# Classical Entanglement Structure in the Wavefunction of Inflationary   Fluctuations

**Authors:** Elliot Nelson, C. Jess Riedel

arXiv: 1704.00728 · 2017-12-13

## TL;DR

This paper demonstrates how classical metric perturbations emerge from quantum vacuum fluctuations during inflation through entanglement and decoherence, leading to a classical, stochastic spacetime structure.

## Contribution

It reveals that entanglement structure and minimal gravitational interactions cause decoherence, producing classical metric perturbations from quantum inflationary fluctuations.

## Key findings

- Exponential records of metric fluctuations on large scales.
- Decoherence leads to classical branches of the wavefunction.
- Accounts for entropy production and stochastic spacetime emergence.

## Abstract

We argue that the preferred classical variables that emerge from a pure quantum state are determined by its entanglement structure in the form of redundant records: information shared between many subsystems. Focusing on the early universe, we ask how classical metric perturbations emerge from vacuum fluctuations in an inflationary background. We show that the squeezing of the quantum state for super-horizon modes, along with minimal gravitational interactions, leads to decoherence and to an exponential number of records of metric fluctuations on very large scales, $\lambda/\lambda_{\rm Hubble}>\Delta_\zeta^{-2/3}$, where $\Delta_\zeta\lesssim 10^{-5}$ is the amplitude of scalar metric fluctuations. This determines a preferred decomposition of the inflationary wavefunction into orthogonal "branches" corresponding to classical metric perturbations, which defines an inflationary entropy production rate and accounts for the emergence of stochastic, inhomogeneous spacetime geometry.

## Full text

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## Figures

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## References

14 references — full list in the complete paper: https://tomesphere.com/paper/1704.00728/full.md

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Source: https://tomesphere.com/paper/1704.00728