pith. sign in

Renyi Entropies for Free Field Theories

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
abstract

Renyi entropies S_q are useful measures of quantum entanglement; they can be calculated from traces of the reduced density matrix raised to power q, with q>=0. For (d+1)-dimensional conformal field theories, the Renyi entropies across S^{d-1} may be extracted from the thermal partition functions of these theories on either (d+1)-dimensional de Sitter space or R x H^d, where H^d is the d-dimensional hyperbolic space. These thermal partition functions can in turn be expressed as path integrals on branched coverings of the (d+1)-dimensional sphere and S^1 x H^d, respectively. We calculate the Renyi entropies of free massless scalars and fermions in d=2, and show how using zeta-function regularization one finds agreement between the calculations on the branched coverings of S^3 and on S^1 x H^2. Analogous calculations for massive free fields provide monotonic interpolating functions between the Renyi entropies at the Gaussian and the trivial fixed points. Finally, we discuss similar Renyi entropy calculations in d>2.

citation-role summary

background 1

citation-polarity summary

fields

hep-th 2

years

2025 2

verdicts

UNVERDICTED 2

roles

background 1

polarities

background 1

representative citing papers

De Sitter Horizon Edge Partition Functions

hep-th · 2025-01-29 · unverdicted · novelty 5.0

Edge partition functions for totally symmetric tensors in dS_{d+1} are decomposed under so(d), with the linearized gravity case receiving contributions from shift-symmetric fields on S^{d-1} suggesting an embedded brane interpretation.

citing papers explorer

Showing 2 of 2 citing papers.

  • De Sitter Horizon Edge Partition Functions hep-th · 2025-01-29 · unverdicted · none · ref 151 · internal anchor

    Edge partition functions for totally symmetric tensors in dS_{d+1} are decomposed under so(d), with the linearized gravity case receiving contributions from shift-symmetric fields on S^{d-1} suggesting an embedded brane interpretation.

  • From Weyl Anomaly to Defect Supersymmetric R\'enyi Entropy and Casimir Energy hep-th · 2025-01-16 · unverdicted · none · ref 30 · internal anchor

    In 6D (2,0) theories, defect supersymmetric Rényi entropy contribution is linear in 1/n and equals a constant times (2b - d2); Casimir energy contribution equals -d2 (up to constant) in the chiral algebra limit.