Back reaction and Hawking radiation from a Vaidya black hole

Details Back reaction and Hawking radiation from a Vaidya black hole Back reaction and Hawking radiation from a Vaidya black hole

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ap%26ss.312..315z&link_type=abstract

Astrophysics and Space Science, Volume 312, Issue 3-4, pp. 315-319

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

Using Damour-Ruffini’s and Hamilton-Jacobi’s methods, Hawking radiation from a Vaidya black hole is investigated. Due to non-stationary black holes, the event horizon r H and the entropy S are all related to both the mass m( υ) and dot{r}H . When the back-reaction of particles’s energy to space-time is considered, we get the emission probability. It is found that the result is different from that of the stationary Schwarzschild black hole, because dot{r}H is the function of mass m( υ).

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