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arXiv · 2004.04956

Firewall From Effective Field Theory

Pei-Ming Ho·Yuki Yokokura
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Abstract

For an effective field theory in the background of an evaporating black hole with spherical symmetry, we consider non-renormalizable interactions and their relevance to physical effects. The background geometry is determined by the semi-classical Einstein equation for an uneventful horizon where the vacuum energy-momentum tensor is small for freely falling observers. Surprisingly, after Hawking radiation appears, the transition amplitude from the Unruh vacuum to certain multi-particle states grows exponentially with time for a class of higher-derivative operators after the collapsing matter enters the near-horizon region, despite the absence of large curvature invariants. Within the scrambling time, the uneventful horizon transitions towards a firewall, and eventually the effective field theory breaks down.

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Pei-Ming Ho, Yuki Yokokura. 2020-04-10. Firewall From Effective Field Theory. https://arxiv.org/abs/2004.04956

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