Wick rotation



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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+ist + i s. After Wick rotation it is the imaginary part ss that replaces the “real” time tt.

graphics grabbed from Fulling-Ruijsenaars 87

This is motivated by the observation that the Minkowski metric (with the 1,1,1,1-1,1,1,1 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 d,1\mathbb{R}^{d,1}/Euclidean space d+1\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 TT (“KMS states”), and then relates this to Euclidean field theory with compact/periodic Euclidean time of length β=1/T\beta = 1/T (see Fulling-Ruijsenaars 87, section 3):

relativistic field theory on Minkowski spacetime d,1 in a thermal equilibrium state at temperatureT} Wick rotation {Euclidean field theory on Euclidean space d×S β 1 with compact/periodic Euclidean time of lengthβ=1/T A T|:Φ(x 1,t)Φ(x 2,t)Φ(x n,t):|T d,1equal-time n-point functionof relativistic fields in thermal equilibrium state |T = 0|Φ(x 1,t)Φ(x 2,t)Φ(x n,t)|0 d×S β 1correlator of Euclidean fields for "Euclidean time" of periodicityβ=1/T \array{ \left. \array{ \text{relativistic field theory} \\ \text{on Minkowski spacetime} \\ \mathbb{R}^{d,1} \\ \text{in a thermal equilibrium state} \\ \text{at temperature}\; T } \right\} & \;\;\;\; \overset{ \text{Wick rotation} }{\leftrightarrow} \;\;\;\; & \left\{ \array{ \text{Euclidean field theory} \\ \text{on Euclidean space} \\ \mathbb{R}^d \times S^1_{\beta} \\ \text{with compact/periodic Euclidean time} \\ \text{of length} \; \beta = 1/T } \right. \\ \phantom{A} \\ \underset{ { \text{equal-time n-point function} \atop \text{of relativistic fields} } \atop \text{ in thermal equilibrium state } \; \vert T\rangle }{ \underbrace{ \left\langle T\vert :\mathbf{\Phi}(x_1,t) \mathbf{\Phi}(x_2,t) \cdots \mathbf{\Phi}(x_n,t) : \vert T \right\rangle_{\mathbb{R}^{d,1}} }} &\;=\;& \underset{ \text{correlator of Euclidean fields} \atop \text{ for "Euclidean time" of periodicity}\; \beta = 1/T }{ \underbrace{ \left\langle 0 \vert \mathbf{\Phi}(x_1,t) \mathbf{\Phi}(x_2,t) \cdots \mathbf{\Phi}(x_n,t) \vert 0 \right\rangle_{\mathbb{R}^{d} \times S^1_{\beta}} }} }

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 1,1,1,1-1,1,1,1 convention for the tensor:

ds 2=(dt) 2+(dx) 2+(dy) 2+(dz) 2d s^{2}= -(d t)^{2} + (d x)^{2} + (d y)^{2} + (d z)^{2}

and the four-dimensional Euclidean metric:

ds 2=dτ 2+(dx) 2+(dy) 2+(dz) 2d s^{2}= d \tau^{2} + (d x)^{2} + (d y)^{2} + (d z)^{2}.

Notice that if dt=idτd t = i\cdot d \tau, the two are equivalent.


A typical method for employing Wick rotation would be to make the substitution t=iτt=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

  • Abel Klein, Lawrence Landau, Periodic Gaussian Osterwalder-Schrader positive processes and the two-sided Markov property on the circle, Pacific Journal of Mathematics, Vol. 94, No. 2, 1981 (DOI: 10.2140/pjm.1981.94.341, pdf)

The idea here apparently goes back to

  • Claude Bloch, Sur la détermination de l’état fondamental d’un système de particules, Nucl. Phys. 7 (1958) 451

This has maybe first been made precise, for the case of 1+1 dimensions, in

  • Raphael Høegh-Krohn, Relativistic Quantum Statistical Mechanics in two-dimensional Space-Time, Communications in Mathematical Physics 38.3 (1974): 195-224 (pdf)

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

Last revised on November 15, 2018 at 09:29:07. See the history of this page for a list of all contributions to it.