# Opacity and Effective Field Theory in Anti-de Sitter Backgrounds

**Authors:** Sylvain Fichet

arXiv: 1905.05779 · 2019-11-07

## TL;DR

This paper demonstrates that in Lorentzian AdS, bulk interactions cause exponential decay of propagators towards the horizon, effectively censoring regions where the 5d effective field theory breaks down, with implications for decay rates.

## Contribution

It shows that exponential suppression of propagators in Lorentzian AdS occurs due to bulk interactions, extending known Euclidean results and impacting EFT validity.

## Key findings

- Exponential decay of propagators in Lorentzian AdS with interactions.
- Gravitational dressing, especially scalar components, causes suppression.
- Decay rates of bulk fields are exponentially suppressed.

## Abstract

We consider quantum field theory in a five-dimensional anti-de Sitter background, possibly truncated by 4d branes. In the Euclidian version of this space, it is known that propagators exponentially decay when they go far enough towards the Poincar\'e horizon, i.e. deep enough into the IR region of the AdS bulk. In this note we show that an analogous property exists in Lorentzian AdS. The exponential suppression is found to occur in the presence of bulk interactions dressing the AdS propagators. We calculate one-loop gravitational dressing and find that the suppression effect comes from the scalar component of the 5d graviton. We then argue that, at least at strong coupling, this exponential decay censors the region of spacetime where the 5d effective field theory would become invalid. As an application we estimate the rate for the cascade decay of bulk fields---which are known to produce soft spherical events with high multiplicity---and find this rate to be exponentially suppressed.

## Full text

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## Figures

2 figures with captions in the complete paper: https://tomesphere.com/paper/1905.05779/full.md

## References

20 references — full list in the complete paper: https://tomesphere.com/paper/1905.05779/full.md

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Source: https://tomesphere.com/paper/1905.05779