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A Neutral Model With Fluctuating Population Size and Its Effective Size
Masaru Iizukaa, Hidenori Tachidab, and Hirotsugu Matsudaca Division of Mathematics, Kyushu Dental College, Kitakyushu 803-8580, Japan,
b Department of Biology, Graduate School of Sciences, Kyushu University, Fukuoka 810-8560, Japan
c Kyushu University, Fukuoka 812-8581, Japan
Corresponding author: Masaru Iizuka, Kyushu Dental College, 2-6-1 Manazuru, Kokurakita-ku, Kitakyushu 803-8580, Japan., iizuka{at}kyu-dent.ac.jp (E-mail)
Communicating editor: W. STEPHAN
| ABSTRACT |
|---|
We consider a diffusion model with neutral alleles whose population size is fluctuating randomly. For this model, the effects of fluctuation of population size on the effective size are investigated. The effective size defined by the equilibrium average heterozygosity is larger than the harmonic mean of population size but smaller than the arithmetic mean of population size. To see explicitly the effects of fluctuation of population size on the effective size, we investigate a special case where population size fluctuates between two distinct states. In some cases, the effective size is very different from the harmonic mean. For this concrete model, we also obtain the stationary distribution of the average heterozygosity. Asymptotic behavior of the effective size is obtained when the population size is large and/or autocorrelation of the fluctuation is weak or strong.
THE average heterozygosity has been one of the most frequently used measures of genetic diversity. A large amount of data have been accumulated to estimate the average heterozygosity of various species using protein electrophoresis (see, for example, ![]()
![]()
![]()
![]()
![]()
![]()
![]()
![]()
![]()
One of the reasons that heterozygosity has been used for measuring genetic diversity is a simple relationship between its expectation and population genetic parameters under the neutrality assumption (![]()
, where u is the mutation rate (![]()
The size of the population is, however, hardly constant and it may fluctuate from generation to generation. In such cases, it is necessary to understand how fluctuation of population size would affect genetic diversity and summary statistics such as H. For this end, the effects of fluctuation of population size on the effective size of population Ne must be clarified and a representation for Ne must be obtained. By this representation, the expected heterozygosity may be expressed as
and it shows how the fluctuation of population size affects H.
Fluctuation of population size is not independent from generation to generation in general as in the case of stochastic selection (![]()
![]()
![]()
![]()
![]()
![]()
![]()
![]()
![]()
![]()
![]()
In this article, we consider the diffusion model with neutral K (2
K
) alleles whose population size is fluctuating randomly, incorporating the effect of mutation. First, we consider a general case with respect to the fluctuation of population size and we show that the effective size defined by the equilibrium average heterozygosity is larger than the harmonic mean of population size but smaller than the arithmetic mean of population size. Then we consider a special case of a two-valued Markov chain as a model of the fluctuation of population size. This simplification enables us to obtain explicit formulas for the stationary distribution of the average heterozygosity and the effective size. We can see quantitatively how the effective size is different from the harmonic mean using the latter formula.
| NEUTRAL MODEL WITH FLUCTUATING POPULATION SIZE |
|---|
Before we introduce the fluctuation of population size, we summarize some of the known results on the constant population model (![]()
![]()
i). Under the diffusion approximation (diffusion model), let xi(t) be the gene frequency of Ai at time t. We denote by
[·] the operation taking the expectation with respect to the random sampling drift. Then the average heterozygosity
![]() |
(1) |
at time t satisfies the differential equation
![]() |
(2) |
(see Appendix A), which has the solution
![]() |
(3) |
and
![]() |
(4) |
where we put
![]() |
(5) |
Note that the case of K =
is the infinite allele model (![]()
and
. By this formula, the population size N can be expressed as
![]() |
(6) |
A large amount of ecological data suggest that numbers of individuals in natural populations fluctuate considerably in each epoch and from generation to generation (![]()
![]()
![]()
![]()
100,000 years in the last 700,000 years. Organismal populations were thought to have responded to such climate shifts by changing their habitats (![]()
![]()
![]()
![]()
Now we consider the cases when population size fluctuates and let N(t) be the size of a haploid population at time t. In this article, we assume that {N(t)}-
<t<
is a stationary stochastic process that does not depend on gene frequencies {(x1(t), x2(t), ... , xK-1(t))}t
0. In other words, the stochastic process that governs the change in population size is independent of the genetic structure of the population. We consider a diffusion model whose population size at time t is N(t) (for the precise meaning of this model, see Appendix A). This model is referred to as the neutral diffusion model with fluctuating population size and the case of K =
is referred to as the infinite allele model with fluctuating population size. For this model, the average heterozygosity H(t) satisfies
![]() |
(7) |
(see Appendix A). The solution of this differential equation is
![]() |
(8) |
Note that {H(t)}t
0 is a stochastic process induced by {N(t)}-
<t<
.
