Stau relic density at the big-bang nucleosynthesis era in the coannihilation scenario and a solution to theLi7problem

We calculate the relic density of stau at the big-bang nucleosynthesis era in the coannihilation scenario of the minimal supersymmetric standard model. In this scenario, stau can be long lived and have significance in the remediation of light elements abundances. The freeze-out of stau is corroborated by solving the Boltzmann equation numerically, and the parameter dependence of the relic density is investigated. The possibility of solving the ⁷Li problem is examined by taking account into the long-lived stau. By adopting an observational value of ⁷Li in [J. Mel\'endez and I. Ram\'{}rez, Astrophys. J. 615, L33 (2004).], we get minimal supersymmetric standard model parameter space in which abundances of both dark matter and all of the light elements are reproduced in accordance with observations. We also address the influence of intergenerational mixing on our calculation.