated form, a general
linear stability analysis seems impossible. However, if
f ¼ f 1 , where
f1 ¼
ð1 þ bgÞ2 ð2y b gÞ
,
gð2 b2 g2 Þ þ bð1 b2 g2 Þ
(17)
then one eigenvalue of p^ ðMÞ equals unity because another
equilibrium, p^ LE , passes through it. If f ¼ f 1 , then
p^ ðMÞ
A ¼
ð1 þ bÞð1 þ gÞ
2ð1 þ bgÞ
(20)
f 0 of ominð1; f 1 Þ.
This is confirmed by numerical results, cf. Fig. 3. They also
suggest that p^ ðMÞ is globally stable if f 4maxð1; f 2 Þ, (14),
and that stability is independent of r.
If f 41, fixation of M from sufficiently high frequency
occurs if f 4f 1 , which translates into a complicated
condition for b. In terms of fitnesses, it is equivalent to
(21)
W ðgÞ4W ðbÞ,
^ ðMÞ
where fitnesses are evaluated at p
.
(18)
and a local stability analysis can be performed if f ¼ f 1 þ
and and s are sufficiently small. It demonstrates that p^ ðMÞ
changes stability as p^ LE passes through at ¼ 0, and p^ ðMÞ
exists and is asymptotically stable if either
f 4maxð1; f 1 Þ
or
(19)
3.1.4. The equilibrium (e)
In general, this fully polymorphic equilibrium cannot be
determined explicitly. Numerical computations indicate
that it is always in linkage equilibrium and that no other
internal equilibrium exists. In the special case b ¼ g, when
the modifier allele M is dominant, p^ LE can be calculated
Fig. 3. Regions of existence and stability of the equilibria. In region Omo , only monomorphic equilibria and those on the edges p1 þ p3 ¼ 1 and p2 þ p4 ¼ 1
can be stable. In region O1 , p^ ðmÞ and an interval of fixed points on the edge p1 þ p3 are stable. In O2 , p^ ðMÞ and an interval of fixed points on the edge
p2 þ p4 ¼ 1 are stable. In region Om , the equilibrium p^ ðmÞ is globally asymptotically stable, and in OM , p^ ðMÞ is globally asymptotically stable. In Om_M , both
p^ ðmÞ and p^ ðMÞ are asymptotically stable, and the fully polymorphic equilibrium p^ LE exists and is unstable. Thus, depending on the initial conditions, either
m or M becomes eventually fixed. In Om^M , both p^ ðmÞ and p^ ðMÞ are unstable, and p^ LE is globally attracting. Parameter values are b ¼ 0:1 and g ¼ 0:2 in the
upper left panel, b ¼ 0:5 and g ¼ 0:6 in the upper right panel, b ¼ 0:5 and g ¼ 1 in the lower left panel, and b ¼ g ¼ 1 in the lower right panel.
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explicitly and a more detailed analysis is performed in
Section 3.2.2.
A bifurcation analysis suggests the following. If bog,
then p^ LE exists if and only if (Appendix A.5)
f 1 of of 2 .
(22)
Hence, existence requires y4b=2. As a function of f, p^ LE
enters the simplex through the equilibrium p^ ðMÞ if f ¼ f 1
and leaves it through p^ ðmÞ if f ¼ f 2 , where p^ ðmÞ
A ¼ ð1 þ bÞ=2
if f ¼ f 2 . The case b ¼ g is degenerate and needs separate
treatment (see below).
Since, in general, p^ LE cannot be calculated explicitly, a
general linear stability analysis seems impossible. Apparently, if p^ LE exists, then it is unstable if f 41, and
asymptotically stable if f o1. It exchanges stability with
p^ ðMÞ and with p^ ðmÞ when it passes through them. For
various combinations of b and g, Fig. 3 displays the regions
of existence and stability of all equilibria as a function of y
and f. The boundary between the regions Om and Om_M is
given by f ¼ f 1 , and the boundary between Om_M and OM
is given by f ¼ f 2 . The critical role of f ¼ 1 is eminent.
If f 41, condition (22) is equivalent to
W ðbÞoW ð0Þ at p^ ðmÞ
and
W ðbÞoW ðgÞ at p^ ðMÞ .
(23)
Thus, the internal equilibrium exists if and only if double
heterozygotes have a lower fitness than the corresponding
heterozygotes at the equilibria p^ ðmÞ and p^ ðMÞ . Then, p^ LE
appears to be unstable and either m or M goes to fixation,
depending on the initial gamete distribution. Similarly, if
f o1, then double heterozygote advantage at p^ ðmÞ and p^ ðMÞ
is necessary for existence of p^ LE . In this case, p^ LE appears
to be globally attracting and a modifier gets stuck at an
intermediate frequency.
3.2. Special cases
3.2.1. Symmetric optimum, y ¼ 0
If y ¼ 0, all equilibria listed in Table 1, except the
internal equilibrium (e), exist for all parameter combinations. The internal equilibrium never exists. The equilibrium p^ ðmÞ is asymptotically stable if and only if f o1.
Because we have f 1 ; f 2 o0 in this case, f 41 is sufficient for
successful invasion and fixation of the modifier. Thus, if
y ¼ 0 and f 41, any modifier increasing dominance invades
and rises to fixation.
3.2.2. M is dominant, b ¼ g
In this case, the internal equilibrium is given by
pffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi
1þg
gð1 þ 2f Þ g3 f 2y
LE
^
;
p
¼
1
¼
p^ LE
,
pffiffiffiffiffipffiffiffiffiffiffiffiffiffiffiffiffiffi
M
A
2
gf 1 g2
D^ LE ¼ 0.
ð24Þ
It exists if and only if
2y g
2y
of o 1,
2
gð2 g Þ
g
(25)
which is impossible if b ¼ g ¼ 1. Thus, y4 2g is a necessary
condition for existence. If f 41, then y4g is a necessary
condition. If f ¼ 2y=g 1, a simple calculation shows that
2yg
^ LE
p^ LE coincides with p^ ðmÞ . If f ¼ gð2g
2 Þ, then p
M ¼ 1 and, due
to the uniqueness of the fixed point p^ ðMÞ on p3 þ p4 ¼ 1,
p^ LE has to (and does) coincide with p^ ðMÞ .
