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Minimal dark matter

Open access
Cirelli, Marco, Fornengo, Nicolao, Strumia, Alessandro·2006·Nuclear Physics B

Abstract

Abstract A few multiplets that can be added to the SM contain a lightest neutral component which is automatically stable and provides allowed DM candidates with a non-standard phenomenology. Thanks to coannihilations, a successful thermal abundance is obtained for well defined DM masses. The best candidate seems to be a SU ( 2 ) L fermion quintuplet with mass 4.4 TeV, accompanied by a charged partner 166 MeV heavier with life-time 1.8 cm , that manifests at colliders as charged tracks disappearing in π ± with 97.7% branching ratio. The cross section for usual NC direct DM detection is σ SI = f 2 1.0 × 10 −43 cm 2 where f ∼ 1 is a nucleon matrix element. We study prospects for CC direct detection and for indirect detection.

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Metadata

Authors
Cirelli, M., Fornengo, N., & Strumia, A.
Venue
Nuclear Physics B
Publisher
Elsevier BV
Published
2006-10
Volume
753
Issue
1-2
Pages
178-194
ISSN
0550-3213 (ISSN-L)
OpenAlex
W1991806240
Cited by
1,002
References
1
FWCI
14.51
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: Minimal dark matter. https://app.cochat.ai/papers/10.1016/j.nuclphysb.2006.07.012
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Cirelli, M., Fornengo, N., & Strumia, A. (2006). Minimal dark matter. Nuclear Physics B. https://doi.org/10.1016/j.nuclphysb.2006.07.012

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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