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What is called Wick rotation (after Gian-Carlo Wick) is a method in physics for finding a construction in relativistic field theory on Minkowski spacetime or, more generally, on Lorentzian manifolds, from a related construction in Euclidean field theory on Riemannian manifolds in a way that involves or generalizes the idea of analytic continuation for the time coordinates.
The complex plane for a complexified time coordinate $t + i s$. After Wick rotation it is the imaginary part $s$ that replaces the “real” time $t$.
graphics grabbed from Fulling-Ruijsenaars 87
This is motivated by the observation that the Minkowski metric (with the $-1,1,1,1$ convention) and the four-Euclidean metric are equivalent if the time components of either are allowed to have imaginary values. Hence Wick rotation, when it applies, involves analytic continuation of n-point functions to complex valued time coordinates.
For relativistic/Euclidean quantum field theory on Minkowski spacetime $\mathbb{R}^{d,1}$/Euclidean space $\mathbb{R}^{d+1}$ Wick rotation is rigorously understood and takes the form of a theorem relating the Wightman axioms for n-point functions in relativistic field theory to the Osterwalder-Schrader axioms for correlators in Euclidean field theory.
See for instance Fulling-Ruijsenaars 87, section 2 for a clear account.
More generally, in this context Wick rotation applies to relativistic field theory in thermal equilibrium states at positive temperature $T$ (“KMS states”), and then relates this to Euclidean field theory with compact/periodic Euclidean time of length $\beta = 1/T$ (see Fulling-Ruijsenaars 87, section 3):
In this form, Wick rotation is also known as thermal quantum field theory. See there for more.
graphics grabbed form Frolov-Zelnikov 11
Wick rotation also applies on suitable black-hole?-spacetimes spring thermodynamics, such as the Bekenstein-Hawking entropy, find elegant explanations, at least at the level of the manipulation of formulas (see e.g. Fulling-Ruijsenaars 87, section 4).
Consider the Minkowski metric with the $-1,1,1,1$ convention for the tensor:
$d s^{2}= -(d t)^{2} + (d x)^{2} + (d y)^{2} + (d z)^{2}$
and the four-dimensional Euclidean metric:
$d s^{2}= d \tau^{2} + (d x)^{2} + (d y)^{2} + (d z)^{2}$.
Notice that if $d t = i\cdot d \tau$, the two are equivalent.
A typical method for employing Wick rotation would be to make the substitution $t=i\tau$ in a problem in Minkowski space. The resulting problem is in Euclidean space and is sometimes easier to solve, after which a reverse substitution can (sometimes) be performed, yielding a solution to the original problem.
Technically, this works for any four-vector comparison between Minkowski space and Euclidean space, not just for space-time intervals.
Wick rotation between relativistic field theory in terms of Wightman axioms for n-point functions on Minkowski spacetime and Euclidean field theory in terms of Osterwalder-Schrader axioms for correlators on Euclidean space is due to
The generalization of this for positive thermal equilibrium vacuum staes?, relating to thermal quantum field theory with compact/periodic Euclidean time is discussed in
The idea here apparently goes back to
This has maybe first been made precise, for the case of 1+1 dimensions, in
Good review on the relation to thermal quantum field theory and black hole thermodynamics is in
S.A. Fulling, S.N.M. Ruijsenaars, Temperature, periodicity and horizons, Physics Reports Volume 152, Issue 3, August 1987, Pages 135-176 (pdf, doi:10.1016/0370-1573(87)90136-0)
Gary Gibbons, Malcolm J. Perry, Black Holes and Thermal Green Functions, Vol. 358, No. 1695 (1978) (jstor:79482)
Discussion of thermal Wick rotation on global anti-de Sitter spacetime (which is already periodic in real time) is in
See also
Dirk Schlingemann, From euclidean field theory to quantum field theory (arXiv:hep-th/9802035)
Graeme Segal, Wick rotation and the positivity of energy in quantum field theory (video)
Edward Witten, The Feynman $i \epsilon$ in String Theory (arXiv:1307.5124)
Last revised on November 15, 2018 at 09:29:07. See the history of this page for a list of all contributions to it.