Abstract

Multi-component dark matter scenarios are studied in the model with U(1)X dark gauge symmetry that is broken into its product subgroup Z2 × Z3 á la Krauss-Wilczek mechanism. In this setup, there exist two types of dark matter fields, X and Y, distinguished by different Z2 × Z3 charges. The real and imaginary parts of the Z2-charged field, XR and XI, get different masses from the U(1)X symmetry breaking. The field Y, which is another dark matter candidate due to the unbroken Z3 symmetry, belongs to the Strongly Interacting Massive Particle (SIMP)-type dark matter. Both XI and XR may contribute to Y’s 3 → 2 annihilation processes, opening a new class of SIMP models with a local dark gauge symmetry. Depending on the mass difference between XI and XR, we have either two-component or three-component dark matter scenarios. In particular two- or three-component SIMP scenarios can be realised not only for small mass difference between X and Y, but also for large mass hierarchy between them, which is a new and unique feature of the present model. We consider both theoretical and experimental constraints, and present four case studies of the multi-component dark matter scenarios.

Highlights

  • The current Universe is composed of only one component

  • Multi-component dark matter scenarios are studied in the model with U(1)X dark gauge symmetry that is broken into its product subgroup Z2 × Z3 á la Krauss-Wilczek mechanism

  • Even if the dark sector of the current Universe is dominated by a singlecomponent DM, there could be more DM species in the earlier Universe that would modify the evolution of the early Universe

Read more

Summary

Generalities

We have four coupled Boltzmann equations for describing the evolution of the system consisting of {Y, XI , XR, Z }.6. The Boltzmann equation for the species i is given by ni + 3Hni = − Γ i→j,k ni nei q nj nk nej q nekq. Where ni (neiq) is the (equilibrium) number density of the species i, H the Hubble parameter, and ≡ d/dt with t being the cosmic time. Σv and σv are the thermally-averaged cross sections, and Γ is the thermallyaveraged decay rate. The thermally-averaged cross section σv for the i, j → l, m process

F spins
Two-component scenario
Three-component scenario
Conclusions
A Three-body decay of XR
Findings
B The full Boltzmann equations
Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call