If bog, then by (22) f 1 is the lower bound of the interval
for f in which the internal equilibrium exists. It is easy to
2yg
see that limb!g f 1 o gð2g
2 Þ, hence f 1 increases discontinuously at b ¼ g. Thus, the treatment in Appendix A.5 does
not extend to the present case, which is degenerate.
In addition, if b ¼ g, p^ LE enters the simplex through
2yg
p^ ðMÞ ‘rapidly’ because for f ¼ gð2g
we have
2 Þ þ ,
pffi pffi
2
g
ð2g
Þ
pffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi
ffi þ OðÞ.
p^ LE
M ¼1
2
ð1g Þð2ygÞ
3.2.3. MM causes complete dominance, g ¼ 1
In this case, the equilibrium (d) has the simple
representation
sffiffiffiffiffiffiffiffiffiffiffi
f y
ðMÞ
^ ðMÞ
; p^ ðMÞ
p^ 3 ¼
¼ 1 p^ 3ðMÞ .
(26)
A ¼ p
4
2f
It exists if and only if f 4y. Local stability of p^ ðMÞ can be
determined under the simplifying assumption of weak
selection (small s). Then, p^ ðMÞ is asymptotically stable if
and only if f 41 (Appendix A.4.2). Numerical results
suggest this to be true for any s.
If, in addition, we assume b ¼ g ¼ 1, a more detailed
analysis can be performed. It follows from (24) and (25)
that the equilibrium p^ LE does not exist in this case. The
eigenvalues of p^ ðMÞ are 1, 1 r, and l1 given by (A.16a).
The eigenvalue 1 results from the fact that M is dominant.
Therefore, the equilibrium p^ ðMÞ is asymptotically stable if
and only if f 41. In fact, it appears to be globally stable in
this case. In particular, p^ ðmÞ is unstable if f 41.
3.3. Deleterious modifiers
Most mutants have slightly deleterious fitness effects.
Here, we study whether and when evolution of dominance
can occur if the modifier is not neutral. We assume that the
fitness of a two-locus genotype is reduced by t, where
tX0 is small, if it carries one M allele, and by 2t if it
carries two M alleles. We require 2t þ sð1 þ jyjÞ2 o1, so
that all genotypes have positive fitnesses irrespective of
their frequency, cf. (1), (5).
If t40, except for the monomorphic equilibria, the edge
equilibria (a) and (b) from Table 1 no longer exist because
the frequency of M decreases along these edges. None of
the monomorphic equilibria can be stable if f 41
(Appendix A.1). Clearly, the equilibria p^ ðmÞ (c) and p^ ðMÞ
(d), which are of most biological interest, remain unchanged by admitting t40, however, their stability properties change. Also an internal equilibrium, corresponding to
(e) may exist if t40. In general, it is not in linkage
equilibrium, and it cannot be calculated explicitly.
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217
In Appendix A.3 it is shown that p^ ðmÞ is unstable, i.e., the
modifier M can invade, if
is asymptotically stable, i.e., the modifier allele M becomes
fixed if sufficiently frequent, if
to12 sbðf 1Þðb WÞð1 W2 Þ þ Oðs2 Þ,
2
^ ðMÞ
to2p^ ðMÞ
A ð1 p
A Þ½W ðgÞ W ðbÞ þ Oðs Þ.
(27)
where W ¼ 2y=ð1 þ f Þ. If f 41, the existence of a positive t
requires that b4W, which is equivalent to (14). If
W ¼ y ¼ 0, then (27) simplifies to
to12 sb2 ðf 1Þ þ Oðs2 Þ.
to12sbðf
(28)
2
The condition
1Þðb WÞð1 W Þ, the leading
order estimate in (27), is easily shown to be equivalent to
ðmÞ
to2p^ A
ð1 p^ ðmÞ
A Þ½W ðbÞ W ð0Þ.
(29)
The latter is fulfilled if and only if the mean fitness of an
invading population with genotype Mm at the modifier
locus is larger than the mean fitness of a resident
population with mm. If t ¼ 0, then (29) reduces to (15).
For the equilibrium p^ ðMÞ , no complete stability analysis
can be performed. A condition analogous to (27) is given in
Appendix A.4.4, however, it involves the allele frequency
p^ ðMÞ
A , which is a complicated solution of a cubic.
Equivalently, and in analogy to (29), we obtain that p^ ðMÞ
(30)
Such positive values of t exist provided (19) holds.
Apparently, if (30) is satisfied but not (27), then an
unstable internal equilibrium exists. By contrast, if (27) is
satisfied but not (30), then a stable internal equilibrium
exists and the modifier M can invade but converges to
some intermediate frequency. This occurs if t is sufficiently
small relative to b but too large relative to g b.
Thus, a (partially) dominant modifier M may get stuck at
intermediate frequency. A deleterious modifier can
never become fixed if g ¼ b, i.e., if it is completely
dominant (this could be proved only for b ¼ g ¼ 1, see
Appendix A.4.2).
Numerical results support the above (approximate)
analytical results and suggest that successful invasion of
the modifier M or fixation from high frequency occur if
(27) or (30) are satisfied, respectively. Fig. 4, which is
analogous to Fig. 3, displays regions of existence and
stability of equilibria for a deleterious modifier.
Fig. 4. Regions of existence and stability of the equilibria for a deleterious modifier. We have s ¼ 0:1 and t ¼ 0:01, all other parameters, as well as
notation, are as in Fig. 3. However, in Omo only p1 ¼ 1 or p2 ¼ 1 can be stable because the edge equilibria do not exist. The reader may note the different
scales for f.
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We note that (27)–(30) provide estimates for the strength
of selection on a neutral modifier close to the respective
equilibria.
dominance than mm. A further case, with t40, is also
displayed in Fig. 5.
