Phase Transitions from the Fifth Dimension
Kaustubh Agashe, Peizhi Du, Majid Ekhterachian, Soubhik Kumar, Raman, Sundrum

TL;DR
This paper investigates the cosmological phase transition in 5D warped compactifications, analyzing bubble nucleation and gravitational wave production, with implications for the hierarchy problem and holographic duality.
Contribution
It introduces a smooth bounce configuration for 5D bubble nucleation, providing a lower bound on transition rates and exploring modifications to the Goldberger-Wise stabilization.
Findings
Slow transition with supercooling in minimal Goldberger-Wise setup
Prompt transition with modified Goldberger-Wise potential
Potential gravitational wave signals from bubble collisions
Abstract
We study the cosmological transition of 5D warped compactifications, from the high-temperature black-brane phase to the low-temperature Randall-Sundrum I phase. The transition proceeds via percolation of bubbles of IR-brane nucleating from the black-brane horizon. The violent bubble dynamics can be a powerful source of observable stochastic gravitational waves. While bubble nucleation is non-perturbative in 5D gravity, it is amenable to semiclassical treatment in terms of a "bounce" configuration interpolating between the two phases. We demonstrate how such a bounce configuration can be smooth enough to maintain 5D effective field theory control, and how a simple ansatz for it places a rigorous lower-bound on the transition rate in the thin-wall regime, and gives plausible estimates more generally. When applied to the Hierarchy Problem, the minimal Goldberger-Wise stabilization of the…
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