Abstract
A dark QCD sector is a relatively minimal extension of the Standard Model
(SM) that admits Dark Matter (DM) candidates but requires no portal to the
visible sector beyond gravitational interactions: A "nightmare scenario" for DM
detection. We consider a secluded dark sector containing a single flavor of
light, vector-like dark quark gauged under $SU(N)$. In the large-$N$ limit,
this single-flavor theory becomes highly predictive, generating two DM
candidates whose masses and dynamics are described by few parameters: A light
quark-antiquark bound state, the dark analog of the $\eta'$ meson, and a heavy
bound state of $N$ quarks, the dark analog of the $\Delta^++$ baryon. We show
that the latter may freeze-in with an abundance independent of the confinement
scale, forming DM-like relics for $N 10$, while the former may
generate DM via cannibalization and freeze-out. We study the interplay of this
two-component DM system and determine the characteristic ranges of the
confinement scale, dark-visible sector temperature ratio, and $N$ that admit
non-excluded DM, once the effects of self-interaction constraints and bounds on
effective degrees of freedom at the BBN and CMB epochs are included.
Users
Please
log in to take part in the discussion (add own reviews or comments).