3.5. Recombination and the rate of evolution
3.4. mm causes dominance
We briefly discuss an extension of our model. For
mathematical simplicity, we assumed so far that in the
presence of mm there is no dominance at the primary locus,
i.e., a ¼ 0. If aa0, the stability analysis of the equilibrium
p^ ðmÞ becomes mathematically equivalent to that of p^ ðMÞ .
Therefore, the invasion condition for a deleterious
modifier is
ðmÞ
^A
Þ½W ðbÞ W ðaÞ þ Oðs2 Þ.
to2p^ ðmÞ
A ð1 p
(31)
If t ¼ 0, y ¼ 0, and a40, then the modifier M can invade if
either b4a or bobc for some bc o0 (see Fig. 5, lower left
panel). Numerical results suggest that bc is always
smaller than a. Apparently, this asymmetry is due to
the position of the fitness minimum which for aa0 is in
general not at 0. Thus, Mm has to induce a higher degree of
Although the conditions for invasion and for fixation
from high frequency are apparently independent of the
recombination rate r (we have a mathematical proof only
for the independence of the invasion condition), linkage
between primary locus and modifier may have a strong
influence on the rate of evolution. If, initially, one of the
primary alleles is rare, tightly linked modifiers invade much
more rapidly and, usually, become fixed more rapidly
(Fig. 6, left panel). The initial steep increase occurs because
first the allele A increases in frequency to approximate
equilibrium proportions at the primary locus, i.e., close to
p^ ðmÞ . Then the modifier starts to increase due to his own,
indirect fitness advantage. If invasion of the modifier starts
near the equilibrium p^ ðmÞ , i.e., the primary locus is close to
equilibrium, then recombination has only a slight influence
on the rate of evolution (Fig. 6, right panel). In any case,
Fig. 5. Regions of invasion of modifier allele M as a function of y and b. In the top row, there is no dominance ða ¼ 0Þ in the absence of M; in the bottom
row, A is slightly dominant ða ¼ 0:1Þ. In the left column, different shadings correspond to regions in which a modifier M with various deleterious effects t
can invade. In the white region, no modifier can invade (even if neutral); light gray to dark gray shadings indicate regions in which modifiers with t ¼ 0,
0.004, 0.015, 0.03, 0.05 can invade. The other parameters are: s ¼ 0:1, r ¼ 0:5 and f ¼ 2. In the right column, different shadings correspond to regions in
which a modifier with deleterious effect t ¼ 0:01 can invade if f assumes the values (from dark gray to light gray) 1.25, 1.5, 2.5, and 6. If f ¼ 6 is replaced
by a larger values, the white region shrinks and, in the limit f ! 1, disappears. The other parameters are: s ¼ 0:1 and r ¼ 0:5.
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219
Fig. 6. Rate of modifier evolution. The frequency of an initially rare modifier allele M is shown for s ¼ 0:1, t ¼ 0, and a ¼ 0. Black curves are for r ¼ 0,
gray curves for r ¼ 0:5. In the left panel we have b ¼ 0:1, g ¼ 0:2, and trajectories start close to the equilibrium p1 ¼ 1, i.e., at ð0:99; 0:003; 0:003; 0:004Þ;
solid lines are for f ¼ 5, y ¼ 0, dotted lines for f ¼ 2:5, y ¼ 0, and dashed lines for f ¼ 5, y ¼ 0:3. In the right panel we have b ¼ 0:5, g ¼ 0:6, and
trajectories start close to the equilibrium p^ ðmÞ ; solid lines are for f ¼ 2:5, y ¼ 0, dotted lines for f ¼ 1:5, y ¼ 0, and dashed lines for f ¼ 2:5, y ¼ 0:6.
stronger frequency dependence (larger f) or a stronger
dominance effect (larger b, gÞ accelerate the sweep.
3.6. Population regulation
If population regulation is taken into account, fitness is
given by
W ðgÞ ¼ F ðNÞ½1 sðg yÞ2 þ sZððg gÞ2 Þ þ V ,
(32)
0
where Z ¼ ZðNÞ ¼ fNF ðNÞ=F ðNÞ and F : ½0; 1Þ !
½0; 1Þ is a strictly decreasing, differentiable function of N
such that F ðNÞ ¼ 1 has a unique positive solution K, the
carrying capacity. For more information, consult Bürger
(2005) and Thieme (2003, Chapter 9). The genetic
dynamics (9) has to be complimented by the demographic
dynamics
N 0 ¼ W N.
(33)
The inclusion of population regulation makes a detailed
mathematical analysis prohibitively complicated. Comprehensive numerical iterations show that, in general, con^ occurs much
vergence to demographic equilibrium, N,
faster than convergence to genetic equilibrium. Concomitantly, during this first phase, ZðNÞ converges to Z^ . Then,
with this value nearly fixed, convergence to genetic
equilibrium occurs as studied above. Since the value of Z^
depends on the equilibrium reached, in principle, equilibrium configurations could occur which do not exist in the
simplified model (cf. Bürger, 2005). However, we did not
find such instances.
Eq. (2.10) in Bürger (2005) shows that the population
size in demographic equilibrium can be approximated by
!
^ þ ðḡ^ yÞ2
V
N^ ¼ K þ sK 2f V^ þ
þ Oðs2 C 2 Þ,
KF 0 ðKÞ
where C ¼ maxððḡ^ yÞ2 ; V^ Þ, a ^ signifies equilibrium
values, and s is small. From this, an approximation for Z^
can be obtained (Bürger, 2005, Eq. (C.4)). For discrete
logistic growth, one obtains to leading order in s (Bürger,
2005, Appendix C):
N^ kðr 1Þ þ ksð2f V^ ðr 1Þ V^ ðḡ^ yÞ2 Þ,
Z^ f ðr 1Þ sf rðV^ þ ðḡ^ yÞ2 Þ.
With f ¼ Z^ , the local stability conditions derived above
apply. Thus, the main features of the full model appear to
be captured by the simplified model with constant
population size.
