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Senescence from Reproduction
John Thoms, Peter Donahue, Naeem Jan
To cite this version:
John Thoms, Peter Donahue, Naeem Jan. Senescence from Reproduction. Journal de Physique I,
EDP Sciences, 1995, 5 (8), pp.935-940. �10.1051/jp1:1995173�. �jpa-00247117�
Classification Physics Abstracts
02.50-r 05.20-y 87.10+e
Short Communication
Senescence ftom Reproduction
John
Thoms,
Peter Donahue and Naeem JanPhysics Department, St. Francis Xavier University, Antigonish, Box 5000, Nova Scotia, B2G 2W5, Canada
(Received
2 June 1995, accepted 7 June1995)
Abstract. We present results from Monte Carlo simulations of a modified
"bit-string"
model of Penna which show that ageing or senescence may be the result of reproduction over anextended period, as expected from mutation accumulation. This mduces an effective form of
antagonistic pleiotropy. We also obtain a double maxima in the distribution of the age at which death occurs. These results may be relevant to current theories of ageing.
The
understanding
of themechanism(s)
ofageing
or senescence is one which is not without interest tobiologists
and others.Ageing
is the termcommonly
used to describe thededining
functional
capacities
of the matureorganism.
Thisproblem, although
mentioned in theBible,
was
recognised
in the scientific literature asearly
as 1870by
RusselWallace,
and his themewas
developed
laterby Weismann, Haldane, Hamilton,
Medawar and othersIll.
Thistheory
asserts that
ageing
is the result of lateacting
deleterious mutations which areweakly
selectedby
natural selection at
reproduction.
The presence of these "bad" mutations in the individual areexpressed
late in life and decrease theability
of the organism to carry out its normalfunctions;
this makes the
organism
moresusceptible
toinjury,
disease and then death. Anothertheory
assumes that genes which are beneficial to the
juvenile
may turn out to be detrimental iii theadult. This
theory
is referred to iii the literature asautagonistic pleiotropy
aud was consideredin various forms
by
Darwin,Medawar, Williams,
Charlesworth and othersIll.
We propose to
study
the consequences of a model of mutation accumulation. The"bit-string"
model of Penna [2] is a suitable
starting point.
In this model we have 64 genes,representing
an
individual,
which may be either "on" or "off"(0
or1).
At the start we generate a random sequence of states,representing optimal
fitness for the environment, which we refer to as theoptimal
sequence. Dur initialpopulation
consists of 20000 individuals half of whom bave theoptimal
sequence. This was necessary to ensure that there wasa
surviving
group alter the first 10 years. In this version of the model we do trot allow for survival over trie age of 64, but with trie parameters considered very few live over trie age of 35 anyway. Eachorganism,
atbirth,
is
given
thegenetic string
of its parent, but weallow,
withequal probability
for either0,
1 or© Les Editions de Physique 1995
936 JOURNAL DE PHYSIQUE I N°8
2
hereditary point
mutations at birth. This is doneby simply switching
arandomly
selected gene of the parent from its present state to theopposite
state.Given a
population
we increment the age, 1, of each individual in thepopulation by
onela year)
and this is
represented by
theexpression
of the i~h gene. Thenewly expressed
gene iscompared
to its counterpart in the
optimal
sequence. Ifthey
agree, then this represents a"good"
genebut if
they disagree,
then this is considered a deleterioushereditary
mutation. All the earlierexpressed
genes are also active and the total deleterioushereditary
mutations is theHamming
distance between the active segment of the
genetic string
and thecorresponding
segment of theoptimal
sequence. Also at each year we allow each member toacquire
a deleterious somatic mutation. A deleterious somatic mutation is one which is detrimental to theorganism
but is not transmitted to itsoff-spring.
This mutation occurs withprobability
0.01 in each year and triesum of these mutations is retained. After each member of trie
population
basaged
we measurethe average number of deleterious mutations per individual. This average is determined from the total deleterious mutations which has occurred to ail the
organisms
so far in their life(hereditary plus somatic).
