
TL;DR
This paper discusses a holographic approach to resolving the black hole information paradox, emphasizing its non-local nature and how external observations can detect deviations from normal radiation.
Contribution
It highlights the non-local aspects of the holographic resolution and how observations outside black holes can reveal these effects.
Findings
Holography offers a potential resolution to the paradox.
External observations can detect non-local effects.
Black holes may not radiate like ordinary bodies.
Abstract
Recent developments in holography have suggested a potential resolution to the black hole information paradox within the context of gravitational effective field theory. We emphasize the non-local nature of this proposed resolution, and highlight the ways in which observations outside the black hole can detect it and conclude that the black hole is not radiating like an ordinary body would.
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Pulsars and Gravitational Waves Research