4. Discussion
Evolution of dominance under frequency-dependent
selection is an old hat. Studies have been initiated already
half a century ago in the context of evolution of mimicry
(e.g., Sheppard, 1958; Clarke, 1964; O’Donald, 1968). In
these models it is assumed that a mimic is best protected
from predators if it has an intermediate, ‘focal’ frequency.
In some of these models, rapid evolution of a modifier has
been demonstrated by numerical examples, and selective
advantages have been estimated to be considerable. This is
in contrast to Fisher’s classical model (Mayo and Bürger,
1997).
In this work, we are concerned with a different scenario,
namely with the evolution of dominance if heterozygotes
are underdominant and maintained by frequency-dependent disruptive selection. Compared with the evolution of
assortative mating and speciation, evolution of dominance
may be a genetically simple and evolutionary fast
alternative to eliminate disadvantageous heterozygotes. It
is known that evolution of dominance can occur on short
time scales, sometimes considerably less than 100 generations. The most prominent case occurred during the spread
of industrial melanism in the moth Biston betularia (e.g.,
Kettlewell, 1965).
We start with a brief summary of our results and restrict
attention to parameter values f 41, so that intraspecific
competition is strong enough to induce disruptive selection.
First, we deal with a neutral modifier, i.e., we assume t ¼ 0.
In contrast to Section 3, here we consider the ecological
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parameters s, f, and y as given (with 0pyo1Þ and ask for
which values of b and/or g the modifier M can invade
successfully and/or becomes fixed. Because heterozygotes
can be modified in both directions, we admit values b and g
such that either 0obpgp1 or 1pgpbo0.
In the absence of the modifier allele M and if a ¼ 0 in (7),
there is no dominance at the primary locus and a
polymorphism, p^ ðmÞ , is maintained whenever f 41. If
y ¼ 0, modifiers inducing any level of dominance will
invade and become fixed. If ya0, this is not so because the
minimum fitness is assumed at g ¼ y=ð1 þ f Þ, which differs
from the genotypic value 0 of the Aa heterozygote. For
ya0, negative b or sufficiently large b40 is necessary for
successful invasion (see Fig. 2). Importantly, invasion of a
neutral modifier also guarantees its eventual fixation.
Indeed, condition (14) or, equivalently, (15) implies global
fixation, i.e., from any initial condition. However, fixation
of an already frequent modifier can occur in a wider
parameter range than invasion, except when b ¼ g ¼ 1
(then invasion and fixation occur whenever f 41Þ. Fixation
from sufficiently high frequency occurs if (19) or,
equivalently, (21) holds. If (22) is valid, an internal unstable
equilibrium exists and the modifier becomes fixed only if it
is initially sufficiently frequent, a scenario which is
biologically not unrealistic and may have occurred in some
cases (Wagner and Bürger, 1985). Therefore, an invasion
analysis is insufficient to predict the evolution of
dominance.
Because a large fraction of mutations is known to be
slightly deleterious, we also investigated modifiers with a
direct deleterious effect on fitness, independent of their
modifying effect. Such modifiers can still invade if they
induce sufficiently strong dominance, i.e., if (29) holds to
leading order in s; for graphical representations, see Figs. 4
and 5. The condition for fixation of a modifier that is
already sufficiently frequent is given by (30).
If the modifier is deleterious, then an internal, stable or
unstable, equilibrium may exist. If the deleterious effect t is
sufficiently small so that M can invade, then M will
converge to some intermediate frequency if g b is too
small to outweigh the deleterious effect 2t of the MM
homozygous genotypes. In contrast, if b is relatively small
and g b is large, then invasion may be impossible but
fixation of a frequent modifier can occur (see Fig. 4). Under
the assumption of an infinitesimally small dominance effect
b, deleterious modifiers can never invade. Also for an
asymmetric optimum, modifiers of very small effect can
invade only if they push the heterozygous effect b in the
direction opposite to y.
In only a few models of modification of dominance can
modifiers with a frequency-independent deleterious effect
invade and become fixed. One, for the evolution of
mimicry, goes back to Sheppard (1958). It assumes that if
a new mutant arises, heterozygotes have a fitness advantage over both homozygotes, and modifiers may be selected
that increase the fitness of one of the homozygotes. It was
proved that such a neutral modifier always invades and
becomes fixed (Bürger, 1983). Thus, a bistable situation
does not occur. In addition, also modifiers with a slightly
deleterious fitness effect can invade and become fixed. The
present model provides another example. As is shown
explicitly by (27) and (28), condition (29) is frequency
independent given the model parameters, although p^ ðmÞ
A
enters. The same applies to (30) and (31). We note that
these conditions are similar in structure to those given by
Otto and Bourguet (1999); e.g., their Eq. (8). Thus, their
model constitutes a third example.
In Otto and Bourguet’s model with soft selection, a
polymorphism with stable underdominance is maintained.
For small migration rates, the authors provided estimates
for the (indirect) selection coefficient of an invading
dominance modifier. For high recombination rates, these
estimates are similar in structure to our condition (31) on
the deleterious effect t which, along with (27)–(30),
provides an estimate of the selection intensity on the
modifier near the respective equilibrium. Interestingly, in
Otto and Bourget’s model the selection coefficients depend
strongly on the recombination rate. Thus, their invasion
conditions depend on the linkage relation, whereas ours do
not. The reason seems to be that one allele is favored in
each deme and migration is weak, thus tight linkage
facilitates invasion and quick fixation of the modifier.
Although, Otto and Bourguet do not mention it, it can be
shown that in their model, in which modifiers have no
direct fitness effects, an internal equilibrium can exist,
which may be stable or unstable; see Peischl (2006).
Van Dooren’s (1999) model and results are difficult to
compare with ours because his parameterization is very
different and he studies the successive invasion of mutants,
as is usual in adaptive dynamics. Still, his general
conclusion, mainly based on numerical examples, that
dominance relations evolve to a certain extent if a
stable polymorphism is maintained, is qualitatively
similar to ours. In addition, he found that for some
parameter combinations alternative ESS with either no
dominance or complete dominance coexist, a situation that
may be related to our finding of an unstable internal
equilibrium.
