A re-analysis of gravitino dark matter in the constrained MSSM

被引:5
作者
Laboratoire de Physique Théorique et Astroparticules, CNRS UMR 5825, Université Montpellier II, F-34095 Montpellier Cedex 5, France [1 ]
不详 [2 ]
不详 [3 ]
不详 [4 ]
机构
[1] Laboratoire de Physique Théorique et Astroparticules, CNRS UMR 5825, Université Montpellier II
[2] Departamento de Física Teórica C-XI, Universidad Autónoma de Madrid, Cantoblanco
[3] Instituto de Física Teórica UAM/CSIC, Universidad Autónoma de Madrid, Cantoblanco
[4] Department of Physics and Astronomy, University of Sheffield, S3 7RH, Sheffield
来源
Chin. Phys. | 2009年 / 6卷 / 2565-2570期
关键词
Fractals; -; Galaxies; Gravitation;
D O I
10.1088/1674-1056/18/6/074
中图分类号
学科分类号
摘要
We re-consider the gravitino as dark matter in the framework of the Constrained MSSM. We include several recently suggested improvements on: (i) the thermal production of gravitinos, (ii) the calculation of the hadronic spectrum from NLSP decay and (iii) the BBN calculation including stau bound-state effects. In most cases we find an upper bound on the reheating temperature TR ≲ a few × 107GeV from over-production of 6Li from bound state effects. We also find an upper limit on the stau lifetime of 3 × 104sec, which is nearly an order of magnitude larger than the simple limit 5 × 103sec often used to avoid the effect of bound-state catalysis. The bound on TR is relaxed to ≲ a few × 108GeV when we use a more conservative bound on 6Li/7Li, in which case a new region at small stau mass at ∼ 100GeV and much longer lifetimes opens up. Such a low stau mass region can be easily tested at the LHC. © 2009 Chin. Phys. Soc. and IOP Publishing Ltd.
引用
收藏
页码:2565 / 2570
页数:5
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