2022
DOI: 10.3390/sym14071299
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Review on Higgs Hidden–Dark Sector Physics at High-Energy Colliders

Abstract: The presence of a hidden or dark sector of phenomena that relates either weakly or in a particular way to Standard Model (SM) fields has theoretical as well as experimental support. Many extensions of SM use hidden or dark sector states to propose a specific candidate for dark matter (DM) in the universe or to explain astrophysical findings. If such a family of Beyond the Standard Model (BSM) particles and interactions exists, it is possible that they will be discovered experimentally at CERN’s Large Hadron Co… Show more

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Cited by 3 publications
(2 citation statements)
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“…An understanding of the universe at the most fundamental level has long been an aim of the physics community. The Standard Model stands as the most complete fundamental description of matter and its interactions, yet many phenomena, including the matter-antimatter asymmetry, gravitational interaction, and the neutrino mass [1], are not well-described within the current framework. This has prompted widespread efforts to search for physics beyond the Standard Model (BSM), which would simultaneously show an inconsistency with the current Standard Model picture while also potentially giving credence to one of many proposed theoretical alternatives [2].…”
Section: Introductionmentioning
confidence: 99%
“…An understanding of the universe at the most fundamental level has long been an aim of the physics community. The Standard Model stands as the most complete fundamental description of matter and its interactions, yet many phenomena, including the matter-antimatter asymmetry, gravitational interaction, and the neutrino mass [1], are not well-described within the current framework. This has prompted widespread efforts to search for physics beyond the Standard Model (BSM), which would simultaneously show an inconsistency with the current Standard Model picture while also potentially giving credence to one of many proposed theoretical alternatives [2].…”
Section: Introductionmentioning
confidence: 99%
“…We need more observational clues for the DM model building [4]. In addition to the cosmological searches [5], there are mainly three types of DM searches: direct detection [6][7][8], indirect detection [9][10][11], and collider search [12][13][14][15], to constrain the couplings between the DM and SM particles [4,16,17]. Most of them are given on the DM coupling with nucleons and hence effectively quarks.…”
Section: Introductionmentioning
confidence: 99%