Following Schneider (2007), a population-genetic study
of long-term evolution, i.e., successive invasions of
modifier alleles, could be performed for our model, because
a, b, and g are parameters. In contrast to adaptivedynamics methodology, in population genetics we need not
assume that the invading type differs only very slightly
from the resident type. In fact, this seems to be an
important aspect because in many empirical examples
dominance relations have changed dramatically within a
short time span, thus ‘modifiers’ seem to have large effects.
In addition, in our model modifiers of arbitrarily small
effect can invade only if they are neutral (or have a direct
beneficial effect on fitness) and if they modify dominance in
one direction (opposite to yÞ. Our population-genetic
analysis reveals that modifiers can invade under much
more general assumptions than a simple invasion analysis
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considering mutations of infinitesimally small effects would
suggest. Moreover, the conditions for invasion and fixation
are not equivalent.
If y ¼ 0, t ¼ 0 and a ¼ 0, then any modifier invades and
becomes fixed that induces some degree of dominance (i.e.,
ba0Þ. If, for instance, a40, modifiers with positive b can
invade if b4a. For negative b, it appears that bo a is a
necessary condition for successful invasion of a modifier.
Thus, only modifiers inducing a higher degree of dominance can invade and we expect that in the long run,
complete dominance of one of the alleles evolves. If yX0,
t ¼ 0, and b ¼ g ¼ 1, then p^ ðMÞ is globally asymptotically
stable and we expect that this is the only stable long-term
equilibrium. For deleterious modifiers the situation becomes more complicated, especially as it cannot be
expected that every new modifier allele has the same fitness
effect.
Evolution of dominance is one of several mechanisms by
which inheritance systems and genetic architectures can
evolve (Bagheri, 2006). Four recent theoretical studies have
shown that the genetic architecture readily evolves under
frequency-dependent disruptive selection. Matessi and
Gimelfarb (2006) studied long-term evolution at a single
multiallelic locus under frequency-dependent selection of
essentially the same form as ours. In their model,
homozygous and heterozygous effects evolve due to a
sequence of new mutations, typically in such a way that at
a long-term equilibrium (i.e., at an equilibrium that cannot
be invaded by further mutations) only the two most
extreme of all possible phenotypes are realized. Their
genetic model is highly flexible, so that different alleles can
code for the same phenotype and thus coexist, and for each
individual the phenotype associated with a given genotype
may be drawn from a distribution. van Doorn and
Dieckmann (2006) investigated numerically a multilocus
soft-selection Levene model, in which Gaussian stabilizing
selection acts on a quantitative trait in each of two patches.
If the fitness optima differ sufficiently much between
patches, after evolutionary branching, one of the loci
evolves larger and larger effects, whereas the others evolve
increasingly small effects. After a sufficiently long time, one
homozygote and the heterozygote become well adapted.
Then, evolution of dominance starts and the phenotype of
second homozygote evolves toward that of the heterozygote. Their study assumes additive genetics, i.e., no
epistasis or dominance. For an ecological scenario as in the
present paper, Kopp and Hermisson (2006) showed that in
multilocus models with epistasis but no dominance,
typically highly asymmetric genetic architectures evolve,
in the sense that one or a few loci have large effects,
whereas the other loci have very small effects. Finally,
Schneider (2007) performed a complete analysis of longterm evolution of the same ecological model as used here
and by Kopp and Hermisson. His genetic model is a
multilocus–multiallele model with no dominance and
epistasis, and he assumes linkage equilibrium. He classifies
all possible long-term equilibria and finds that a highly
asymmetric genetic architecture, as in van Doorn and
Dieckmann (2006) and Kopp and Hermisson (2006),
evolves only if the range of possible effects at some locus
is sufficiently large to span the full range of ecologically
favored phenotypes.
The above findings provide further support for the
suggestion of Wilson and Turelli (1986) that stable
underdominance could mediate rapid evolution of dominance, although an analytical proof within their model
seems impracticable. These findings show that evolution of
dominance or, more generally, evolution of genetic
architecture is a potent mechanism to remove unfit
heterozygotes which naturally occur under disruptive
selection. Whether and when evolution of dominance is
indeed more efficient or rapid than evolution of assortative
mating remains to be studied.
Acknowledgment
We thank J. Hermisson, K. Schneider, and T. van
Dooren for useful comments on the manuscript. This
work was supported by grant P16474-N04 of the
Austrian Science Foundation (FWF) and by a grant of
the Vienna Science and Technology Fund (WWTF). The
Program for Evolutionary Dynamics is supported by
Jeffrey Epstein.
Appendix A. Existence and stability of equilibria
We do not give complete algebraic proofs here, which
would be very lengthy. However, all the formulas given can
be easily checked with Mathematica or similar software.
Unless otherwise stated, we admit aa0 and tX0.
A.1. Monomorphic equilibria
The eigenvalues of the four monomorphic equilibria
are readily determined and are quite simple, even if
initially there is some degree of dominance, i.e., aa0,
and the modifier is deleterious, i.e., t40. Clearly,
the two edges of equilibria do not exist if the modifier is
deleterious.
The eigenvalues of p1 ¼ 1 are
l1 ¼
ð1 rÞf1 t þ s½ð1 bÞ2 f ðb yÞ2 g
,
1 sð1 þ yÞ2
l2 ¼ 1
l3 ¼
t
,
1 sð1 þ yÞ2
1 þ s½ð1 þ aÞ2 f ða yÞ2
.
1 sð1 þ yÞ2
(A.1a)
(A.1b)
(A.1c)
Obviously, all eigenvalues are positive and l2 o1. Further,
2
1sð1þyÞ
we have l1 o1 if and only if r4rc1 ¼ 1 1tþs½ð1bÞ
.
2
f ðbyÞ2
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It can easily be seen that rc1 o0 if and only if
f of r1
l3 ¼
t
b 1 2y
.
þ
¼
2
1þb
sð1 þ bÞ
(A.2)
The eigenvalue l3 is smaller than 1 if and only if
f of c1 ¼
a 1 2y
.
