Wick rotation in the lapse, admissible complex metrics, and foliation changing diffeomorphisms
Rudrajit Banerjee, Max Niedermaier
TL;DR
The authors introduce a lapse-based Wick rotation on foliated manifolds that keeps the manifold’s real atlas while smoothly interpolating between Lorentzian and Euclidean geometries via a phase rotation of the lapse. By formulating the rotated metric as a rank-one perturbation and analyzing foliation-changing diffeomorphisms, they achieve a covariant description of $g^{\theta}$ across equivalent foliations. They prove three notions of admissibility for the complex metric in a minimally coupled scalar theory: damping of the action, positivity of the linear response, and sectoriality of the complex Hessian, with the Hessian spectrum confined to a wedge in the upper half-plane and explicit behavior near Minkowski and Friedmann-Lemaître backgrounds. The work predicts modified propagators compared to the standard $i\epsilon$ prescription and suggests broad applicability to other fields and to gravity via heat-kernel methods, offering a unified framework for Lorentzian-to-Euclidean transitions on foliated spaces.
Abstract
A Wick rotation in the lapse (not in time) is introduced that interpolates between Riemannian and Lorentzian metrics on real manifolds admitting a codimension-one foliation. The definition refers to a fiducial foliation but covariance under foliation changing diffeomorphisms can be rendered explicit in a reformulation as a rank one perturbation. Applied to scalar field theories a Lorentzian signature action develops a positive imaginary part thereby identifying the underlying complex metric as ``admissible''. This admissibility is ensured in non-fiducial foliations in technically distinct ways also for the variation with respect to the metric and for the Hessian. The Hessian of the Wick rotated action is a complex combination of a generalized Laplacian and a d'Alembertian, which is shown to have spectrum contained in a wedge of the upper complex half plane. Specialized to near Minkowski space the induced propagator differs from the one with the Feynman $iε$ prescription and on Friedmann-Lemaître backgrounds the difference to a Wick rotation in time is illustrated.
