Lorentzian spectral zeta functions on asymptotically Minkowski spacetimes

preprint2022arXivOpen access

Abstract

In this note, we consider perturbations of Minkowski space as well as more general spacetimes on which the wave operator □g\square_g is essentially self-adjoint. We review a recent result which gives the meromorphic continuation of the Lorentzian spectral zeta function density, i.e. of the trace density of complex powers α↦(□g−iε)−αα\mapsto (\square_g-i \varepsilon)^{-α}. In even dimension n≥4n\geq 4, the residue at n2−1\frac{n}{2}-1 is shown to be a multiple of the scalar curvature in the limit ε→0+\varepsilon\to 0^+. This yields a spectral action for gravity in Lorentzian signature.

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