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DarMM
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Sorry, I should have explained this better. There is still a "regularisation" of sorts, but no physical cutoff.Demystifier said:In particular, at the top of page 180 the author writes:
"This is an ultraviolet "regularization" in the usual terminology. It should be stressed, however, that here this is a consequence of the causal distribution splitting and not an ad hoc recipe".
That is the original form of the Epstein-Glaser approach, if you are interested the modern form of the Epstein-Glaser approach is as follows.Therefore, I do not think it is correct to say that there is no regularization in the Epstein-Glaser approach. It's only that the regularization is mathematically better justified.
More technically, the Epstein-Glaser approach starts from the observation that time ordering of field operators introduces step functions theta(t-t'), which are ill defined at zero. Therefore, the theta functions are replaced by certain better defined regularized functions, which avoid problematic UV divergences.
Let's say the propagator of a scalar field theory is ##D(x-y)##, then the bubble second order diagram in ##\phi^4## theory in position space is:
##\int{D(x_1 - x_3)D(x_2 - x_3)D^{2}(x_3 - x_4)D(x_4 - x_5)D(x_4 - x_6)d^{4}x_{3}d^{4}x_{4}}##
Of course ##S(x_1,x_2,x_3,x_4,x_5,x_6) = D(x_1 - x_3)D(x_2 - x_3)D^{2}(x_3 - x_4)D(x_4 - x_5)D(x_4 - x_6)## is not a well-defined distribution on ##\mathbb{R}^{24}##, in the sense that there are some test functions that when integrated against it have a divergent result.
So you restrict the space of test functions from ##\mathcal{D}(\mathbb{R}^{24})## to some subspace ##\mathcal{A}## on which ##S(x_1,x_2,x_3,x_4,x_5,x_6)## is a sensible linear functional, typically the space of test functions which vanish on the ##x_i = x_j## hyperplanes. This is the regularisation in the Epstein-Glaser approach, but hopefully you can see why it's not really a physical cutoff. I don't know what it would correspond to physically.
You then prove that there is essentially a unique distribution ##\tilde{S}## defined on all test functions in ##\mathcal{D}(\mathbb{R}^{24})## which:
1. Agrees with ##\tilde{S}## on ##\mathcal{A}##.
2. Obeys relativity and causality.
Essentially ##S## has extensions thanks to the Hahn-Banach theorem to all of ##\mathcal{D}(\mathbb{R}^{24})##, but only one (up to a constant) obeys relativity and causality.
Hence we have renormalization via Hahn-Banach + Relativity.
However really the only way to work with a QFT without any regulator at all, is to know in advance which Hilbert Space it is defined on. On that Hilbert space there will be no divergences. However we aren't really able to do this at the moment, except with Algebraic QFT, which removes Hilbert Spaces but at the cost of being so general you can't work with a specific QFT.