Composite dark matter from a model with composite Higgs boson
Maxim Yu. Khlopov, Chris Kouvaris

TL;DR
This paper explores a composite dark matter model based on a minimal walking technicolor framework, focusing on techni-O-helium atoms as the primary dark matter component and addressing experimental detection discrepancies.
Contribution
It extends previous work by analyzing mixed dark matter scenarios, cosmological bounds on techniparticle masses, and potential explanations for direct detection experiment discrepancies.
Findings
Techni-O-helium dominates dark matter in the model.
Bound states of techniparticles are a minor dark matter component.
Proposed explanation for DAMA/NaI and DAMA/LIBRA experimental results.
Abstract
In a previous paper \cite{Khlopov:2007ic}, we showed how the minimal walking technicolor model (WTC) can provide a composite dark matter candidate, by forming bound states between a -2 electrically charged techniparticle and a . We studied the properties of these \emph{techni-O-helium} "atoms", which behave as warmer dark matter rather than cold. In this paper we extend our work on several different aspects. We study the possibility of a mixed scenario where both and bound states between +2 and -2 electrically charged techniparticles coexist in the dark matter density. We argue that these newly proposed bound states solely made of techniparticles, although they behave as Weakly Interacting Massive Particles (WIMPs), due to their large elastic cross section with nuclei, can only account for a small percentage of the dark matter density. Therefore we conclude that…
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