What is the objective of renormalization group theory?

In summary, renormalization group theory is a method used in quantum field theory to remove infinities and account for the dependence of physical parameters on energy scales. It involves a regularization process and the use of "bare parameters" which are then renormalized to obtain observable quantities that are independent of the regularization. This can also be interpreted as integrating out irrelevant degrees of freedom in the path integral of the action. Renormalization group theory is necessary even for finite theories and is not just a "dirty trick." Other methods besides renormalization group theory can also be used to deal with singular perturbation problems.
  • #1
ndung200790
519
0
Please teach me this:
It seem to me that the objective of renormalization were the exclusion the infinities.But in renormalization group theory,they consider the dependence of physics parameters(e.g the interaction constant lamda,the mass parameter) on momentum p.Then I do not understand what is the objective(meaning) of renormalization group theory?
Thank you very much in advance.
 
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  • #2
Renormalization inorer to remove infinities is just a dirty trick. The renormalization group itself says that you can look at a theory at different energy scales E and E' (or at different length scales which is the same) and renromalize masses and coupling constants g(E) and g'(E') such that the predictions of both theories are the same. Essentially they are THE SAME theory.

This can e.g. be interpreted as "integrating out" degrees of freedom and hiding their contribution in the renormalization of parameters. Have a look at http://en.wikipedia.org/wiki/Renormalization_group#Block_spin_renormalization_group
 
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  • #3
Then,it seem to me there is an unclear in ''finite'' characteristic(''already renormalization'') in renormalization group theory.They pose a renormalization ''condition'' p^2=-M^2,then leading to Callan-Symazik...ect.So,the ''finite characteristic'' of the theory depends on the renormalizable nature of concrete QTF theory that we consider.
 
  • #4
I would put it this way.

To make renormalization, you first need to do a regularization. Any regularization involves some arbitrary energy-scale parameter, such as the cut off. The physical result should not depend on the choice of the value of that parameter. But this requirement is not trivial at all. It turns out that this requirement has a consequence that some physical quantities depend on energy in a physical process in a specific way. This dependence is what the renormalization group equation describes.
 
  • #5
... and this dependence does exist even if regularization is NOT required.
 
  • #6
Renormalization is not (only) a "dirty trick" to get rid of infinities in S-matrix elements or other observable quantities but necessary even for perfectly finite quantities. The reason is that in perturbation theory one uses parameters of fictitious objects called "bare particles", i.e., of free particles, and one has to adapt the wave-function normalization when considering interactions. This you can see even in usual quantum mechanics when you do, e.g., the "old fashioned" perturbation theory of stationary states (Schrödinger perturbation theory).

In quantum field theory, in addition one can absorb the infinities into the "bare parameters", that are unobservable, but as Demystifier pointed out, that requires the introduction of a energy/momentum scale. It does not come from the regularization, because the renormalized theory should be independent of the regularization used. A clearer picture is BPHZ renormalization, where you don't go over an intermediate step of a regularization, but interpret the Feynman rules as expressions for the integrands of loop integrals and subtract the divergences and subdivergences systematically before you do the integrations by using Zimmermann's Forest Formula.

These subtractions can usually be done only at a non-zero spacelike four momentum due to the analytic properties of the vertex functions and the demand that the counterterms, contributing to the wave-function-normalization factors, masses, and coupling constants must be real in order to have a self-adjoint Hamilton operator which guarantees a unitary S matrix. In this way you always introduce an energy-momentum scale, and this choice is in principle arbitrary, but the values of the "dressed parameters" depend on this choice of the scale. Changing the scale thus leads to finite renormalizations of these parameters, such that the prediction for observable quantities (S-matrix elements) don't change. The renormalization-group equations describe this change of the renormalized parameters of the theory such that the observable quantities do not change.

In the context of perturbation theory that independence in principle holds true only up to the order of the expansion parameter (e.g., some coupling or [itex]\hbar[/tex], etc.) taken into account in the calculation. The solution of the renormalization group equation with the "anomalous dimensions" given by perturbation theory are however usually to any order or the expansion parameter. One can show that this corresponds to a certain resummation of perturbation theory, summing up leading logarithms (see, e.g., Weinberg, Quantum Theory of Fields, Vol. II).

Another interpretation, originating from the work of K. Wilson, is that "irrelevant degrees of freedom" are integrated out in the path integral of the action. This can, e.g., be "hard modes" and thus the meaning is to coarse grain over small-range correlations lower than a certain energy scale. This is particularly intuitive in the context of many-body applications, where one looks at collective modes of a system rather than at the many microscopic degrees of freedom making up this collective behavior since if one restricts oneself only to observations below a certain energy or momentum scale (equivalent to the resolution of time and space dependences of observables) the complicated microscopic degrees of freedom become irrelevant concerning the collective behavior at the resolution of the observation.
 
  • #7
tom.stoer said:
... and this dependence does exist even if regularization is NOT required.
True. But when regularization is not needed (as in solid state physics) then even renormalization is not necessary. In this case, renormalization is only a convenient trick that simplifies certain calculations.
 
  • #8
Let me ask you a question, too: Which other methods besides renormalization group theory do you know to deal with singular perturbation problems?
 

1. What is renormalization group theory?

Renormalization group theory is a mathematical framework used in theoretical physics and statistical mechanics to study how physical systems behave at different scales. It allows us to understand the behavior of a system at a larger scale by examining its behavior at smaller scales.

2. What is the main objective of renormalization group theory?

The main objective of renormalization group theory is to study the scaling behavior of physical systems, which describes how a system's properties change as its size or energy scale changes. It helps us understand the universal properties of systems and how they behave under different conditions.

3. How does renormalization group theory work?

Renormalization group theory works by breaking down a system into smaller components and studying how they interact with each other. By analyzing these interactions, we can understand how the system behaves as a whole. This approach allows us to make predictions and gain insights about the behavior of the system at different scales.

4. What are the applications of renormalization group theory?

Renormalization group theory has a wide range of applications in various fields of physics, such as condensed matter physics, particle physics, and cosmology. It is also used in other fields, such as economics and biology, to study complex systems and their behavior at different scales.

5. What are the limitations of renormalization group theory?

While renormalization group theory is a powerful tool for understanding the behavior of physical systems, it does have its limitations. It relies on approximations and simplifications, and its predictions may not always be accurate for systems with strong interactions or at extreme scales. Additionally, it does not provide a complete description of a system, but rather focuses on its universal properties.

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