Evolution: Cosmic, Biological,
Social
13
bones, neurons, muscles, gases, etc. (see also Hall and Fagen 1956). In many
cases we are dealing with very complex systems that are found in many places
(Haken 2005: 16). The emergence of forms of greater complexity results from
the transition from one evolutionary level to another. The general principles re-
lated to the functioning and development of such objects can be described by
general system theory. The concepts of self-organization and transition from
equilibrium to a non-equilibrium state are also relevant in this respect. In addi-
tion, both biotic and abiotic systems show complex interactions with their envi-
ronment that can be described in terms of general principles.
In the fourth place, mega-evolutionary trajectories can be considered as
components of a single process, and their different phases can be regarded as dif-
ferent types of macroevolution that could be similar in terms of their main trends
and directions as well as particular mechanisms. This will be discussed in more
detail below.
In the fifth place, we can speak about common vectors of megaevolution as
well as common causes and conditions during the transition from one level of
organization to another.
11
There is a number of very important categories that
are relevant for the analysis of all phases of megaevolution, most notably self-
organization, stable and chaotic states, phase transition, bifurcation, etc.
Because of our rapidly growing knowledge of the universe, on the one hand,
and, simultaneously, our lack of reliable information about many of its aspects,
on the other hand, arguments regarding the issue of whether our world is
‘strange’, fortuitous (see, e.g., Davies 1982, 1985, etc.), or ‘regular’ remain ra-
ther polarized (see, in particular, Kazyutinsky 1994). At present, we are dealing
with conflicting paradigms that are hard to falsify, while even the very notion of
what ‘regular’ means is not sufficiently rigorously defined (see Grinin and Ko-
rotayev 2009: ch. 1 for more detail). For this reason, modern cosmological the-
ories and hypotheses sometimes exhibit directly opposing ideas. For example,
according to Panov (2008a), the cosmological theory of ‘chaotic inflation’ im-
plies that there is not just one universe, but in fact, an unlimited number of
them, while all those universes can possess entirely different physics. As
a result, life may be possible in some universes and impossible in others. Since
we emerged in a universe where the life was possible, we observe the set of pa-
rameters that corresponds to the so-called ‘anthropic principle’.
12
However, it
may be that the
cosmologies of inflation, the multiverse, and string theory do not
have any relevance for reality as we observe it. The fundamental constants may
11
The problem of evolutionary transitions from one level of megaevolution to another is discussed
in a number of contributions to the present Almanac (Spier, Snooks, Grinin, Markov, Korotayev,
Heylighen).
12
The anthropic principle (that does not have any generally accepted wording yet) maintains
the presence of a link between the large-scale properties of the expanding universe and the emer-
gence of life, intelligence, and civilizations within it (see, e.g., Kazyutinsky 1994).
Introduction. Evolutionary Megaparadigms
14
simply have the observed values just because they cannot have any other values
due to some yet unknown fundamental physical laws (Panov 2008а: 54–55).
At least five basic aspects can be identified that help us to recognize sub-
stantial similarities between different evolutionary forms and processes:
13
1) the ‘starting’ level/aspect, consisting of a minimum number of general
characteristics of matter and energy that are, apparently, determined at the very
beginning of space and time. These fundamental characteristics allow us to
identify the most basic common denominator for different evolutionary levels in
terms of entropy/energy, self-organization potential, etc.;
2) ‘genetic-hierarchical’ levels/aspects, because any new form of evolution
must be connected with the previous ones;
3) ‘interaction and adaptation’: emerging levels of organization may ‘tune
up’ their parameters compared to preceding evolutionary forms, while at
the same time all forms of evolution depend on each other; hence, there is a cer-
tain kind of ‘accommodation’ between them;
4) ‘behavioral’ aspects: different forms of matter can sometimes behave ra-
ther similarly in certain conditions. They can acquire similar structures, while it
may also be possible to detect similar phases, cycles, rhythms and patterns. As
a result, by concentrating on similarities instead of differences in details we
may be able to formulate certain general principles concerning the ‘behavior’
of objects at various levels of evolution;
5) trends in, and possible direction of, evolution: this aspect has attracted
the attention of especially those evolutionists who seek to define evolution in
terms of transitions from less complex/developed systems to more com-
plex/developed ones. Major issues include the following questions: Are these
trends large-scale (for example of intergalactic level) or more localized, such as
of the planetary scale and below? Is this dynamics cyclical or linear, like, for
example, the rise and demise of certain societies? Do we need the anthropic
principle to explain this? Currently, no consensus exists on these and many other
issues of this kind. However, there can be no doubt that a great number of
trends can be observed in megaevolution, which needs to be explained.
* * *
We can now provide a fuller, yet still preliminary, characterization of evolu-
tionary megaparadigms. First of all, this involves general evolutionary laws,
characteristics, and principles; vectors, levels, and rhythms of mega- and mac-
roevolution as well as similarities of ‘behavior’ of different forms of matter in
13
In particular, many processes that take place at different evolutionary levels are described by
similar basic models; their phase portraits are also often very similar, which makes it possible to
detect a number of important common traits in many different evolutionary processes (Cher-
navsky 2004: 83).