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Cosmological phase transitions at three loops: the final verdict on perturbation theory

5 Pith papers cite this work. Polarity classification is still indexing.

5 Pith papers citing it
abstract

We complete the perturbative program for equilibrium thermodynamics of cosmological first-order phase transitions by determining the finite-temperature effective potential of gauge-Higgs theories at next-to-next-to-next-to-next-to-leading order (N$^4$LO). The computation of the three-loop effective potential required to reach this order is extended to generic models in dimensionally reduced effective theories in a companion article. Our N$^4$LO result is the last perturbative order before confinement renders electroweak gauge-Higgs theories non-perturbative at four loops. By contrasting our analysis with non-perturbative lattice results, we find a remarkable agreement. As a direct application for predictions of gravitational waves produced by a first-order transition, our computation provides the final fully perturbative results for the phase transition strength and speed of sound.

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years

2026 5

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Polyakov Loops Tame Phase Transitions

hep-ph · 2026-07-07 · conditional · novelty 6.0

Polyakov loop contributions to the thermal effective potential soften electroweak phase transitions, disfavoring first-order transitions and suppressing gravitational-wave signals.

Constraining the real scalar singlet extension of the SM

hep-ph · 2026-06-10 · unverdicted · novelty 4.0

Real scalar singlet extension of SM permits strong first-order EWPT for singlet masses up to ~1 TeV; HL-LHC tests large fraction of space while FCC offers discovery reach.

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