We next check the members of trie
population
for survival. There are several hurdles: We compute a deathprobability,
pd~~
exp(r(b a))
+ 1 ~~~where b is trie average number of mutations per individual and a is the number of mutations of trie individual concerned and r, which is set
equal
to 10 in thiswork, plays
trie role of an inversetemperature for our Fermi function [3]. This value of r
gives
a lowprobability
of survival for those individuals below the average fitness andcorrspondingly
ahigh probability
of survival for those whose fitness is greater than b. If a random number is less than pd then trieorganism
is removed from the
population.
Environmental limitationsplaced
onfood,
space, andnesting
sites are taken into account
by
an ageindependent
Verhulst term whichgives
each invididuala
probability
ofil N(t)/k)
ofstaying
alive. k is the carryingcapacity
of the environment which is set to100,000
at the onset, andN(t)
is thepopulation
at the year t. k is about 10 timeslanger
than triesteady
statepopulation
which isapproximately
8500. Triesurviving
members are those who are able to avoid these two hurdles.
After the
grim
reaper we consider birth. Each member of thepopulation
in the age group ii to 25 isgiven
a 50 percentprobability
togive
birth to anoff-spring.
Theoff-spring
isgiven
moreor less the same
genetic
sequence as the parent. The maximum number of point mutations allowed in thebaby
is 2 and as we havedescribed,
thissimply
means that a maximum of 2 genesare switched from their present state. No further
hereditary point
mutations are allowed for this individualduring
its life time, thus all other deleterious mutations that occur are somatic.We now discuss the results from
simulating
this model. We have monitored thepopulation
to establish that we have reached thesteady
state.Figure
i shows thesteady
state age distribution after 2000 years. Similar curves are obtained alter 1000 years. Note theexponential decay
and also that very few members survive after the age of 25.Figure
2 shows the average number ofdeletenous mutations in the
steady
statepopulation
with age. Weclearly
see that the average number of mutations in thejuvenile (less
thon10)
is verysmall,
whereas the average number of deleterious mutations increasesrapidly
after the age of là- We measure the average number of deleterioushereditary
mutations per individual between the ages of I and 12 and report 0.157,whereas,
between the ages of13 and 25 we find 1.712.Figure
3 shows thefrequency
at which death occurs with age. We collected these data over 1000 years in thesteady
state. There are twopeaks
one near the age of 5 and the other nearAGE DISTRIBUTION
900
800 °
700
> 6°° °
O °
~z
500 °
Q o
~
~ 400 °
o o
300 °
o o
200 o
°
o o
100 o
~ °
o o
~ o
0 5 10 15 20 25 30 35
AGE
Fig. i. The age distribution of the population at 2000 years.
the age of 21. As far as we are aware, this is the first report of such a curve from theoretical considerations of a model of
ageing.
Asexpected, (Fig. I),
very few individuals survive after the age of 25. In order to understand the nature of the firstpeak
we show inFigure
4 thenumber of mutations in each age group. We have not normalised
by
the number of membersin each age group. We see that the
interplay
between thepopulation
distribution with age and theprobability
ofexpressing
a deleterious mutation, which increases with age, isresponsible
for the firstpeak.
The secondpeak
reflects the upper limit of selection at the onset ofinfertility.
Here we sec clear demonstration of the mutation accumulation without selection pressure trie individuals become unfit. This is reinforced in
Figure
5 where we show trie survivalratio,
N(t)/(N(t I)).
Here we see a more or less constant survival ratio up to trie age of 15 and this decreases toapproximately
o-S at age 25. This is trie random limit where trieprobability
of a deleterious mutation is o-S in the
steady
statepopulation.
We have shown that the Penna
"bit-string"
model is well suited forsimulating
the consequences of the mutation accumulationtheory
ofageing.
We have included a fitness function whichis
responsive
to trie overall fitness of triepopulation.
This is a natural method to include trie RedQueen
[4] effect as thepopulation
evolves tohigher
fitness. We are also able toimpose environmental tolerance to an individual's deviation from the average fitness. This is
accomplished by simply tuning
the r parameter in our Fermi function. We observed the total number of deleterious mutations per individual under trie age of12 and between trie ages of 13 and 25 and find that it differsby
a factor of 10. We mayinterpret
this asreflecting
a type ofantagonistic pleiotropy.