Let
![]() |
(9) |
and
![]() |
(10) |
be the arithmetic mean and the harmonic mean of N(t), respectively. Here E[·] is the operation taking the expectation with respect to the probability law of N(t). On the other hand, the effective size of population Ne can be defined as
![]() |
(11) |
by (6). Then we have
![]() |
(12) |
(see Appendix B). The effective size of the population is larger than the harmonic mean but smaller than the arithmetic mean by (12). Note that this result holds for any fluctuation of N(t) as far as 1/N(t) is integrable and H(t) is described by (7). This result is general in this sense but we cannot see how much Ne is larger than Nh or how much it is smaller than Na. For this end, we must consider a concrete example of the fluctuation of N(t), which is discussed in the next section. As we noted before, the effective size is said to be equal to the harmonic mean of the population size when population sizes are not constant in the literature (![]()
![]()
![]()
![]()
![]()
| TWO-VALUED MARKOV CHAIN MODEL |
|---|
To see how the effective size of population Ne depends on the probability law of {N(t)}-
<t<
and to what extent Ne is different from Nh and Na, we consider a special case of a continuous time two-valued Markov chain for {N(t)}-
<t<
. Let {N(t)}-
<t<
be a Markov chain on {N1, N2} such that
![]() |
(13) |
(
t
0), where N1 < N2. Here,
i is the jump rate from the state Ni to Nj (j
i) and lim
t
0 (o(
t)/
t) = 0. Note that the stationary probabilities for N(t) = N1 and N(t) = N2 are
![]() |
(15) |
![]() |
(16) |
respectively, where we put
![]() |
(17) |
Note that r = 1/2 for the symmetric case of
1 =
2. The autocorrelation of {N(t)}-
<t<
can be defined by
![]() |
(18) |
where Var[N(0)] and Cov[N(0), N(t)] are the variance of N(0) and the covariance of N(0) and N(t), respectively. Since
![]() |
(19) |
where
![]() |
(20) |
we have
![]() |
(21) |
and N(t1) and N(t2) are positively autocorrelated (t1
t2).
Let p(h, Ni) and p(h) be the stationary probability density functions of (H(t), N(t)) and H(t), respectively (i = 1, 2). Applying the results of ![]()
![]() |
(22) |
![]() |
(23) |
and
![]() |
(24) |
(H1 < h < H2), where
![]() |
(25) |
![]() |
(26) |
and
![]() |
(27) |
is the beta function (p, q > 0; see Appendix C). The stationary probability density function p(h) of the average heterozygosity is presented in Fig 1 for the case of K =
, 2N1u = 0.1 (H1 = 0.09), and 2N2u = 1 (H2 = 0.5). The solid line, the dotted line, and the dashed line represent the cases of
1 =
2 = 0.5,
1 =
2 = 1, and
1 =
2 = 2, respectively. The stationary probability density function p(h) is bell shaped if
1,
2 > 1 (the jump rates
1 and
2 are large) and it is U shaped if 0 <
1,
2 < 1 (the jump rates
1 and
2 are small). Note that the equilibrium heterozygosity H(
) is a random variable due to the stochastic fluctuation of population size and the distribution function of H(
) is
![]() |
(28) |
|
(H1 < h < H2). Then we have
![]() |
(29) |
and
![]() |
(30) |
where
![]() |
(31) |
As noted above, the variance is due to the stochastic fluctuation of population size. Thus, the variance quantifies the extent of variation expected among average heterozygosities of independent populations whose sizes obey the same probability law. The variance should not be mixed up with that among the average heterozygosities of respective loci in one species, because those loci are considered to have experienced the same population history. The conditional stationary probability density function of H(t) given N(t) = N1 is
![]() |
(32) |
and that given N(t) = N2 is
![]() |
(33) |
Then the conditional expectation of H(
) given the population size being N1 is
![]() |
(34) |
and that given the population size being N2 is
![]() |
(35) |
Note that E[H(
)|Ni] is the expectation of the equilibrium average heterozygosity knowing that the population size at the observation time is Ni. It is easy to see
![]() |
(36) |
as we expect. On the other hand, the conditional stationary probabilities of N(t) = N1 and N(t) = N2 given H(t) = h are
![]() |
(37) |
and
![]() |
(38) |
respectively. Note that p(Ni|h) is the stationary probability that the population size is Ni knowing that the average heterozygosity is h.
