Is our universe likely to decay within 20 billion years?
Don N. Page · 2008 · Physical Review D, 78(6), 063535
This source is used as supports evidence across 1 linked claim and 3 related evidence hubs. Its citation record is marked verified; that verifies the source trail, not the truth of any linked claim.
Summary
Argues that to avoid the conclusion that we are typical Boltzmann-brain observers, our current vacuum must decay on a timescale comparable to or shorter than the natural Boltzmann-brain nucleation timescale — in some models, less than ~20 Gyr.
How this source is used on the map
The clearest statement of how the Boltzmann-brain count is tamed by a finite vacuum lifetime; companion paper to 'Return of the Boltzmann brains'.
Citation record
- Authors
- Don N. Page
- Year
- 2008
- Publication
- Physical Review D, 78(6), 063535
- Source type
- Journal article
- Map role
- supports
- Credibility level
- primary
- Citation status
- Verified
- DOI
- 10.1103/PhysRevD.78.063535
- PubMed
- Not recorded
- Not recorded
Linked claims
Related evidence hubs
Related sources
Sets up one of the main physical pathways for resolving the paradox — vacuum decay into terminal states before BBs can dominate.
One of the canonical modern statements of the Boltzmann-brain comparison and its implications for inflation.
The paper that reignited modern interest in the Boltzmann-brain problem by linking it directly to the accelerating expansion of our universe.
The default scholarly reference for what Many-Worlds actually claims and where it is contested.
The standard reference for the cognitive-instability resolution and the philosophical case against taking Boltzmann-brain dominance as a real prediction.
Major physical objection to Boltzmann-brain dominance: the static de Sitter vacuum is sterile, so the mathematical fluctuation probability does not translate into real observers.