A Hidden Dark Matter Sector, Dark Radiation, and the CMB
Zackaria Chacko, Yanou Cui, Sungwoo Hong, Takemichi Okui

TL;DR
This paper explores a dark matter model with a hidden sector that contributes to dark radiation, affecting the CMB, and proposes observable signals in upcoming experiments, compatible with current Planck data.
Contribution
It introduces a scenario where dark matter annihilates into hidden sector states, which impact the CMB and can be tested with future cosmological and collider experiments.
Findings
Hidden sector states can contribute to dark radiation detectable via CMB signals.
The model's predictions align with Planck data and are testable by upcoming CMB experiments.
Higgs decays into hidden states provide a collider probe for the scenario.
Abstract
We consider theories where dark matter is composed of a thermal relic of weak scale mass, whose couplings to the Standard Model (SM) are however too small to give rise to the observed abundance. Instead, the abundance is set by annihilation to light hidden sector states that carry no charges under the SM gauge interactions. In such a scenario the constraints from direct and indirect detection, and from collider searches for dark matter, can easily be satisfied. The masses of such light hidden states can be protected by symmetry if they are Nambu-Goldstone bosons, fermions, or gauge bosons. These states can then contribute to the cosmic energy density as dark radiation, leading to observable signals in the cosmic microwave background (CMB). Furthermore, depending on whether or not the light hidden sector states self-interact, the fraction of the total energy density that free-streams is…
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