False-Vacuum Decay Lifetime When the Decay Integral Has an Upper Temperature Cutoff

The bounce actions span from 208 in the shallow case to 8527 in the deep case, and the lifetimes vary correspondingly over an enormous range because the action sits in an exponential. The intermediate case gives a decay probability of 10^-279 per Hubble four-volume at its reference epoch, corresponding to a lifetime of 10^279 Hubble times, comfortably stable. In all three cases the epochs that dominate the decay probability lie at or below the scale set by the potential itself, far below the ceiling temperature. Removing the formal history above the ceiling therefore changes the survival conclusion in none of the three cases: potentials that are stable remain stable, and the shallow case, which decays promptly, does so at low temperature where the truncation is irrelevant. This study is simulated and computed from stated assumptions; it is not a measurement.

Authors

Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-11-11
DOI
https://doi.org/10.5281/zenodo.24145317
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
0.00
Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
NOV
article

False-Vacuum Decay Lifetime When the Decay Integral Has an Upper Temperature Cutoff

William Alexander Aldred
Zenodo (CERN European Organization for Nuclear Research)
Cosmology and Gravitation Theories
article

False-Vacuum Decay Lifetime When the Decay Integral Has an Upper Temperature Cutoff

William Alexander Aldred
article en

Abstract

The bounce actions span from 208 in the shallow case to 8527 in the deep case, and the lifetimes vary correspondingly over an enormous range because the action sits in an exponential. The intermediate case gives a decay probability of 10^-279 per Hubble four-volume at its reference epoch, corresponding to a lifetime of 10^279 Hubble times, comfortably stable. In all three cases the epochs that dominate the decay probability lie at or below the scale set by the potential itself, far below the ceiling temperature. Removing the formal history above the ceiling therefore changes the survival conclusion in none of the three cases: potentials that are stable remain stable, and the shallow case, which decays promptly, does so at low temperature where the truncation is irrelevant. This study is simulated and computed from stated assumptions; it is not a measurement.

Zenodo (CERN European Organization for Nuclear Research)
Cosmology and Gravitation Theories
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.

Laika access coming soon