Dual-temperature acceleration radiation. (arXiv:2102.00158v2 [gr-qc] UPDATED)
<a href="http://arxiv.org/find/gr-qc/1/au:+Good_M/0/1/0/all/0/1">Michael R.R. Good</a>, <a href="http://arxiv.org/find/gr-qc/1/au:+Mitra_A/0/1/0/all/0/1">Ayan Mitra</a>, <a href="http://arxiv.org/find/gr-qc/1/au:+Zarikas_V/0/1/0/all/0/1">Vasileios Zarikas</a>
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.
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.
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