B physics and Supersymmetry
| dc.creator | Ko, P. | |
| dc.date | 2004-11-27 | |
| dc.date | 2005-01-18 | |
| dc.date.accessioned | 2026-07-07T03:53:58Z | |
| dc.date.available | 2026-07-07T03:53:58Z | |
| dc.description | In SUSY models, it is still possible to have large signals even if the current data on $K$ and $B$ systems are consistent with the CKM paradigm for flavor mixing and CP violation. I first discuss $b\to d$ and $b\to s$ transitions including time-dependent CP asymmetries in $B_d \to ϕK_s$, and usefulness of $B_s \to μ^+ μ^-$ to distinguish various SUSY breaking mechanisms. Then I will discuss 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 $B (B_s \to μ^+ μ^-)$. | |
| dc.description | Plenary talk at SUSY04, to appear in the proceeding; references added | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0411351 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0411351 | |
| dc.identifier | J.Korean Phys.Soc. 45 (2004) S410-S416 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/44053 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | B physics and Supersymmetry | |
| dc.type | text |