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- W1494955780 abstract "When a black hole radiates particles, it losses energy and shrinks, the horizon contracts from its original radius to a new smaller radius. This leads to the separation between the initial and final radii, which sets the barrier for the particles to tunnel We develop the work of Parikh [Phys. Rev. Lett. 85 (2000) 5042; Gen. Rel. Grav. 36 (2004) 2419] to a Horowitz-Strominger black hole, i.e. applying the Wentzel-Kramers-Brillouin approximation and semi-classical method to calculate the rate of the Hawking radiation. The result agrees with Г～e^-21mf=e^△SBH. It is also proven that the energy spectrum deviates from exact thermality." @default.
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- W1494955780 date "2005-01-01" @default.
- W1494955780 modified "2023-09-23" @default.
- W1494955780 title "Hawking Radiation from the Horowitz-Strominger Black Hole" @default.
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