Partially acoustic dark matter, interacting dark radiation, and large scale structure

Chacko, Zackaria; Cui, Yanou; Hong, Sungwoo; Okui, Takemichi; Tsai, Yuhsinz

doi:10.1007/JHEP12(2016)108

Title: Partially acoustic dark matter, interacting dark radiation, and large scale structure

Journal Article · Wed Dec 21 00:00:00 EST 2016 · Journal of High Energy Physics (Online)

DOI:https://doi.org/10.1007/JHEP12(2016)108· OSTI ID:1368037

Chacko, Zackaria ^[1]; Cui, Yanou ^[2]; Hong, Sungwoo ^[1]; Okui, Takemichi ^[3]; Tsai, Yuhsinz ^[1]

Univ. of Maryland, College Park, MD (United States). Dept. of Physics. Maryland Center for Fundamental Physics
Univ. of Maryland, College Park, MD (United States). Dept. of Physics. Maryland Center for Fundamental Physics; Univ. of California, Riverside, CA (United States). Dept. of Physics and Astronomy; Perimeter Inst., North Waterloo, ON (Canada)
Florida State Univ., Tallahassee, FL (United States). Dept. of Physics

The standard paradigm of collisionless cold dark matter is in tension with measurements on large scales. In particular, the best fit values of the Hubble rate H₀ and the matter density perturbation σ₈ inferred from the cosmic microwave background seem inconsistent with the results from direct measurements. We show that both problems can be solved in a framework in which dark matter consists of two distinct components, a dominant component and a subdominant component. The primary component is cold and collisionless. The secondary component is also cold, but interacts strongly with dark radiation, which itself forms a tightly coupled fluid. The growth of density perturbations in the subdominant component is inhibited by dark acoustic oscillations due to its coupling to the dark radiation, solving the σ₈ problem, while the presence of tightly coupled dark radiation ameliorates the H₀ problem. The subdominant component of dark matter and dark radiation continue to remain in thermal equilibrium until late times, inhibiting the formation of a dark disk. We present an example of a simple model that naturally realizes this scenario in which both constituents of dark matter are thermal WIMPs. Our scenario can be tested by future stage-IV experiments designed to probe the CMB and large scale structure.

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Research Organization:: Florida State Univ., Tallahassee, FL (United States); Univ. of Maryland, College Park, MD (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF)

Contributing Organization:: Univ. of California, Riverside, CA (United States); Perimeter Inst., North Waterloo, ON (Canada)

Grant/Contract Number:: SC0010102; PHY-1315155; PHY-1066293

OSTI ID:: 1368037

Journal Information:: Journal of High Energy Physics (Online), Vol. 2016, Issue 12; ISSN 1029-8479

Publisher:: Springer BerlinCopyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 60 works

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