Dark matter in UED: The role of the second KK level

G. Bélanger*, M. Kakizaki, A. Pukhov

*この論文の責任著者

研究成果: ジャーナルへの寄稿学術論文査読

63 被引用数 (Scopus)

抄録

We perform a complete calculation of the relic abundance of the KK-photon LKP in the universal extra dimension model including all coannihilation channels and all resonances. We show that the production of level 2 particles which decay dominantly into SM particles contribute significantly to coannihilation processes involving level 1 KK-leptons. As a result the preferred dark matter scale is increased to R-1 = 1.3 TeV. A dark matter candidate at or below the TeV scale can only be found in the non-minimal model by reducing the mass splittings between the KK-particles and the LKP. The LKP nucleon scattering cross section is typically small, σ < 10-10 pb, unless the KK-quarks are nearly degenerate with the LKP.

本文言語英語
論文番号009
ジャーナルJournal of Cosmology and Astroparticle Physics
2011
2
DOI
出版ステータス出版済み - 2011/02

ASJC Scopus 主題領域

  • 天文学と天体物理学

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