Origin of Hawking Radiation: Firewall or Atmosphere?
Wontae Kim

TL;DR
This paper clarifies that Hawking radiation originates from the atmosphere near the horizon rather than the horizon itself, and discusses the conditions under which a firewall can exist due to infinite blueshift effects.
Contribution
It demonstrates through an exactly solvable model that the firewall arises from the Unruh vacuum's negative ingoing flux, and clarifies the true origin of Hawking radiation.
Findings
Hawking radiation originates from the atmosphere, not the horizon.
Firewall can be supported by infinite Tolman temperature due to blueshifted ingoing flux.
Hawking radiation and firewall are compatible under certain conditions.
Abstract
The Unruh vacuum not admitting any outgoing flux at the horizon implies that the origin of the outgoing Hawking radiation is the atmosphere of a near-horizon quantum region without resort to the firewall; however, the existence of the firewall of superplanckian excitations at the horizon can be supported by the infinite Tolman temperature at the horizon. In an exactly soluble model, we explicitly show that the firewall necessarily emerges out of the Unruh vacuum so that the Tolman temperature in the Unruh vacuum is divergent in essence due to the infinitely blueshifted negative ingoing flux crossing the horizon rather than the outgoing flux. We also show that the outgoing Hawking radiation in the Unruh vacuum indeed originates from the atmosphere, not just at the horizon, which is of no relevance to the infinite blueshift. Consequently, the firewall from the infinite Tolman temperature…
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