Current status and muon g - 2 explanation of lepton portal dark matter

In this paper, we summarize phenomenology in lepton portal dark matter (DM) models, where DM couples to leptons and extra leptons/sleptons. There are several possible setups: a DM field is either a complex/real scalar or a Dirac/Majorana fermion, and chiralities of leptons that couple to the DM are different according to the spin of the DM. We discuss the prediction of each model and compare it with the latest experimental constraints from the DM detections, the LHC, and the flavor experiments. We also propose simple setups to resolve the discrepancy in the anomalous magnetic moment of muon.

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Publication Details

Journal
OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information)
Published
2024-11-25
DOI
https://doi.org/10.1007/jhep08%282020%29042
Citations
49
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article

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article

Current status and muon g - 2 explanation of lepton portal dark matter

Junichiro Kawamura
49 citations
OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information)
Dark Matter and Cosmic Phenomena
article

Current status and muon g - 2 explanation of lepton portal dark matter

Junichiro Kawamura
article en
49 citations

Abstract

In this paper, we summarize phenomenology in lepton portal dark matter (DM) models, where DM couples to leptons and extra leptons/sleptons. There are several possible setups: a DM field is either a complex/real scalar or a Dirac/Majorana fermion, and chiralities of leptons that couple to the DM are different according to the spin of the DM. We discuss the prediction of each model and compare it with the latest experimental constraints from the DM detections, the LHC, and the flavor experiments. We also propose simple setups to resolve the discrepancy in the anomalous magnetic moment of muon.

OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information)
Office of Scientific and Technical Information (US), Keio University (JP), The Ohio State University (US)
U.S. Department of Energy, Ministry of Education, Culture, Sports, Science and Technology, Natural Sciences and Engineering Research Council of Canada, Japan Society for the Promotion of Science
Dark Matter and Cosmic Phenomena
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