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Electric shocks: bounding Einstein-Maxwell theory with time delays on boosted RN backgrounds

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arxiv 2312.17328 v1 pith:H5RDFGBN submitted 2023-12-28 hep-th

classification hep-th
keywords backgroundstimetheorydelayfieldshockwaveboostedbounds
verification ladder T0 review T1 audit T2 compute T3 formal

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The requirement that particles propagate causally on non-trivial backgrounds implies interesting constraints on higher-derivative operators. This work is part of a systematic study of the positivity bounds derivable from time delays on shockwave backgrounds. First, we discuss shockwaves in field theory, which are infinitely boosted Coulomb-like field configurations. We show how a positive time delay implies positivity of four-derivative operators in scalar field theory and electromagnetism, consistent with the results derived using dispersion relations, and we comment on how additional higher-derivative operators could be included. We then turn to gravitational shockwave backgrounds. We compute the infinite boost limit of Reissner-Nordstr\"om black holes to derive charged shockwave backgrounds. We consider photons traveling on these backgrounds and interacting through four-derivative corrections to Einstein-Maxwell theory. The inclusion of gravity introduces a logarithmic term into the time delay that interferes with the straightforward bounds derivable in pure field theory, a fact consistent with CEMZ and with recent results from dispersion relations. We discuss two ways to extract a physically meaningful quantity from the logarithmic time delay -- by introducing an IR cutoff, or by considering the derivative of the time delay -- and comment on the bounds implied in each case. Finally, we review a number of additional shockwave backgrounds which might be of use in future applications, including spinning shockwaves, those in higher dimensions or with a cosmological constant, and shockwaves from boosted extended objects.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Can weak-gravity, causality-violation arguments constrain modified gravity?

    hep-th 2025-06 conditional novelty 6.0 of 10

    Eikonal amplitude-based causality constraints on dynamical Chern-Simons gravity apply only at large impact parameters in weak gravity, making them less stringent than current astrophysical bounds.

  2. Causality bounds from charged shockwaves in 5d

    hep-th 2024-12 conditional novelty 5.0 of 10

    Causality on 5d charged shockwaves gives positivity bounds on four-derivative Einstein-Maxwell couplings, with gravity weakening the pure-field-theory bounds and near-horizon photons providing the strongest constraints.

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