Excluding Electroweak Baryogenesis in the MSSM
David Curtin, Prerit Jaiswal, Patrick Meade
TL;DR
This paper assesses whether electroweak baryogenesis (EWBG) can occur in the MSSM, arguing that the only viable realization is the Light Stop Scenario (LSS) which links a strong first-order phase transition to stop-sector dynamics and Higgs couplings. It then uses LHC Higgs data, particularly correlations among loop-induced and tree-level Higgs processes, to test the MSSM EWBG hypothesis in a largely model-independent way. By combining ATLAS and CMS Higgs searches, the authors find strong tension with EWBG in both non-decoupling and decoupling limits, excluding EWBG at the 90–95% confidence level under a ~125 GeV Higgs assumption, and nearly the entire EWBG parameter space at >90% CL even without that assumption except for a narrow mh window around 117–119 GeV. The work identifies a distinct “fingerprint” of EWBG in Higgs observables, offering a practical route to falsify EWBG in the MSSM with current and near-future Higgs measurements.
Abstract
In the context of the MSSM the Light Stop Scenario (LSS) is the only region of parameter space that allows for successful Electroweak Baryogenesis (EWBG). This possibility is very phenomenologically attractive, since it allows for the direct production of light stops and could be tested at the LHC. The ATLAS and CMS experiments have recently supplied tantalizing hints for a Higgs boson with a mass of ~ 125 GeV. This Higgs mass severely restricts the parameter space of the LSS, and we discuss the specific predictions made for EWBG in the MSSM. Combining data from all the available ATLAS and CMS Higgs searches reveals a tension with the predictions of EWBG even at this early stage. This allows us to exclude EWBG in the MSSM at greater than (90) 95% confidence level in the (non-)decoupling limit, by examining correlations between different Higgs decay channels. We also examine the exclusion without the assumption of a ~ 125 GeV Higgs. The Higgs searches are still highly constraining, excluding the entire EWBG parameter space at greater than 90% CL except for a small window of m_h ~ 117 - 119 GeV.
