UNIVERSAL ENTROPY BOUND AND DISCRETE SPACETIME
UNIVERSAL ENTROPY BOUND AND DISCRETE SPACETIME
Starting from the universal entropy bounds suggested by Bekenstein and Susskind and applying them to the black-body radiation situation, we get a cut-off of space $ Δx \geq χl_{\mathrm{P}}$ with $χ\geq 0.1$. We go further to get a cut-off of time $ Δt \geq χl_{\mathrm{P}}/c $, thus, the discrete space-time …