The two faces of Hawking radiation

Abstract

What happens when Alice falls into a black hole? In spite of recent challenges by Almheiri et al. -- the ""firewall" hypothesis -- the consensus on this question tends to remain "nothing special". Here I argue that something rather special can happen near the horizon, already at the semiclassical level: besides the standard Hawking outgoing modes, Alice can records a quasi-thermal spectrum of ingoing modes, whose temperature and intensity diverges as Alice's Killing energy $E$ goes to zero. I suggest that this effect can be thought of in terms a "horizon-infinity duality", which relates the perception of near-horizon and asymptotic geodesic observers -- the two faces of Hawking radiation.

Honorable Mention in the Gravity Research Foundation 2013 Essay Competition

References in corpus (2)

• Minimal conditions for the existence of a Hawking-like flux
• Quantum nature of black holes

Cited by in corpus (6)

• Excluding Black Hole Firewalls with Extreme Cosmic Censorship
• Something special at the event horizon
• The effective Tolman temperature in curved spacetimes
• Quantum frictionless trajectories versus geodesics
• Excavations at the gravitationally collapsed site: Recent findings
• Quantum fields in curved space-time, semiclassical gravity, quantum gravity phenomenology, and analogue models: Report on session D4 at GR20