Boltzmann brains and the scale-factor cutoff measure of the multiverse

TL;DR

This paper evaluates the scale-factor cutoff measure in the multiverse by calculating the ratio of Boltzmann brains to normal observers, ensuring the measure predicts a universe like ours with a finite and acceptable observer ratio.

Contribution

It provides a quantitative analysis of Boltzmann brain prevalence using the scale-factor cutoff measure, deriving conditions for acceptable observer ratios in the multiverse.

Findings

The ratio of Boltzmann brains to normal observers is finite under this measure.

Derived an expression relating the ratio to nucleation and decay rates.

Discussed parameter conditions for the measure to produce realistic predictions.

Abstract

To make predictions for an eternally inflating "multiverse", one must adopt a procedure for regulating its divergent spacetime volume. Recently, a new test of such spacetime measures has emerged: normal observers - who evolve in pocket universes cooling from hot big bang conditions - must not be vastly outnumbered by "Boltzmann brains" - freak observers that pop in and out of existence as a result of rare quantum fluctuations. If the Boltzmann brains prevail, then a randomly chosen observer would be overwhelmingly likely to be surrounded by an empty world, where all but vacuum energy has redshifted away, rather than the rich structure that we observe. Using the scale-factor cutoff measure, we calculate the ratio of Boltzmann brains to normal observers. We find the ratio to be finite, and give an expression for it in terms of Boltzmann brain nucleation rates and vacuum decay rates. We discuss the conditions that these rates must obey for the ratio to be acceptable, and we discuss estimates of the rates under a variety of assumptions.