Planckian Scattering and Black Holes
Sebastian de Haro (Utrecht University)

TL;DR
This paper extends 't Hooft's black hole S-matrix to include transverse effects, showing it reproduces correct dynamics and amplitudes, and reveals a holographic, non-commutative structure on the horizon.
Contribution
It introduces a string theory model with an antisymmetric tensor background that captures both longitudinal and transverse black hole scattering dynamics beyond the eikonal approximation.
Findings
Reproduces correct momentum transfer in scattering processes.
Amplitude matches Veneziano amplitude in a certain limit.
Operators of horizon degrees of freedom are non-commuting, with a modified uncertainty principle.
Abstract
Recently, 't Hooft's S-matrix for black hole evaporation, obtained from the gravitational interactions between the in-falling particles and Hawking radiation, has been generalised to include transverse effects. The action describing the collision turned out to be a string theory action with an antisymmetric tensor background. In this article we show that the model reproduces both the correct longitudinal and transverse dynamics, even when one goes beyond the eikonal approximation or particles collide at nonvanishing incidence angles. It also gives the correct momentum tranfer that takes place in the process. Including a curvature on the horizon provides the action with an extra term, which can be interpreted as a dilaton contribution. The amplitude of the scattering is seen to reproduce the Veneziano amplitude in a certain limit, as in earlier work by 't Hooft. The theory resembles a…
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