UV And IR Effects On Hawking Radiation
arXiv:2207.07122 · doi:10.1007/JHEP03(2023)002
Abstract
We study the time-dependence of Hawking radiation for a black hole in the Unruh vacuum, and find that it is not robust against certain UV and IR effects. If there is a UV cutoff at the Planck scale, Hawking radiation is turned off after the scrambling time. In the absence of a UV cutoff, Hawking radiation is sensitive to the IR cutoff through a UV/IR connection due to higher-derivative interactions in the effective theory. Furthermore, higher-derivative interactions with the background contribute to a large amplitude of particle creation that changes Hawking radiation. This unexpected large effect is related to a peculiar feature of the Hawking particle wave packets.
35 pages, 5 figures, references added, minor modification
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Cited by in corpus (6)
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- UV Dispersive Effects on Hawking Radiation
- A Stringy Effect on Hawking Radiation
- Towards Hamiltonian Formalism for String Field Theory and Nonlocality
- UV Effects and Short-Lived Hawking Radiation: Alternative Resolution of Information Paradox