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Non-commutative corrections to the classical expression for the fuzzy spherearea are found out through the asymptotic expansion for its heat kernel trace.As an important consequence, some quantum gravity deviations in the luminosityof black holes must appear. We calculate these deviations for a static,spherically symmetric, black-hole with a horizon modeled by a fuzzy sphere. Theresults obtained could be verified through the radiation of black holes formedin the Large Hadron Collider (LHC).

A note on the fuzzy sphere area spectrum, black hole luminosity, and the quantum nature of spacetime