Editing Quantum gravity (section)

=== Nonrenormalizability of gravity ===
{{Further|Renormalization|Asymptotic safety in quantum gravity}}
General relativity, like [[electromagnetism]], is a [[classical field theory]]. One might expect that, as with electromagnetism, the gravitational force should also have a corresponding [[quantum field theory]].

However, gravity is perturbatively [[nonrenormalizable]].<ref>{{Cite book |last=Feynman |first=Richard P. |title=Feynman Lectures on Gravitation |publisher=Addison-Wesley |year=1995 |isbn=978-0201627343 |location=Reading, Massachusetts |pages=xxxvi–xxxviii, 211–212 |language=en-us}}</ref><ref>{{ cite book | last= Hamber | first= H. W. | title= Quantum Gravitation – The Feynman Path Integral Approach | publisher = Springer Nature | date=2009 | isbn=978-3-540-85292-6 }}</ref> For a quantum field theory to be well defined according to this understanding of the subject, it must be [[asymptotic freedom|asymptotically free]] or [[asymptotic safety|asymptotically safe]]. The theory must be characterized by a choice of ''finitely many'' parameters, which could, in principle, be set by experiment. For example, in [[quantum electrodynamics]] these parameters are the charge and mass of the electron, as measured at a particular energy scale.

On the other hand, in quantizing gravity there are, in [[perturbation theory]], ''infinitely many independent parameters'' (counterterm coefficients) needed to define the theory. For a given choice of those parameters, one could make sense of the theory, but since it is impossible to conduct infinite experiments to fix the values of every parameter, it has been argued that one does not, in perturbation theory, have a meaningful physical theory. At low energies, the logic of the [[renormalization group]] tells us that, despite the unknown choices of these infinitely many parameters, quantum gravity will reduce to the usual Einstein theory of general relativity. On the other hand, if we could probe very high energies where quantum effects take over, then ''every one'' of the infinitely many unknown parameters would begin to matter, and we could make no predictions at all.<ref>{{Cite journal|doi=10.1016/0370-2693(85)91470-4|last1=Goroff|first1=Marc H.|last2=Sagnotti|first2=Augusto|last3=Sagnotti|first3=Augusto|title=Quantum gravity at two loops|date=1985|journal=[[Physics Letters B]]|volume=160|issue=1–3|pages=81–86|bibcode = 1985PhLB..160...81G }}</ref>

It is conceivable that, in the correct theory of quantum gravity, the infinitely many unknown parameters will reduce to a finite number that can then be measured. One possibility is that normal [[perturbation theory]] is not a reliable guide to the renormalizability of the theory, and that there really ''is'' a [[UV fixed point]] for gravity. Since this is a question of [[non-perturbative]] quantum field theory, finding a reliable answer is difficult, pursued in the [[Asymptotic safety in quantum gravity|asymptotic safety program]]. Another possibility is that there are new, undiscovered symmetry principles that constrain the parameters and reduce them to a finite set. This is the route taken by [[string theory]], where all of the excitations of the string essentially manifest themselves as new symmetries.<ref>{{Cite web|url=https://golem.ph.utexas.edu/~distler/blog/archives/000639.html|title=Motivation|last=Distler|first=Jacques|author-link=Jacques Distler|date=2005-09-01|website=golem.ph.utexas.edu|language=en|access-date=2018-02-24|archive-date=2019-02-11|archive-url=https://web.archive.org/web/20190211070351/https://golem.ph.utexas.edu/~distler/blog/archives/000639.html|url-status=live}}</ref>{{Better source needed|date=February 2019}}