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JHEP05(2008)036 doi: 10.1088/1126-6708/2008/05/036
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Abstract. The axino dark matter hypothesis in RSII brane model is studied. Within the framework of CMSSM we assume that the lightest neutralino or stau is the NLSP, and that the axino production has a single contribution from the NLSP decay. It is found that the axino can play the role of dark matter in the universe and we determine what the axino mass should be for different values of the five-dimensional Planck mass. An upper bound is obtained for the latter.
Key words: Cosmology of Theories beyond the SM; Supersymmetric Standard Model
Received 15 February 2008, accepted for publication 3 May 2008| Post to CiteUlike | | Post to Connotea | | Post to Bibsonomy |
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