From configuration to dynamics -- Emergence of Lorentz signature in classical field theory
Shinji Mukohyama, Jean-Philippe Uzan

TL;DR
This paper explores how Lorentzian spacetime structure can emerge from a fundamentally Riemannian metric at the microscopic level, leading to effective relativistic dynamics in classical field theories.
Contribution
It introduces a model where Lorentzian geometry arises as an effective property in a fundamentally Euclidean space, extending classical field theory and including a novel approach to gravity.
Findings
Lorentzian dynamics emerge from a Riemannian metric in certain regions.
Constructed classical field theories for scalars, vectors, and spinors in flat spacetime.
Gravity can be incorporated, resulting in a covariant Galileon type theory.
Abstract
The Lorentzian metric structure used in any field theory allows one to implement the relativistic notion of causality and to define a notion of time dimension. This article investigates the possibility that at the microscopic level the metric is Riemannian, i.e. locally Euclidean, and that the Lorentzian structure, that we usually consider as fundamental, is in fact an effective property that emerges in some regions of a 4-dimensional space with a positive definite metric. In such a model, there is no dynamics nor signature flip across some hypersurface; instead, all the fields develop a Lorentzian dynamics in these regions because they propagate in an effective metric. It is shown that one can construct a decent classical field theory for scalars, vectors and (Dirac) spinors in flat spacetime. It is then shown that gravity can be included but that the theory for the effective…
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