Magnetic Fields at First Order Phase Transition: A Threat to Electroweak Baryogenesis
Andrea De Simone, Germano Nardini, Mariano Quiros, Antonio Riotto

TL;DR
This paper demonstrates that magnetic fields generated during a first order electroweak phase transition can significantly weaken baryon asymmetry preservation, challenging the viability of electroweak baryogenesis in the MSSM.
Contribution
It reveals the impact of magnetic fields on sphaleron transitions, showing they can undermine electroweak baryogenesis in the MSSM, and emphasizes the need for future experimental and theoretical studies.
Findings
Magnetic fields lower sphaleron energy, increasing washout of baryon asymmetry.
In the presence of magnetic fields, the Higgs mass needed for baryogenesis is below current experimental bounds.
Electroweak baryogenesis in MSSM is threatened by magnetic field effects, requiring further investigation.
Abstract
The generation of the observed baryon asymmetry may have taken place during the electroweak phase transition, thus involving physics testable at LHC, a scenario dubbed electroweak baryogenesis. In this paper we point out that the magnetic field which is produced in the bubbles of a first order phase transition endangers the baryon asymmetry produced in the bubble walls. The reason being that the produced magnetic field couples to the sphaleron magnetic moment and lowers the sphaleron energy; this strengthens the sphaleron transitions inside the bubbles and triggers a more effective wash out of the baryon asymmetry. We apply this scenario to the Minimal Supersymmetric extension of the Standard Model (MSSM) where, in the absence of a magnetic field, successful electroweak baryogenesis requires the lightest CP-even Higgs and the right-handed stop masses to be lighter than about 127 GeV and…
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