Neutralino dark matter scattering and $B_s \to μ^+ μ^-$ in SUSY models
| dc.creator | Baek, Seungwon | |
| dc.creator | Kim, Yeong Gyun | |
| dc.creator | Ko, P. | |
| dc.date | 2004-06-03 | |
| dc.date | 2005-03-07 | |
| dc.date.accessioned | 2026-07-07T10:49:06Z | |
| dc.date.available | 2026-07-07T10:49:06Z | |
| dc.description | It is pointed out that there is a strong correlation between the neutralino dark matter scattering cross section $σ_{\tildeχ p}$ and the branching ratio for $B_s \to μ^+ μ^-$ within minimal supergravity (mSUGRA) and its extensions. This correlation arises mainly from $\tanβ$ and heavy neutral Higgs mass dependence, and shows a nice interplay between vastly different two observables within supersymmetric models. Current upper limit on $B(B_s \to μ^+ μ^-) < 5.8 \times 10^{-7}$ excludes substantial parameter space where $σ_{\tildeχ p}$ is within the CDMS sensitivity region. | |
| dc.description | version to appear in JHEP | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0406033 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0406033 | |
| dc.identifier | JHEP0502:067,2005 | |
| dc.identifier | doi:10.1088/1126-6708/2005/02/067 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/184108 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Neutralino dark matter scattering and $B_s \to μ^+ μ^-$ in SUSY models | |
| dc.type | text |