The Cardy-Verlinde equation in a spherical symmetric gravitational collapse
arXiv:1007.4142 · doi:10.1142/S0217751X10050986
Abstract
The Cardy-Verlinde formula is analyzed in the contest of the gravitational collapse. Starting from the holographic principle, we show how the equations for a homogeneous and isotropic gravitational collapse describe the formation of the black hole entropy. Some comments on the role of the entangled entropy and the connection with the c-theorem are made.
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