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Flaxino dark matter and stau decay

Authors
Chun, Eung JinKim, Hang BaeKohri, KazunoriLyth, David H.
Issue Date
Mar-2008
Publisher
Springer Verlag
Keywords
supersymmetry phenomenology; cosmology of theories beyond the SM
Citation
Journal of High Energy Physics, no.3, pp 1 - 15
Pages
15
Indexed
SCIE
SCOPUS
Journal Title
Journal of High Energy Physics
Number
3
Start Page
1
End Page
15
URI
https://scholarworks.bwise.kr/hanyang/handle/2021.sw.hanyang/178908
DOI
10.1088/1126-6708/2008/03/061
ISSN
1126-6708
1029-8479
Abstract
If the spontaneous breaking of Peccei-Quinn symmetry comes from soft supersymmetry breaking, the fermionic partners of the symmetry-breaking fields have mass of order the gravitino mass, and are called flatinos. The lightest flatino, called here the flaxino, is a CDM candidate if it is the lightest supersymmetric particle. We here explore flaxino dark matter assuming that the lightest ordinary supersymmetric particle is the stau, with gravity-mediated supersymmetry breaking. The decay of the stau to the flaxino is fast enough not to spoil the standard predictions of Big Bang Nucleosynthesis, and its track and decay can be seen in future colliders.
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