2017
DOI: 10.1007/jhep04(2017)041
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Electroweak Kaluza-Klein dark matter

Abstract: Abstract:In models with universal extra dimensions (UED), the lightest Kaluza-Klein excitation of neutral electroweak gauge bosons is a stable, weakly interacting massive particle and thus is a candidate for dark matter thanks to Kaluza-Klein parity. We examine concrete model realizations of such dark matter in the context of non-minimal UED extensions. The boundary localized kinetic terms for the electroweak gauge bosons lead to a non-trivial mixing among the first Kaluza-Klein excitations of the SU(2) W and … Show more

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Cited by 24 publications
(22 citation statements)
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References 79 publications
(131 reference statements)
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“…In the context of a non-minimal model of universal extra dimensions, enriched by the presence boundary localized kinetic terms [72][73][74], the authors of Ref. [75] were able to give a more stringent bound on the compactification scale: 2.4 TeV R −1 .…”
Section: With Both Cases Taken Intomentioning
confidence: 99%
“…In the context of a non-minimal model of universal extra dimensions, enriched by the presence boundary localized kinetic terms [72][73][74], the authors of Ref. [75] were able to give a more stringent bound on the compactification scale: 2.4 TeV R −1 .…”
Section: With Both Cases Taken Intomentioning
confidence: 99%
“…Additional constraints from cosmology (that the B 1 must have a relic density compatible with the estimated dark matter density from CMB measurements) require the mass of the B 1 to be below ∼1.6 TeV [9,23,31]. Thus, taken all results together, the allowed parameter space for the B 1 to constitute the only component of dark matter in the Universe is currently quite restricted, but non-minimal UED models, not probed here, can still provide viable dark matter candidates [10].…”
Section: Data Selectionmentioning
confidence: 79%
“…(B 1 ), the first excitation of the scalar gauge boson in the theory [5,6,7,8,9,10]. Usually denoted as the lightest Kaluza-Klein particle (LKP), it can have a mass in the range from a few hundred GeV (limit from rare decay processes [11,12]) to a few TeV (to avoid overclosing the Universe), the mass being proportional to 1/R, where R is the size of the extra dimension.…”
Section: Introductionmentioning
confidence: 99%
“…Furthermore, a lot of effort has been put in the investigation of such model from the perspective of DM [40,41], Z-boson decay to b-quarks [42], rare decays of top quarks [43,44], gauge fixing [45], decays of B-meson [46,47] and more recently R(D (⋆) ) anomalies [48]. In [49], authors have done a detailed analysis of KK-dark matter in the light of various experimental constraints. Productions of KK-excitations of the strongly interacting KK-quarks and KK-gluons at the LHC have been investigated in [50].…”
Section: Introductionmentioning
confidence: 99%