Bubble Wall Profiles in Supersymmetric Models
Peter John (University of Heidelberg)
TL;DR
This paper computes bubble wall profiles in supersymmetric models, specifically the MSSM and NMSSM, using numerical methods to understand phase transition dynamics relevant for early universe cosmology.
Contribution
It provides new numerical solutions for bubble wall profiles in both minimal and non-minimal supersymmetric models, advancing the understanding of phase transitions in these theories.
Findings
Numerical solutions for MSSM and NMSSM bubble walls are presented.
Methodology for solving equations of motion for bubble profiles is detailed.
Results contribute to understanding electroweak phase transitions in supersymmetric models.
Abstract
We present solutions to the equations of motion for bubble wall profiles in the minimal and a non minimal supersymmetric extension of the Standard model. We discuss the method of the numerical approach and present results for the two models (MSSM and NMSSM). Calculations for the NMSSM were done in collaboration with S.J. Huber and M.G. Schmidt.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Methane Hydrates and Related Phenomena · Astro and Planetary Science