2019
DOI: 10.1007/jhep02(2019)186
|View full text |Cite
|
Sign up to set email alerts
|

LHC-friendly minimal freeze-in models

Abstract: We propose simple freeze-in models where the observed dark matter abundance is explained via the decay of an electrically charged and/or coloured parent particle into Feebly Interacting Massive Particles (FIMP). The parent particle is long-lived and yields a 1 The HL-LHC is expected to produce ∼ 10 8 Higgs bosons. Typical freeze-in values for yχ lie in the O(10 −13 − 10 −7 ) range, would yield less than 10 −4 DM events at the HL-LHC in our scenario.2 Since, as we will see later on, the DM production at the LHC… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
1
1

Citation Types

2
136
0

Year Published

2020
2020
2024
2024

Publication Types

Select...
6
1

Relationship

1
6

Authors

Journals

citations
Cited by 98 publications
(140 citation statements)
references
References 201 publications
(275 reference statements)
2
136
0
Order By: Relevance
“…We note that ATLAS can reconstruct tracks as short as ∼ 12 cm, while for the CMS tracker the minimum reconstructed track length is ∼ 25 − 30 cm (see e.g. the discussion in [31,80]). As a result, the ATLAS search can constrain smaller lifetimes than the CMS study.…”
Section: Disappearing Track Signaturesmentioning
confidence: 91%
See 3 more Smart Citations
“…We note that ATLAS can reconstruct tracks as short as ∼ 12 cm, while for the CMS tracker the minimum reconstructed track length is ∼ 25 − 30 cm (see e.g. the discussion in [31,80]). As a result, the ATLAS search can constrain smaller lifetimes than the CMS study.…”
Section: Disappearing Track Signaturesmentioning
confidence: 91%
“…As previously mentioned, there are several important cosmological constraints on this class of freeze-in DM scenarios (for a discussion of such constraints in similar scenarios, see also [30,31]). The first constraint we need to consider comes from Big Bang Nucleosynthesis (BBN), which accurately explains the measured primordial abundances of light elements in the Universe 13 (see e.g.…”
Section: Constraints On Dark Matter Freeze-in From Cosmologymentioning
confidence: 98%
See 2 more Smart Citations
“…We note that several works exist in the literature on supersymmetric U (1) extensions of MSSM and their implications on dark matter and collider searches (see, e.g., [29]). Also, several works on signatures of long-lived particles at colliders with freeze-in dark matter have appeared recently [30][31][32][33][34][35] as well as scenarios testing for freeze-in via direct detection [36][37][38][39][40] and indirect detection [41,42]. The analysis of this work is significantly different from these.…”
Section: Introductionmentioning
confidence: 99%