Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
2010-01-08
Phys.Rev.D82:115030,2010
Physics
High Energy Physics
High Energy Physics - Phenomenology
9 pages, 5 figures, figure 5 corrected
Scientific paper
10.1103/PhysRevD.82.115030
We calculate the relic density of stau at the beginning of the Big-Bang Nucleosynthesis (BBN) era in the coannihilation scenario of minimal supersymmetric standard model (MSSM). In this scenario, stau can be long-lived and form bound states with nuclei. We put constraints on the parameter space of MSSM by connecting the calculation of the relic density of stau to the observation of the light elements abundance, which strongly depends on the relic density of stau. Consistency between the theoretical prediction and the observational result, both of the dark matter abundance and the light elements abundance, requires the mass difference between the lighter stau and the lightest neutralino to be around 100MeV, the stau mass to be 300 -- 400 GeV, and the mixing angle of the left and right-handed staus to be $\sin\theta_{\tau} = (0.65 \textrm{--} 1)$.
Jittoh Toshifumi
Kohri Kazunori
Koike Masafumi
Sato Joe
Shimomura Takashi
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