2005/04/30 by Yasaman Farzan, Farzan, Yasaman · 1 citation
Physics and Astronomy · #Dark Matter and Cosmic Phenomena #FOS: Physical sciences #High Energy Physics - Phenomenology (hep-ph) #Neutrino Physics Research #Particle physics theoretical and experimental studies #hep-ph
paper · pdf · doi:10.48550/arxiv.hep-ph/0505004
6 pages, 3 figures, talk presented at the XXXXth Moriond conference on electroweak interactions and unified theories; v2: minor changes
openalex publication_date 2005/04/30 · arxiv created 2005/05/10 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
To embed the seesaw mechanism in the MSSM, two or three right-handed neutrino supermultiplets, Ni, have to be added to the model. In this framework, the supersymmetry breaking potential will include a new term called neutrino B-term: MBνN N/2. In this talk, we present a toy model that generates a large neutrino B-term keeping other supersymmetry breaking parameters small. We then review the consequences of having a large neutrino B-term on the electroweak symmetry breaking parameters and electric dipole moments (EDMs) of elementary particles.