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We derive the general form of Hawking temperature for Vaidya black hole inthe tunneling pictures. This kind of black hole is regarded as the descriptionof a more realistic one since it's time dependent decreasing mass due to theevaporation process. Clearly, the temperature would be time dependent as ourfindings. We use the semiclassical methods, namely radial null geodesic andcomplex paths methods. Both methods are found to give the same results. Then,we discuss the possible form of corresponding entropy.

Semiclassical Methods for Hawking Radiation from a Vaidya Black Hole