Editing Renormalization (section)

== Renormalizability ==
From this philosophical reassessment, a new concept follows naturally: the notion of renormalizability.  Not all theories lend themselves to renormalization in the manner described above, with a finite supply of counterterms and all quantities becoming cutoff-independent at the end of the calculation.  If the Lagrangian contains combinations of field operators of high enough [[dimensional analysis|dimension]] in energy units, the counterterms required to cancel all divergences proliferate to infinite number, and, at first glance, the theory would seem to gain an infinite number of free parameters and therefore lose all predictive power, becoming scientifically worthless. Such theories are called ''nonrenormalizable''.

The [[Standard Model]] of particle physics contains only renormalizable operators, but the interactions of [[general relativity]] become nonrenormalizable operators if one attempts to construct a field theory of [[quantum gravity]] in the most straightforward manner (treating the metric in the [[Einstein–Hilbert Lagrangian]] as a perturbation about the [[Minkowski metric]]), suggesting that [[perturbation theory (quantum mechanics)|perturbation theory]] is not satisfactory in application to quantum gravity.

However, in an [[effective field theory]], "renormalizability" is, strictly speaking, a [[misnomer]]. In nonrenormalizable effective field theory, terms in the Lagrangian do multiply to infinity, but have coefficients suppressed by ever-more-extreme inverse powers of the energy cutoff.  If the cutoff is a real, physical quantity—that is, if the theory is only an effective description of physics up to some maximum energy or minimum distance scale—then these additional terms could represent real physical interactions.  Assuming that the dimensionless constants in the theory do not get too large, one can group calculations by inverse powers of the cutoff, and extract approximate predictions to finite order in the cutoff that still have a finite number of free parameters.  It can even be useful to renormalize these "nonrenormalizable" interactions.

Nonrenormalizable interactions in effective field theories rapidly become weaker as the energy scale becomes much smaller than the cutoff.  The classic example is the [[Fermi's interaction|Fermi theory]] of the [[weak nuclear force]], a nonrenormalizable effective theory whose cutoff is comparable to the mass of the [[W particle]].  This fact may also provide a possible explanation for ''why'' almost all of the particle interactions we see are describable by renormalizable theories.  It may be that any others that may exist at the [[Grand Unified Theory|GUT]] or Planck scale simply become too weak to detect in the realm we can observe, with one exception: [[gravity]], whose exceedingly weak interaction is magnified by the presence of the enormous masses of [[star]]s and [[planet]]s.{{Citation needed|date=February 2010}}