# Dimensional regularization

In theoretical physics, dimensional regularization is a method introduced by Giambiagi and Bollini[1] as well as – independently and more comprehensively[2] – by 't Hooft and Veltman[3] for regularizing integrals in the evaluation of Feynman diagrams; in other words, assigning values to them that are meromorphic functions of a complex parameter d, the analytic continuation of the number of spacetime dimensions.

Dimensional regularization writes a Feynman integral as an integral depending on the spacetime dimension d and the squared distances (xixj)2 of the spacetime points xi, ... appearing in it. In Euclidean space, the integral often converges for −Re(d) sufficiently large, and can be analytically continued from this region to a meromorphic function defined for all complex d. In general, there will be a pole at the physical value (usually 4) of d, which needs to be canceled by renormalization to obtain physical quantities. Etingof (1999) showed that dimensional regularization is mathematically well defined, at least in the case of massive Euclidean fields, by using the Bernstein–Sato polynomial to carry out the analytic continuation.

Although the method is most well understood when poles are subtracted and d is once again replaced by 4, it has also led to some successes when d is taken to approach another integer value where the theory appears to be strongly coupled as in the case of the Wilson-Fisher fixed point. A further leap is to take the interpolation through fractional dimensions seriously. This has led some authors to suggest that dimensional regularization can be used to study the physics of crystals that macroscopically appear to be fractals.[4]

If one wishes to evaluate a loop integral which is logarithmically divergent in four dimensions, like

${\displaystyle \int {\frac {d^{d}p}{(2\pi )^{d}}}{\frac {1}{\left(p^{2}+m^{2}\right)^{2}}},}$

one first rewrites the integral in some way so that the number of variables integrated over does not depend on d, and then we formally vary the parameter d, to include non-integral values like d = 4 − ε.

This gives

${\displaystyle \int _{0}^{\infty }{\frac {dp}{(2\pi )^{4-\varepsilon }}}{\frac {2\pi ^{(4-\varepsilon )/2}}{\Gamma \left({\frac {4-\varepsilon }{2}}\right)}}{\frac {p^{3-\varepsilon }}{\left(p^{2}+m^{2}\right)^{2}}}={\frac {2^{\varepsilon -4}\pi ^{{\frac {\varepsilon }{2}}-1}}{\sin({\frac {\pi \varepsilon }{2}})\Gamma (1-{\frac {\varepsilon }{2}})}}m^{-\varepsilon }={\frac {1}{8\pi ^{2}\varepsilon }}-{\frac {1}{16\pi ^{2}}}\left(\ln {\frac {m^{2}}{4\pi }}+\gamma \right)+{\mathcal {O}}(\varepsilon ).}$

Emilio Elizalde has shown that Zeta regularization and dimensional regularization are equivalent since they use the same principle of using analytic continuation in order for a series or integral to converge.

## Notes

1. ^ Bollini 1972, p. 20.
2. ^ Bietenholz, Wolfgang; Prado, Lilian (2014-02-01). "Revolutionary physics in reactionary Argentina". Physics Today. 67 (2): 38–43. Bibcode:2014PhT....67b..38B. doi:10.1063/PT.3.2277. ISSN 0031-9228.
3. ^ 't Hooft 1972
4. ^ Le Guillo, J.C.; Zinn-Justin, J. (1987). "Accurate critical exponents for Ising-like systems in non-integer dimensions". Journal de Physique. 48.