Significant effects of second KK particles on LKP dark matter physics
Mitsuru Kakizaki, Shigeki Matsumoto, Yoshio Sato, Masato Senami
TL;DR
In universal extra dimensions, second KK states can significantly modify LKP dark matter physics. By computing the annihilation cross section including the $s$-channel resonance from $h^{(2)}$ and solving the Boltzmann equation, the authors show that the annihilation rate is enhanced, reducing the relic density $ obreak \\Omega h^2$ and shifting the WMAP-compatible LKP mass to about $950$ GeV (roughly $900$–$1000$ GeV for $0.5\%<\delta<2\%$). They also discuss how second KK states affect coannihilation, indirect detection signals, and collider phenomenology, highlighting a robust, intrinsic resonance mechanism in UEDs. This work provides a concrete, testable framework linking KK physics to cosmological relic abundance and to potential observational signatures at colliders and in indirect detection experiments.
Abstract
We point out that Kaluza-Klein (KK) dark matter physics is drastically affected by second KK particles. In this work various interesting phenomena caused by the second KK modes are discussed. In particular, we reevaluate the annihilation cross section and thermal relic density of the KK dark matter quantitatively in universal extra dimensions, in which all the standard model particles propagate. In these models, the first KK mode of $B$ boson is a viable dark matter candidate by virtue of KK-parity. We demonstrate that the KK dark matter annihilation cross section can be enhanced, compared with the tree level cross section mediated only by first KK particles. The dark matter mass consistent with the WMAP observation is increased.
