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Effective Tolman temperature induced by trace anomaly
Myungseok Eune, Yongwan Gim, Wontae Kim
Despite the finiteness of stress tensor for a scalar field on the four-dimensional Schwarzschild black hole in the Israel-Hartle-Hawking vacuum, the Tolman temperature in thermal e…
Hawking, Fiducial, and Free-fall Temperatures of Black Hole on Gravity's Rainbow
Yongwan Gim, Wontae Kim
On gravity's rainbow, the energy of particles affects the geometry of black hole in such a way that the Hawking temperature of black hole is appropriately modified. It means that t…
A Quantal Tolman Temperature
Yongwan Gim, Wontae Kim
The conventional Tolman temperature based on the assumption of the traceless condition of energy-momentum tensor for matter fields is infinite at the horizon if Hawking radiation i…
Black Hole Complementarity in Gravity's Rainbow
Yongwan Gim, Wontae Kim
To see how the gravity's rainbow works for black hole complementary, we evaluate the required energy for duplication of information in the context of black hole complementarity by…