2011
DOI: 10.1103/physrevd.84.051702
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Dark matter in anomalousU(1)models with neutral mixing

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Cited by 3 publications
(4 citation statements)
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“…We choose these ranges because in the SM all the charges are of this order. Furthermore in [5] we have found that −1 Q Hu 1 for the model to be consistent with the WMAP data on dark matter. Then, out of simplicity we have used the same region for the other two charges.…”
Section: Dependence On the Chargessupporting
confidence: 78%
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“…We choose these ranges because in the SM all the charges are of this order. Furthermore in [5] we have found that −1 Q Hu 1 for the model to be consistent with the WMAP data on dark matter. Then, out of simplicity we have used the same region for the other two charges.…”
Section: Dependence On the Chargessupporting
confidence: 78%
“…From the cross section of the process, that can be found in Appendix A, we can see that the amplitude is proportional to the fourth power of the charges. So, the equations (2)- (5) imply that the asymmetry must be a rational function in which both the numerator and denominator are fourth grade polynomials in the charges:…”
Section: General Casementioning
confidence: 99%
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“…Our analysis is restricted to non-anomalous extension of the Standard Model (for the anomalous case see e.g. [69][70][71][72][73][74]). In the analysis that follows we will assume the kinetic mixing is absent and instead investigate the pure Stueckelberg sector in the absence of mass mixing of the hypercharge B with the Stueckelberg sector.…”
Section: Jhep01(2012)038mentioning
confidence: 99%