THE REACTION TO THE SCHWARZSCHILD SPACE-TIME BY THE HAWKING EVAPORATION
考虑Hawking蒸发对Schwarzschild时空反作用后的静态球对称度规

For the black hole having Hawking radiation, it must have effect on the space-time metric (the so-called back-reaction). By combination of the result from themodynamical approach with the back-reaction of the black hole and the semiclassical Einstein equation, we get the modified Schwarzschild space-time metric. This method is much more simple and convenient than that of Jork's.