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Dark matter in supersymmetric models with axino LSP in Randall-Sundrum II brane model

Jin U Kang et al JHEP05(2008)036   doi: 10.1088/1126-6708/2008/05/036  Help

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Jin U Kang1,2 and Grigoris Panotopoulos2
1 Department of Physics, Kim Il Sung University, Pyongyang, Democratic People's Republic of Korea
2 ASC, Department of Physics LMU, Theresienstr. 37, 80333 Munich, Germany
E-mail: Grigoris.Panotopoulos@physik.uni-muenchen.de

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
Published 9 May 2008

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