4.6 Article

Magnetic fields at first order phase transition: a threat to electroweak baryogenesis

Journal

Publisher

IOP PUBLISHING LTD
DOI: 10.1088/1475-7516/2011/10/030

Keywords

baryon asymmetry; magnetic fields; supersymmetry and cosmology

Funding

  1. Swiss National Science Foundation [200021-125237]
  2. Spanish Consolider-Ingenio Programme [CSD2007-00042]
  3. CICYT, Spain [FPA 2008-01430]
  4. Belgian IISN convention of FNRS [4.4514.08]
  5. ICREA Funding Source: Custom

Ask authors/readers for more resources

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 120 GeV, respectively. We show that even for moderate values of the magnetic field, the Higgs mass required to preserve the baryon asymmetry is below the present experimental bound. As a consequence electroweak baryogenesis within the MSSM should be confronted on the one hand to future measurements at the LHC on the Higgs and the right-handed stop masses, and on the other hand to more precise calculations of the magnetic field produced at the electroweak phase transition.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.6
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

No Data Available
No Data Available