A toolbox for black hole scattering
Nava Gaddam, Nico Groenenboom
TL;DR
This work constructs a comprehensive toolbox for black hole scattering by deriving near-horizon graviton propagators in a complete partial-wave basis for all parity and multipole modes, and by identifying which graviton sectors couple at leading order. It then shows how the interacting sector can be recast as an effective scalar theory with a four-vertex, dramatically simplifying the computation of elastic and inelastic amplitudes and enabling ladder-like resummations. A key outcome is that black hole entropy can be interpreted as arising from the multiplicity of external legs in dominant 2→2N amplitudes, linking microphysical scattering to thermodynamic entropy. The framework opens paths to compute higher-point and loop amplitudes efficiently, extend to other fields, and explore signatures such as gravitational echoes and Post-BH corrections, with potential relevance to near-horizon quantum gravity phenomenology.
Abstract
Hawking's free field theory is expected to break down after Page time. In previous work, we have shown that a primary dynamical reason for this breakdown is the dominance of graviton fluctuations of the horizon that mediate scattering processes. In this article, we present a toolbox for such `black hole scattering' computations. The toolbox comprises of explicit expressions for the graviton propagator near the horizon in an angular momentum basis for all angular momentum modes of either parity, the leading interaction rules, and most importantly a rewriting of the theory in terms of a scalar theory with an interesting four-vertex. We demonstrate how this rewriting drastically reduces the number of diagrams to be calculated in the original formulation. Finally and perhaps most remarkably, we observe that the black hole entropy appears to emerge from the multiplicity of external legs of the dominant $2\rightarrow2N$ amplitudes in this theory.
