On-shell Equation of the Lorentzian Classicalized Holographic Tensor Network

In the Lorentzian classicalized holographic tensor network (cHTN), we derive its relativistic on-shell equation from its Lorentzian action in the presence of a relativistic massive particle in the bulk spacetime: -\sigma \hbar \theta=Mc^۲.Here, \sigma is the von Neumann entropy of the cHTN per site in nats, \theta is the real-proper-time expansion of the cHTN defined along the world line of the particle, and M is the non-zero mass of the particle.We explain the physical properties, interpretation, and consequences of this equation.Specifically, from this equation we derive the properties of the on-shell proper acceleration of another massive particle in the bulk spacetime as those of the gravitational acceleration induced by the original massive particle.