Suppressing Hawking radiation by quantum Zeno effect

We present evidence that quantum Zeno effect, otherwise working only for microscopic systems, may also work for large black holes (BH's). The expectation that a BH geometry should behave classically at time intervals larger than the Planck time tPltPl indicates that the quantum process of measurement of classical degrees of freedom takes time of the order of tPltPl. Since BH has only a few classical degrees of freedom, such a fast measurement makes a macroscopic BH strongly susceptible to the quantum Zeno effect, which repeatedly collapses the quantum state to the initial one, the state before the creation of Hawking quanta. By this mechanism, Hawking radiation from a BH of mass M   is strongly suppressed by a factor of the order of mPl/MmPl/M.