Direct Detection of Mirror Matter in Twin Higgs Models
Zackaria Chacko, David Curtin, Michael Geller, Yuhsin Tsai

TL;DR
This paper investigates the potential for direct detection experiments to identify mirror baryons and electrons in Twin Higgs models, considering their sub-nano-charged nature and various galactic distributions, to uncover the mirror dark matter's properties.
Contribution
It introduces a framework for detecting sub-nano-charged mirror particles in direct detection experiments, analyzing different galactic distributions and their impact on detection prospects.
Findings
Mirror dark matter could be detected via nuclear and electron recoil experiments.
Different galactic distributions (halo or disk) affect detection rates.
Recoil energy analysis can reveal mirror particle masses and charges.
Abstract
We explore the possibility of discovering the mirror baryons and electrons of the Mirror Twin Higgs model in direct detection experiments, in a scenario in which these particles constitute a subcomponent of the observed DM. We consider a framework in which the mirror fermions are sub-nano-charged, as a consequence of kinetic mixing between the photon and its mirror counterpart. We consider both nuclear recoil and electron recoil experiments. The event rates depend on the fraction of mirror DM that is ionized, and also on its distribution in the galaxy. Since mirror DM is dissipative, at the location of the Earth it may be in the form of a halo or may have collapsed into a disk, depending on the cooling rate. For a given mirror DM abundance we determine the expected event rates in direct detection experiments for the limiting cases of an ionized halo, an ionized disk, an atomic halo and…
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