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The power of chance

My interest in natural science dates back to my early childhood. My father, a school teacher (mathematics, industrial arts, physical exercise) was always ready to answer the usual questions of little ones in a satisfying way. Soon, I developed my own theories on the world around me. When I switched from elementary to secondary school, I was conviced that our physical world was an endless row of universes. I imagined our solar system as an atom with the sun as nucleus and the planets as electrons. Similarly, I was speculating about inhabitants on the planets in our body and all objects around, living on the electrons of the atoms constituting ordinary matter.
I was careful enough to keep this theory to myself, as long as I had no proof for it. Nevertheless, I was ready to propose a much easier way to look for extra-terrestrial civilizations than to struggle with distances of dozens and hundreds of lightyears and the rather limited velocity of light. We just should keep an eye on our own microscopic worlds and explore in more detail the surfaces of its electrons. The final nail in the coffin of my secret Matroschka theory of the world was convincingly provided by quantum theory. But every time when I think about a 'theory of everything', this old concept of mine comes to mind.
Also another approach to deal with our reality has deep roots in my curriculum. In the early eighties, during my thesis, evaluating the results of experiments was still predominately some paper & pencil work. My old lab notes are full of hand-made diagrams. When I was confronted with the problem of fitting experimental data to a non-linear function with 4 parameters, I turned to our high end electronic instrument, an HP 35 pocket calculator. Based on intuition, I wrote a program that allowed the iterative adaptation of the 4 parameters according to random numbers ('Monte Carlo simulation'). I obtained plausible solutions after hours of run time.
Unfortunately, it soon turned out that the results of each run differed from each other considerably. It took me days and weeks of calculation time to explore a landscape of plausible results, pointing to the existence of an absolute minimum. At this stage of my endavor I looked for help at our IT department, where I was introduced to the iterative curve fitting methods as used by Gauss & Newton already at the beginning of the 18th century. I was granted access to the local 'super-computer' and introduced to the fabrication of punched cards ('Lochkarten') to enter my data.
Happily I retured to the lab with a stack of computer printouts and enjoyed the now accessible 'true' values, including even the standard deviations (from the diagonal elements of the matrix). I was able to teach our famous pocket calculator the new technique. Basically, the procedure solved 4 equations with 4 variables. Even secondary school knowledge would have allowed me to do this, some hours of careful pencil & paper work included (the calculator was done with it in a few seconds).
In the year 2020, the COVID-19 crisis rekindled my interest in fitting data to non-linear functions. I collected the pandemic-related death toll from 28 nations (Wiki, WHO) and fitted the time course to an exponential function with an increasing number of terms. I started with the good old Gauss-Newton algorithm on my HP 28S; later, I switched to the more powerful web site originally conceptualized by John Pezzullo. When the emergency state was over, I used the data as material to resurrect my old idea: fitting parameters in a random way.
Some time courses resulted in multiple solutions of almost identical fitting quality. I came to these results offline on an old notebook (Microsoft Excel 2010), after having written the first 'macro' in my life. Fitting reached Gauss-Newton quality after run times of 30-60 min. Most functions consisted of 4-6 terms each requiring 3 parameters. This was quite some progress in comparison with my first allempt of random fitting back in the eighties. This time, the 'Monte Carlo' approach added some specific quality to the matter, something the Gauss-Newton method was unable to yield.
Extracting facts on the basis of data and models is always an insecure procedure. Data contain measurement error, and models are mostly chosen by intuition. Allowing random variation during complex fitting procedures adds a certain quantum of realism into the analysis. On the one hand, the obtained result will disappoint our hope for clarity; on the other, it will prevent us from premature conclusions. It is old mathematic wisdom that you cannot secure more parameters out of an analysis than the number of independent relationships analyzed. The essence is to spell out all relationships in precise detail, but often knowledge about them is limited (if not totally missing)..
In case of further dimensions in addition to our conventional 4-dimensional space-time (as suggested in earlier accounts of mine), we may collect data on the influence of observation and communication, but analysis will be hampered by the absence of any formalism expressing potential connections or dependencies. Instead of expecting direct relationships allowing the setup of equations, we rather may be left with stochastic approaches. In the realm of observation and communication it is mostly a question of yes or no (digital instead of analog). Instead of measurement, the preferred tool will probably be the (very rough) estimate of probabilities.
Of course, we will not get out more than we invested. Also the (hopefully) obtained results will treat more dimensions than our conventional space-time. For hard-core natural scientists, they will have some casual, non-scientific appeal. This would not be the case, if we would interact with non-terrestrial civilizations by speed-of-light channels (which is not possible). Interaction with non-solar civilizations (see link below 'On the likelihood...') will only be possible in a full-dimensional way (whatever that means).
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On the likelihood of rare events
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