Triejuvenile
issimple
fitter on average thon the adult. This seems to be a natural consequence of mutation accumulation. We intend to indude in a futurestudy
trie effects of a
slowly evolving
environment. We will allow the"optimal"
sequence toslowly
mutate with time. This will introduce aspects of the
Bak-Sneppen
[Si model where co-evolutionof a
self-organised
critical system leads to extinction on all scales. Anothertopic
of interest is whathappens
when aparental
care factor is introduced into the model.Any youth
with a938 JOURNAL DE PHYSIQUE I N°8
Ave~ge Mu~tion w& Age
D.Q
° o
0.8
~ ~ o
o
à Ù-fi o
fl S o
f
0.5ce °
fi
g o
< °.~
o 0.3
o
0.2 Q
o
°
0.1
~ ~ o ° ° ~
~ o o o o °
~ o ° °
0
0 5 10 15 20 25 30 35
AGE
Fig. 2. The average number of mutations per individual for each age group with the fertility range being from Ii to 25. Note trie rapta increase at 15 years.
AGE ATDEATH
o
o ~
6000 ° °
o
o ~
5000 °
o o
~
~ o
o o ° °
° ° o o ~
4000 z
" o
à
j~ 3000 °
o
2000
o
1000 o
o
o
° o o
~
o 5 10 15 20 25 30 35 40
AGE
Fig. 3. The frequeucy of death with age for the case where the fertility range is from Ii to 25. The first peak is sensitive to number of hereditary point mutations allowed at birth.
Tata Mutations withAge 35
o o
o o
30 °
o
~ o
25 °
o o
°
o ~
fl 20 ° °
o
O °
P °
~ o ~
1
15° o
o io
o
5 o
o o
o °
0 5 10 15 20 25 30 35
AGE
Fig. 4. The sum of the mutations for the individuals in each age group, independent of the size of each group.
Sumkal Ratio wth Age
o o
o o-fi
S ~ o o
4 o ~ o
% É
z o o
0.4
~ o
0.2
0
0 5 10 15 20 25 30 35
AGE
Fig. 5. The survival ratio as a function of age for the case where the fertility range is from ii to 25.
940 JOURNAL DE PHYSIQUE I N°8
living
parent would have a greater chance ofsurviving.
Acknowledgments
We welcome the opportuuity to thank Professor Stauffer
(who
isperformiug self-experimeuts
ou
ageing)
and his collaboratorsPenna,
Moss de Oliveria and Bemardes forkeepiug
us informed of their work aud also for encouragement. This research issupported
in partby
NSERC ofCanada and a UCR grant from St. Francis Xavier
University.
References
Ill
Rose M.R., Evolution Biology of Aging(Oxford
University Press, Oxford, 1991), and see refer-ences therein for earlier literature; Charlesworth B., Evolution
in Age-Structured Populations, 2nd edition
(Cambridge
University Press, Cambridge,1994).
[2] Penna T.J.P., J. Star. Phys. 78
(1995)
1629; Bernardes A.T. and Staulfer D., submitted(1995);
Penna T.J. and Staulfer D., Înt. J. Med. Phys. C6
(1995)
233; Moss de Oliveria S., Penna T.J.P.and Staulfer D., Physica A215
(1995)
298. Earlier simulations are reviewed by Staulfer D., Braz.J. Phys. 26
(1994)
900.[3] Amitrano Ç., Peliti L. and Saber M., Molecular Evolution on Rugged Landscapes: Proteins, ANA
and the Immune System, A.S. Perelson and S-A- Kaulfman, Eds.
(Addison-Wesley
Publishing Co.,Redwood City,
1991).
[4] Ridley M., Trie Red Queen
(Macmillan
Publishing Co., New York,1993).
[5] Bak P. and Sneppen K., Phys. Reu. Lent. 71
(1993)
4083; Ray T.S, and Jan N., Phys. Reu. Lent.72