Emission from the D1D5 CFT
Steven G. Avery, Borun D. Chowdhury, Samir D. Mathur
TL;DR
This work builds a concrete bridge between the D1D5 CFT at the orbifold point and its gravity dual by formulating how flat-space fields couple to the CFT and by constructing explicit vertex operators for minimally coupled supergravity scalars. Using spectral flow, the authors map between Ramond and NS sectors to simplify calculations, then compute CFT amplitudes for emission from simple and highly excited states, including nonextremal microstates. They derive the emission rate formulas, perform careful combinatorics over the orbifold copies, and demonstrate exact agreement with gravity predictions in the dual geometry, reinforcing the AdS/CFT correspondence for dynamical emission processes. The framework is then extended to nonextremal states, showing Bose-enhancement in the emission rate and linking the CFT results to Hawking-like radiation from corresponding microstates. The methodology provides a robust toolkit for computing a wide class of CFT emission amplitudes and paves the way for exploring deformations away from the orbifold point. Overall, the paper solidifies the microscopic CFT description of D1D5 radiation and exemplifies precise matches with gravity across extremal and nonextremal regimes.
Abstract
It is believed that the D1D5 brane system is described by an 'orbifold CFT' at a special point in moduli space. We first develop a general formulation relating amplitudes in a d-dimensional CFT to absorption/emission of quanta from flat infinity. We then construct the D1D5 vertex operators for minimally coupled scalars in supergravity, and use these to compute the CFT amplitude for emission from a state carrying a single excitation. Using spectral flow we relate this process to one where we have emission from a highly excited initial state. In each case the radiation rate is found to agree with the radiation found in the gravity dual.
