Supersymmetry, flavor physics and dark matter
| dc.creator | Ko, P. | |
| dc.date | 2005-02-24 | |
| dc.date.accessioned | 2026-07-07T03:54:27Z | |
| dc.date.available | 2026-07-07T03:54:27Z | |
| dc.description | In this talk, I first discuss $b\to d$, $b\to s$ and $s\to d$ transitions including time-dependent CP asymmetries in $B_d \to ϕK_s$ and Re ($ε^{'}/ε_K$). Then I show that the decay $B_s \to μ^+ μ^-$ is useful to distinguish various SUSY breaking mechanisms. I will also describe some possible connections between B physics and cosmology: (i) B physics and electroweak baryogenesis within SUSY models, and (ii) the correlation between the neutralino dark matter scattering and $B (B_s \to μ^+ μ^-)$. In particular, we point out that the current upper bound on $B (B_s \to μ^+ μ^-)$ form CDF and D0 collaborations can constrain the spin-independent neutralino scattering cross section more strongly than the CDMS bound. | |
| dc.description | Talk at the 1st GUC workshop, Cairo, Egypt | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0502228 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0502228 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/44241 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Supersymmetry, flavor physics and dark matter | |
| dc.type | text |