Towards a gauge invariant volume-weighted probability measure for eternal inflation
Andrei Linde
TL;DR
Eternal inflation yields infinities and gauge-dependent cut-offs that blur probabilistic predictions across the multiverse. The paper proposes a stationary, gauge-invariant volume-weighted measure that ties probabilities to volume growth during inflation and the onset of stationarity, rendering results largely independent of time parametrization for $β>0$. In a simple three-minima model, the relative volumes obey $P(φ_1)/P(φ_5) = Γ_{32} e^{3N_{21}} / (Γ_{34} e^{3N_{45}})$, with the youngness paradox removed when clocks are reset at stationarity; the same principle extends to slow-roll stages and generalizes to temperatures via volume factors. This stationary approach offers a robust framework for comparing vacua in the landscape and clarifies when different volume-weighted measures agree, while pointing to extensions to more complex tunneling scenarios and slow-roll dynamics.
Abstract
An improved volume-weighted probability measure for eternal inflation is proposed. For the models studied in this paper it leads to simple and intuitively expected gauge-invariant results.
