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  Are these two aspects of traditional renormalization only technical conveniences in light of our modern understanding?

+ 6 like - 0 dislike

1. Sending cutoff to infinity:In modern perspective, is it enough to just set cutoff to be a large but definite scale, while imposing renormalization conditions? And we know sending cutoff to infinity can't always be done (even at perturbative level?) if there is a Landau pole. So sending cutoff to infinity is probably just for calculational convenience?

2. Renormalizability in the sense that quantum corrections do not generate new counter-terms: We would like to have such renormalizability because such theories are qualitatively correct at tree level, so that we have good control of the theories just by inspecting their Lagrangians?

The above have been in my head for a while and they seem to make sense. However I haven't found materials explicitly phrasing it this way, so I put it here to check if I am having any misunderstanding.

asked Sep 27, 2014 in Theoretical Physics by Jia Yiyang (2,635 points) [ no revision ]

Sending cutoff to infinity is not allowable anymore and renormalizability requirement is forbidden too. New counter-terms with their cutoff dependencies might be necessary to fit our theories to experiments because we do not know physics. We must keep our options maximally open.

The explanation is that the effective theory is only valid at a certain range of scales and when you go beyond towards higher energies for example, new operators (terms) can become relevant as there is a new fixed point.

1 Answer

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In a renormalizable theory (with or without Landau pole), the perturbative results change only by $O(\Lambda^{-1})$ when you move the cutoff to $\infty$ and adjust the finitely many counterterms accordingly. Thus one could always work at some finite $\Lambda$ and stay within the experimental bounds.

However, Poincare invariance (and in not gauge invariant renormalization schemes also gauge invariance) is then violated by $O(\Lambda^{-1})$, too. This means that $\Lambda$ has to be large enough to respect the very stringent experimental bounds on a violation of Poincare invariance. 

Thus the limit $\Lambda\to\infty$ is primarily needed to have exact symmetries. In a sense, this means that it is needed only for theoretical reasons of elegance, since if Poincare invariance were broken it would call for an explanation why it is so extremely well satisfied. 

Nonrenormalizable theories show precisely the same behavior, except that infinitely many counterterms are needed to get a finite limit as $\Lambda\to\infty$. This is not a disaster for predictability as all but a few of these counterterms are suppressed by high powers of the mass scale of the theory (such as the Planck mass for gravity).

All this is valid on the perturbative level.

Nonperturbatively things could go wrong if there is a Landau pole, but the existence of a Landau pole for $\Phi^4$ theory or QED is proved only in low order perturbation theory. Hence in fact nothing mathematically convincing is known about the obstructions to nonperturbative QFTs (whose observable fields satisfy the Wightman axioms).

My personal belief is that QED (or at least a variant of QED that contains nuclei in addition to electrons, with simplified interactions and conserved nucleon number - i.e., excluding radioactivity) must exist since it is the most accurate theory that we have.

answered Oct 4, 2014 by Arnold Neumaier (12,890 points) [ no revision ]
Most voted comments show all comments

Thanks! To clarify my thought on my 2nd question, I guess it can be formulated this way: if non-renormalizable interactions that keep generating new counter terms are perfectly legitimate, what is the value of t'Hooft and Veltman's work on renormalizabilty of Yang-Mills? Trying to explain this to myself led to the thought I wrote down in the main post. 

From the newer EFT point of view as I understand it, not being able to send $\Lambda \rightarrow \infty$ is no longer that bad as it just means that a new EFT (with potentially different (un)broken symmetries too) kicks in at high energy scales.

There is a video (a little bit long, but interesting) about ups and downs in QFT understanding and developments. It is a talk given by S. Weinberg at CERN. I give a reference to a clip.

Renormalizability means very few constants that need to be fit to experiment, and hence great predictivity at any accuracy. (Of course, whether experiment agrees to that accuracy is a different question.) Nonrenormalizable theories need more and more constants (and, consequently, more messy computations) as one increases the desired accuracy. Thus renormalizability is always a significant advantage.

However, at the time  t'Hooft and Veltman proved renormalization of nonabelian gauge theories, renormalization was considered an essential requirement for consistency. Proving it was the breakthrough that made QCD a standard rather than just a possibility.

Only later, Weinberg made the nonrenormalizable case respectable again.

I meant with renormalizability not power counting (which is only a necessary condition) but the absence of infinities in the higher order contributions when one removes the cutoff. This is nontrivial, and was in the setting before causal perturbation theory even hard for $\Phi^4$ theory. That they proved it for QCD was indeed remarkable. (That QCD has a favorable power counting is obvious.)

But at tree level, there is no difference. The difference is that in higher orders, one doesn't get additional renormalization ambiguities, that would arise when one had to remove additional infinities.

I never claimed that their work has only historical value. In my answer I had mentioned the advantages of being renormalizable. But it is not better accuracy but well-definedness to all orders with a few parameters only.

Most recent comments show all comments

@jiaYiyang: Yukawa interactions without bare $\phi^4$ still has a Fermion box diagram with four scalars and Fermions going in a loop which gives a logarithmically growing scattering to 2 $\phi$ particles to 2 $\phi$ particles. Even if it at some subtraction point this gives zero $\lambda$ for the $\phi^4$ interaction, this condition is not preserved under running, and if you change the scale of subtraction to a very high one, you always find a large $\lambda$ at this subtraction scale.

@RonMaimon, yes, that's why I said I thought it was not qualitatively correct at tree level. But then the QED example shows it is probably not a useful way of looking at it.

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