Abstract

We study the effect of electromagnetic interactions on the classical soft theorems on an asymptotically AdS background in 4 spacetime dimensions, in the limit of a small cosmological constant or equivalently a large AdS radius l. This identifies 1/l2 perturbative corrections to the known asymptotically flat spacetime leading and subleading soft factors. Our analysis is only valid to leading order in 1/l2. The leading soft factor can be expected to be universal and holds beyond tree level. This allows us to derive a 1/l2 corrected Ward identity, following the known equivalence between large gauge Ward identities and soft theorems in asymptotically flat spacetimes.

Highlights

  • Of the single soft photon theorem to subleading order in four spacetime dimensions [20]: Seflmat = Seflmat;leading + Seflmat;subleading, with

  • We study the effect of electromagnetic interactions on the classical soft theorems on an asymptotically Anti-de Sitter (AdS) background in 4 spacetime dimensions, in the limit of a small cosmological constant or equivalently a large AdS radius l

  • We find the effect of the small AdS potential on the classical soft photon theorem

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Summary

Perturbations of AdS Reissner-Nordström spacetime

We are interested in studying the classical soft photon theorem in asymptotically AdS backgrounds. Since we are interested in studying the radiation emitted by the scattering of a probe particle moving in an unbounded trajectory on the spacetime (from the point of view of an asymptotic observer) we introduce isotropic coordinates. We refer the reader to [33] for further justification on choosing this particular coordinate system In these coordinates, the resulting radiation will be isotropic in all spatial directions. Retaining terms up to leading order in φ and 1/l2, we find that the metric components in (2.8) take the form ρ2 g00 = − 1 + 2φ + l2 , g0i = 0 , ρ2 gij = δij 1 − 2φ + 2l2. Note that the spacetime metric in (2.12) provides the leading AdS correction about an asymptotically flat spacetime and in isotropic coordinates it just behaves like the AdSSchwarzschild metric with a gauge potential. √ 3The equality of GQ and GM holds in the extremal limit

Perturbations of Einstein-Maxwell equations
Solutions of the field equations
Classical soft photon factor
Classical soft graviton factor
Ward identities from soft photon factors
Conclusion and open questions
A Classical soft graviton theorem
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