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Автор Sean Bailly
Дата выпуска 2011-03-01
dc.description We present supersymmetric scenarios with gravitino LSP and stau NLSP in the case of a non-standard model of cosmology with the addition of a dark component in the pre-BBN era. In the context of the standard model of cosmology, gravitino LSP has drawn quite some attention as it is a good candidate for dark matter. It is produced in scattering processes during reheating after inflation and from the decay of the stau. With a long lifetime, the stau decays during Big Bang Nucleosynthesis. It is strongly constrained by the abundance of light elements but can however address the known ``BBN lithium problem''. It requires fairly massive staus m<sub></sub>≳ 1TeV and puts an upper bound on the reheating temperature T<sub>R</sub> ≃ 10<sup>7</sup> GeV which does not satisfy the requirements for thermal leptogenesis. For the non-standard cosmological scenario, the reheating temperature bound can be strongly relaxed T<sub>R</sub> ≫ 10<sup>9</sup>GeV and the lithium-7 problem solved with a stau typical mass of m<sub></sub> ∼ 600–700 GeV and down to ∼ 400GeV with a very important dark component that could enable possible production and detection at the LHC.
Формат application.pdf
Издатель Institute of Physics Publishing
Название Gravitino dark matter and the lithium primordial abundance within a pre-BBN modified expansion
Тип paper
DOI 10.1088/1475-7516/2011/03/022
Electronic ISSN 1475-7516
Журнал Journal of Cosmology and Astroparticle Physics
Том 2011
Первая страница 22
Последняя страница 022
Аффилиация Sean Bailly; Laboratoire de Physique Théorique LAPTH, Université de Savoie, CNRS (UMR 5108), BP 110, F-74941 Annecy-Le-Vieux Cedex, France
Выпуск 03

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