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Causality Violation, Gravitational Shockwaves and UV Completion

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arxiv 1512.04952 v2 pith:ZOFIBWGT submitted 2015-12-15 hep-th

classification hep-th
keywords causalityeffectivetimeactionactionsbackgroundenergiesgravitational
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The effective actions describing the low-energy dynamics of QFTs involving gravity generically exhibit causality violations. These may take the form of superluminal propagation or Shapiro time advances and allow the construction of "time machines", i.e. spacetimes admitting closed non-spacelike curves. Here, we discuss critically whether such causality violations may be used as a criterion to identify unphysical effective actions or whether, and how, causality problems may be resolved by embedding the action in a fundamental, UV complete QFT. We study in detail the case of photon scattering in an Aichelburg-Sexl gravitational shockwave background and calculate the phase shifts in QED for all energies, demonstrating their smooth interpolation from the causality-violating effective action values at low-energy to their manifestly causal high-energy limits. At low energies, these phase shifts may be interpreted as backwards-in-time coordinate jumps as the photon encounters the shock wavefront, and we illustrate how the resulting causality problems emerge and are resolved in a two-shockwave time machine scenario. The implications of our results for ultra-high (Planck) energy scattering, in which graviton exchange is modelled by the shockwave background, are highlighted.

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  1. Microcausality without Lorentz invariance

    hep-th 2025-02 conditional novelty 8.0 of 10

    Microcausality in Lorentz-violating states is equivalent to specific analyticity and exponential boundedness of spatial Fourier transforms of commutators, with explicit EFT constraints.

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