
162 7. Birth and Population Increase from Matrix Population Models
P
s−1
w
s−1
= λw
s
.
Since w can be scaled at will, let w
1
= 1, and then solve for successive
values. This gives the stable age distribution, with abundances of each age
class measured relative to the abundance of the first:
w
1
=1
w
2
= P
1
λ
−1
w
3
= P
1
P
2
λ
−2
.
.
.
w
s
= P
1
P
2
···P
s−1
λ
−s+1
, (7.2.5)
which is directly analogous to (5.1.1),
.
i
P
i
corresponding to l(x)andλ
−i
corresponding to e
−rx
.
7.2.3 Imprimitive Matrices
An imprimitive matrix A has d eigenvalues with the same absolute mag-
nitude, where d is the index of imprimitivity. Only one of these eigenvalues
(λ
1
) is real and positive; the others form angles in the complex plane of
θ =2π/d, 4π/d,...,(d − 1)2π/d, and are thus either complex or, if d =2,
negative. The common magnitude of this set of d eigenvalues is strictly
greater than the magnitude of any of the remaining eigenvalues, so as
t →∞only the d leading eigenvalues have any influence on population
dynamics.
Cull and Vogt (1973, 1974, 1976) and Svirezhev and Logofet (1983) dis-
cuss the resulting dynamics in detail. Because of the complex eigenvalues,
the stage distribution does not converge, but instead oscillates with a pe-
riod d, as does the total population size. Suppose that d = 3, and consider
(7.2.3). The eigenvalues λ
2
and λ
3
are now complex, and |λ
2
| = |λ
3
| = λ
1
.
Using (7.1.31) for λ
t
i
, the limit (7.2.4) is replaced by
n(t)
λ
t
1
→ c
1
w
1
+ c
2
(cos θt + i sin θt)w
2
+ c
3
(cos θt − i sin θt)w
3
(7.2.6)
as t →∞.Sincew
2
and w
3
and c
2
and c
3
are complex conjugates, the
imaginary parts of (7.2.6) cancel out, so that n(t) is real, as it should be.
From (7.2.6) it follows that w
1
is still a stable stage distribution in the
sense that, if n(0) is proportional to w
1
,sothatc
2
= c
3
= 0, the population
will remain at that structure for all time. However, w
1
is not stable in the
sense that an initial population not proportional to w
1
will converge to it.
Instead, the limit in (7.2.6) is periodic, with period d.
Cull and Vogt (1973) show that a running average of n(t), with the
average taken over the period of the oscillation, converges to w
1
and grows