Pith. sign in

REVIEW 1 cited by

Is Our Universe Likely to Decay within 20 Billion Years?

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv hep-th/0610079 v2 pith:3GHNYGXY submitted 2006-10-09 hep-th astro-phgr-qc

Is Our Universe Likely to Decay within 20 Billion Years?

classification hep-th astro-phgr-qc
keywords universeasymptoticdecayfluctuationshighlylikelyobservationsrate
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
0 comments
read the original abstract

Observations that we are highly unlikely to be vacuum fluctuations suggest that our universe is decaying at a rate faster than the asymptotic volume growth rate, in order that there not be too many observers produced by vacuum fluctuations to make our observations highly atypical. An asymptotic linear e-folding time of roughly 16 Gyr (deduced from current measurements of cosmic acceleration) would then imply that our universe is more likely than not to decay within a time that is less than 19 Gyr in the future.

discussion (0)

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

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Dark Energy Bubble as Dynamical Dark Energy: Properties and CMB Constraints

    astro-ph.CO 2026-07 conditional novelty 6.0

    A late-time bubble of lower dark energy density can mimic DESI BAO features, but CMB dipole, kSZ, and sound-horizon constraints exclude the required parameters.