Now we have an explicit expression for Ne. By (11) and (29), we have
![]() |
(39) |
since
![]() |
(40) |
Note that Ne depends on the mutation rate u. By (39), Ne is an increasing function of the measure of autocorrelation
(a decreasing function of
) if we fix the value of r (note that Nh does not depend on
if we fix the value of r). To see how much Ne > Nh, we consider the ratio of the effective size to the harmonic mean
![]() |
(41) |
where
![]() |
(42) |
and
![]() |
(43) |
The dependence of log10(Ne/Nh) on log10(N2/N1) is presented in Fig 2 for the case of
1 =
2, K =
, and
2 = 1. The solid line, the dotted line, and the dashed line represent the cases of
2 = 0.1,
2 = 1, and
2 = 10, respectively. The ratio Ne/Nh can be very large if N1 << N2 and the jump rate
is not large. For example,
if
and
. On the other hand,
if
and
. Note that Ne/Nh and log10(Ne/Nh) are decreasing functions of the scaled mutation rate
2 and the values of log10(Ne/Nh) for
2 < 1 are larger than those in Fig 2 if we fix log10(N2/N1) and
2.
|
Noting that
![]() |
(44) |
we can express Ne in terms of Na and Nh,
![]() |
(45) |
where
![]() |
(46) |
and
![]() |
(47) |
(0 < RK < 1). Note that we have obtained explicit expressions for Ne [i.e., (39) and (45)] by introducing the two-valued Markov chain model.
The size of population N(t) may be very large in natural populations. Further, the autocorrelation of {N(t)}-
<t<
may be very weak or strong. In such cases, we can consider the asymptotic behavior of Ne. For this end, we parameterize N1, N2, Ne, Nh, Na,
1,
2,
, V, u, and RK by
(
0) such as N
1, N
2, N
e, N
h, N
a, 
1, 
2, 
, V
, u
, and R
K. Here, we assume that
and
do not depend on
for simplicity. Note that N
a/N
h does not depend on
in this case. For simplicity, we assume that the limits
![]() |
(48) |
and
![]() |
(49) |
exist (0
,
). By
![]() |
(50) |
and (45), it is easy to see that
![]() |
(51) |
if
=
or
=
,
![]() |
(52) |
if
= 0 and
= 0. The cases that
=
, 0 <
<
, and
= 0 are referred to as weak autocorrelation, moderate autocorrelation, and strong autocorrelation limits, respectively. In the same way, the cases that
= 0, 0 <
<
, and
=
are referred to as weak mutation, moderate mutation, and strong mutation limits, respectively. By (51) and (52), the effective size is asymptotically equal to the harmonic mean in the case of weak autocorrelation or strong mutation and the effective size is asymptotically equal to the arithmetic mean in the case of strong autocorrelation and weak mutation. Note that, in the case that r and b do not depend on
, weak, moderate, and strong autocorrelation limits correspond to lim
0
, and lim
0
, respectively.
