Entanglement entropy due to near horizon degrees of freedom
arXiv:1405.6461 · doi:10.1140/epjp/i2015-15154-9
Abstract
Assuming that the dominant contribution, to the entropy due to entanglement across a spherical hypersurface, comes from the near horizon degrees of freedom, we analytically derive the entropy of a free massless scalar field in Minkowski spacetime across a spherical entangling surface. The resulting entanglement entropy is found to be proportional to the entangling surface as expected. A logarithmic subleading term with positive coefficient is also found through numerical computation. We have extended the analysis to higher dimensions as well.
Substantially revised version, title and abstract modified, new conclusions
References in corpus (8)
- Towards a derivation of holographic entanglement entropy
- Generalized gravitational entropy
- Universal terms for the entanglement entropy in 2+1 dimensions
- Power-law corrections to entanglement entropy of horizons
- Where are the black hole entropy degrees of freedom ?
- Zero modes and divergence of entanglement entropy
- Corrections to Bekenstein-Hawking entropy --- Quantum or not-so quantum?
- Entanglement entropy for non-zero genus topologies