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Title: Black Holes, Hawking Radiation and the Information Paradox

Technical Report ·
DOI:https://doi.org/10.2172/808686· OSTI ID:808686

This talk is about results obtained by Kirill Melnikov and myself pertaining to the canonical quantization of a massless scalar field in the presence of a Schwarzschild black hole. After a brief summary of what we did and how we reproduce the familiar Hawking temperature and energy flux, I focus attention on how our discussion differs from other treatments. In particular I show that we can define a system which fakes an equilibrium thermodynamic object whose entropy is given by the A/4 (where A is the area of the black hole horizon), but for which the assignment of a classical entropy to the system is incorrect. Finally I briefly discuss a discretized version of the theory which seems to indicate that things work in a surprising way near r=0.

Research Organization:
SLAC National Accelerator Lab., Menlo Park, CA (United States)
Sponsoring Organization:
USDOE Office of Science (US)
DOE Contract Number:
AC03-76SF00515
OSTI ID:
808686
Report Number(s):
SLAC-PUB-9595; TRN: US200308%%117
Resource Relation:
Other Information: PBD: 19 Nov 2002
Country of Publication:
United States
Language:
English

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