THE ROLE OF THE PLANCK SCALE IN BLACK HOLE RADIANCE
Abstract
Lorentz invariance plays a pivotal role in the derivation of the Hawking effect, which crucially requires an integration in arbitrarily small distances or, equivalently, in unbounded energies. New physics at the Planck scale could, therefore, potentially modify the emission spectrum. We argue, however, that the kinematic invariance can be deformed in such a way that the thermal spectrum remains insensitive to trans-Planckian physics.
This essay received an "honorable mention" in the 2007 Essay Competition of the Gravity Research Foundation.
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