Constraining the interaction strength between dark matter and visible matter. II: Scalar, vector and spin-3/2 dark matter
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Publication:447336
DOI10.1016/j.nuclphysb.2012.02.016zbMath1246.83279arXiv1112.6052OpenAlexW1967620349MaRDI QIDQ447336
Xiao-Jun Bi, Jia-Ming Zheng, Dao-Xin Yao, Hong-Hao Zhang, Zhao-Huan Yu, Zhi Bing Li
Publication date: 3 September 2012
Published in: Nuclear Physics. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1112.6052
Related Items (4)
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 scalar case ⋮ Simplified models of dark matter with a long-lived co-annihilation partner
Cites Work
- Dark matter, proton decay and other phenomenological constraints in \({\mathcal F}\)-\(SU(5)\)
- Gamma ray line constraints on effective theories of dark matter
- Constraining the interaction strength between dark matter and visible matter: I. Fermionic dark matter
- Model-independent implications of the \(e^{\pm }\), \(\bar{p}\) cosmic ray spectra on properties of Dark Matter
- PHYSICS OF DARK MATTER IN THE LIGHT OF DARK ATOMS
- Fermi Decay of Higher Spin Particles
- On the theory of higher spin fields
- On a Theory of Particles with Half-Integral Spin
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