The Wright-Fisher model with fluctuating population size is investigated by ![]()
![]() |
(53) |
The effective size N*e is smaller than the harmonic mean if the change in population size is negatively autocorrelated, it is larger than the harmonic mean if the change is positively autocorrelated, and it is equal to the harmonic mean if the change is uncorrelated. These results are consistent with those for the diffusion model in this section. Note that the change in population size is positively autocorrelated in our formulation through the diffusion model in this section. In other words, the introduction of the fluctuation of population size after the diffusion approximation implies that this fluctuation cannot be uncorrelated or negatively autocorrelated. There are some properties on asymptotic behavior of the Wright-Fisher model with fluctuating population size that are consistent with those of the diffusion model in this section. For example, the effective size is asymptotically equal to the harmonic mean in the case of weak autocorrelation for both models (see ![]()
The Wright-Fisher model with fluctuating population size is more fundamental than the diffusion model with fluctuating population size since the stochastic effect of fluctuation of population size is introduced after the diffusion approximation for the latter model. It seems not to be easy, however, to incorporate the effect of mutation into the Wright-Fisher model with fluctuating population size. It is easy to incorporate the effect of mutation into the diffusion model with fluctuating population size since the differential equation for H(t) is linear. Furthermore, we can consider a very general pattern of fluctuation of population size for the diffusion model with fluctuating population size as we have shown in this article.
| DISCUSSION |
|---|
Here, we discuss some biological relevance of our results. Suppose that we are interested in effects of selection on genetic variation in a species. Effects of weak selection depend on population size (![]()
![]()
![]()
![]()
![]()
![]()
![]()
![]()
![]()
![]()
![]() |
(54) |
is expressed as
![]() |
(55) |
where E[H(
)]u
u(1-z) is the value of E[H(
)] with the total mutation rate u being replaced by u(1 - z). Then we can obtain the joint frequencies of alleles by (6) of ![]()
![]() |
(56) |
since
![]() |
(57) |
and
![]() |
(58) |
where
is the value of
and
is the value of dE[H(
)]/du when u = 0. The same method may be applied to microsatellite allele frequencies. For example, (11a) of ![]()
![]()
![]()
2m, where µ and
2m are the parameters describing the mutation scheme for microsatellite alleles.
| ACKNOWLEDGMENTS |
|---|
We thank A. Shimizu for noting the result of ![]()
Manuscript received August 13, 2001; Accepted for publication February 11, 2002.
| APPENDIX A |
|---|
Let f(x1(t), x2(t), ... , xK-1(t)) be an arbitrary function of gene frequencies in the neutral diffusion model. We denote by
[·] the operation taking the expectation with respect to the random sampling drift. By the general theory of diffusion processes (see ![]()
![]()
![]() |
(A1) |
where
![]() |
(A2) |

Substituting
![]() |
(A3) |
for f(x1, x2, ... , xK-1) in (A1), we have
![]() |
(A4) |
Noting that
![]() |
(A5) |
we have (2) by (A1).
The neutral diffusion model with fluctuating population size is defined as a diffusion model with a random parameter by replacing N in (A2) with the stationary stochastic process N(t). In other words, this model is defined as a diffusion process in random environments. We have (7) in the same way as we have (2).
| APPENDIX B |
|---|
For a function f(x) with
![]() |
(B1) |
for any x, y, and t (x
y, 0 < t < 1), and for a random variable X, we have
![]() |
(B2) |
unless
almost surely (see ![]()
![]()
, we have
![]() |
(B3) |
and
![]() |
(B4) |
By (B4) and the definition of Ne in (11), we have
![]() |
(B5) |
By using the inequality (B2) again for
, we have
![]() |
(B6) |
and
![]() |
(B7) |
Then we have
![]() |
(B8) |
by (B7) and (11).
| APPENDIX C |
|---|
For the two-valued Markov chain model, (7) can be expressed as
![]() |
(C1) |
if
, where
![]() |
(C2) |
We can regard (C1) as an ordinary differential equation, one of whose parameters stochastically changes. Note that H1
H(t)
H2 if H1
H(0)
H2.
By (2.17) of ![]()
![]() |
(C3) |
(H1 < h < H2), where C is the normalization constant. By this formula, we have (22) and (23).
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, and
. The solid line, the dotted line, and the dashed line represent the cases of
, and
, respectively.















, and
. The solid line, the dotted line, and the dashed line represent the cases of
, and 































