TY - JOUR
ID - 340
TI - On-shell Equation of the Lorentzian Classicalized Holographic Tensor Network
JO - Journal of Holography Applications in Physics
JA - JHAP
LA - en
SN - 2783-4778
AU - Konishi, Eiji
AD - Graduate School of Human and Environmental Studies, Kyoto University
Y1 - 2023
PY - 2023
VL - 3
IS - 3
SP - 37
EP - 44
KW - Holographic Principle
KW - Quantum Entanglement
KW - Holographic Tensor Network
KW - Classicalization
DO - 10.22128/jhap.2023.679.1052
N2 - 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: $-\sigma \hbar \theta=Mc^2$.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.
UR - https://jhap.du.ac.ir/article_340.html
L1 - https://jhap.du.ac.ir/article_340_32d95622308c9d447e20d3a641a0def3.pdf
ER -