Techni-dilaton as Dark Matter
Ki-Young Choi, Deog Ki Hong, Shinya Matsuzaki

TL;DR
This paper proposes a new dark matter candidate called the light decoupled techni-dilaton, arising from walking technicolor theories, which is weakly interacting and can account for dark matter in a specific mass range.
Contribution
It introduces the techni-dilaton as a novel dark matter candidate from conformal technicolor models and analyzes its cosmological and astrophysical viability.
Findings
Techni-dilaton is extremely weakly interacting.
Produced mainly through non-thermal mechanisms.
Mass range suitable for dark matter is approximately 0.01 eV to 500 eV.
Abstract
We propose a new dark matter candidate, {\it light decoupled techni-dilaton}, which arises from the almost scale-invariant/conformal (walking) technicolor. We investigate its characteristic nature and discuss several cosmological and astrophysical constraints. It turns out that techni-dilatons are extremely weakly interacting and produced dominantly by the non-thermal mechanism to be the main component of dark matter with mass range between around 0.01 eV and 500 eV for typical walking technicolor scenarios.
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