malawi_glenn said:
What are the "real" problems in physics? Can these problems we solved solely by mathematicians? What are your thoughts on that?
Knowing that one does not know what one does not know. It applies to a current situation of some physics (a natural phenomenon) that has been overlooked, probably because it was/is unexpected.
coquelicot said:
The tendency to present a jungle of equations as a well established theory. The problem is real: you have to spend two years to understand the equation jungle, just to realize that there is no clear directing idea behind them. And the worse is that you can even not criticize the theory, because you will be considered as an idiot for not understanding the (alleged) idea behind the equations. The book of de Groot I am trying to study may be an example of that (not sure, I'm just beginning). That's bad for the physics, because some problems may be considered to be solved while they are actually not
Not so much 'well-establish', but perhaps established enough to solve a problem (behavior of a physical system in which a multitude of phenomena are occurring, and one would like to describe different aspects in an economical way). Economical can mean solving a problem on a workstation (multicore), or a small cluster or work stations, and not a supercomputer with 100,000 cores, and I want an answer within 24 hour (or less ideally) and not a week, or weeks, or longer. And the solution shouldn't take MWh (MJ) of energy, but maybe many kWh (KJ).
Is the argument about how physicists use mathematics or describe the mathematics (or mathematical tools) employed in solving a problem, or describing a problem.
When I began studying physics in earnest, in high school then university, I quickly realized that I needed a firm background in mathematics, at least calculus, and then advanced calculus, but I didn't seen the need for subjects like group theory.
Consider some 'small' problems, or pieces of physics, involving photon interactions in matter, and simultaneously, interactions of electrons (and positrons) in the same matter, and the response of that matter to the population of photons, electrons and positrons moving through it (I haven't introduced neutrons yet). I have dozens of elements (atoms) jiggling about. Ideally they stay near there initial location before the photons, electrons, positrons (and neutrons) starting flying about. And there's more physics to add - transmutation of atoms (one element to another) and cations wanting to meet up with anions.
Consider the mathematics in this text describing the theory applied in the PENELOPE code.
https://www.oecd-nea.org/upload/doc...mulation_of_electron_and_photon_transport.pdf
It only covers part of the physics of photons, electrons, positrons (and doesn't involve neutrons, atomic displacements/diffusion, nuclear transmutations, nuclear fission, chemical reactions). The output is generally the energy deposition (dose) in some structure of matter, which could be simply a volume of water, air, human tissue, medical plastics, a detector material (NaI, GeLi, . . . ), semiconductors, ceramics (e.g., SiC) stainless steels, Zr-alloys, nuclear fuel (UO
2). When high Z materials are involved, the problem takes hours to run on a small PC (Intel I7-6600U CPU @ 2.60 GHz).
PENELOPE has been incorporated into GEANT4.
https://twiki.cern.ch/twiki/bin/genpdf/Geant4/LowePenelope
https://twiki.cern.ch/twiki/bin/view/Geant4/LowePenelope
Another code similar to PENELOPE is EGS5 (5th version of EGS, Electron-Gamma Shower).
https://rcwww.kek.jp/research/egs/egs5_manual/slac730-160113.pdf
Just one example of application -
https://www.sciencedirect.com/science/article/pii/S027288422030883X
I'm interested in the effects of radiation on the evolution of structural materials and their performance in rather aggressive environments, and in particularly, how high energy gamma rays (and coincident/consequential electrons/positrons) change the atomic microstructure (crystal lattices and grain structure) of structural materials. The above codes PENELOPE does not yet consider photoneutron or photofission reactions, which only become significant in the presence of very light atoms (isotopes of Z=1 through Z=8) and heavy atoms (Z≥92), nor have the codes. EGS5 does appear to do photoneutron reactions.
Nuclear reactor core simulation codes do not consider photonuclear reactions necessarily, and in some cases, the cross section data libraries are incomplete.
Now if we turn to simulating the evolution of all the stars (do we consider the influence/perturbations of planets?) in all the galaxies in the universe over say a billion years - that's a much bigger problem. Or we could pick a small problem and just do all the stars in the galaxy in which we find ourselves. Or we pick a piece of a large problem and see if our mathematical models are sufficiently rigorous and robust to predict the behavior and outcome (describe the physics) we observe now and in the future.