Constraining the interaction strength between dark matter and visible matter: I. Fermionic dark matter

DOI10.1016/j.nuclphysb.2011.09.009zbMath1229.83090arXiv1012.2022OpenAlexW2064304114MaRDI QIDQ659371

Jia-Ming Zheng, Xiao-Jun Bi, Zhao-Huan Yu, Jun-Wen Shao, Hong-Hao Zhang, Zhi Bing Li

Publication date: 18 January 2012

Published in: Nuclear Physics. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1012.2022

Mathematics Subject Classification ID

Unified quantum theories (81V22) Relativistic cosmology (83F05)

Related Items (7)

The 750 GeV diphoton excess at the LHC and dark matter constraints ⋮ Classification of effective operators for interactions between the standard model and dark matter ⋮ CEPC precision of electroweak oblique parameters and weakly interacting dark matter: the fermionic case ⋮ The new formulation of Higgs effective field theory ⋮ Constraining the interaction strength between dark matter and visible matter. II: Scalar, vector and spin-3/2 dark matter ⋮ Simplified models of dark matter with a long-lived co-annihilation partner ⋮ PHYSICS OF DARK MATTER IN THE LIGHT OF DARK ATOMS

Cites Work

• Dark matter direct detection rate in a generic model with micrOMEGAs 2.2
• Model-independent implications of the \(e^{\pm }\), \(\bar{p}\) cosmic ray spectra on properties of Dark Matter

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