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VOLUME 29 (1979) | ISSUE 3 | PAGE 196
The hydrodynamics of black hole vaporization
An approximate spherically-symmetric solution is obtained for the equations of relativistic hydrodynamics which describe the latter stage of the quantum vaporization of a black hole. The hydrodynamic state—terminating at temperatures of the order of the π-meson mass—provides means for finding the energy distribution of scattering particles.