Constraints to Dark Matter from Inert Higgs Doublet Model

Díaz, M. A.; Koch, Benjamin; Urrutia-Quiroga, Sebastián

doi:10.48550/arxiv.1511.04429

Cited by 10 publications

(13 citation statements)

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“…In fact, there are many possible extensions of the SM predicting WIMP DM candidates, e.g. wino, bino and higgsino in supersymmetric models [1,2], Kaluza-Klein particles in extra dimension models [3,4], inert scalars in extended Higgs models [5][6][7][8][9], and so on. In these extended models, DM is often accompanied with extra charged or colored particles, which mediates interaction between DM and SM.…”

Section: Introductionmentioning

confidence: 99%

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

Kawamura,

Okawa,

Omura

2020

Preprint

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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: complex/real scalar DM and Dirac/Majorana fermion DM. In addition, there are choices for the lepton chirality that couples to DM. We discuss the prediction of each model and compare it with the latest experimental constraints from the DM, the LHC, and the flavor experiments. We also propose a simple setup to achieve the discrepancy in the anomalous magnetic moment of muon.

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Section: Introductionmentioning

confidence: 99%

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

Kawamura,

Okawa,

Omura

2020

Preprint

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“…There are many studies in literature which look at the DM aspect of IHDM. A recent study [59] has treated the non-SM CP even scalar in the IHDM as the DM candidate and found out allowed parameter space satisfying the relic density. Part of this parameter space gets ruled out from the direct detection and collider physics constraints.…”

Section: Inert Higgs Doublet Model For Low λ U Vmentioning

confidence: 99%

Can dark matter be an artifact of extended theories of gravity?

2016

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In this article, we propose different background models of extended theories of gravity, which are minimally coupled to the SM fields, to explain the possibility of genesis of dark matter without affecting the SM particle sector. We modify the gravity sector by allowing quantum corrections motivated from (1) local f (R) gravity and (2) non-minimally coupled gravity with SM sector and dilaton field. Next we apply conformal transformation on the metric to transform the action back to the Einstein frame. We also show that an effective theory constructed from these extended theories of gravity and SM sector looks exactly the same. Using the relic constraint observed by Planck 2015, we constrain the scale of the effective field theory (Λ U V ) as well as the dark matter mass (M ). We consider two cases-(1) light dark matter (LDM) and (2) heavy dark matter (HDM), and deduce upper bounds on thermally averaged cross section of dark matter annihilating to SM particles. Further we show that our model naturally incorporates self interactions of dark matter. Using these self interactions, we derive the constraints on the parameters of the (1) local f (R) gravity and (2) non-minimally coupled gravity from dark matter self interaction. Finally, we propose some different UV complete models from a particle physics point of view, which can give rise to the same effective theory that we have deduced from extended theories of gravity.

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“…The lightest scalar Higgs in the IDM, as a dark matter candidate, needs to be able to reconstruct the correct DM relic abundance. In Ref [12,13], they found that three allowed mass regimes for the lightest Higgs satisfy the requirement of relic abundance. The scalar dark matter particle has also been explored by various direct, indirect experiments and high energy colliders.…”

Section: Introductionmentioning

confidence: 99%

Searches for dark matter via charged Higgs pair production in the Inert Doublet Model at $γγ$ collider

Yang¹,

Song²,

Li³

et al. 2020

Preprint

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The Inert Doublet Model(IDM) is one of the simplest extensions beyond Standard Model(SM) with an extended scalar sector, which provide a scalar dark matter particle candidate. In this paper, we investigate the double charged Higgs production at γγ collider. By scanning the whole parameter space, we obtain the parameter points corresponding to the correct relic abundance of dark matter. After applying all theoretical and experimental constraints, the parameter space for the existence of dark matter is extremely restricted. We perform the analysis for the signal of H + H − production in the IDM and the SM backgrounds, and the optimized selection conditions are chosen in kinematic variables to maximize signal significance. Comparing signal with backgrounds, we obtain the parameter points which can be detected at future γγ collider experiments.

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Constraints to Dark Matter from Inert Higgs Doublet Model

Cited by 10 publications

References 0 publications

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

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

Can dark matter be an artifact of extended theories of gravity?

Searches for dark matter via charged Higgs pair production in the Inert Doublet Model at $γγ$ collider

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