1þa
(A.3)
Since f c1 is monotonically increasing in a, we have f r1 4f c1 .
Therefore, p1 ¼ 1 is asymptotically stable if and only if
f of c1 ; in particular, stability does not depend on r.
The eigenvalues of p2 ¼ 1 are
l1 ¼
ð1 rÞf1 t s½ð1 bÞ2 f ðb yÞ2 g
,
1 sð1 yÞ2
l2 ¼ 1
t
,
1 sð1 yÞ2
(A.4a)
(A.4c)
2
1sð1yÞ
have l1 o1 if and only if r4rc2 ¼ 1 1ts½ðbyÞ
.
2
ð1bÞ2 f
We have l1 o1 for every rX0 if and only if
t
2y 1 b
.
þ
1b
sð1 bÞ2
(A.5)
In addition, l3 o1 if and only if
2y 1 a
.
1a
(A.6)
to 2sðbaÞð1bÞð1yÞ
.
1a
It follows that f r2 of c2 if and only if
Thus, for sufficiently small r and t, it is possible that
l1 414l3 . Hence, stability may depend on r. A necessary
condition for stability is f of c2 .
The eigenvalues of p3 ¼ 1 are
l1 ¼
ð1 rÞf1 þ t þ s½ð1 þ bÞ2 f ðb yÞ2 g
,
1 2t sð1 þ yÞ2
(A.7a)
t
,
1 2t sð1 þ yÞ2
(A.7b)
1 2t s½ðg yÞ2 f ð1 þ gÞ2
,
l3 ¼
1 2t sð1 þ yÞ2
(A.7c)
l2 ¼ 1 þ
and those of p4 ¼ 1 are
l1 ¼
ð1 rÞf1 t s½ð1 þ bÞ2 f ðb yÞ2 g
,
1 2t sð1 yÞ2
l2 ¼ 1 þ
t
,
1 2t sð1 yÞ2
If t40, then l2 41 holds in both cases because fitnesses of
all genotypes have to be nonnegative, i.e., 2t þ sð1 þ
jyjÞ2 p1 must hold. Thus, neither p3 ¼ 1 nor p4 ¼ 1 can
be locally stable.
If t ¼ 0, one eigenvalue is always unity because of the
two edges of equilibria. In this case, it can be shown that no
monomorphic equilibrium can be stable if
a 1 2y 2y 1 a g 1 2y 2y 1 g
;
;
;
f 4max
.
1þa
1a
1þg
1g
(A.9)
As a consequence of our constraints on the parameters,
monomorphic equilibria can never be stable if f 41, i.e., if
there is disruptive selection.
A.2. Edge equilibria
Again, all eigenvalues are positive and l2 o1. Here, we
f of c2 ¼
(A.8c)
(A.4b)
1 þ s½ða yÞ2 ð1 þ aÞ2 f
.
l3 ¼
1 sð1 yÞ2
f of r2 ¼
1 2t s½ðg yÞ2 f ð1 gÞ2
.
1 2t sð1 yÞ2
(A.8a)
(A.8b)
Here, we assume t ¼ 0 because otherwise no equilibria
exist on the edges p1 þ p3 ¼ 1 and p2 þ p4 ¼ 1 except the
monomorphic ones. Because the edges p1 þ p3 ¼ 1 and
p2 þ p4 ¼ 1 consist of equilibria, one eigenvalue is always
1. The other two are the solutions of complicated quadratic
polynomials. Under the assumption of weak selection,
however, relatively simple expressions are obtained that
allow simple conclusions. To leading order in s, the two
nontrivial eigenvalues on p1 þ p3 ¼ 1 are given by 1 r þ
OðsÞ and
1 þ sf2ð1 þ yÞ½1 þ að1 pM Þ2 þ 2bpM ð1 pM Þ þ gp2M
þ ðf 1Þ½1 þ aða þ 2Þð1 pM Þ2 þ 2bðb þ 2ÞpM ð1 pM Þ
þ gðg þ 2Þp2M g þ Oðs2 Þ.
The latter clearly is 41 whenever f 41. Hence, none of the
equilibria can be stable.
To leading order in s, the two nontrivial eigenvalues on
p2 þ p4 ¼ 1 are given by 1 r þ OðsÞ and
1 þ sf2ð1 yÞ½1 að1 pM Þ2 2bpM ð1 pM Þ gp2M
þ ðf 1Þ½1 þ aða 2Þð1 pM Þ2
þ 2bðb 2ÞpM ð1 pM Þ þ gðg 2Þp2M g þ Oðs2 Þ.
Here, the latter is 41 whenever f 41 because 1 þ aða 2Þ
X0 for a 2 ½1; 1. Hence, again, none of the equilibria can
be stable if f 41.
Numerical iterations suggest that if both monomorphic
equilibria are stable/unstable, the same holds for all
equilibria in between. If one is stable and the other is
unstable, then stability changes exactly once on this edge.
Examples are given and proved in Peischl (2006).
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A.3. The equilibrium p^ ðmÞ
A.3.1. The case a ¼ 0
This case is much simpler than aa0 because the
equilibrium can be calculated explicitly if a ¼ 0. It is given
by (10). The eigenvalue determining stability within the
edge p1 þ p2 ¼ 1 is
2
l1 ¼ 1
223
If t ¼ 0 and under the assumption of weak selection
(small s), asymptotic stability of p^ ðmÞ changes as f passes
through f 2 ðaÞ, where
f 2 ðaÞ ¼
ð1 þ abÞ2 ð2y a bÞ
,
að2 a2 b2 Þ þ bð1 b2 a2 Þ
(A.12)
cf. Sections A.4.3 and A.4.4 for more details.
2
sð1 þ f Þ½ð1 þ f Þ 4y
.
