http://arxiv.org/abs/2102.00158
We solve for a system that emits acceleration radiation at two different temperatures. The equilibrium states occur asymptotically in Planck distributions and transition non-thermally. The model is simple enough to obtain a global solution for the radiation spectrum analytically. We present it as a potentially useful model for investigation of non-thermal vacuum acceleration radiation in the presence of final(initial) asymptotic thermodynamic horizon(less) states in equilibrium.
M. Good, A. Mitra and V. Zarikas
Tue, 2 Feb 21
28/86
Comments: Accepted to Astronomy Reports. 10 pages, 4 figures