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&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;{{Short description|Procedure in quantum field theory that removes infinities by redefining physical parameters such as mass and charge}}&lt;br /&gt;
&lt;br /&gt;
{{Quantum book backlink|Quantum field theory}}&lt;br /&gt;
&amp;#039;&amp;#039;&amp;#039;Renormalization in quantum field theory&amp;#039;&amp;#039;&amp;#039; is the systematic procedure used to handle divergences that arise in perturbative calculations by absorbing them into redefined physical parameters such as mass, charge, and field normalization.&amp;lt;ref name=&amp;quot;peskin&amp;quot;&amp;gt;Peskin, M. E.; Schroeder, D. V. &amp;#039;&amp;#039;An Introduction to Quantum Field Theory&amp;#039;&amp;#039; (1995).&amp;lt;/ref&amp;gt; It allows quantum field theories to produce finite, physically meaningful predictions.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;div style=&amp;quot;float:right; border:1px solid #ccc; padding:4px; background:#fff8dc; margin:0 0 1em 1em; width:420px;&amp;quot;&amp;gt;&lt;br /&gt;
[[File:Renormalization_flow_diagram.jpg|400px]]&lt;br /&gt;
&amp;lt;div style=&amp;quot;font-size:90%;&amp;quot;&amp;gt;Renormalization: scale-dependent behavior of physical parameters and absorption of divergences into redefined quantities&amp;lt;/div&amp;gt;&lt;br /&gt;
&amp;lt;/div&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Origin of divergences ==&lt;br /&gt;
In quantum field theory, higher-order corrections involve integrals over all possible momenta. These integrals often diverge at high energies (ultraviolet divergences).&amp;lt;ref name=&amp;quot;weinberg&amp;quot;&amp;gt;Weinberg, S. &amp;#039;&amp;#039;The Quantum Theory of Fields&amp;#039;&amp;#039; (1995).&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
For example, loop diagrams in perturbation theory can produce expressions such as:&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
\int^\infty \frac{d^4p}{p^2 - m^2}&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
which are not finite without additional procedures.&lt;br /&gt;
&lt;br /&gt;
== Regularization ==&lt;br /&gt;
The first step in renormalization is regularization, where divergences are controlled by introducing a parameter that makes the integrals finite.&lt;br /&gt;
&lt;br /&gt;
Common methods include:&lt;br /&gt;
&lt;br /&gt;
* momentum cutoff  &lt;br /&gt;
* dimensional regularization  &lt;br /&gt;
* Pauli–Villars regularization  &lt;br /&gt;
&lt;br /&gt;
For instance, a momentum cutoff replaces divergent integrals with:&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
\int^{\Lambda} d^4p&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\Lambda&amp;lt;/math&amp;gt; is a finite cutoff scale.&amp;lt;ref name=&amp;quot;schwartz&amp;quot;&amp;gt;Schwartz, M. D. &amp;#039;&amp;#039;Quantum Field Theory and the Standard Model&amp;#039;&amp;#039; (2014).&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Renormalization procedure ==&lt;br /&gt;
After regularization, divergences are absorbed into redefined parameters:&lt;br /&gt;
&lt;br /&gt;
* bare mass &amp;lt;math&amp;gt;m_0&amp;lt;/math&amp;gt; → physical mass &amp;lt;math&amp;gt;m&amp;lt;/math&amp;gt;  &lt;br /&gt;
* bare charge &amp;lt;math&amp;gt;e_0&amp;lt;/math&amp;gt; → physical charge &amp;lt;math&amp;gt;e&amp;lt;/math&amp;gt;  &lt;br /&gt;
&lt;br /&gt;
The Lagrangian is rewritten in terms of renormalized quantities plus counterterms:&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
\mathcal{L} = \mathcal{L}_{\text{ren}} + \mathcal{L}_{\text{counter}}&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
These counterterms cancel the divergences arising in loop calculations.&amp;lt;ref name=&amp;quot;peskin&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Running coupling constants ==&lt;br /&gt;
Renormalization introduces a dependence of physical parameters on the energy scale. This is described by the renormalization group.&lt;br /&gt;
&lt;br /&gt;
For example, the coupling constant becomes scale-dependent:&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
\alpha(\mu)&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\mu&amp;lt;/math&amp;gt; is the renormalization scale.&lt;br /&gt;
&lt;br /&gt;
The evolution of parameters with scale is governed by equations such as:&lt;br /&gt;
&amp;lt;math&amp;gt;&lt;br /&gt;
\mu \frac{d g}{d\mu} = \beta(g)&lt;br /&gt;
&amp;lt;/math&amp;gt;&lt;br /&gt;
&lt;br /&gt;
where &amp;lt;math&amp;gt;\beta(g)&amp;lt;/math&amp;gt; is the beta function.&amp;lt;ref name=&amp;quot;zee&amp;quot;&amp;gt;Zee, A. &amp;#039;&amp;#039;Quantum Field Theory in a Nutshell&amp;#039;&amp;#039; (2010).&amp;lt;/ref&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Renormalizable theories ==&lt;br /&gt;
A theory is called renormalizable if all divergences can be absorbed into a finite number of parameters.&lt;br /&gt;
&lt;br /&gt;
Examples include:&lt;br /&gt;
&lt;br /&gt;
* quantum electrodynamics (QED)  &lt;br /&gt;
* quantum chromodynamics (QCD)  &lt;br /&gt;
&lt;br /&gt;
Non-renormalizable theories can still be useful as effective field theories valid at a limited energy scale.&amp;lt;ref name=&amp;quot;weinberg&amp;quot;/&amp;gt;&lt;br /&gt;
&lt;br /&gt;
== Physical interpretation ==&lt;br /&gt;
Renormalization reflects the fact that physical measurements depend on the energy scale at which they are performed.&lt;br /&gt;
&lt;br /&gt;
Quantum fluctuations at different scales modify the effective values of parameters, leading to observable effects such as charge screening in QED.&lt;br /&gt;
&lt;br /&gt;
== Conceptual importance ==&lt;br /&gt;
Renormalization is one of the central concepts of modern quantum field theory. It explains how:&lt;br /&gt;
&lt;br /&gt;
* infinities are handled consistently  &lt;br /&gt;
* physical predictions remain finite  &lt;br /&gt;
* interactions depend on scale  &lt;br /&gt;
&lt;br /&gt;
It also provides the foundation for the renormalization group and modern effective field theory approaches.&lt;br /&gt;
&lt;br /&gt;
==See also==&lt;br /&gt;
{{#invoke:PhysicsQC|tocHeadingAndList|Physics:Quantum basics/See also}}&lt;br /&gt;
&lt;br /&gt;
==References==&lt;br /&gt;
{{reflist|3}}&lt;br /&gt;
{{Author|Harold Foppele}}&lt;br /&gt;
&lt;br /&gt;
{{Sourceattribution|Quantum field theory (QFT) core|1}}&lt;/div&gt;</summary>
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