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arXiv · hep-ph/0610155

Mixed Dark Matter in Universal Extra Dimension Models with TeV Scale $W_{R}$ and $Z'$

Ken Hsieh·R. N. Mohapatra·Salah Nasri
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Abstract

We show that in a class of universal extra dimension (UED) models that solves both the neutrino mass and proton decay problems using low scale left-right symmetry, the dark matter of the Universe consists of an admixture of KK photon and KK right-handed neutrinos. We present a full calculation of the dark matter density in these models taking into account the co-annihilation effects due to near by states such as the scalar partner of the KK photon as well as fermion states near the right-handed KK neutrino. Using the value of the relic CDM density, we obtain upper limits on $R^{-1}$ of about 400-650 GeV and $M_{Z'}\leq 1.5$ TeV, both being accessible to LHC. For a region in this parameter space where the KK right-handed neutrino contributes significantly to the total relic density of dark matter, we obtain a lower bound on the dark matter-nucleon scattering cross section of $10^{-44}$ cm$^2$, which can be probed by the next round of dark matter search experiments.

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Ken Hsieh, R. N. Mohapatra, Salah Nasri. 2006-10-16. Mixed Dark Matter in Universal Extra Dimension Models with TeV Scale $W_{R}$ and $Z'$. https://doi.org/10.1088/1126-6708%2F2006%2F12%2F067

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