Entanglement Entropy of Two Spheres
Noburo Shiba
TL;DR
We address the entanglement structure of a massless free scalar field in vacuum for two separated spheres. Using a Bombelli-style lattice approach with Gaussian reduced density matrices, we compute the entanglement entropies and show that the mutual information $S_{A;B}$ between the two spheres is UV-cutoff independent and scales as the product of their surface areas at large separation, i.e., $S_{A;B} \propto R_1^{d-1} R_2^{d-1} / r^{2d-2}$ for dimension $d$. Numerical results in $d=3$ reveal $S_{A;B} \approx - g R_1^2 R_2^2 / r^4$ with $g \approx 0.26$, while in $d=2$ the decay is $-S_{A;B} \approx 0.37 R_1 R_2 / r^2$, and interior regions contribute nonuniformly to mutual information. These findings inform potential connections to black-hole entanglement and yield a scalable method for computing entanglement in arbitrary geometries.
Abstract
We study the entanglement entropy S_{AB} of a massless free scalar field on two spheres A and B whose radii are R_1 and R_2, respectively, and the distance between the centers of them is r. The state of the massless free scalar field is the vacuum state. We obtain the result that the mutual information S_{A;B}:=S_A+S_B-S_{AB} is independent of the ultraviolet cutoff and proportional to the product of the areas of the two spheres when r>>R_1,R_2, where S_A and S_B are the entanglement entropy on the inside region of A and B, respectively. We discuss possible connections of this result with the physics of black holes.
