4–6 May 2015
University of Pittsburgh
US/Eastern timezone

CMB Signals of a Hidden Dark Matter Sector

5 May 2015, 14:00
15m
G26 (University of Pittsburgh)

G26

University of Pittsburgh

Pittsburgh, PA 15260
parallel talk Cosmology III

Speaker

Mr Sungwoo Hong (University of Maryland at College Park)

Description

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 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. If the hidden sector includes Goldstone bosons, fermions or vector gauge bosons, these particles can naturally be light, their masses being protected by symmetries. These states can then contribute to the total energy density in 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 either decreased or increased, leading to characteristic effects on both the scalar and tensor components of the CMB anisotropy. In particular, we show that the locations of the CMB peaks are shifted, with the sign of the shift depending on whether or not these new light hidden sector states carry self-interactions. The magnitude of these signals depends on the number of light degrees of freedom in the hidden sector, and on the temperature at which it kinetically decouples from the SM. We consider a simple model that realizes this scenario, based on a framework in which the SM and hidden sector are initially in thermal equilibrium through the Higgs portal, and show that both the energy density and self-interaction signals can be compatible with recent Planck results, while large enough to be detected in upcoming experiments such as CMBPol and CMB Stage-IV.

Authors

Mr Sungwoo Hong (University of Maryland at College Park) Prof. Takemichi Okui (Florida State University) Dr Yanou Cui (Perimeter Institute for Theoretical Physics) Prof. Zackaria Chacko (University of Maryland at College Park)

Presentation materials