2ð1 þ f Þ2 þ s½ð1 þ f Þ2 ð2f 1Þ þ 2yð1 2f f 2 Þ
(A.10a)
We have l1 o1 if and only if f 42jyj 1, i.e., whenever this
equilibrium exists. The other two eigenvalues are the
solutions of a complicated quadratic equation. To leading
order in s, they are given by
(A.13)
o1 ¼ 2½1 þ f þ g2 ð3f 1Þ þ 2gð3f þ yÞ,
ðA:10bÞ
2
þ 14st½ð2f 1Þð2 W2 Þ þ f 2 W2 þ Oðs2 Þ,
hðxÞ:¼o0 þ o1 x þ o2 x2 þ o3 x3 ¼ 0,
o0 ¼ ð1 þ gÞð1 þ f þ gðf 1Þ þ 2yÞ,
þ rð1 2b2 þ 2bW W2 Þ
l3 ¼ 1 t þ 12sbðf 1Þðb WÞð1 W Þ
A.4.1. Existence
On the edge p3 þ p4 ¼ 1, where M is fixed, an internal
equilibrium is a solution p3 ¼ x 2 ð0; 1Þ of
where
l2 ¼ ð1 rÞð1 tÞ þ 12sðf 1Þ½bðb WÞð1 þ W2 Þ
þ 14stð1 rÞ½ð2f 1Þð2 W2 Þ þ f 2 W2 þ Oðs2 Þ,
A.4. The equilibrium p^ ðMÞ
o2 ¼ 12gf ð1 þ gÞ,
o3 ¼ 8g2 f .
We have
ðA:10cÞ
where W ¼ 2y=ð1 þ f Þ. Unless r is small relative to s, it
follows that l3 determines stability, and (27) is
obtained immediately. If t ¼ 0, then conditions (13a) are
obtained.
For general s, the characteristic polynomial evaluated at
x ¼ 1 is given by
s2 bðf 1Þ½ð1 þ f Þ2 4y2 ½bð1 þ f Þ 2yA
p1 ¼
,
½ð1 þ f Þ2 ð2 þ sð2f 1Þ 2sy2 Þ þ 4sy2 3
where
A ¼ sbðf 2 1Þ½bð1 þ f Þ 2y
rf2 2sðb yÞ2 þ f ð4 þ s 2sb2 Þ
þ 2f 2 ½1 þ sð1 þ b2 2by y2 Þ þ f 3 sð1 þ 2b2 Þg.
Because p^ ðmÞ exists only if ð1 þ f Þ2 44y2 , the stability
properties of p^ ðmÞ can change only if f ¼ 1 or f ¼ f 2 or
A ¼ 0.
However,
we
have
Ao0
whenever
ðf 1Þ½bð1 þ f Þ 2yo0, which is satisfied if and only if
one of conditions (13a) is fulfilled. Therefore, stability is
independent of r and always given by (13a).
A.3.2. The case aa0
The analysis of this case is mathematically equivalent to the
analysis of the equilibrium p^ ðMÞ , but with g and a exchanged
(see below). Therefore (16), p^ ðmÞ exists if and only if
2y 1 a a 1 2y
;
.
(A.11)
f 4max 0;
1a
1þa
Each of the following conditions is sufficient for existence:
f 41, jyjo12, or 2y 1oao2y þ 1.
hð0Þ ¼ o0 o0
if and only if
f4
g 1 2y
.
1þg
(A.14)
In addition, we get
hð1Þ ¼ ð1 gÞð1 þ g þ f ð1 gÞ 2yÞ40
if and only if
f4
2y 1 g
.
1g
(A.15)
Thus, if f 40, then hð0Þ40 and hð1Þo0 cannot hold.
If h has no or one critical point, then it is strictly
monotonically increasing because it is a cubic and o3 40.
Hence, a unique equilibrium exists if and only if hð0Þo0
and hð1Þ40.
Otherwise, h has two critical points, y1 oy2 , with
h0 ðy1 Þ ¼ h0 ðy2 Þ ¼ 0. Because h00 ðxÞ ¼ 24gf ð1 þ g 2gxÞ,
we have h00 ðy1 Þo0, h00 ðy2 Þ40 and y2 41. Hence, y1 is a
local maximum and y2 is a local minimum. Consequently,
if hð0Þo0 and hð1Þ40, then there exists a unique solution
of hðxÞ ¼ 0 in ð0; 1Þ. If hð0Þo0 and hð1Þo0, the following
argument shows that no solution exists in ð0; 1Þ. Because
hð0Þohð1Þ, we have hð0Þohð1Þo0 if and only if (A.15) is
violated, i.e., if and only if
b1 ¼ 12½f ð1 gÞ þ 1 þ goy.
This requires f o1 and y40. In addition, a simple
rearrangement shows that
pffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffiffi!
g2 þ 2f 1 2gy
1
1
pffiffiffiffiffi
y1 ¼
1þ
41
2
g
3f g
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S. Peischl, R. Bürger / Journal of Theoretical Biology 251 (2008) 210–226
(assuming, of course, g2 þ 2f 1 2gyX0Þ is equivalent to
b2 ¼
g2 1 f ð1 6g þ 3g2 Þ
oy.
2g
p^ ðMÞ
A ðÞ ¼
Another simple calculation shows that b2 ob1 if f o1, thus
hð0Þohð1Þo0 implies y1 41, and therefore no solution in
ð0; 1Þ can exist. In the third and last possible case, hð0Þ40
and hð1Þ40, no solution in ð0; 1Þ exists because y2 41.
Summarizing, a unique equilibrium exists if and only if
hð0Þo0 and hð1Þ40, i.e., if both (A.14) and (A.15) hold.
Simple calculations show that each of the following
conditions is sufficient for existence: f 41, jyjo12, or
g þ 142y4g 1.
A.4.2. Stability if g ¼ 1
If g ¼ 1, we obtain hðxÞ ¼ 4ð1 xÞðf þ y 4fxþ 2fx2 Þ,
and p^ ðMÞ is given by (26). Then, the eigenvalues can be
calculated explicitly. The eigenvalue determining stability
within the edge p3 þ p4 ¼ 1 is
pffiffiffiffiffi pffiffiffiffiffiffiffiffiffiffiffi
4sðf yÞ3=2 ð 2f f yÞ
.
