Cosmological Phase Transitions and their Properties in the NMSSM

TL;DR

This paper investigates the nature of cosmological phase transitions in the NMSSM, analyzing their properties and implications for electroweak baryogenesis, using an effective field theory approach and considering current experimental constraints.

Contribution

It provides a detailed analysis of phase transition structures, bubble wall properties, and velocities in the NMSSM, highlighting conditions favorable for electroweak baryogenesis.

Findings

Possible one- or two-step first-order phase transitions.

Bubble wall velocities are often sub-luminal and sub-sonic.

Conditions for successful electroweak baryogenesis are identified.

Abstract

We study cosmological phase transitions in the Next-to-Minimal Supersymmetric Standard Model (NMSSM) in light of the Higgs discovery. We use an effective field theory approach to calculate the finite temperature effective potential, focusing on regions with significant tree-level contributions to the Higgs mass, a viable neutralino dark matter candidate, 1-2 TeV stops, and with the remaining particle spectrum compatible with current LHC searches and results. The phase transition structure in viable regions of parameter space exhibits a rich phenomenology, potentially giving rise to one- or two-step first-order phase transitions in the singlet and/or $SU(2)$ directions. We compute several parameters pertaining to the bubble wall profile, including the bubble wall width and $\Delta\beta$ (the variation of the ratio in Higgs vacuum expectation values across the wall). These quantities can vary significantly across small regions of parameter space and can be promising for successful electroweak baryogenesis. We estimate the wall velocity microphysically, taking into account the various sources of friction acting on the expanding bubble wall. Ultra-relativistic solutions to the bubble wall equations of motion typically exist when the electroweak phase transition features substantial supercooling. For somewhat weaker transitions, the bubble wall instead tends to be sub-luminal and, in fact, likely sub-sonic, suggesting that successful electroweak baryogenesis may indeed occur in regions of the NMSSM compatible with the Higgs discovery.