The spectral function in a strongly coupled, thermalising CFT
Alice Bernamonti, Ben Craps, Joris Vanhoof

TL;DR
This paper investigates the time-dependent spectral function and effective temperature in a thermalising two-dimensional conformal field theory using holographic duality, extending previous work to dynamic, non-equilibrium settings.
Contribution
It extends the calculation of spectral functions and effective temperatures to a time-dependent, thermalising CFT dual to AdS3-Vaidya spacetime, employing geodesic approximation and novel analytic continuation methods.
Findings
Computed spectral functions during thermalisation process
Demonstrated evolution of effective temperature over time
Extended holographic techniques to non-equilibrium dynamics
Abstract
In relation to the fluctuation-dissipation theorem, we discuss a time-dependent notion of spectral function and effective temperature. Extending recent results from arXiv:1212.6066, we work out these quantities in a two-dimensional thermalising CFT dual to AdS3-Vaidya spacetime which interpolates between a black brane geometry at early times and a higher temperature black brane at late times. The computation is carried out in the gravitational holographic dual in the geodesic approximation and using a non-standard analytic continuation.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Noncommutative and Quantum Gravity Theories