(A.16a)
l1 ¼ 1
f ½1 þ sð2f 1 y2 Þ
Recall that existence of p^ ðMÞ requires f 4y. It is readily
shown that l1 40 and l1 o1 if and only if f 4jyj. The
other two eigenvalues are the solutions of a complicated quadratic equation. To leading order in s and t,
they are
l2 ¼ ð1 rÞð1 þ tÞ þ OðsÞ þ Oðt2 Þ,
(A.16b)
pffiffiffiffiffiffiffiffiffiffiffi
l3 ¼ 1 þ t sð1 f 1 Þð1 b2 Þ f y
pffiffiffiffiffi pffiffiffiffiffiffiffiffiffiffiffi
ð 2f f yÞ þ Oðs2 Þ þ OðstÞ þ Oðt2 Þ.
ðA:16cÞ
If t is sufficiently much smaller than r, then stability is
determined by l3 . Therefore, p^ ðMÞ is asymptotically stable
if, approximately,
tosð1 f 1 Þð1 b2 Þ
pffiffiffiffiffiffiffiffiffiffiffi pffiffiffiffiffi pffiffiffiffiffiffiffiffiffiffiffi
f yð 2f f yÞ.
(A.17)
Because yp1, the right-hand side is positive if f 41. It
increases nearly linearly in f. Therefore, p^ ðMÞ is locally
asymptotically stable if t is sufficiently small. If t ¼ 0, then
p^ ðMÞ is asymptotically stable whenever f 41.
If b ¼ g ¼ 1, then the eigenvalues can be calculated
explicitly, and we obtain
l3 ¼ 1 þ
t
1 2t sð1 2f þ y2 Þ
is given by
through p^ ðMÞ . If f ¼ f 1 þ , p^ ðMÞ
A
(A.18)
and l2 ¼ ð1 rÞl3 . Thus, M cannot become fixed
if t40.
ð1 þ bÞð1 þ gÞ
þ a,
2ð1 þ bgÞ
(A.19)
where a is a complicated expression. The eigenvalue
determining stability within the edge p3 þ p4 ¼ 1 is
given by
l1 ¼ 1 s
ð1 b2 Þð1 g2 Þa1
2ð1 þ bgÞ2 ½gð2 g2 b2 Þ þ bð1 b2 g2 Þ
þ Oðs2 Þ þ OðsÞ þ Oð2 Þ,
where
a1 ¼ g½1 þ 3g2 2g4 þ 3bgð1 g2 Þ þ 6bg
þ b2 ð3 þ bg þ 3g2 þ bg3 Þ
þ 2yð1 4g2 þ 2g4 3bg 3b2 g2 b3 g3 Þ.
We have l1 o1 whenever f 1 41 because this implies
yXb þ gX0. Since, a1 40 if y ¼ 0 and if y ¼ 1, it follows
that a1 40 for every y 2 ½0; 1.
The value of the characteristic polynomial for the other
two eigenvalues at l ¼ 1 can be shown to be
rsðg bÞð1 b2 Þð1 g2 Þ
½gð2 g2 b2 Þ þ bð1 b2 g2 Þ2 þ 4að1 g2 Þð1 þ bgÞ3 ð2y b gÞ
2ð1 þ bgÞ4 ½gð2 g2 b2 Þ þ bð1 b2 g2 Þ
þOðs2 Þ þ Oð2 Þ.
Therefore, the equilibrium changes stability at ¼ 0 as
increases from below 0 to above 0, i.e., as p^ LE enters the
simplex. In fact, numerical evaluation of the nominator
shows that it is always positive (although a is negative).
Because the derivative of the characteristic polynomial at 1
is r þ OðsÞ, it follows that p^ ðMÞ becomes stable as p^ LE moves
through, i.e., if 40.
A.4.4. Deleterious modifier M
By comparing the mean fitness of a population which is
in equilibrium with respect to the first locus and is
homozygous for M with an analogous population which
heterozygous at the modifier locus, we find that the
condition for fixation of M should be given by (30). If
fitnesses are calculated explicitly, this becomes
^ ðMÞ
to2p^ ðMÞ
A ð1 p
A Þsðg bÞ½ðb þ gÞðf 1Þ þ 2ðy þ f Þ
^ ðMÞ
4f p^ ðMÞ
A ð1 þ gð1 p
A ÞÞ,
ðA:20Þ
ðMÞ
where p^ A
is given as the unique solution of the cubic
(A.13). The same stability result is obtained by calculating
the (otherwise very complicated) eigenvalues to first order
in s and in t (also omitting terms of order st).
A.5. The equilibrium p^ LE
A.4.3. Stability near f ¼ f 1
Here, we assume t ¼ 0. As f increases from below f 1 (17)
to above f 1 , the equilibrium p^ LE traverses into the simplex
Here, we assume a ¼ 0 and t ¼ 0. With Mathematica it is
straightforward to check that if f ¼ f 2 ð40Þ and bo1,
ARTICLE IN PRESS
S. Peischl, R. Bürger / Journal of Theoretical Biology 251 (2008) 210–226
then the following internal equilibrium exists:
p^ LE
A ¼
1þb
ðg bÞgb2
þ
þ Oð2 Þ,
2
2
2
4½ygðg bÞ þ b ð1 b Þð2y bÞ
(A.21a)
p^ LE
M ¼
b3
þ Oð2 Þ,
2½ygðg bÞ þ b2 ð1 b2 Þð2y bÞ
LE
D^ ¼ Oð2 Þ.
(A.21b)
(A.21c)
A similar analysis can be performed for f ¼ f 1 þ .
Then, the internal equilibrium is given by
p^ LE
A ¼
ð1 þ bÞð1 þ gÞ
þ a1 þ Oð2 Þ,
2ð1 þ bgÞ
(A.22a)
2
p^ LE
M ¼ 1 ðg bÞa2 þ Oð Þ,
(A.22b)
LE
D^ ¼ Oð2 Þ,
(A.22c)
where a1 and a2 are complicated, positive expressions in b,
g and y. Eqs. (A.22) do not give a valid equilibrium in the
case b ¼ g, which turns out to be degenerate, see Section
3.2.2.
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