2011
DOI: 10.1007/jhep02(2011)100
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Dark matter and a new gauge boson through kinetic mixing

Abstract: We consider a hidden sector model of dark matter which is charged under a hidden U(1)_X gauge symmetry. Kinetic mixing of U(1)_X with the Standard Model hypercharge U(1)_Y is allowed to provide communication between the hidden sector and the Standard Model sector. We present various limits on the kinetic mixing parameter and the hidden gauge coupling constant coming from various low energy observables, electroweak precision tests, and the right thermal relic density of the dark matter. Saturating these constra… Show more

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Cited by 116 publications
(121 citation statements)
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“…It could be interesting to notice that in any of the cases discussed above, the direct detection rate is largely suppressed. Indeed, this rate can become important for a kinetic mixing around δ ≃ 10 −3 [29][30][31][32][33] and could even explain DAMA/CoGENT excess with δ ≃ 10 −2 . However, in the model we are considering, the "portal" between the dark matter sector and the visible one does not go through this kinetic mixing, but through the trivectorial couplings generated in eq.…”
Section: Z ′ < M ψmentioning
confidence: 96%
See 1 more Smart Citation
“…It could be interesting to notice that in any of the cases discussed above, the direct detection rate is largely suppressed. Indeed, this rate can become important for a kinetic mixing around δ ≃ 10 −3 [29][30][31][32][33] and could even explain DAMA/CoGENT excess with δ ≃ 10 −2 . However, in the model we are considering, the "portal" between the dark matter sector and the visible one does not go through this kinetic mixing, but through the trivectorial couplings generated in eq.…”
Section: Z ′ < M ψmentioning
confidence: 96%
“…The Dark Matter (DM) candidate ψ 0 could be the lightest (and thus stable) particle of this secluded sector. Such a mixing has been justified in recent string constructions [18][19][20][21][22], but has also been studied within a model independent approach [23][24][25][26][27][28][29][30][31][32][33] or in a supersymmetric extension [34][35][36][37].…”
Section: Introductionmentioning
confidence: 99%
“…It leads to several consequences, most importantly, the possibility of detecting the DM particles in the laboratory [21]. Barring the possibility of fine tuning, the predicted DM cross section would be within reach for the next generation of DM direct detection experiments.…”
Section: Jhep10(2015)046mentioning
confidence: 99%
“…For a vector interaction the only quarks that play a role are those of the valence (up and down), while for a scalar interaction the sea quarks are also important for the entire process. Since the up and down quarks are not present in the proton and neutron in the same fraction, one can express f p and f n as follows [57],…”
Section: Si Interactionsmentioning
confidence: 99%