2006/05/31 by Seyed Yaser Ayazi, Yasaman Farzan
Physics and Astronomy · #Baryogenesis #Dark Matter and Cosmic Phenomena #Electroweak interaction #Neutrino Physics Research #Particle physics #Particle physics theoretical and experimental studies #Physics #hep-ph
paper · pdf · doi:10.1103/physrevd.74.055008
published as Phys.Rev.D74:055008,2006 · 33 pages, 12 figures
arxiv created 2006/06/09 · openalex publication_date 2006/09/28 · arxiv updated 2014/11/17 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
The possibility of cancellation between different contributions to de, dn and dHg is reconsidered with special emphasis on the region that is phenomenologically interesting (intermediate values of tan\ensuremathβ and sub-TeV sfermion masses). It is found that in the range favored by electroweak baryogenesis (i.e., |\ensuremathμ|\ensuremath≃M1 or |\ensuremathμ|\ensuremath≃M2), sin[\ensuremathθ_\ensuremathμ+\ensuremathθ_M1]\ensuremath∼1 can be compatible with the EDM bounds even for slepton masses below 500 GeV. Such large values of the phases promise a successful electroweak baryogenesis. The possibility of large CP-odd effects at linear collider is also discussed.