Exploring the Rindler vacuum and the Euclidean Plane

Abstract

In flat spacetime, two inequivalent vacuum states which arise rather naturally are the Rindler vacuum (R) and the Minkowski vacuum (M). We disuss several aspects of the Rindler vacuum, concentrating on the propagator and Schwinger (heat) kernel defined using R, both in the Lorentzian and Euclidean sectors. We start by exploring an intriguing result due to Candelas and Raine , viz., that $G_R$, the Feynman propagator corresponding to R, can be expressed as a curious integral transform of $G_M$, the Feynman propagator in M. We show that, this relation actually follows from the well known result that, $G_M$ can be written as a periodic sum of $G_R$, in the Rindler time $\tau$, with the period $2\pi i$. We further show that, the integral transform result holds for a wide class of pairs of bi-scalars $(F_M,F_R)$, provided $F_M$ can be represented as a periodic sum of $F_R$ with period $2\pi i$. We provide an explicit procedure to retrieve $F_R$ from its periodic sum $F_M$, for a wide class of functions. An example of particular interest is the pair of Schwinger kernels $(K_M,K_R)$, corresponding to the Minkowski and the Rindler vacua. We obtain explicit expression for $K_R$ and clarify several conceptual and technical issues related to these biscalars both in the Euclidean and Lorentzian sector. In particular we address the issue of retrieving the information contained in all the four wedges of the Rindler frame in the Lorentzian sector, starting from the Euclidean Rindler (polar) coordinates. This is possible but require four different types of analytic continuations, based on one unifying principle. Our procedure allows generalisation of these results to any (bifurcate Killing) horizon in curved spacetime.

arXiv commentver. 2: to appear in J. Math. Phys., 37 pages, 6 figures, 1 table

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• Thermality of the Rindler horizon: A simple derivation from the structure of the inertial propagator
• Vacuum currents in partially compactified Rindler spacetime with an application to cylindrical black holes
• Wigner distributions in Rindler spacetime and nonvacuum Minkowski states