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Well, renormalization is primarily not about the divergences, which only occur, because physicists tend to handle distribution (generalized functions) sloppily. You have to renormalize in any case when doing any perturbation theory, and you can indeed do the calculations of perturbative QFT without any divergences occurring at any stage. You just have to handle the distributions, particularly taking products of them, carefully.ilper said:Math in QFT is bringing much artificial renormalizations in the end and enormous calculations. Surely the nature does it not that way.
I have a question apart from mathematical formulation. Is the QFT field a field of probabilities? Operator valued field is a field in math but what I want to know is what is it in reality? The collapse is possible only for probabilities.
The traditional approach is to do some regularization of the distributions first and then taking limits to the physical parameters after renormalization, which by construction is finite. For perturbative calculations the most convenient techniques of this kind is dimensional regularization or the zeta-function renormalization, which is closely related to Schwinger's proper-time method.
Another systematic scheme is to interpret the naive Feynman rules, leading to divergent "loop integrals", as rules for the integrands of the expression expressed by the diagrams and then doing the necessary subtractions, leading to the renormalized expressions for these integrands and integrating the (then of course finite) expressions over the loop momenta. This technique also works for resummed perturbation theory (like the 2PI/CJT formalism).
An alternative more modern approach is the "causal Epstein-Glaser" approach, where you work with physical fields, i.e., normalizable states and not with distributions. This is a very physical idea.
Last but not least there's also the functional renormalization-group approach, which corresponds to the most physical approach towards renormalization, which is Wilson's approach.
All these techniques to remedy the UV divergences lead to the same result for a given renormalization scheme, and all these schemes lead to the same physical results (S-matrix elements) to the order of perturbation theory calculated.
If massless fields are involved in the theory (as is the case for all gauge theories with un-Higgsed local gauge theories) you also have to take care about infrared and colinear divergences, which is done traditionally by summing up soft-photon contributions all contributing at the same order of the expansion parameter (powers of the coupling constant or rather powers of ##\hbar##). A more modern (equivalent) approach is to work with the correct "asymptotic free states", which are not the naive plane waves usually used but a specific kind of "dressed states" taking into account the non-trivial asymptotics due to the long-range nature of gauge interactions (socalled "infra-particles").