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

被引:41
作者
Bailly, Sean [1 ]
Choi, Ki-Young [2 ,3 ]
Jedamzik, Karsten [1 ]
Roszkowski, Leszek [4 ]
机构
[1] Univ Montpellier 2, Lab Phys Theor & Astroparticules, CNRS, UMR 5825, F-34095 Montpellier 5, France
[2] Univ Autonoma Madrid, Dept Fis Teor C 11, E-28049 Madrid, Spain
[3] Univ Autonoma Madrid, Inst Fis Teor, CSIC, E-28049 Madrid, Spain
[4] Univ Sheffield, Dept Phys & Astron, Sheffield S3 7RH, S Yorkshire, England
关键词
Cosmology of Theories beyond the SM; Supersymmetric Effective Theories; COSMOLOGICAL CONSTRAINTS; SPECTRAL DISTORTIONS; SUPERSYMMETRY; NUCLEOSYNTHESIS; THERMALIZATION; SAVE;
D O I
10.1088/1126-6708/2009/05/103
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
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 T-R less than or similar to a few x 10(7) GeV from over-production of Li-6 from bound state effects. We also find an upper limit on the stau lifetime of 3 x 10(4) sec, which is nearly an order of magnitude larger than the simple limit 5 x 10(3) sec often used to avoid the effect of bound-state catalysis. The bound on T R is relaxed to less than or similar to a few x 10(8) GeV when we use a more conservative bound on Li-6/Li-7, in which case a new region at small stau mass at similar to 100GeV and much longer lifetimes opens up. Such a low stau mass region can be easily tested at the LHC.
引用
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页数:17
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