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Some interesting overview information in "Complexity Measures in Manufacturing Systems" by DeTony et al. (Not sure how accurate some of the characterizations of the different complexity measures are.)
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Evolutionary informatics, a branch of information theory, studies the informational requirements of evolutionary processes. Its most significant result is a conservation principle. According to this principle, the information needed to find a successful search is never less than the information required to make the original search successful. Consequently, the higher-level search for a search is never easier than the original lower-level search. Conservation of information implies that information, like money or energy, is a commodity that obeys strict accounting principles. Accordingly, searches, in successfully locating targets, cannot expend more information than originally deposited. Conservation of information has far-reaching implications for evolutionary theory, pointing out that the success of evolutionary processes in exploring biological configuration space always depends on preexisting information. In particular, evolutionary processes cannot create the information required for their success from scratch.
- William Dembski, "What Does Information Tell Us About ID?", Salvo
Treating the empirical time scale of the evolution theoretically as infinity they have then an easy game, apparently to avoid the concept of purposesiveness. While they pretend to stay in this way completely ‘scientific’ and ‘rational’, they become actually very irrational, particularly because they use the word ‘chance’, not any longer combined with estimations of a mathematically defined probability, in its application to very rare single events more or less synonymous with the old word ‘miracle’.”
-- Wolfgang Pauli to Niels Bohr, 2/15/1955, letter 2015 in von Meyenn (2001), p.105
Physicists love to think about systems that take only a little information to describe. So when they get a system that takes a lot of information to describe, they use a trick called 'statistical mechanics', where you try to ignore most of this information and focus on a few especially important variables. For example, if you hand a physicist a box of gas, they'll try to avoid thinking about the state of each atom, and instead focus on a few macroscopic quantities like the volume and total energy. Ironically, the mathematical concept of information arose first here—although they didn't call it information back then; they called it 'entropy'. The entropy of a box of gas is precisely the amount of information you've decided to forget when you play this trick of focusing on the macroscopic variables. Amazingly, remembering just this—the sheer amount of information you've forgotten—can be extremely useful... at least for the systems physicists like best.He goes on to say that in biology, there is a lot less information in the system that can be forgotten... This goes back somewhat to the use of "entropy" to correlate to different kinds of information. The (average) loss of uncertainty/entropy in Shannon information, for example. He goes on to talk about alleles as rival hypotheses.
The analogy is mathematically precise, and fascinating. In rough terms, it says that the process of natural selection resembles the process of Bayesian inference. A population of organisms can be thought of as having various 'hypotheses' about how to survive—each hypothesis corresponding to a different allele. (Roughly, an allele is one of several alternative versions of a gene.) In each successive generation, the process of natural selection modifies the proportion of organisms having each hypothesis, according to Bayes' rule!It appears that this approach looks at information in terms of a distance from a destination state of stability. So in that sense, it is more about relative information.
But what does all this have to do with information? . . . first discovered by Ethan Atkin. Suppose evolution as described by the replicator equation brings the whole list of probabilities pi — let's call this list p —closer and closer to some stable equilibrium, say q. Then if a couple of technical conditions hold, the entropy of q relative to p keeps decreasing, and approaches zero. Remember what I told you about relative entropy. In Bayesian inference, the entropy q relative to p is how much information we gain if we start with p as our prior and then do an experiment that pushes us to the posterior q. So, in simple rough terms: as it approaches a stable equilibrium, the amount of information a species has left to learn keeps dropping, and goes to zero! . . . You can find [precise details] in Section 3.5, which is called "Kullback-Leibler Divergence is a Lyapunov function for the Replicator Dynamic". . . . 'Kullback-Leibler divergence' is just another term for relative entropy. 'Lyapunov function' means that it keeps dropping and goes to zero. And the 'replicator dynamic' is the replicator equation I described above. . . . [This approach] uses information geometry to make precise the sense in which evolution is a process of acquiring information.Baez offers some background to this in Gavin E. Crooks' Measuring thermodynamic length and in part 1 of his series.
But when we’ve got lots of observables, there’s something better than the variance of each one. There’s the covariance matrix of the whole lot of them! Each observablefluctuates around its mean value
… but these fluctuations are not independent! They’re correlated, and the covariance matrix says how.
All this is very visual, at least for me. If you imagine the fluctuations as forming a blurry patch near the point, this patch will be ellipsoidal in shape, at least when all our random fluctuations are Gaussian. And then the shape of this ellipsoid is precisely captured by the covariance matrix! In particular, the eigenvectors of the covariance matrix will point along the principal axes of this ellipsoid, and the eigenvalues will say how stretched out the ellipsoid is in each direction!
I am not a physicist, but I suppose it is possible to theorize about an atomic nucleus with a million protons. But what if I want to create one? It appears that producing transuranic elements takes huge amounts of time/energy and the greater the number of protons, the more time/energy it takes. It is even conceivable (to me at least) that there is not enough time/energy available (at least on earth) to actually produce one. Like the prime factorization ofIn his 1979 paper "Time, Space, and Randomness," Adleman develops an idea about "K-potency" motivated by an analogy with thermodynamics, specifically chemical reactions that take much less time going in one direction than the other., it may exist in theory but not in reality. On the other hand, physicists from Russia and America, using lots of time/energy, have created an atomic nucleus with 118 protons called Ununoctium. Ununoctium is analogous to Childers’ prime factorization; both exist in reality; both were very costly to create.
Conscious understanding is a comparatively slow process, but it can cut down considerably the number of alternatives that need to be seriously consideredand thereby greatly increase the effective depth calculation.In other words, a flash of insight can cross large distances of "logical depth" a la Charles H. Bennett. Insight is like a wormhole, a directed wormhole, through solution space.
Another thing: If it is an easy thing to make a protein for any particular effect, why isn't it exceptionally easy to make a protein that really gums up the works? either ties itself into a useless little knot or turns into something that binds with all sorts of things it shouldn't and kills its organism (slowly or quickly)? The need to maintain the structural and functional integrity of an evolving protein severely restricts the repertoire of acceptable amino-acid substitutions1, 2, 3, 4. However, it is not known whether these restrictions impose a global limit on how far homologous protein sequences can diverge from each other. Here we explore the limits of protein evolution using sequence divergence data. We formulate a computational approach to study the rate of divergence of distant protein sequences and measure this rate for ancient proteins, those that were present in the last universal common ancestor. We show that ancient proteins are still diverging from each other, indicating an ongoing expansion of the protein sequence universe. The slow rate of this divergence is imposed by the sparseness of functional protein sequences in sequence space and the ruggedness of the protein fitness landscape: ~98 per cent of sites cannot accept an amino-acid substitution at any given moment but a vast majority of all sites may eventually be permitted to evolve when other, compensatory, changes occur. Thus, ~3.5 × 109 yr has not been enough to reach the limit of divergent evolution of proteins, and for most proteins the limit of sequence similarity imposed by common function may not exceed that of random sequences.