2021
DOI: 10.1007/jhep04(2021)269
|View full text |Cite
|
Sign up to set email alerts
|

Exploring properties of long-lived particles in inelastic dark matter models at Belle II

Abstract: The inelastic dark matter model is one kind of popular models for the light dark matter (DM) below O(1) GeV. If the mass splitting between DM excited and ground states is small enough, the co-annihilation becomes the dominant channel for thermal relic density and the DM excited state can be long-lived at the collider scale. We study scalar and fermion inelastic dark matter models for $$ \mathcal{O} $$ O (1) GeV DM at Belle II with U(1)D dark gauge symmetry broken into its Z2 s… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1

Citation Types

0
27
0

Year Published

2021
2021
2023
2023

Publication Types

Select...
8
1

Relationship

2
7

Authors

Journals

citations
Cited by 21 publications
(27 citation statements)
references
References 77 publications
0
27
0
Order By: Relevance
“…We assume q X is a real number and q X = 0, 1 such that all X 1 , X 2 and Φ are charged under U (1) X . On the other hand, in order to simplify our discussion, we don't [19,35,69,70]. These operators need special treatments or care.…”
Section: A Scalar C2cdm Modelsmentioning
confidence: 99%
“…We assume q X is a real number and q X = 0, 1 such that all X 1 , X 2 and Φ are charged under U (1) X . On the other hand, in order to simplify our discussion, we don't [19,35,69,70]. These operators need special treatments or care.…”
Section: A Scalar C2cdm Modelsmentioning
confidence: 99%
“…• Dark-flavour non-diagonal production: as an example, consider inelastic dark matter coupled to a dark photon, e + e − → γA , A → χ 2 χ 1 , where χ 1 is a stable invisible particle and χ 2 is the LLP [24][25][26][27][28][29][30][31]77]. This example is an illustrative model that predicts only a single LLP, showing the importance of single-LLP searches (N dv = 1) where possible.…”
Section: Jhep09(2021)154mentioning
confidence: 99%
“…For example, if we consider the case of a dark photon that is kinetically mixed with the SM photon, there are strong constraints on the model if the dark photon decays either exclusively through its coupling to the SM [14][15][16][17][18], or invisibly to unseen hidden-sector states [19][20][21]. If, however, the dark photon decays to hidden-sector states that partially decay back to the SM (for example, in the case of inelastic DM [22][23][24][25][26][27][28][29][30][31]), then neither search strategy applies, and the parameter space can be relatively unconstrained. Indeed, truly model-independent constraints from electroweak precision tests [32] and deep inelastic scattering [33] are sufficiently weak that they do not completely exclude dark photons as an explanation for the 4σ discrepancy between theory and experiment in (g − 2) µ [34,35].…”
Section: Introductionmentioning
confidence: 99%
“…For past studies of LLPs at Belle II, see, e.g., refs. [63][64][65][66][67][68][69][70][71][72][73]. Experimental LLP searches conducted at BaBar and Belle appear in refs.…”
Section: Introductionmentioning
confidence: 99%