pith. sign in

arxiv: 1708.02265 · v3 · pith:SSW36S5Onew · submitted 2017-08-07 · ✦ hep-th · astro-ph.CO· gr-qc· hep-ph· quant-ph

Entangled de Sitter from Stringy Axionic Bell pair I: An analysis using Bunch Davies vacuum

classification ✦ hep-th astro-ph.COgr-qchep-phquant-ph
keywords entanglemententropybellbunchdaviesquantumsitteranalysis
0
0 comments X p. Extension
pith:SSW36S5O Add to your LaTeX paper What is a Pith Number?
\usepackage{pith}
\pithnumber{SSW36S5O}

Prints a linked pith:SSW36S5O badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more

read the original abstract

In this work, we study the quantum entanglement and compute entanglement entropy in de Sitter space for a bipartite quantum field theory driven by axion originating from ${\bf Type~ IIB}$ string compactification on a Calabi Yau three fold (${\bf CY^3}$) and in presence of ${\bf NS5}$ brane. For this compuation, we consider a spherical surface ${\bf S}^2$, which divide the spatial slice of de Sitter (${\bf dS_4}$) into exterior and interior sub regions. We also consider the initial choice of vaccum to be Bunch Davies state. First we derive the solution of the wave function of axion in a hyperbolic open chart by constructing a suitable basis for Bunch Davies vacuum state using Bogoliubov transformation. We then, derive the expression for density matrix by tracing over the exterior region. This allows us to compute entanglement entropy and R$\acute{e}$nyi entropy in $3+1$ dimension. Further we quantify the UV finite contribution of entanglement entropy which contain the physics of long range quantum correlations of our expanding universe. Finally, our analysis compliments the necessary condition for the violation of Bell's inequality in primordial cosmology due to the non vanishing entanglement entropy for axionic Bell pair.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.