zonde said:
Can you expand this?
Do you mean particle number is conserved statistically? And what empirical data do you have in mind?
By particle number, I mean the number of particles minus the number of anti-particles in a state. Strictly, I would say that charges are conserved, which imply the conservation of particle number. I would take the conservation of electrical charge —absolutely, not statistically— to be an empirical principle that is essentially unquestioned. Electric charge is of course intimately related to the U(1) gauge group in the standard formalisms. Physical states apparently can be mixtures of states that have different charges, but they cannot be superpositions of states that have different charges, which is just to say that there is a superselection principle for electric charge.
As far as the conservation of other charges is concerned, of electroweak and color charges, or perhaps of hadron number conservation, I would regard these as more open to question, but, in the absence of any definite reason, it suits me for now to give the Standard Model of Particle Physics the benefit of the doubt. My understanding of the detailed phenomenology of Particle Physics needs a lot of brushing up.
I take it to be a significant key to how we should construct theories that electric charge is an integer multiple of the charge on the electron in almost all circumstances.
zonde said:
I am not sure I understand your position. Where do you see physical significance of quanta then?
Surely you must take that there is some physical significance of quanta at least in interactions (photon absorption by electron for example).
I have to say that I have some rude ideas how energy can be physically allocated to quanta but these are for my own comfort so to say.
And do you have some link with introduction in random fields? I looked into wikipedia but it is very short about this topic. Maybe there is any of your own papers that are not very specific?
Where did you last see a photon absorbed by an electron? It's a standard way of talking, of course, justified by a naive interpretation of a tree level Feynman diagram, but if we introduce loop level Feynman diagrams, and get past renormalization, a similarly naive interpretation would have to say that there are infinite numbers of electrons and photons of infinitely varied energies, both on and off shell, interacting together, which is just messy.
At the empirical level, I would be (somewhat) more happy to say that a photon was absorbed by a macroscopic object, causing a thermodynamic transition from a ready state to an excited state that I can see with a microscope, or that is amplified electrically to the point that a computer memory bit is modified. There's always a question whether any given event was caused by a cosmic ray, was a result of an internal fluctuation of the macroscopic object, was caused by a stray electron, neutron, neutrino, or whatever, from an unshielded piece of apparatus in the room, etc.. If we see the rate of events change just after we turn on a light, we can only say that a particular discrete thermodynamic transition was quite likely caused by the light being turned on, not that it was definitely caused by a photon. I'm happy saying that the change of the statistics was caused by turning on the light, but we should be careful what we say about individual events.
As I said a few messages back, I take there to be three fairly incontrovertible discrete structures, charges, discrete spectra (something like the spectrum of Hydrogen, say, which are modeled as the eigenvalues of observables), and thermodynamic transitions of macroscopic objects. The idea that there are "quanta" is too vague to be thrown around without any indication of what mathematics we're using. Insofar as Planck's constant is what we're talking about when we talk about "quanta", I take it to be a measure of irreducible quantum fluctuations, which have effects on most small-scale Physics, which can be observed in large-scale Physics when we take appropriate steps to engineer amplification. My papers talk about this in an evolving way that is not entirely coherent over time.
As far as references on random fields are concerned, please get back to me immediately if you find something accessible on the web or in the literature! My own attempts at explaining random fields only scratch at the surface of the mathematics. There are a number of books in the Yale libraries,
Preston, Christopher J., Random fields, Springer-Verlag, 1976.
Vanmarcke, Erik., Random fields, analysis and synthesis, MIT Press, c1983.
Rozanov, Yu. A, Random fields and stochastic partial differential equations, Kluwer Academic, c1998.
Spitzer, Frank Ludwig, Random fields and interacting particle systems, Mathematical Association of America, 1971.
Another book is Stanley P. Gudder, Stochastic Methods in Quantum Mechanics, North-Holland, 1979, which I have taken to citing in papers, referring particularly to chapter 6, because the discussion of random fields is quite nicely done and geared to quantum field theory ways of thinking.
As you see, most of these references are from 20-30 years ago.
The algebraic methods I'm using to construct random fields and states over them, of creation and annihilation operators, are not in the literature in any direct way to my knowledge, although they are not particularly difficult mathematics. People haven't much thought it would be interesting to work with random fields, so finding effective ways of using them has not been investigated. The mathematics I'm using is partly just that of commutative *-algebras, for the field observables, whereas the algebra of creation and annihilation operators are very similar to what is used in quantum field theory. The literature of C*-algebras to a limited extent applies also to *-algebras, although the lack of a norm for the local observables has plenty of consequences.
Andrei Khrennikov has been using a mathematics that can be thought of as random fields, although I have not liked his formalism much. His papers can be found on arXiv.
Random fields are used in Physics at the Cosmological scale (indeed it was someone who works on Cosmology who was the second person to point out this mathematics to me, about six years ago), but I don't know whether there is a standard reference for random fields in that literature. So I've written to that person to find out whether there's a standard reference to cite or for sending graduate students to it.