Cérebros de Boltzmann

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

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.
Comments:32 pp, 2 figs The work has been significantly improved and extended. In discussing the Boltzmann Brain (BB) nucleation rate, we corrected the statement and the implications of the Bekenstein bound. Other additions include a toy model based on an ideal gas, discussions of BB's in Schwarzschild-de Sitter space and the stability of BB's against expansion, and the generalization of dominant vacua
Subjects:High Energy Physics - Theory (hep-th); Cosmology and Extragalactic Astrophysics (astro-ph.CO); General Relativity and Quantum Cosmology (gr-qc)
Report number:MIT-CTP-3975, SU-ITP-08/20
Cite as:arXiv:0808.3778v2 [hep-th]


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