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Numerical Computations of Entanglement Measures in Curved Space

Suresh Govindarajan, Sreehari A Padinhareveettil, Raghotham A Kulkarni

TL;DR

This work develops a covariant, lattice-like numerical framework to compute entanglement entropy and logarithmic negativity for scalar and abelian gauge fields in curved backgrounds, extending Srednicki's flat-space results to AdS$_4$, RT surfaces in AdS$_3$, and dS$_4$. The method discretizes space via proper distance, builds quadratic Hamiltonians, and diagonalizes reduced-density matrices across angular modes to obtain EE and E_N. It demonstrates a clear area-law scaling $S\sim \kappa R^2$, with the slope controlled by the AdS radius $L$ and reconcilable with flat-space limits when $L\to\infty$, and it verifies the universal term predictions using heat-kernel coefficients. The study also reveals divergences in the negativity in 3+1d and above, while showing convergent behavior in 2+1d, providing a bridge between numerical entanglement measures in curved spacetimes and analytic heat-kernel analyses.

Abstract

We numerically compute the entanglement entropy and negativity for scalar fields and abelian gauge fields in a variety of situations. These extend computations of Srednicki to situations involving curved space. We discretize space in a covariant way. Finally, we compare some of our results with those obtained via the heat kernel coefficients.

Numerical Computations of Entanglement Measures in Curved Space

TL;DR

This work develops a covariant, lattice-like numerical framework to compute entanglement entropy and logarithmic negativity for scalar and abelian gauge fields in curved backgrounds, extending Srednicki's flat-space results to AdS, RT surfaces in AdS, and dS. The method discretizes space via proper distance, builds quadratic Hamiltonians, and diagonalizes reduced-density matrices across angular modes to obtain EE and E_N. It demonstrates a clear area-law scaling , with the slope controlled by the AdS radius and reconcilable with flat-space limits when , and it verifies the universal term predictions using heat-kernel coefficients. The study also reveals divergences in the negativity in 3+1d and above, while showing convergent behavior in 2+1d, providing a bridge between numerical entanglement measures in curved spacetimes and analytic heat-kernel analyses.

Abstract

We numerically compute the entanglement entropy and negativity for scalar fields and abelian gauge fields in a variety of situations. These extend computations of Srednicki to situations involving curved space. We discretize space in a covariant way. Finally, we compare some of our results with those obtained via the heat kernel coefficients.
Paper Structure (25 sections, 167 equations, 16 figures)

This paper contains 25 sections, 167 equations, 16 figures.

Figures (16)

  • Figure 1: Foliation of a constant $t$ slice using constant $\eta$ and $x$ surfaces. $L$ is taken to be 1 here. Constant $\eta$ surfaces (red) are RT surfaces. Both $\eta$ and $x$ can take values from $-\infty$ to $\infty$.
  • Figure 2: Entanglement entropy of scalar field in a sphere in flat space time vs. radius. Entanglement entropy increases linearly with $R^2$.
  • Figure 3: Entanglement entropy vs. $R^2$ for different masses. Addition of mass reduces the entanglement entropy.
  • Figure 4: Fitting the dependence of entanglement entropy on mass (i) $1/(1+p\hat{m}^b)$ with $p=0.6339, \ b=1.6649$, (ii)$ce^{-\hat{m}d}$ with $c=0.9943,\ d= 0.5013$.
  • Figure 5: Entanglement entropy vs. $R^2$ calculated from working with discretizing proper distance $u$ in radial direction for different values of AdS radius. We see the area law, ie. entanglement entropy $\propto R^2$. We also observe the slope is a function of the AdS radius $L$.
  • ...and 11 more figures