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The CGHS black hole has a spectrum and temperature that corresponds to anaccelerated reflecting boundary condition in flat spacetime. The betacoefficients are identical to a moving mirror model where the acceleration isexponential in laboratory time. The center and the event horizon of the blackhole are at the same location modeled by the perfectly reflecting regularitycondition that red-shifts the field modes. In addition to computing the energyflux, we find the corresponding parameter associated with the black hole massand the cosmological constant in the gravitational analog system. Generalizedto any mirror trajectory we derive the self-force (Lorentz-Abraham-Dirac) andexpress it and the power (Larmor) in connection with entanglement entropy,inviting an interpretation of acceleration radiation in terms of informationflow. The mirror self-force and radiative power are applied to the particularCGHS black hole analog moving mirror which reveals the physics of informationat the horizon during asymptotic approach to thermal equilibrium.

Relativistic quantum information as radiation reaction: entanglement entropy and self-force of a moving mirror analog to the CGHS black hole